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Log canonical models and variation of GIT for genus four canonical curves

Sebastian Casalaina-Martin University of Colorado, Department of Mathematics, Boulder, CO 80309-0395 casa@math.colorado.edu David Jensen Stony Brook University, Department of Mathematics, Stony Brook, NY 11794 djensen@math.sunysb.edu  and  Radu Laza Stony Brook University, Department of Mathematics, Stony Brook, NY 11794 rlaza@math.sunysb.edu
(Date: July 25, 2025)
Abstract.

We discuss GIT for canonically embedded genus four curves and the connection to the Hassett–Keel program. A canonical genus four curve is a complete intersection of a quadric and a cubic, and, in contrast to the genus three case, there is a family of GIT quotients that depend on a choice of linearization. We discuss the corresponding VGIT problem and show that the resulting spaces give the final steps in the Hassett–Keel program for genus four curves.

The first author was partially supported by NSF grant DMS-1101333. The third author was partially supported by NSF grant DMS-0968968 and a Sloan Fellowship

Introduction

The Hassett–Keel program aims to give modular interpretations of certain log canonical models of M¯g\overline{M}_{g}, the moduli space of stable curves of fixed genus gg, with the ultimate goal of giving a modular interpretation of the canonical model for the case g0g\gg 0. The program, while relatively new, has attracted the attention of a number of researchers, and has rapidly become one of the most active areas of research concerning the moduli of curves. Perhaps the most successful approach so far has been to compare these log canonical models to alternate compactifications of MgM_{g} constructed via GIT on the spaces Hilbg,νm\operatorname{Hilb}_{g,\nu}^{m}, the so-called mm-th Hilbert spaces of ν\nu-canonically embedded curves of genus gg, for “small” ν\nu and mm (e.g. [HH09], [HH08], [AH12]).

For large genus, completing the program in its entirety still seems somewhat out of reach. On the other hand, the case of low genus curves affords a gateway to the general case, providing motivation and corroboration of expected behavior. The genus 22 and 33 cases were completed recently ([Has05], [HL10b]). In this paper, we study the genus 44 case by focusing on the spaces Hilb4,1m\operatorname{Hilb}_{4,1}^{m}; i.e. we study GIT quotients of canonically embedded genus 44 curves. The main result is a complete description of GIT stability on Hilb4,1m\operatorname{Hilb}_{4,1}^{m} for all mm, as well as a proof that the resulting GIT quotients give the final steps in the Hassett–Keel program for genus 44. Together with previous work on the subject (see [HL10a], [Fed12], [CMJL12]), this completes the program in genus 44 outside of a small range.

One of the key features of this paper is the technique employed. Using a space we denote by E\mathbb{P}E (a smooth, elementary, birational model of the Hilbert scheme parameterizing complete intersections) we fit all of the Hilbert quotients for canonical genus 44 curves into a single variation of GIT problem (VGIT). In other words, the final steps of the Hassett–Keel program in genus 44 are described by a VGIT problem on a single space. Also of interest is a technical point that arises: we are forced to do VGIT for linearizations that lie outside of the ample cone. A priori this leads to an ambiguity in the meaning of Mumford’s numerical criterion for stability. However we are able to circumvent this issue to provide a complete analysis of the stability conditions on E\mathbb{P}E.

While examples of GIT for hypersurfaces are abundant in the literature (e.g. [MFK94, §4.2], [Sha80], [All03], [Laz09]), this appears to be one of the first examples of GIT for complete intersections (see however [AM99] and [MM93] for (2,2)(2,2) complete intersections, and Benoist [Ben11] for some generic stability results in a situation similar to ours). Furthermore, unlike the projective spaces parameterizing hypersurfaces or the Grassmannian parameterizing complete intersections of type (d,,d)(d,\dots,d), the natural parameter space in our situation has Picard rank two, and thus provides a natural setting for variation of GIT. We believe the techniques we develop in this paper for studying VGIT for spaces of complete intersections will have a number of further applications beyond moduli spaces of curves.

The Hassett–Keel program for genus 44 curves: known and new results

To put our results in context, we recall some background on the Hassett–Keel program. Namely, for α[0,1]\alpha\in[0,1], the log minimal models of M¯g\overline{M}_{g} are defined to be the projective varieties

M¯g(α):=Proj(n=0H0(n(KM¯g+αδ))),\overline{M}_{g}(\alpha):=\operatorname{Proj}\left(\bigoplus_{n=0}^{\infty}H^{0}\left(n(K_{\overline{M}_{g}}+\alpha\delta)\right)\right),

where δ\delta is the boundary divisor in M¯g\overline{M}_{g}. Hassett and Hyeon have explicitly constructed the log minimal models M¯g(α)\overline{M}_{g}(\alpha) for α710ϵ\alpha\geq\frac{7}{10}-\epsilon (see [HH09, HH08]). Hyeon and Lee have also described the next stage of the program in the specific case that g=4g=4 (see [HL10a]): as α\alpha decreases from 23+ϵ\frac{2}{3}+\epsilon to 23\frac{2}{3}, they construct a map that contracts the locus of Weierstrass genus 2 tails, replacing them with A4A_{4} singularities. Thus, the known spaces for the Hassett–Keel program in genus 44 are:

(0.1) M¯4=M¯4[1,911)\textstyle{\overline{M}_{4}=\overline{M}_{4}[1,\frac{9}{11})\ignorespaces\ignorespaces\ignorespaces\ignorespaces}M¯4ps=M¯4[911,710)\textstyle{\overline{M}_{4}^{ps}=\overline{M}_{4}[\frac{9}{11},\frac{7}{10})\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces}M¯4hs=M¯4(710,23)\textstyle{\overline{M}_{4}^{hs}=\overline{M}_{4}(\frac{7}{10},\frac{2}{3})\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces}M¯4cs=M¯4(710)\textstyle{\overline{M}_{4}^{cs}=\overline{M}_{4}(\frac{7}{10})}M¯4(23)\textstyle{\overline{M}_{4}(\frac{2}{3})}

where the notation M¯g(I)\overline{M}_{g}(I) for an interval II means M¯g(α)M¯g(β)\overline{M}_{g}(\alpha)\cong\overline{M}_{g}(\beta) for all α,βI\alpha,\beta\in I. The double arrows correspond to divisorial contractions, the single arrows to small contractions, and the dashed arrows to flips.

The main result of the paper is the construction of the log minimal models M¯4(α)\overline{M}_{4}(\alpha) for α59\alpha\leq\frac{5}{9} via a VGIT analysis of canonically embedded curves in 3\mathbb{P}^{3}.

Main Theorem.

For α59\alpha\leq\frac{5}{9}, the log minimal models M¯4(α)\overline{M}_{4}(\alpha) arise as GIT quotients of the parameter space E\mathbb{P}E. Moreover, the VGIT problem gives us the following diagram:

(0.2) M¯4(59,2344)\textstyle{\overline{M}_{4}(\frac{5}{9},\frac{23}{44})\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces}M¯4(2344,12)\textstyle{\overline{M}_{4}(\frac{23}{44},\frac{1}{2})\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces}M¯4(12,2960)\textstyle{\overline{M}_{4}(\frac{1}{2},\frac{29}{60})\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces}M¯4(59)\textstyle{\overline{M}_{4}(\frac{5}{9})}M¯4(2344)\textstyle{\overline{M}_{4}(\frac{23}{44})}M¯4(12)\textstyle{\overline{M}_{4}(\frac{1}{2})}M¯4[2960,817)\textstyle{\overline{M}_{4}[\frac{29}{60},\frac{8}{17})\ignorespaces\ignorespaces\ignorespaces\ignorespaces}M¯4(817)={}\textstyle{\overline{M}_{4}(\frac{8}{17})=\{*\}}

More specifically,

  • i)

    the end point M¯4(817+ϵ)\overline{M}_{4}(\frac{8}{17}+\epsilon) is obtained via GIT for (3,3)(3,3) curves on 1×1\mathbb{P}^{1}\times\mathbb{P}^{1} as discussed in [Fed12];

  • ii)

    the other end point M¯4(59)\overline{M}_{4}(\frac{5}{9}) is obtained via GIT for the Chow variety of genus 4 canonical curves as discussed in [CMJL12];

  • iii)

    the remaining spaces M¯4(α)\overline{M}_{4}(\alpha) for α\alpha in the range 817<α<59\frac{8}{17}<\alpha<\frac{5}{9} are obtained via appropriate Hilb4,1m\operatorname{Hilb}^{m}_{4,1} quotients, with the exception of α=2344\alpha=\frac{23}{44}.

Thus in genus 44, the remaining unknown range for the Hassett–Keel program is the interval α(59,23)\alpha\in(\frac{5}{9},\frac{2}{3}). Using the geometric meaning of the spaces M¯4(α)\overline{M}_{4}(\alpha) for α59\alpha\leq\frac{5}{9} and the predictions of [AFS10], we expect that there are exactly two more critical values: α=1929\alpha=\frac{19}{29}, when the divisor δ2\delta_{2} should be contracted to a point, and α=4983\alpha=\frac{49}{83}, when the locus of curves with hyperelliptic normalization obtained by introducing a cusp at a Weierstrass point should be flipped, being replaced by curves with A6A_{6} singularities. We do not expect that these models can be obtained by further varying the GIT problem we consider here. In fact, since each of these predicted models arises prior to the predicted flip of the hyperelliptic locus (α=59\alpha=\frac{5}{9}), they should be unrelated to spaces of canonical curves. It is believed that each of these two intermediate models ought to correspond to a quotient of the Hilbert scheme of bicanonical curves.

GIT for canonical genus 44 curves

As already mentioned, GIT for pluricanonical curves has long been used to produce projective models for the moduli space of curves. For example Mumford used asymptotic stability for ν\nu-canonical curves, with ν5\nu\geq 5, to show the projectivity of M¯g\overline{M}_{g}, and recently the case ν<5\nu<5 has been used in the Hassett–Keel program. The basic idea is that as the values ν\nu and mm decrease one should obtain the log minimal models M¯g(α)\overline{M}_{g}(\alpha) for progressively smaller values of α\alpha (e.g. [FS10, Table 1]). Thus from the perspective of the Hassett–Keel program, it is of interest to understand GIT for canonically embedded curves. This turns out to be difficult, and to our knowledge the only case where the stability conditions have been described completely prior to this paper is for genus 33. On the other hand, it was recently proved (see [AFS12]) that the generic non-singular canonical curve of arbitrary genus is stable. In this paper, we completely describe the stability conditions for genus 44 canonical curves.

We set up the analysis of the GIT stability for canonical genus 44 curves as follows. The canonical model of a smooth, non-hyperelliptic genus 44 curve is a (2,3)(2,3)-complete intersection in 3\mathbb{P}^{3}. A natural parameter space for complete intersections is a projective bundle E9\mathbb{P}E\to\mathbb{P}^{9} on which G=SL(4,)G=\mathrm{SL}(4,\mathbb{C}) acts naturally. Since rank(Pic(E))=2\mathrm{rank}(\operatorname{Pic}(\mathbb{P}E))=2, the GIT computation involves a choice of linearization parameterized by t+{0}t\in\mathbb{Q}_{+}\cup\{0\} (corresponding to the linearization η+th\eta+th, where η\eta is the pullback of 𝒪(1)\mathscr{O}(1) from the space of quadrics 9\mathbb{P}^{9} and hh is the relative 𝒪(1)\mathscr{O}(1)). In this paper, we analyze the geometry of the quotients E//tSL(4)\mathbb{P}E/\!\!/_{t}\mathrm{SL}(4) as the linearization varies and relate them to the Hassett–Keel spaces M¯(α)\overline{M}(\alpha). We note that a related setup for GIT for complete intersections occurs in recent work of Benoist [Ben11].

One naturally identifies two special cases. First, for 0<t10<t\ll 1 one easily sees that E//tSL(4)\mathbb{P}E/\!\!/_{t}\mathrm{SL}(4) coincides with the GIT quotient for (3,3)(3,3) curves on 1×1\mathbb{P}^{1}\times\mathbb{P}^{1}; this was analyzed by Fedorchuk [Fed12]. At the other extreme, the case t=23t=\frac{2}{3} was shown in [CMJL12] to be isomorphic to both the quotient of the Chow variety for genus 44 canonical curves, as well as to the Hassett–Keel space M¯4(59)\overline{M}_{4}(\frac{5}{9}). The content of this paper is to describe the GIT quotient for the intermediary values t(0,23)t\in(0,\frac{2}{3}). We work with E\mathbb{P}E, but show that all of the quotients of type Hilb4,1m//SL(4)\operatorname{Hilb}^{m}_{4,1}/\!\!/\mathrm{SL}(4) arise in this way. The advantage of working with E\mathbb{P}E is that we have VGIT on a single, elementary space, where the stability computation is straightforward and corresponds directly to the variation of parameters.

Geometric description of the birational maps in the main theorem

As mentioned, the Hassett–Keel program aims to give modular interpretations to the spaces M¯g(α)\overline{M}_{g}(\alpha) and to the birational maps between them. Essentially, as α\alpha decreases, it is expected that M¯g(α)\overline{M}_{g}(\alpha) parameterizes curves with increasingly complicated singularities, and at the same time special curves from M¯g\overline{M}_{g} are removed (e.g. curves with elliptic tails, or hyperelliptic curves, etc.). In the situation of our main result, the maps of the diagram (0.2) are intuitively described as follows. In M¯4(59)\overline{M}_{4}(\frac{5}{9}), the hyperelliptic locus is contracted, as is the locus of elliptic triboroughs, and the locus of curves in Δ0\Delta_{0} with hyperelliptic normalization obtained by gluing two points that are conjugate under the hyperelliptic involution. The next map flips these loci, replacing them with curves that have A8A_{8}, D4D_{4}, and A7A_{7} singularities, respectively.

The second flip (at α=2344\alpha=\frac{23}{44}) removes the locus of cuspidal curves whose normalization is hyperelliptic, replacing them with curves possessing a separating A7A_{7} singularity. The third flip (at α=12\alpha=\frac{1}{2}) removes the locus of nodal curves whose normalization is hyperelliptic, replacing them with the union of a conic and a double conic. Finally, the map to M¯4(2960)\overline{M}_{4}(\frac{29}{60}) contracts the Gieseker–Petri divisor to a point, corresponding to a triple conic. This geometric description of the various maps is summarized in Tables 2 and 3 in §3.

We note that the critical slopes occurring in our analysis are in concordance with the general predictions of Alper–Fedorchuk–Smyth [AFS10]. We also note that at α=59\alpha=\frac{5}{9} and α=2344\alpha=\frac{23}{44}, we observe a phenomenon that first occurs in genus 44. Namely, the critical values at which the separating A5A_{5} and A7A_{7} singularities appear differ from those at which the non-separating singularities appear.

Acknowldegements

The authors are grateful to O. Benoist and M. Fedorchuk for discussions relevant to this paper, and for specific comments on an earlier draft. We also thank the referees for detailed comments that have improved the paper.

Table of spaces

The following table, relating the parameters α\alpha, tt and mm, describes the relationships among the various spaces occurring in this paper. Note that the following relations (see Proposition 1.8 and Theorem 7.1) hold:

t=34α1633α14,α=14t1633t34,t={m2m+12m4,2m28m+83m29m+8m5.t=\frac{34\alpha-16}{33\alpha-14},\ \ \alpha=\frac{14t-16}{33t-34},\ \ t=\left\{\begin{array}[]{ll}\frac{m-2}{m+1}&2\leq m\leq 4,\\ &\\ \frac{2m^{2}-8m+8}{3m^{2}-9m+8}&m\geq 5.\\ \end{array}\right.
M¯g(α)E//tSL(4)mHilb4,1m//ΛmSL(4)Other5923Chow4,1//ΛSL(4)(2344,59)(611,23)(17+1294,)8234461117+1294(12,2344)(25,611)(4,17+1294)5,6,7122544(2960,12)(29,25)(207,4)3(817,2960](0,29](2,207]|𝒪1×1(3,3)|//SO(4)817022\begin{array}[]{|c|c|c|c|c|}\hline\cr\overline{M}_{g}(\alpha)&\mathbb{P}E/\!\!/_{t}\mathrm{SL}(4)&m&\operatorname{Hilb}_{4,1}^{m}/\!\!/_{\Lambda_{m}}\mathrm{SL}(4)&\text{Other}\\ \hline\cr\hline\cr\frac{5}{9}&\frac{2}{3}&\infty&-&\operatorname{Chow}_{4,1}/\!\!/_{\Lambda_{\infty}}\mathrm{SL}(4)\\ \hline\cr\left(\frac{23}{44},\frac{5}{9}\right)&\left(\frac{6}{11},\frac{2}{3}\right)&\left(\frac{17+\sqrt{129}}{4},\infty\right)&\geq 8&\\ \hline\cr\frac{23}{44}&\frac{6}{11}&\frac{17+\sqrt{129}}{4}&-&\\ \hline\cr\left(\frac{1}{2},\frac{23}{44}\right)&\left(\frac{2}{5},\frac{6}{11}\right)&\left(4,\frac{17+\sqrt{129}}{4}\right)&5,6,7&\\ \hline\cr\frac{1}{2}&\frac{2}{5}&4&4&\\ \hline\cr\left(\frac{29}{60},\frac{1}{2}\right)&\left(\frac{2}{9},\frac{2}{5}\right)&\left(\frac{20}{7},4\right)&3&\\ \hline\cr\left(\frac{8}{17},\frac{29}{60}\right]&\left(0,\frac{2}{9}\right]&\left(2,\frac{20}{7}\right]&-&\left|\mathscr{O}_{\mathbb{P}^{1}\times\mathbb{P}^{1}}(3,3)\right|/\!\!/\mathrm{SO}(4)\\ \hline\cr\frac{8}{17}&0&2&2&\\ \hline\cr\end{array}
Table 1. Relationship among the spaces appearing in this paper.

1. E\mathbb{P}E and its geometry

In this section we recall the projective bundle E\mathbb{P}E considered in [CMJL12] (see also [Ben11] for a more general setup) parameterizing subschemes of 3\mathbb{P}^{3} defined by a quadric and a cubic. The primary aim is to describe various rational maps from E\mathbb{P}E to projective space and their induced polarizations in terms of standard generators for the Picard group.

1.1. Preliminaries

We start by recalling the definition of the bundle E\mathbb{P}E from [CMJL12] and establishing some basic properties. We fix the notation

Vd:=H0(3,𝒪3(d))V_{d}:=H^{0}(\mathbb{P}^{3},\mathscr{O}_{\mathbb{P}^{3}}(d))

for each dd\in\mathbb{Z}, and define 𝒬\mathcal{Q} to be the universal quadric:

𝒬3×V2π2V2=V2.\begin{CD}\mathcal{Q}@>{}>{}>\mathbb{P}^{3}\times\mathbb{P}V_{2}\\ @V{}V{}V@V{}V{\pi_{2}}V\\ \mathbb{P}V_{2}=\mathbb{P}V_{2}.\end{CD}

There is an exact sequence of sheaves

(1.1) 0𝒬𝒪3×V2𝒪𝒬0.0\to\mathcal{I}_{\mathcal{Q}}\to\mathscr{O}_{\mathbb{P}^{3}\times\mathbb{P}V_{2}}\to\mathscr{O}_{\mathcal{Q}}\to 0.

Setting π1:3×V23\pi_{1}:\mathbb{P}^{3}\times\mathbb{P}V_{2}\to\mathbb{P}^{3} (resp. π2:3×V2V2\pi_{2}:\mathbb{P}^{3}\times\mathbb{P}V_{2}\to\mathbb{P}V_{2}) to be the first (resp. second) projection, then tensoring (1.1) by π1𝒪3(3)\pi_{1}^{*}\mathscr{O}_{\mathbb{P}^{3}}(3) and projecting with π2\pi_{2*} we obtain an exact sequence:

(1.2) 0π2(𝒬π1𝒪3(3))π2(π1𝒪3(3))π2(𝒪𝒬π1𝒪3(3))0.0\to\pi_{2*}(\mathcal{I}_{\mathcal{Q}}\otimes\pi_{1}^{*}\mathcal{O}_{\mathbb{P}^{3}}(3))\to\pi_{2*}(\pi_{1}^{*}\mathcal{O}_{\mathbb{P}^{3}}(3))\to\pi_{2*}(\mathscr{O}_{\mathcal{Q}}\otimes\pi_{1}^{*}\mathcal{O}_{\mathbb{P}^{3}}(3))\to 0.

We will define the projective bundle E\mathbb{P}E using the locally free sheaf on the right.

Definition 1.3.

In the notation above, let :=π2(𝒪𝒬π1𝒪3(3))\mathscr{E}:=\pi_{2*}(\mathscr{O}_{\mathcal{Q}}\otimes\pi_{1}^{*}\mathcal{O}_{\mathbb{P}^{3}}(3)), E:=Spec¯V2()E:=\underline{\operatorname{Spec}}_{\mathbb{P}V_{2}}(\mathscr{E}^{\vee}) and E:=Proj¯V2()\mathbb{P}E:=\underline{\operatorname{Proj}}_{\mathbb{P}V_{2}}(\mathscr{E}^{\vee}). We denote the natural projection as π:EV2\pi:\mathbb{P}E\to\mathbb{P}V_{2}.

Remark 1.4.

Points of E\mathbb{P}E correspond to pairs ([q],[f])([q],[f]) where [q]V2[q]\in\mathbb{P}V_{2} is the class of a non-zero element qV2q\in V_{2}, and [f]E[q][f]\in\mathbb{P}E_{[q]} is the class of a non-zero element fV3/x0q,x1q,x2q,x3qf\in V_{3}/\langle x_{0}q,x_{1}q,x_{2}q,x_{3}q\rangle. Sometimes we will instead consider ff as an element of V3V_{3} not lying in the span of x0q,x1q,x2q,x3q\langle x_{0}q,x_{1}q,x_{2}q,x_{3}q\rangle. We will often write (q,f)(q,f) rather than ([q],[f])([q],[f]) if there is no chance of confusion. This description motivates calling E\mathbb{P}E the space of (2,3)(2,3)-subschemes in 3\mathbb{P}^{3}. Throughout, we will write UEU\subset\mathbb{P}E for the open subset of points (q,f)(q,f) such that qq and ff do not have a common factor. Note there is a non-flat family of sub-schemes of 3\mathbb{P}^{3} over E\mathbb{P}E that restricts to a flat family over UU.

We point out that

(1.5) π2(π1𝒪3(3))V3𝒪V2and π2(𝒬π1𝒪3(3)))V1𝒪V2(1),\pi_{2*}(\pi_{1}^{*}\mathcal{O}_{\mathbb{P}^{3}}(3))\cong V_{3}\otimes_{\mathbb{C}}\mathscr{O}_{\mathbb{P}V_{2}}\ \ \text{and }\ \ \pi_{2\ast}\left(\mathcal{I}_{\mathcal{Q}}\otimes\pi_{1}^{*}\mathcal{O}_{\mathbb{P}^{3}}(3))\right)\cong V_{1}\otimes_{\mathbb{C}}\mathscr{O}_{\mathbb{P}V_{2}}(-1),

so (1.2) can be written as

(1.6) 0V1𝒪V2(1)V3𝒪V20.0\to V_{1}\otimes_{\mathbb{C}}\mathscr{O}_{\mathbb{P}V_{2}}(-1)\to V_{3}\otimes_{\mathbb{C}}\mathscr{O}_{\mathbb{P}V_{2}}\to\mathscr{E}\to 0.
Remark 1.7.

With this description of \mathscr{E}, it is easy to describe many of the invariants of EE and E\mathbb{P}E. Setting x=c1(𝒪V2(1))x=c_{1}(\mathscr{O}_{\mathbb{P}V_{2}}(1)), the Chern character of EE is ch(E)=204k=0(1)kxkk!\operatorname{ch(E)}=20-4\sum_{k=0}^{\infty}\frac{(-1)^{k}x^{k}}{k!}. Denoting the line bundles η=π𝒪V2(1)\eta=\pi^{*}\mathscr{O}_{\mathbb{P}V_{2}}(1) and h=𝒪E(1)h=\mathscr{O}_{\mathbb{P}E}(1), it is standard that Pic(E)ηh\operatorname{Pic}(\mathbb{P}E)\cong\mathbb{Z}\eta\oplus\mathbb{Z}h, and

KE=14η16h.K_{\mathbb{P}E}=-14\eta-16h.

We define the slope of a line bundle aη+bha\eta+bh (with a0a\neq 0) to be equal to t=bat=\frac{b}{a}.

1.2. Morphisms to projective space

As mentioned above, there is a family

𝒞3×Eπ2E=E.\begin{CD}\mathcal{C}@>{}>{}>\mathbb{P}^{3}\times\mathbb{P}E\\ @V{}V{}V@V{}V{\pi_{2}}V\\ \mathbb{P}E=\mathbb{P}E.\end{CD}

of (2,3)(2,3)-subschemes of 3\mathbb{P}^{3} parameterized by E\mathbb{P}E that is flat exactly over the locus UU of points ([q],[f])([q],[f]) such that qq and ff do not have a common linear factor. Consequently, there is a birational map

EHilb4,1\mathbb{P}E\dashrightarrow\operatorname{Hilb}_{4,1}

whose restriction to UU is a morphism; here Hilb4,1\operatorname{Hilb}_{4,1} is the component of the Hilbert scheme containing genus 44 canonical curves.

1.2.1. The moduli space of curves

The rational map Hilb4,1M¯4\operatorname{Hilb}_{4,1}\dashrightarrow\overline{M}_{4} induces a rational map

EM¯4.\mathbb{P}E\dashrightarrow\overline{M}_{4}.

Setting λ\lambda and δ\delta to be the pull-backs of the corresponding classes on M¯4\overline{M}_{4} one can check (e.g. [CMJL12, §1]) that

λ\displaystyle\lambda =\displaystyle= 4η+4h,\displaystyle 4\eta+4h,
δ\displaystyle\delta =\displaystyle= 33η+34h.\displaystyle 33\eta+34h.

Conversely, η=172λδ\eta=\frac{17}{2}\lambda-\delta and h=334λ+δh=-\frac{33}{4}\lambda+\delta.

1.2.2. Grassmannians

For each point in Hilb4,1\operatorname{Hilb}_{4,1}, we have an associated ideal sheaf 𝒪3\mathcal{I}\subseteq\mathscr{O}_{\mathbb{P}^{3}}. The generic point of Hilb4,1\operatorname{Hilb}_{4,1} corresponds to a canonical curve, so that \mathcal{I} is the sheaf associated to a homogeneous ideal of the form (q,f)[X0,,X3](q,f)\subseteq\mathbb{C}[X_{0},\ldots,X_{3}] where qq is a quadric and ff is a cubic. Since qq and ff have no common irreducible factors in this case, we get the following resolution of the ideal sheaf \mathcal{I}:

0𝒪3(5)(f,q)𝒪3(2)𝒪3(3)(qf)0.0\longrightarrow\mathscr{O}_{\mathbb{P}^{3}}(-5)\stackrel{{\scriptstyle(f,-q)}}{{\longrightarrow}}\mathscr{O}_{\mathbb{P}^{3}}(-2)\oplus\mathscr{O}_{\mathbb{P}^{3}}(-3)\stackrel{{\scriptstyle\binom{q}{f}}}{{\longrightarrow}}\mathcal{I}\longrightarrow 0.

It follows that

km:=h0((m))=(m+13)+(m3)(m23).k_{m}:=h^{0}(\mathcal{I}(m))=\binom{m+1}{3}+\binom{m}{3}-\binom{m-2}{3}.

Set

nm=h0(𝒪3(m))=(m+33).n_{m}=h^{0}(\mathscr{O}_{\mathbb{P}^{3}}(m))=\binom{m+3}{3}.

With this notation, there is a rational map ψm:Hilb4,1𝔾(km,nm)\psi_{m}:\operatorname{Hilb}_{4,1}\dashrightarrow\mathbb{G}(k_{m},n_{m}), and recall that Hilb4,1m\operatorname{Hilb}_{4,1}^{m} is defined to be the closure of the image of ψm\psi_{m}. The Plücker embedding induces a linearization Λm\Lambda_{m} on Hilb4,1m\operatorname{Hilb}_{4,1}^{m}. Composing the rational map EHilb4,1\mathbb{P}E\dashrightarrow\operatorname{Hilb}_{4,1} with ψm\psi_{m} defines a rational map

φm:EHilb4,1m\varphi_{m}:\mathbb{P}E\dashrightarrow\operatorname{Hilb}_{4,1}^{m}

that restricts to a morphism on the open set UEU\subseteq\mathbb{P}E.

Since E\mathbb{P}E is smooth, and codimE(EU)2\operatorname{codim}_{\mathbb{P}E}(\mathbb{P}E\setminus U)\geq 2, each line bundle on UU has a unique extension to a line bundle on E\mathbb{P}E; in other words, the restriction map Pic(E)Pic(U)\operatorname{Pic}(\mathbb{P}E)\to\operatorname{Pic}(U) is an isomorphism. Since the restriction of φm\varphi_{m} to UU is regular, there is a well defined pull-back

φm:Pic(Hilb4,1m)Pic(E)\varphi_{m}^{*}:\operatorname{Pic}(\operatorname{Hilb}^{m}_{4,1})\to\operatorname{Pic}(\mathbb{P}E)

given by the composition Pic(Hilb4,1m)(φm|U)Pic(U)Pic(E)\operatorname{Pic}(\operatorname{Hilb}^{m}_{4,1})\xrightarrow{(\varphi_{m}|_{U})^{*}}\operatorname{Pic}(U)\to\operatorname{Pic}(\mathbb{P}E).

Proposition 1.8.

For all mm\in\mathbb{N} there is a rational map

φm:EHilb4,1m\varphi_{m}:\mathbb{P}E\dashrightarrow\operatorname{Hilb}_{4,1}^{m}

that restricts to a morphism on the open set UEU\subseteq\mathbb{P}E of points ([q],[f])([q],[f]) such that qq and ff do not have a common linear factor. The pull-back of the polarization Λm\Lambda_{m} on Hilb4,1m\operatorname{Hilb}_{4,1}^{m} is given by the formula

φmΛm=((m+13)(m23))η+((m3)(m23))h,\varphi_{m}^{*}\Lambda_{m}=\left(\binom{m+1}{3}-\binom{m-2}{3}\right)\eta+\left(\binom{m}{3}-\binom{m-2}{3}\right)h,

where we use the convention that (ab)=0\binom{a}{b}=0 if a<ba<b. In particular, the slope of φmΛm\varphi^{*}_{m}\Lambda_{m} is given by

t={m2m+12m42m28m+83m29m+8m5.t=\left\{\begin{array}[]{ll}\frac{m-2}{m+1}&2\leq m\leq 4\\ &\\ \frac{2m^{2}-8m+8}{3m^{2}-9m+8}&m\geq 5.\\ \end{array}\right.
Proof.

This follows directly from the construction of φm\varphi_{m} and is left to the reader. ∎

1.2.3. The Chow variety

The Hilbert-Chow morphism ψ:Hilb4,1Chow4,1\psi_{\infty}:\operatorname{Hilb}_{4,1}\to\operatorname{Chow}_{4,1} induces a birational map φ:EChow4,1\varphi_{\infty}:\mathbb{P}E\dashrightarrow\operatorname{Chow}_{4,1}. We will denote by Λ\Lambda_{\infty} the canonical polarization on the Chow variety. The following was established in the proof of [CMJL12, Thm. 2.11].

Proposition 1.9 ([CMJL12]).

The birational map

φ:EChow4,1\varphi_{\infty}:\mathbb{P}E\dashrightarrow\operatorname{Chow}_{4,1}

restricts to a morphism on the locus of points ([q],[f])([q],[f]) such that qq and ff do not have a common linear factor. The pull-back of the canonical polarization Λ\Lambda_{\infty} on Chow4,1\operatorname{Chow}_{4,1} is proportional to 3η+2h3\eta+2h.∎

Remark 1.10.

There is a constant c+c\in\mathbb{Q}_{+} such that limm13m2ψmΛm=cψΛ\lim_{m\to\infty}\frac{1}{3m^{2}}\psi_{m}^{*}\Lambda_{m}=c\psi_{\infty}^{*}\Lambda_{\infty} (cf. [KM76, Thm. 4]). This is reflected in the slopes in Propositions 1.8 and 1.9.

1.3. Cones of divisors on E\mathbb{P}E

We now consider the nef cone and pseudoeffective cone of E\mathbb{P}E. Benoist [Ben11] has determined the nef cones of more general spaces of complete intersections. We state a special case of his result here, together with a basic observation on the pseudoeffective cone.

Proposition 1.11 ([Ben11, Thm 2.7]).

The nef cone of E\mathbb{P}E has extremal rays of slope 0 and 12\frac{1}{2}. The pseudoeffective cone of E\mathbb{P}E has an extremal ray of slope 0 and contains the ray of slope 3433\frac{34}{33}.

Proof.

The computation of the nef cone is in [Ben11, Thm 2.7]. For the pseudoeffective cone, on the one hand, η\eta is effective (in fact semi-ample), but not big, so it generates one boundary of the pseudoeffective cone. The discriminant divisor δ\delta is effective, establishing the other claim. ∎

1.4. The Rojas–Vainsencher resolution

Rojas–Vainsencher [RV02] have constructed an explicit resolution WW of the rational map EHilb4,1\mathbb{P}E\dashrightarrow\operatorname{Hilb}_{4,1}, giving a diagram:

W\textstyle{W\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces}π1\scriptstyle{\pi_{1}}π2\scriptstyle{\pi_{2}}E\textstyle{\mathbb{P}E\ignorespaces\ignorespaces\ignorespaces\ignorespaces}Hilb4,1.\textstyle{\operatorname{Hilb}_{4,1}.}

It is shown in [RV02, Thm. 3.1] that WW can be obtained from E\mathbb{P}E via a sequence of seven blow-ups along SL(4)\mathrm{SL}(4)-invariant smooth subvarieties, and the resulting space WW is isomorphic to E\mathbb{P}E along UEU\subseteq\mathbb{P}E, the locus of complete intersections. In particular, SL(4)\mathrm{SL}(4) acts on WW (compatibly with the action on E\mathbb{P}E), and WW is non-singular.

2. Singularities of (2,3)(2,3)-complete intersections

In this section we discuss the possible isolated singularities of (2,3)(2,3)-complete intersections in 3\mathbb{P}^{3}. Recall that given such a complete intersection, the quadric is uniquely determined by the curve, while the cubic is only determined modulo the quadric. In the GIT analysis, the only relevant cases are when the quadric and cubic are not simultaneously singular, by which we mean that they have no common singular points. In this case, we can choose either the quadric or cubic to obtain local coordinates and view the singularities of CC as planar singularities.

2.1. Double Points

The only planar singularities of multiplicity two are the AkA_{k} singularities. We will see later in our GIT analysis that when kk is odd, it is important to distinguish between two types of AkA_{k} singularities, those that separate the curve and those that do not.

Proposition 2.1.

There exists a reduced (2,3)(2,3)-complete intersection possessing a non-separating singularity of type AkA_{k} if and only if k8k\leq 8. Moreover, if CC is a (2,3)(2,3)-complete intersection with a separating AkA_{k} singularity at a smooth point of the quadric on which it lies, then one of the following holds:

  1. (1)

    k=9k=9, and CC is the union of two twisted cubics.

  2. (2)

    k=7k=7, and CC is the union of a quartic and a conic.

  3. (3)

    k=5k=5, and CC is the union of a quintic and a line.

Proof.

The local contribution of an AkA_{k} singularity to the genus is k2\lfloor\frac{k}{2}\rfloor. Since the arithmetic genus of a (2,3)(2,3)-complete intersection is 4, it follows that it cannot admit an AkA_{k} singularity if k10k\geq 10. Conversely, it is easy to see that there exist (2,3)(2,3)-complete intersections with non-separating singularities of type AkA_{k} for each k8k\leq 8 (e.g. see [Fed12, §2.3.7]).

If CC possesses a separating singularity of type A2n1A_{2n-1}, then C=C1C2C=C_{1}\cup C_{2}, where C1C_{1} and C2C_{2} are connected curves meeting in a single point with multiplicity nn. A case by case analysis of the possibilities gives the second statement of the proposition. It is straightforward to check that there is no (2,3)(2,3)-complete intersection with a separating node or tacnode. ∎

2.2. Triple Points

Let CC be a (2,3)(2,3)-complete intersection with a singularity of multiplicity 3, which does not contain a line component meeting the residual curve only at the singularity. Notice that projection from the singularity maps CC onto a cubic in 2\mathbb{P}^{2}. It follows that CC is contained in the cone over this cubic. We choose specific coordinates so that the singular point is p=(1,0,0,0)p=(1,0,0,0) and the tangent space to the quadric at pp is given by x3=0x_{3}=0. Now, consider the 1-PS with weights (1,0,0,1)(1,0,0,-1). The flat limit of CC under this one-parameter subgroup is cut out by the equations:

x0x3+q(x1,x2)=f(x1,x2)=0x_{0}x_{3}+q^{\prime}(x_{1},x_{2})=f^{\prime}(x_{1},x_{2})=0

where qq^{\prime} and ff^{\prime} are forms in the variables x1,x2x_{1},x_{2}. We see that this limit is the union of three (not necessarily distinct) conics meeting at the points pp and (0,0,0,1)(0,0,0,1).

Following [Fed12] we will refer to these unions of conics as tangent cones. In our GIT analysis we will see that, for a given linearization, the semistable tangent cones are precisely the polystable (i.e. semi-stable with closed orbit) curves with triple point singularities. Note that the conics are distinct if and only if the original triple point is of type D4D_{4}.

2.3. Curves on Singular Quadrics

As we vary the GIT parameters, we will see that certain subloci of curves on singular quadrics are progressively destabilized. In this section we briefly describe each of these loci. The first locus to be destabilized is the set of curves lying on low-rank quadrics.

Proposition 2.2.

The only reduced (2,3)(2,3)-complete intersections with more than one component of positive genus consist of two genus one curves meeting in 3 points. Such a curve necessarily lies on a quadric of rank 2, and moreover the general complete intersection of a cubic and a rank 2 quadric is such a curve.

Proof.

Suppose that C=C1C2C=C_{1}\cup C_{2} is the union of two positive genus curves. Neither curve may have degree 2 or less, and hence both have degree 3. Any degree 3 curve that spans 3\mathbb{P}^{3} is rational, and hence the two curves are both plane cubics. Since CC is contained in a unique quadric, it follows that this quadric must be the union of two planes, and hence CC is as described above. ∎

Following [AFS10], we refer to such curves as elliptic triboroughs. The locus of elliptic triboroughs is expected to be flipped in the Hassett–Keel program at the critical value α=59\alpha=\frac{5}{9}. This is exactly what we will prove in the following sections.

We now consider curves on a quadric of rank 3. More specifically, we will see that a curve lies on a quadric cone if and only if its normalization admits a Gieseker–Petri special linear series. The proposition below follows by a standard argument. The result is not needed in the ensuing proofs, but is useful in giving a geometric interpretation to the stability computations in later sections.

Proposition 2.3.

Let C3C\subset\mathbb{P}^{3} be a complete intersection of a cubic and a quadric of rank at least 3, non-singular everywhere except possibly one point. Then the following hold:

  1. (1)

    If CC is smooth, it has a vanishing theta-null if and only if it lies on a quadric cone.

  2. (2)

    The normalization of CC is a hyperelliptic genus 3 curve if and only if CC lies on a quadric cone and has a node or cusp at the vertex.

  3. (3)

    CC is a tacnodal curve such that the two preimage points of the tacnode via the normalization are conjugate under the hyperelliptic involution if and only if CC lies on a quadric cone and has a tacnode at the vertex.

3. The two boundary cases

In this section we describe two previously studied birational models for M¯4\overline{M}_{4} that are obtained via GIT for canonically embedded genus 44 curves (see [Fed12] and [CMJL12]). In the later sections we will see that these two models coincide with the “boundary cases” in our GIT problem. In other words, each of the models is isomorphic to a quotient of E//SL(4)\mathbb{P}E/\!\!/\mathrm{SL}(4) for a certain choice of linearization, and all of the other linearizations we consider are effective combinations of these two.

3.1. Chow Stability, following [CMJL12]

Let Chow4,1\operatorname{Chow}_{4,1} denote the irreducible component of the Chow variety containing genus 4 canonical curves. In [CMJL12], the authors study the GIT quotient Chow4,1//ΛSL(4)\operatorname{Chow}_{4,1}/\!\!/_{\Lambda_{\infty}}\mathrm{SL}(4) and obtain the following:

Theorem 3.1 ([CMJL12, Thm. 3.1]).

The stability conditions for the quotient Chow4,1//ΛSL(4)\operatorname{Chow}_{4,1}/\!\!/_{\Lambda_{\infty}}\mathrm{SL}(4) are described as follows:

  • (0)

    Every semi-stable point cChow4,1c\in\operatorname{Chow}_{4,1} is the cycle associated to a (2,3)(2,3)-complete intersection in 3\mathbb{P}^{3}. The only non-reduced (2,3)(2,3)-complete intersections that give a semi-stable point cChow4,1c\in\operatorname{Chow}_{4,1} are the genus 44 ribbons (all with associated cycle equal to the twisted cubic with multiplicity 22).

Assume now CC is a reduced (2,3)(2,3)-complete intersection in 3\mathbb{P}^{3}, with associated point cChow4,1c\in\operatorname{Chow}_{4,1}. Let Q3Q\subseteq\mathbb{P}^{3} be the unique quadric containing CC. The following hold:

  • (0’)

    cc is unstable if CC is the intersection of a quadric and a cubic that are simultaneously singular. Thus, in items (1) and (2) below we can assume CC has only planar singularities.

  • (1)

    cc is stable if and only if rankQ3\mathrm{rank}Q\geq 3 and CC is a curve with at worst A1,,A4A_{1},\ldots,A_{4} singularities at the smooth points of QQ and at worst an A1A_{1} or A2A_{2} singularity at the vertex of QQ (if rankQ=3\mathrm{rank}Q=3).

  • (2)

    cc is strictly semi-stable if and only if

    • i)

      rankQ=4\mathrm{rank}Q=4 and

      • (α\alpha)

        CC contains a singularity of type D4D_{4} or A5A_{5}, or,

      • (β\beta)

        CC contains a singularity of type AkA_{k}, k6k\geq 6, and CC does not contain an irreducible component of degree 2\leq 2, or,

    • ii)

      rankQ=3\mathrm{rank}Q=3, CC has at worst an AkA_{k}, kk\in\mathbb{N}, singularity at the vertex of QQ and

      • (α\alpha)

        CC contains a D4D_{4} or an A5A_{5} singularity at a smooth point of QQ or an A3A_{3} singularity at the vertex of QQ, or,

      • (β\beta)

        CC contains a singularity of type AkA_{k}, k6k\geq 6, at a smooth point of QQ or a singularity of type AkA_{k}, k4k\geq 4, at the vertex of QQ, and CC does not contain an irreducible component that is a line, or,

    • iii)

      rankQ=2\mathrm{rank}Q=2 and CC meets the singular locus of QQ in three distinct points.

Remark 3.2.

In the example from [BE95, §7], it is shown that up to change of coordinates there is only one canonically embedded ribbon of genus 4. Moreover, it is shown that the ideal of this ribbon (again, up to change of coordinates) is generated by the quadric q=x1x3x22q=x_{1}x_{3}-x_{2}^{2} and the cubic

f=det(x3x2x1x2x1x0x1x00).f=\det\left(\begin{array}[]{ccc}x_{3}&x_{2}&x_{1}\\ x_{2}&x_{1}&x_{0}\\ x_{1}&x_{0}&0\\ \end{array}\right).
Remark 3.3.

The closed orbits of semi-stable curves fall into 3 categories (see also [CMJL12, Rem. 3.2, 3.3]):

  1. (1)

    The curve CD=V(x0x3,x13+x23)C_{D}=V(x_{0}x_{3},x_{1}^{3}+x_{2}^{3}), consisting of three pairs of lines meeting in two D4D_{4} singularities;

  2. (2)

    The maximally degenerate curve C2A5=V(x0x3x1x2,x0x22+x12x3)C_{2A_{5}}=V(x_{0}x_{3}-x_{1}x_{2},x_{0}x_{2}^{2}+x_{1}^{2}x_{3}) with two A5A_{5} singularities;

  3. (3)

    The curves CA,B=V(x22x1x3,Ax13+Bx0x1x2+x02x3)C_{A,B}=V(x_{2}^{2}-x_{1}x_{3},Ax_{1}^{3}+Bx_{0}x_{1}x_{2}+x_{0}^{2}x_{3}), of which there is a pencil parameterized by 4A/B24A/B^{2}. If 4A/B20,14A/B^{2}\neq 0,1, then CA,BC_{A,B} has an A5A_{5} singularity at a smooth point of the singular quadric, and an A3A_{3} singularity at the vertex of the cone. If 4A/B2=04A/B^{2}=0, then CA,BC_{A,B} has an A5A_{5} and A1A_{1} singularity at smooth points of the singular quadric, and an A3A_{3} singularity at the vertex of the cone. If 4A/B2=14A/B^{2}=1 the curve CA,BC_{A,B} is the genus 44 ribbon, and the associated point in Chow4,1\operatorname{Chow}_{4,1} is the twisted cubic with multiplicity 22. Note also that the orbit closures of curves corresponding to cases (2) i) (β\beta) and (2) ii) (β\beta) contain the orbit of the ribbon.

Moreover, we can describe the degenerations of the strictly semi-stable points cChow4,1c\in\operatorname{Chow}_{4,1}. Let CC be a (2,3)(2,3)-scheme with strictly semi-stable cycle cChow4,1c\in\operatorname{Chow}_{4,1}. If CC contains a D4D_{4} singularity, or lies on a rank 22 quadric, then cc degenerates to the cycle associated to CDC_{D}. If CC lies on a quadric QQ of rank at least 33, and either CC contains an A5A_{5} singularity at a smooth point of QQ, or an A3A_{3} singularity at the vertex of QQ (if rankQ=3\mathrm{rank}Q=3), then cc degenerates to either the cycle associated to C2A5C_{2A_{5}} or to the cycle associated to some CA,BC_{A,B} with 4A/B214A/B^{2}\neq 1. Otherwise, cc degenerates to CA,BC_{A,B} with 4A/B2=14A/B^{2}=1, a non-reduced complete intersection supported on a rational normal curve.

Additionally, it is shown in [CMJL12] that the quotient of the Chow variety coincides with one of the Hassett–Keel spaces, specifically:

(3.4) Chow4,1//ΛSL(4)M¯4(59).\operatorname{Chow}_{4,1}/\!\!/_{\Lambda_{\infty}}\mathrm{SL}(4)\cong\overline{M}_{4}\left(\frac{5}{9}\right).

For the reader’s convenience, we briefly describe the birational contraction M¯4Chow4,1//SL(4)\overline{M}_{4}\dashrightarrow\operatorname{Chow}_{4,1}/\!\!/\mathrm{SL}(4) in Table 2. In order to make sense of the table, we need to recall some standard terminology. Specifically, a tail of genus ii is a genus ii connected component of a curve that meets the residual curve in one point. Similarly, a bridge of genus ii is a genus ii connected component of a curve that meets the residual curve in two points. By conjugate points on a hyperelliptic curve, we mean points that are conjugate under the hyperelliptic involution. An elliptic triborough is a genus 11 connected component of a curve that meets the residual curve in three points.

Semi-stable Singularity Locus Removed in M¯4\overline{M}_{4}
A2A_{2} elliptic tails
A3A_{3} elliptic bridges
A4A_{4} genus 2 tails attached at a Weierstrass point
non-separating A5A_{5} genus 2 bridges attached at conjugate points
separating A5A_{5} general genus 2 tails
A6A_{6} hyperelliptic genus 3 tails attached at a Weierstrass
point
non-separating A7A_{7} curves in Δ0\Delta_{0} with hyperelliptic normalization glued
at conjugate points
A8A_{8}, A9A_{9}, ribbons hyperelliptic curves
D4D_{4} elliptic triboroughs
Table 2. The birational contraction M¯4Chow4,1//SL(4)\overline{M}_{4}\dashrightarrow\operatorname{Chow}_{4,1}/\!\!/\mathrm{SL}(4)
Remark 3.5.

We note in particular that the rational map M¯4Chow4,1//SL(4)\overline{M}_{4}\dashrightarrow\operatorname{Chow}_{4,1}/\!\!/\mathrm{SL}(4) contracts the boundary divisors Δ1\Delta_{1} and Δ2\Delta_{2}, the closure of the hyperelliptic locus, and the locus of elliptic triboroughs.

3.2. Terminal Stability (i.e. stability for (3,3)(3,3) curves on quadric surfaces) following [Fed12]

Recall that every canonically embedded curve CC of genus 4 is contained in a quadric in 3\mathbb{P}^{3}. If this quadric is smooth, then it is isomorphic to 1×1\mathbb{P}^{1}\times\mathbb{P}^{1}, and CC is a member of the class |𝒪1×1(3,3)||\mathcal{O}_{\mathbb{P}^{1}\times\mathbb{P}^{1}}(3,3)|. The automorphism group of the quadric is SO(4)\mathrm{SO}(4), which is isogenous to SL(2)×SL(2)\mathrm{SL}(2)\times\mathrm{SL}(2). The GIT quotient |𝒪(3,3)|//SO(4)|\mathcal{O}(3,3)|/\!\!/\mathrm{SO}(4) was studied in detail by Fedorchuk in [Fed12]. Because this GIT quotient appears as the last stage of the log minimal model program for M¯4\overline{M}_{4}, we refer to curves that are (semi)stable with respect to this action as terminally (semi)stable. We summarize the results of [Fed12] here.

Theorem 3.6 (Fedorchuk [Fed12, §2.2]).

Let C|𝒪(3,3)|C\in|\mathcal{O}(3,3)|. CC is terminally stable if and only if its has at worst double points as singularities and it does not contain a line component LL meeting the residual curve C=CL¯C^{\prime}=\overline{C\setminus L} in exactly one point. CC is terminally semi-stable if and only if it contains neither a double-line component, nor a line component LL meeting the residual curve CC^{\prime} in exactly one point, which is also a singular point of CC^{\prime} (i.e. LC={p}L\cap C^{\prime}=\{p\} and pSing(C)p\in\mathrm{Sing}(C^{\prime})).

Remark 3.7.

The closed orbits of strictly semi-stable curves fall into 44 categories:

  1. (1)

    The maximally degenerate curve C2A5=V(x0x3x1x2,x0x22+x12x3)C_{2A_{5}}=V(x_{0}x_{3}-x_{1}x_{2},x_{0}x_{2}^{2}+x_{1}^{2}x_{3}) with 2 A5A_{5} singularities (same curve as in Rem. 3.3(2));

  2. (2)

    The triple conic V(x0x3x1x2,x33)V(x_{0}x_{3}-x_{1}x_{2},x_{3}^{3});

  3. (3)

    Unions of a smooth conic and a double conic meeting transversally. As discussed in Remark 2.4 in [Fed12], there is a one-dimensional family of such curves;

  4. (4)

    Unions of three conics meeting in two D4D_{4} singularities V(x0x3x1x2,x13+x23)V(x_{0}x_{3}-x_{1}x_{2},x_{1}^{3}+x_{2}^{3}) (analogue of the case of Rem. 3.3(1)).

As mentioned above, Fedorchuk [Fed12] showed that this GIT quotient is the final non-trivial step in the Hassett–Keel program for genus 44, specifically:

(3.8) |𝒪(3,3)|//SO(4)M¯4[2960,817)M¯4(817)={}.|\mathcal{O}(3,3)|/\!\!/\mathrm{SO}(4)\cong\overline{M}_{4}\left[\frac{29}{60},\frac{8}{17}\right)\to\overline{M}_{4}\left(\frac{8}{17}\right)=\{\ast\}.

In this paper we are interested in describing the behavior of the Hassett–Keel program for genus 44 curves in the interval α[817,59]\alpha\in\left[\frac{8}{17},\frac{5}{9}\right] (with endpoints described by (3.8) and (3.4) respectively). In particular, in the following sections, we will give an explicit factorization of the birational map

Ψ:M¯4(59)Chow4,1//SL(4)|𝒪(3,3)|//SO(4)M¯4[2960,817)\Psi:\overline{M}_{4}\left(\frac{5}{9}\right)\cong\operatorname{Chow}_{4,1}/\!\!/\mathrm{SL}(4)\dashrightarrow|\mathcal{O}(3,3)|/\!\!/\mathrm{SO}(4)\cong\overline{M}_{4}\left[\frac{29}{60},\frac{8}{17}\right)

as the composition of two flips and a divisorial contraction.

For the moment, by comparing the stability conditions given by Theorems 3.1 and 3.6 and by simple geometric considerations, we obtain a rough description of the birational map Ψ\Psi as summarized in Table 3 (see also [Fed12, Table 1]). The first three lines of the table correspond to strictly semi-stable points of Chow4,1\operatorname{Chow}_{4,1} that are all flipped by the map M¯4(59ϵ)M¯4(59)\overline{M}_{4}(\frac{5}{9}-\epsilon)\to\overline{M}_{4}(\frac{5}{9}). Then, note that every Chow-stable curve contained in a quadric cone is terminally unstable. There are three types of such curves: those that do not meet the vertex of the cone, those that meet it in a node, and those that meet it in a cusp. These correspond to the latter three lines in the table, as well as the three critical slopes in our VGIT problem. These last three lines correspond, in order, to the flip at α=2344\alpha=\frac{23}{44}, the flip at α=12\alpha=\frac{1}{2}, and the divisorial contraction at α=2960\alpha=\frac{29}{60}.

Semi-stable Singularity Locus Removed
non-separating A5A_{5} tacnodal curves glued at conjugate points
A6A_{6}, non-sep. A7A_{7}, A8A_{8}, A9A_{9} ribbons (see Rem. 3.3(3))
D4D_{4} elliptic triboroughs
separating A7A_{7} cuspidal curves with hyperelliptic normalization
contains a double conic nodal curves with hyperelliptic normalization
triple conic curves with vanishing theta-null
Table 3. The birational map Chow4,1//SL(4)|𝒪(3,3)|//SO(4)\operatorname{Chow}_{4,1}/\!\!/\mathrm{SL}(4)\dashrightarrow|\mathcal{O}(3,3)|/\!\!/\mathrm{SO}(4)

4. Numerical stability of Points in E\mathbb{P}E

In this section we determine the stability conditions on E\mathbb{P}E as the slope tt of the linearization varies by using the Hilbert–Mumford numerical criterion. We note that a discussion of the Hilbert–Mumford index in a related and more general situation than ours was done by Benoist [Ben11], whose results we are using here.

A technical issue arises in this section. Namely, we are interested in applying the numerical criterion for slopes t(0,23]t\in\left(0,\frac{2}{3}\right]. However, by Proposition 1.11, the linearizations of slope t12t\geq\frac{1}{2} are not ample. Thus, for t12t\geq\frac{1}{2}, special care is needed to define a GIT quotient E//tSL(4)\mathbb{P}E/\!\!/_{t}\mathrm{SL}(4) and to understand the stability conditions by means of the numerical criterion. In this section we make the necessary modifications to handle this non-standard GIT case. Namely, here we work with “numerical” (semi-)stability instead of the usual (Mumford) (semi-)stability. Then, in Section 6, we prove that there is no difference between the two notions of stability and that everything has the expected behavior. In short, for slopes t(0,12)t\in\left(0,\frac{1}{2}\right) everything works as usual, since the linearization is ample. For t12t\geq\frac{1}{2} one can still proceed as in the ample case, but this is justified only a posteriori by the results of Section 6.

4.1. The numerical criterion for E\mathbb{P}E

Let us start by recalling the Hilbert–Mumford index for hypersurfaces. That is, we consider the case of SL(r+1)\mathrm{SL}(r+1) acting on H0(r,𝒪r(d))\mathbb{P}H^{0}(\mathbb{P}^{r},\mathscr{O}_{\mathbb{P}^{r}}(d)). In this case, given a one-parameter subgroup (1-PS) λ:𝔾mSL(r+1)\lambda:\mathbb{G}_{m}\to\mathrm{SL}(r+1), the action on H0(r,𝒪r(1))H^{0}(\mathbb{P}^{r},\mathscr{O}_{\mathbb{P}^{r}}(1)) can be diagonalized. We describe the action of λ\lambda in these coordinates with a weight vector α=(α0,α1,,αr)\alpha=(\alpha_{0},\alpha_{1},\ldots,\alpha_{r}). For a monomial xa=x0a0xrarH0(r,𝒪r(d))x^{a}=x_{0}^{a_{0}}\cdots x_{r}^{a_{r}}\in H^{0}(\mathbb{P}^{r},\mathscr{O}_{\mathbb{P}^{r}}(d)) in these coordinates, we define the λ\lambda-weight of xax^{a} to be

wtλ(xa)=α.a=α0a0+α1a1++αrar.wt_{\lambda}(x^{a})=\alpha.a=\alpha_{0}a_{0}+\alpha_{1}a_{1}+\ldots+\alpha_{r}a_{r}.

The Hilbert–Mumford invariant associated to a non-zero homogeneous form FH0(r,𝒪r(d))F\in H^{0}(\mathbb{P}^{r},\mathscr{O}_{\mathbb{P}^{r}}(d)) and a 1-PS λ\lambda is then given by

μ(F,λ)=maxxa monomials in Fwtλ(xa).\mu(F,\lambda)=\max_{x^{a}\text{ monomials in }F}wt_{\lambda}(x^{a}).

Following [Ben11], the Hilbert–Mumford index for complete intersections V(f,q)V(f,q) has a simple expression in terms of the indices for the associated hypersurfaces.

Proposition 4.1 ([Ben11, Prop 2.15]).

The Hilbert–Mumford index of a point ([q],[f])E([q],[f])\in\mathbb{P}E is given by

μaη+bh(([q],[f]),λ)=aμ(q,λ)+bμ(f,λ),\mu^{a\eta+bh}(([q],[f]),\lambda)=a\mu(q,\lambda)+b\mu(f,\lambda),

where fH0(3,𝒪(3))f\in H^{0}(\mathbb{P}^{3},\mathcal{O}(3)) is a representative of [f][f] of minimal λ\lambda-weight.

Recall from §1.1 that the slope of the line bundle aη+bha\eta+bh is defined to be t=bat=\frac{b}{a}. Throughout we will write μt(([q],[f]),λ)\mu^{t}(([q],[f]),\lambda) for the Hilbert–Mumford index with respect to the linearization η+th\eta+th.

Definition 4.2.

We say that ([q],[f])([q],[f]) is numerically tt-stable (resp. numerically tt-semi-stable) if, for all non-trivial one-parameter subgroups λ\lambda,

μt(([q],[f]),λ)>0 (resp. 0 ).\mu^{t}(([q],[f]),\lambda)>0\text{ (resp. }\geq 0\text{ )}.

While we will typically only refer to numerical (semi-)stability for points of E\mathbb{P}E, we will occasionally want to refer to this notion in more generality. Recall that the definition can be made in the situation where one has a reductive group GG acting on a proper space XX with respect to a linearization LL ([MFK94, Def. 2.1, p.48]). We will use the notation XnssX^{nss} and XnsX^{ns} to refer to the numerically semi-stable, and numerically stable loci respectively.

Remark 4.3.

We recall that for the general GIT set-up, with a reductive group GG acting on a space XX with respect to a linearization LL, Mumford [MFK94, Def. 1.7] defines a point xXx\in X to be semi-stable (and a similar definition for stable) if there exists an invariant section σH0(X,Ln)\sigma\in H^{0}(X,L^{\otimes n}) such that σ(x)0\sigma(x)\neq 0 and XσX_{\sigma} is affine. We will use the standard notation X(s)sX^{(s)s} to denote the (semi-)stable points in this sense. To emphasize the distinction with numerical (semi-)stability, and avoid confusion, we will sometimes refer to this as Mumford (semi-)stability. For ample line bundles on projective varieties, the Hilbert–Mumford numerical criterion ([MFK94, Thm. 2.1]) gives that numerical (semi-)stability agrees with (semi-)stability. If LL is not ample, however, the notions may differ (see e.g. Remark 4.4). In our situation, we work with numerical stability, since it is easily computable; in the end (using the results in Section 6), we will prove that this is same as Mumford stability. Of course, this distinction is only relevant in the non-ample case (i.e. linearizations of slopes t12t\geq\frac{1}{2}).

Remark 4.4.

The following simple example illustrates some of the differences between numerical stability and Mumford stability. Let GG be a reductive group acting on a smooth projective variety XX with dim(X)2\dim(X)\geq 2, and let LL be an ample linearization. Consider the blow-up π:XX\pi:X^{\prime}\to X along a closed GG-invariant locus ZZ (with codimZ2\mathrm{codim}Z\geq 2) that contains at least one semi-stable point pZXssp\in Z\cap X^{ss}. Note that the rings of invariant sections R(X,L)GR(X,L)^{G} and R(X,πL)GR(X^{\prime},\pi^{*}L)^{G} agree via pullback of sections, and the Hilbert-Mumford indices agree by functoriality ([MFK94, iii), p.49]). It follows that any point qq in the fiber π1(p)\pi^{-1}(p) (contained in the exceptional divisor EE) will be numerically semi-stable. But no such point can be Mumford semi-stable, because the pull-back of a section σ\sigma that does not vanish at qq does not vanish on π1(p)\pi^{-1}(p), and consequently XσX^{\prime}_{\sigma} can not be affine.

Notation 4.5.

When considering GIT quotients, we will use the notation X//LGX/\!\!/_{L}G for the categorical quotient of the semi-stable locus XssX^{ss} ([MFK94, Thm. 1.10]); we will call this the (categorical) GIT quotient. Note this may not necessarily agree with ProjR(X,L)G\operatorname{Proj}R(X,L)^{G} when LL is not ample.

4.2. Application of the numerical criterion

We begin our discussion by identifying points of E\mathbb{P}E that fail to be numerically semi-stable for any linearization. Note that in order to show that a certain pair ([q],[f])([q],[f]) is not tt-numerically semi-stable, it suffices to find a 11-PS λ\lambda and a representative ff such that μ(q,λ)+tμ(f,λ)<0\mu(q,\lambda)+t\mu(f,\lambda)<0, since for any representative ff, one has μt(([q],[f]),λ)μ(q,λ)+tμ(f,λ)\mu^{t}(([q],[f]),\lambda)\leq\mu(q,\lambda)+t\mu(f,\lambda) (cf. Proposition 4.1).

Proposition 4.6.

If qq is a reducible quadric, then (q,f)(q,f) is not numerically tt-semi-stable for any t<23t<\frac{2}{3}. Moreover, if qq and ff share the common linear factor x0x_{0}, then (q,f)(q,f) is destabilized by the 1-parameter subgroup with weights (3,1,1,1)(-3,1,1,1) for any t23t\leq\frac{2}{3}.

Proof.

Suppose that qq is singular along the line x2=x3=0x_{2}=x_{3}=0, and consider the 1-PS λ\lambda with weights (1,1,1,1)(1,1,-1,-1). Then μ(q,λ)=2\mu(q,\lambda)=-2 and μ(f,λ)3\mu(f,\lambda)\leq 3. Hence μt((q,f),λ)<0\mu^{t}((q,f),\lambda)<0, so (q,f)(q,f) is not numerically tt-semi-stable.

To see the second statement, let λ\lambda be the 1-PS with weights (3,1,1,1)(-3,1,1,1) and note that μ(q,λ)2\mu(q,\lambda)\leq-2, μ(f,λ)1\mu(f,\lambda)\leq-1. ∎

Note that, as a consequence, every numerically tt-semi-stable point of E\mathbb{P}E for t<23t<\frac{2}{3} is a complete intersection. The only points of E\mathbb{P}E that do not correspond to complete intersections are those where qq and ff share a common linear factor. Henceforth, we will refer interchangeably to stability of the point (q,f)E(q,f)\in\mathbb{P}E and stability of the curve C=V(q,f)C=V(q,f).

Proposition 4.7.

If qq and ff are simultaneously singular, then (q,f)(q,f) is not numerically tt-semi-stable for any t23t\leq\frac{2}{3}.

Proof.

Suppose that qq and ff are both singular at the point (1,0,0,0)(1,0,0,0), and consider the 1-PS with weights (3,1,1,1)(3,-1,-1,-1). Then μ(q,λ)=2\mu(q,\lambda)=-2 and μ(f,λ)1\mu(f,\lambda)\leq 1. Hence μt((q,f),λ)43<0\mu^{t}((q,f),\lambda)\leq-\frac{4}{3}<0, so (q,f)(q,f) is not numerically tt-semi-stable. ∎

Proposition 4.8.

Suppose that qq is a quadric cone and ff passes through the singular point pp of qq. If pp is not a node or a cusp of CC, then (q,f)(q,f) is not numerically tt-semi-stable for any t<23t<\frac{2}{3}.

Proof.

Without loss of generality, we may assume that q=x1x3x22q=x_{1}x_{3}-x_{2}^{2}. We write the cubic in coordinates as

f=a+b+c+d=3αa,b,c,dx0ax1bx2cx3d.f=\sum_{a+b+c+d=3}\alpha_{a,b,c,d}x_{0}^{a}x_{1}^{b}x_{2}^{c}x_{3}^{d}.

If p=(1,0,0,0)p=(1,0,0,0) is not a node of CC, then the projectivized tangent cone to CC at pp is a double line contained in the quadric cone. Hence, the tangent space to the cubic at pp meets the quadric in a double line. We may therefore assume that this tangent space is the plane x3=0x_{3}=0. It follows that α3,0,0,0=α2,1,0,0=α2,0,1,0=0\alpha_{3,0,0,0}=\alpha_{2,1,0,0}=\alpha_{2,0,1,0}=0. Since pp is not a cusp, we have α1,2,0,0=0\alpha_{1,2,0,0}=0 as well. Now, consider the 1-PS with weights (3,1,1,3)(3,1,-1,-3). Then μ(q,λ)=2\mu(q,\lambda)=-2 and μ(f,λ)3\mu(f,\lambda)\leq 3. It follows that μt((q,f),λ)<0\mu^{t}((q,f),\lambda)<0, so (q,f)(q,f) is not numerically tt-semi-stable. ∎

Corollary 4.9.

Ribbons are not numerically tt-semi-stable for any t<23t<\frac{2}{3}.

Proof.

This follows from Remark 3.2 and the proposition above. ∎

Proposition 4.10.

Suppose that CC contains a line LL and let C=C\L¯C^{\prime}=\overline{C\backslash L} be the residual curve. If pLCp\in L\cap C^{\prime} is a singular point of CC^{\prime}, then CC is not numerically tt-stable for any t23t\leq\frac{2}{3}. If, in addition, LL meets CC^{\prime} with multiplicity 33 at pp, then CC is not numerically tt-semi-stable for any t23t\leq\frac{2}{3}. In particular, if CC contains a double line, then it is not numerically tt-semi-stable for any t23t\leq\frac{2}{3}.

Proof.

By Propositions 4.6 and 4.8, we may assume that the singular point p=(1,0,0,0)p=(1,0,0,0) is a smooth point of the quadric qq. Without loss of generality, we may assume that the line LL is cut out by x2=x3=0x_{2}=x_{3}=0 and that the tangent plane to qq at pp is cut out by x3=0x_{3}=0. As above, we write the cubic in coordinates as

f=a+b+c+d=3αa,b,c,dx0ax1bx2cx3d.f=\sum_{a+b+c+d=3}\alpha_{a,b,c,d}x_{0}^{a}x_{1}^{b}x_{2}^{c}x_{3}^{d}.

By replacing ff with a cubic of the form f(αx0+βx1)qf-(\alpha x_{0}+\beta x_{1})q for suitable choices of α\alpha and β\beta, we obtain a representative for ff such that α2,0,0,1=α1,1,0,1=0\alpha_{2,0,0,1}=\alpha_{1,1,0,1}=0. From the assumption that CC contains LL, we may conclude that αa,3a,0,0=0\alpha_{a,3-a,0,0}=0 (a=0,1,2,3a=0,1,2,3). From the assumption that CC^{\prime} is singular at pp, we may further conclude that α2,0,1,0=α1,1,1,0=0\alpha_{2,0,1,0}=\alpha_{1,1,1,0}=0. Now consider the 1-PS λ\lambda with weights (1,0,0,1)(1,0,0,-1). Then μ(q,λ)0\mu(q,\lambda)\leq 0 and μ(f,λ)0\mu(f,\lambda)\leq 0. It follows that μt((q,f),λ)0\mu^{t}((q,f),\lambda)\leq 0, so (q,f)(q,f) is not numerically tt-stable.

Let us now assume further that LL meets CC^{\prime} with multiplicity 3 at pp. Then we obtain in addition that α0,2,1,0=0\alpha_{0,2,1,0}=0. Considering the 1-PS λ\lambda with weights (3,1,1,3)(3,1,-1,-3), we see that μ(q,λ)0\mu(q,\lambda)\leq 0 and μ(f,λ)1\mu(f,\lambda)\leq-1. It follows that μt((q,f),λ)<0\mu^{t}((q,f),\lambda)<0, so (q,f)(q,f) is not numerically tt-semi-stable.

The case of a double line follows by taking the reduced line and its residual curve; i.e. C=2L+C′′=L+CC=2L+C^{\prime\prime}=L+C^{\prime} where C=L+C′′C^{\prime}=L+C^{\prime\prime}. ∎

Proposition 4.11.

If CC has a singularity of multiplicity greater than two, it is not numerically tt-stable for any t23t\leq\frac{2}{3}. Moreover, if CC has a singularity of multiplicity greater than three, it is not numerically tt-semi-stable for any t23t\leq\frac{2}{3}.

Proof.

Without loss of generality, we may assume that the singular point is p=(1,0,0,0)p=(1,0,0,0) and by Proposition 4.10 we may assume that CC does not contain a line LL through pp.

Let us first consider the case where pp is a triple point. Because CC does not contain any lines LL such that LC\L¯={p}L\cap\overline{C\backslash L}=\{p\}, projection from pp maps CC onto a cubic in 2\mathbb{P}^{2}. Hence, CC is contained in the cone over this cubic. Consequently, this cone gives a representative ff for [f][f], which we will fix for the computations that follow. Suppose now that the tangent space to the quadric at pp is given by x3=0x_{3}=0. Then consider the 1-PS with weights (1,0,0,1)(1,0,0,-1). We see that both μ(q,λ)0\mu(q,\lambda)\leq 0 and μ(f,λ)0\mu(f,\lambda)\leq 0 and hence CC is not numerically tt-stable for any tt.

Now let us consider the case where pp has multiplicity 44. Projection from pp maps CC onto a conic in 2\mathbb{P}^{2}. Since CC is contained in the cone over this conic, it follows that pp is the singular point of a quadric cone containing CC. We have already seen, however, that unless pp is a node or cusp of CC, then CC is not numerically tt-semi-stable. ∎

We now consider three curves that are terminally semi-stable, but not Chow semi-stable. We determine those values of tt at which they become numerically unstable.

Proposition 4.12.

If CC contains a conic CC^{\prime} that meets C\C¯\overline{C\backslash C^{\prime}} in an A7A_{7} singularity, it is numerically tt-unstable for all t>611t>\frac{6}{11}. If qq is a quadric cone and CC has a cusp at the singular point of qq, it is numerically tt-unstable for all t<611t<\frac{6}{11}.

Proof.

First, consider the case where CC contains a conic CC^{\prime} meeting the residual curve in an A7A_{7} singularity. Without loss of generality, we assume that the conic is contained in the plane x3=0x_{3}=0, the singularity occurs at the point (1,0,0,0)(1,0,0,0), and the quadric fx3\frac{f}{x_{3}} contains the line x2=x3=0x_{2}=x_{3}=0. By assumption, the tangent space to qq at this point contains this line, and the quadric fx3\frac{f}{x_{3}} is singular. Now, consider the 1-PS with weights (7,3,1,9)(7,3,-1,-9). Then μ(q,λ)6\mu(q,\lambda)\leq 6 and μ(f,λ)11\mu(f,\lambda)\leq-11. It follows that

μt((q,f),λ)11t+6\mu^{t}((q,f),\lambda)\leq-11t+6

which is negative when t>611t>\frac{6}{11}.

Now, consider the case where qq is a quadric cone and CC has a cusp at the singular point of qq. Without loss of generality, we may assume that q=x1x3x22q=x_{1}x_{3}-x_{2}^{2}. We write a representative for the cubic in coordinates as

f=a+b+c+d=3αa,b,c,dx0ax1bx2cx3d.f=\sum_{a+b+c+d=3}\alpha_{a,b,c,d}x_{0}^{a}x_{1}^{b}x_{2}^{c}x_{3}^{d}.

As above, we may assume that the tangent space to the cubic at the cone point of qq is the plane x3=0x_{3}=0. It follows that α3,0,0,0=α2,1,0,0=α2,0,1,0=0\alpha_{3,0,0,0}=\alpha_{2,1,0,0}=\alpha_{2,0,1,0}=0. Consider the 1-PS with weights (9,1,3,7)(9,1,-3,-7). Then μ(q,λ)=6\mu(q,\lambda)=-6 and μ(f,λ)11\mu(f,\lambda)\leq 11. It follows that

μt(([q],[f]),λ)11t6\mu^{t}(([q],[f]),\lambda)\leq 11t-6

which is negative when t<611t<\frac{6}{11}. ∎

Remark 4.13.

We will see in Theorem 6.3 (3) that the minimal orbit of the above strictly semi-stable curves at t=611t=\frac{6}{11} is given by

x12+x0x2=x22x3+x0x32=0.x_{1}^{2}+x_{0}x_{2}=x_{2}^{2}x_{3}+x_{0}x_{3}^{2}=0.

This curve consists of two components meeting in a separating A7A_{7} singularity. One of the components is a conic. The other is a quartic with a cusp at the vertex of the cone.

Proposition 4.14.

If CC contains a double conic component, it is numerically tt-unstable for all t>25t>\frac{2}{5}. If qq is a quadric cone and ff passes through the singular point of the cone, then it is is numerically tt-unstable for all t<25t<\frac{2}{5}.

Proof.

First, consider the case where CC contains a double conic component. Without loss of generality, we may assume that the conic is contained in the plane x0=0x_{0}=0. Consider the 1-PS with weights (3,1,1,1)(-3,1,1,1). Then μ(q,λ)2\mu(q,\lambda)\leq 2, and, since ff is divisible by x02x_{0}^{2}, we have μ(f,λ)5\mu(f,\lambda)\leq-5. It follows that

μt((q,f),λ)5t+2\mu^{t}((q,f),\lambda)\leq-5t+2

which is negative when t>25t>\frac{2}{5}.

Now, consider the case where qq is a quadric cone and ff passes through the singular point. Without loss of generality, we may assume that the singularity occurs at the point p=(1,0,0,0)p=(1,0,0,0). Consider the 1-PS with weights (3,1,1,1)(3,-1,-1,-1). Then, since qq is singular at pp, μ(q,λ)=2\mu(q,\lambda)=-2. Furthermore, since ff contains pp, μ(f,λ)5\mu(f,\lambda)\leq 5, so

μt((q,f),λ)5t2\mu^{t}((q,f),\lambda)\leq 5t-2

which is negative when t<25t<\frac{2}{5}. ∎

Remark 4.15.

We will see in Theorem 6.3 (4) that here, the relevant minimal orbit of strictly semi-stable curves is given by the union of two rulings of a quadric cone and a double conic:

q(x0,x1,x2)=x0x32=0.q(x_{0},x_{1},x_{2})=x_{0}x_{3}^{2}=0.
Proposition 4.16.

If CC is a triple conic, then it is numerically tt-unstable for all t>29t>\frac{2}{9}. If qq is singular, then (q,f)(q,f) is numerically tt-unstable for all t<29t<\frac{2}{9}.

Proof.

First, consider the case where CC is a triple conic. Without loss of generality, we may assume that f=x03f=x_{0}^{3}. Consider the 1-PS with weights (3,1,1,1)(-3,1,1,1). Then μ(q,λ)2\mu(q,\lambda)\leq 2 and μ(f,λ)=9\mu(f,\lambda)=-9. Hence

μt((q,f),λ)9t+2\mu^{t}((q,f),\lambda)\leq-9t+2

which is negative when t>29t>\frac{2}{9}.

Now, consider the case where qq is singular. Without loss of generality, we may assume that the singular point is the point p=(1,0,0,0)p=(1,0,0,0). Consider the 1-PS with weights (3,1,1,1)(3,-1,-1,-1). Then, since qq is singular at pp, we have μ(q,λ)=2\mu(q,\lambda)=-2 and μ(f,λ)9\mu(f,\lambda)\leq 9, so

μt((q,f),λ)9t2\mu^{t}((q,f),\lambda)\leq 9t-2

which is negative when t<29t<\frac{2}{9}. ∎

We now change directions, and establish stability in some cases. First, we recall a basic result from GIT.

Lemma 4.17.

Let XX be a scheme (of finite type over an algebraically closed field kk) and let GG be a reductive algebraic group (over kk) acting on XX. Suppose LL is a GG-linearized line bundle on XX. There is a natural induced action of GG on XssX^{ss} and an induced linearization on L|XssL|_{X^{ss}} so that there is an isomorphism of categorical quotients X//LGXss//L|XssGX/\!\!/_{L}G\cong X^{ss}/\!\!/_{L|_{X^{ss}}}G. Moreover, if XX is complete, LL is ample, and XssX^{ss}\neq\emptyset, then there exists m,n0m,n_{0}\in\mathbb{N} such that for all nn0n\geq n_{0}, H0(Xss,(Lssm)n)G=H0(X,(Lm)n)GH^{0}(X^{ss},(L_{ss}^{\otimes m})^{\otimes n})^{G}=H^{0}(X,(L^{\otimes m})^{\otimes n})^{G}.

Proof.

First we consider the GIT quotients X//LGX/\!\!/_{L}G and Xss//L|XssGX^{ss}/\!\!/_{L|_{X^{ss}}}G. If Xss=X^{ss}=\emptyset, then the statement of the lemma is vacuous, so we may assume XssX^{ss}\neq\emptyset. Then the injective restriction maps H0(X,Ln)GH0(Xss,L|Xssn)GH^{0}(X,L^{\otimes n})^{G}\to H^{0}(X^{ss},L|_{X^{ss}}^{\otimes n})^{G} make it clear that any xXssx\in X^{ss} is semi-stable for the GG-linearization of L|XssL|_{X^{ss}}. Thus the semi-stable loci agree. Since the GG-action on XssX^{ss} is induced from that on XX, one concludes there is an isomorphism X//LGXss//L|XssGX/\!\!/_{L}G\cong X^{ss}/\!\!/_{L|_{X^{ss}}}G of the categorical quotients.

Now let us consider the spaces of global sections

H0(Xss,(Lssm)n)G and H0(X,(Lm)n)G.H^{0}(X^{ss},(L_{ss}^{\otimes m})^{\otimes n})^{G}\ \ \text{ and }\ \ H^{0}(X,(L^{\otimes m})^{\otimes n})^{G}.

We are now assuming that XX is complete, LL is ample and XssX^{ss}\neq\emptyset. First, note that there is a surjection π:XssX//LG\pi:X^{ss}\to X/\!\!/_{L}G. Moreover, we have a line bundle 𝒪(1)\mathscr{O}(1) on X//LGX/\!\!/_{L}G such that (up to rescaling LL) we have π𝒪(1)=Lss\pi^{*}\mathscr{O}(1)=L_{ss}. By construction of Proj\operatorname{Proj}, and using the assumption that XX is complete and LL is ample, so that X//LG=ProjR(X,L)GX/\!\!/_{L}G=\operatorname{Proj}R(X,L)^{G}, we get H0(X//LG,𝒪(n))=H0(X,Ln)GH^{0}(X/\!\!/_{L}G,\mathscr{O}(n))=H^{0}(X,L^{\otimes n})^{G} (for n0n\gg 0). Finally, by construction, H0(Xss,Lssn)G=H0(X//LG,𝒪(n))H^{0}(X^{ss},L_{ss}^{\otimes n})^{G}=H^{0}(X/\!\!/_{L}G,\mathscr{O}(n)) completing the proof. ∎

We use this lemma in the following.

Lemma 4.18.

If 0<t<290<t<\frac{2}{9}, then (q,f)(q,f) is tt-(semi)stable if and only if qq is smooth and f|qf|_{q} is terminally (semi)stable.

Proof.

Note that, when 0<t<290<t<\frac{2}{9}, the line bundle η+th\eta+th is ample, so in this case numerical (semi-)stability is the same as actual (semi-)stability. Let QQ be the smooth quadric defined by x02+x12+x22+x32=0x_{0}^{2}+x_{1}^{2}+x_{2}^{2}+x_{3}^{2}=0 and write i:EQEi:\mathbb{P}E_{Q}\hookrightarrow\mathbb{P}E for the inclusion of the fiber of E\mathbb{P}E over QQ. Write G=SL(4)G=\mathrm{SL}(4) and G=SO(4)G^{\prime}=\mathrm{SO}(4) for the stabilizer of QQ. Consider the quasi-projective variety EQ~=G×GEQ\widetilde{\mathbb{P}E_{Q}}=G\times_{G^{\prime}}\mathbb{P}E_{Q}, which is the quotient of G×EQG\times\mathbb{P}E_{Q} by the free action of GG^{\prime}: h(g,x)=(gh1,hx)h(g,x)=(gh^{-1},hx) for hGh\in G^{\prime}. There is a natural identification of the ring of invariants (cf. [Kir09, p.10 Eq. (3)]):

(4.19) R:=n0H0(EQ,ni(η+th))Gn0H0(EQ~,n(η+th))G.R^{\prime}:=\bigoplus_{n\geq 0}H^{0}(\mathbb{P}E_{Q},ni^{*}(\eta+th))^{G^{\prime}}\cong\bigoplus_{n\geq 0}H^{0}(\widetilde{\mathbb{P}E_{Q}},n(\eta+th))^{G}.

Notice that EQ\mathbb{P}E_{Q} has Picard rank 1, so i(η+th)=𝒪(d)i^{*}(\eta+th)=\mathcal{O}(d) for some d0d\geq 0.

Now, observe that EQ~\widetilde{\mathbb{P}E_{Q}} is isomorphic to the open set VEV\subset\mathbb{P}E parameterizing pairs (q,f)(q,f) where qq is smooth. To see this, note that G×EQG\times\mathbb{P}E_{Q} admits a GG^{\prime}-invariant map to this space sending (g,f)(g,f) to (gQ,gf)(g\cdot Q,g\cdot f). This map induces an isomorphism on the quotient because the quadric qq is uniquely determined by an element of G/GG/G^{\prime}.

Finally, note that when t<29t<\frac{2}{9}, every numerically tt-semi-stable point lies on a smooth quadric. From the computations above it follows that EssV\mathbb{P}E^{ss}\subseteq V. Thus, by virtue of Lemma 4.17,

H0(E,n(η+th))GH0(V,n(η+th))GH^{0}(\mathbb{P}E,n(\eta+th))^{G}\cong H^{0}(V,n(\eta+th))^{G}

for these values of tt. Hence

E//tG=Projn0H0(E,n(η+th))G=Projn0H0(V,n(η+th))G\mathbb{P}E/\!\!/_{t}G=\operatorname{Proj}\bigoplus_{n\geq 0}H^{0}(\mathbb{P}E,n(\eta+th))^{G}=\operatorname{Proj}\bigoplus_{n\geq 0}H^{0}(V,n(\eta+th))^{G}
=Projn0H0(EQ,𝒪(n))G=EQ//G.=\operatorname{Proj}\bigoplus_{n\geq 0}H^{0}(\mathbb{P}E_{Q},\mathcal{O}(n))^{G^{\prime}}=\mathbb{P}E_{Q}/\!\!/G^{\prime}.

5. Quotients of the Hilbert Scheme

A standard approach to constructing birational models of M¯g\overline{M}_{g} is to consider the pluricanonical image of a curve as a point in a Chow variety or Hilbert scheme. One can then construct the GIT quotient of this Chow variety or Hilbert scheme by the group of automorphisms of the ambient projective space. This approach can be found, for example, in both Mumford’s and Gieseker’s constructions of M¯g\overline{M}_{g} as an irreducible projective variety (see [Mum77], [Gie82]). It is also the method by which Schubert [Sch91] constructed the moduli space of pseudostable curves M¯gps\overline{M}_{g}^{ps}, and Hassett and Hyeon [HH08] constructed the first flip in the Hassett–Keel program. In our situation, we will consider the GIT quotients Hilb4,1m//ΛmSL(4)\operatorname{Hilb}_{4,1}^{m}/\!\!/_{\Lambda_{m}}\operatorname{SL}(4). Recall that points of Hilb4,1m\operatorname{Hilb}_{4,1}^{m} are called mm-th Hilbert points.

5.1. Numerical criterion for finite Hilbert stability

A criterion for stability of Hilbert points was worked out in [HHL10]. We briefly review their results.

Let XNX\subset\mathbb{P}^{N} be a variety with Hilbert polynomial P(m)P(m). We will write km=(N+mm)P(m)k_{m}=\binom{N+m}{m}-P(m). For any vN+1v\in\mathbb{R}^{N+1}, we define an ordering <v<_{v} on the set of monomials in N+1N+1 variables as follows:

xa<vxbx^{a}<_{v}x^{b} if

  1. (1)

    degxa<degxb\deg x^{a}<\deg x^{b};

  2. (2)

    degxa=degxb\deg x^{a}=\deg x^{b} and v.a<v.bv.a<v.b;

  3. (3)

    degxa=degxb\deg x^{a}=\deg x^{b}, v.a=v.bv.a=v.b, and xa<Lexxbx^{a}<_{Lex}x^{b} in the lexicographic order.

In particular, given a 1-PS λ\lambda with weight vector α=(α0,α1,,αN)\alpha=(\alpha_{0},\alpha_{1},\ldots,\alpha_{N}), the monomial order <λ<_{\lambda} is the lexicographic order associated to the weight α\alpha. For each polynomial ff, let in<λ(f)in_{<_{\lambda}}(f) denote the largest term of ff with respect to <λ<_{\lambda}. For an ideal II, we define in<λ(I)=in<λ(f)|fIin_{<_{\lambda}}(I)=\langle in_{<_{\lambda}}(f)|f\in I\rangle.

Proposition 5.1 ([HHL10]).

A point IHilb4,1m𝔾(km,nm)I\in\operatorname{Hilb}^{m}_{4,1}\subset\mathbb{G}(k_{m},n_{m}) is semi-stable if and only if, for every 1-PS λ\lambda, we have

xain<λ(I)wtλ(xa)0\sum_{x^{a}\in in_{<_{\lambda}}(I)}wt_{\lambda}(x^{a})\geq 0

where the left-hand sum is over the monomials xax^{a} of degree mm in in<λ(I)in_{<_{\lambda}}(I).

Note that when km=1k_{m}=1, this criterion coincides with the criterion for hypersurfaces described in §4.

Proposition 5.2.

If IHilb4,1mI\in\operatorname{Hilb}^{m}_{4,1} is not the mthm^{th} Hilbert point of a (2,3)(2,3)-complete intersection, then it is not mm-Hilbert semi-stable for any m2m\geq 2. Similarly, if XChow4,1X\in\operatorname{Chow}_{4,1} is not a complete intersection, then it is not Chow-semi-stable.

Proof.

Let IHilb4,1m𝔾(km,nm)I\in\operatorname{Hilb}^{m}_{4,1}\subset\mathbb{G}(k_{m},n_{m}) be a vector space. We note that there is a quadric qq and a cubic ff, not divisible by qq, such that II contains all monomials of the form qxaqx^{a} and fxbfx^{b}, where xax^{a} is a monomial of degree m2m-2 and xbx^{b} is a monomial of degree m3m-3. Indeed, this condition is closed in 𝔾(km,nm)\mathbb{G}(k_{m},n_{m}), so it is satisfied by every element of Hilb4,1m\operatorname{Hilb}^{m}_{4,1}. If qq and ff do not share a common linear factor, then II is necessarily the mthm^{th} Hilbert point of the intersection q=f=0q=f=0.

Assume that qq and ff share a common linear factor. We may choose coordinates such that q=x0x1q=x_{0}x_{1}, and ff is divisible by x0x_{0}. We may further assume that ff has a nonzero x0x32x_{0}x_{3}^{2} term. Now, consider the 1-PS λ\lambda with weights (3,1,1,1)(-3,1,1,1). By definition, II contains all of the monomials of the form x0x1xax_{0}x_{1}x^{a}, where xax^{a} is a monomial of degree m2m-2, and of the form x0x32xbx_{0}x_{3}^{2}x^{b}, where xbx^{b} is a monomial of degree m3m-3. The number of such monomials is

(m+13)+(m3)(m13)=16(m1)(m2+4m6)\binom{m+1}{3}+\binom{m}{3}-\binom{m-1}{3}=\frac{1}{6}(m-1)(m^{2}+4m-6)

and the total weight of these monomials is

2(m+13)(m3)=12m2(m1).-2\binom{m+1}{3}-\binom{m}{3}=-\frac{1}{2}m^{2}(m-1).

It follows that

xain<λ(I)wtλ(xa)\sum_{x^{a}\in in_{<_{\lambda}}(I)}wt_{\lambda}(x^{a})
m[(m+33)(6m3)16(m1)(m2+4m6)]12m2(m1)\leq m\left[\binom{m+3}{3}-(6m-3)-\frac{1}{6}(m-1)(m^{2}+4m-6)\right]-\frac{1}{2}m^{2}(m-1)
=12m(m2)(m3)12m2(m1)=m(2m3).=\frac{1}{2}m(m-2)(m-3)-\frac{1}{2}m^{2}(m-1)=-m(2m-3).

Since this is negative for all m2m\geq 2, we see that II is not mm-Hilbert semi-stable for these same mm. We obtain the analogous result for the Chow variety by noting that limmm(2m3)m2<0.\lim_{m\to\infty}\frac{-m(2m-3)}{m^{2}}<0.

We would like to compare the numerical criterion for points in the Hilbert scheme to the numerical criterion for points on E\mathbb{P}E. To this end, we have the following:

Proposition 5.3.

Suppose yHilb4,1y\in\operatorname{Hilb}_{4,1} corresponds to a (2,3)(2,3)-complete intersection C3C\subseteq\mathbb{P}^{3}. Denote also by yy the corresponding point in E\mathbb{P}E. There exists a positive constant cc\in\mathbb{Q} such that for any 1-parameter subgroup λ\lambda, we have μ23(y,λ)cμψΛ(y,λ)\mu^{\frac{2}{3}}(y,\lambda)\geq c\mu^{\psi_{\infty}^{*}\Lambda_{\infty}}(y,\lambda).

Proof.

This follows directly from Benoist [Ben11, Prop. 4.3] and Remark 1.10. ∎

6. Quotients of the Rojas–Vainsencher resolution

In this section we complete the arguments needed in Section 4 (esp. for Theorem 6.3) to handle GIT for non-ample bundles on E\mathbb{P}E. The main point is to use the results on Hilbert stability of the previous section together with the Rojas–Vainsencher resolution WW of the rational map EHilb4,1\mathbb{P}E\dashrightarrow\operatorname{Hilb}_{4,1} (see §1.4):

Wπ1π2EHilb4,1.\lx@xy@svg{\hbox{\raise 2.5pt\hbox{\kern 10.38194pt\hbox{\ignorespaces\ignorespaces\ignorespaces\hbox{\vtop{\kern 0.0pt\offinterlineskip\halign{\entry@#!@&&\entry@@#!@\cr&&\\&&\crcr}}}\ignorespaces{\hbox{\kern-3.0pt\raise 0.0pt\hbox{\hbox{\kern 0.0pt\raise 0.0pt\hbox{\hbox{\kern 3.0pt\raise-2.5pt\hbox{$\textstyle{}$}}}}}}}{\hbox{\kern 34.38194pt\raise 0.0pt\hbox{\hbox{\kern 0.0pt\raise 0.0pt\hbox{\hbox{\kern 3.0pt\raise-2.5pt\hbox{$\textstyle{W\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces\ignorespaces}$}}}}}}}\ignorespaces\ignorespaces\ignorespaces{}\ignorespaces\ignorespaces{\hbox{\lx@xy@drawline@}}\ignorespaces\ignorespaces\ignorespaces{\hbox{\kern 7.57475pt\raise-14.15277pt\hbox{{}\hbox{\kern 0.0pt\raise 0.0pt\hbox{\hbox{\kern 3.0pt\hbox{\hbox{\kern 0.0pt\raise-1.00694pt\hbox{$\scriptstyle{\pi_{1}}$}}}\kern 3.0pt}}}}}}\ignorespaces{\hbox{\kern 8.19267pt\raise-30.98611pt\hbox{\hbox{\kern 0.0pt\raise 0.0pt\hbox{\lx@xy@tip{1}\lx@xy@tip{-1}}}}}}\ignorespaces\ignorespaces{\hbox{\lx@xy@drawline@}}\ignorespaces{\hbox{\lx@xy@drawline@}}\ignorespaces\ignorespaces\ignorespaces{}\ignorespaces\ignorespaces{\hbox{\lx@xy@drawline@}}\ignorespaces\ignorespaces\ignorespaces{\hbox{\kern 66.12106pt\raise-14.15277pt\hbox{{}\hbox{\kern 0.0pt\raise 0.0pt\hbox{\hbox{\kern 3.0pt\hbox{\hbox{\kern 0.0pt\raise-1.00694pt\hbox{$\scriptstyle{\pi_{2}}$}}}\kern 3.0pt}}}}}}\ignorespaces{\hbox{\kern 83.16174pt\raise-30.87498pt\hbox{\hbox{\kern 0.0pt\raise 0.0pt\hbox{\lx@xy@tip{1}\lx@xy@tip{-1}}}}}}\ignorespaces\ignorespaces{\hbox{\lx@xy@drawline@}}\ignorespaces{\hbox{\lx@xy@drawline@}}{\hbox{\kern 89.88895pt\raise 0.0pt\hbox{\hbox{\kern 0.0pt\raise 0.0pt\hbox{\hbox{\kern 3.0pt\raise-2.5pt\hbox{$\textstyle{}$}}}}}}}{\hbox{\kern-10.38194pt\raise-38.31943pt\hbox{\hbox{\kern 0.0pt\raise 0.0pt\hbox{\hbox{\kern 3.0pt\raise-2.5pt\hbox{$\textstyle{\mathbb{P}E\ignorespaces\ignorespaces\ignorespaces\ignorespaces}$}}}}}}}\ignorespaces\ignorespaces\ignorespaces{}\ignorespaces\ignorespaces{\hbox{\lx@xy@drawline@}}\ignorespaces{\hbox{\kern 75.21529pt\raise-38.31943pt\hbox{\hbox{\kern 0.0pt\raise 0.0pt\hbox{\lx@xy@tip{1}\lx@xy@tip{-1}}}}}}\ignorespaces\ignorespaces{\hbox{\lx@xy@drawline@}}\ignorespaces{\hbox{\lx@xy@drawline@}}{\hbox{\kern 39.79861pt\raise-38.31943pt\hbox{\hbox{\kern 0.0pt\raise 0.0pt\hbox{\hbox{\kern 3.0pt\raise-2.5pt\hbox{$\textstyle{}$}}}}}}}{\hbox{\kern 75.21529pt\raise-38.31943pt\hbox{\hbox{\kern 0.0pt\raise 0.0pt\hbox{\hbox{\kern 3.0pt\raise-2.5pt\hbox{$\textstyle{\operatorname{Hilb}_{4,1}}$}}}}}}}\ignorespaces}}}}\ignorespaces.

6.1. Study of GIT stability on WW

Generally speaking, the key to understanding GIT quotients for non-ample bundles is to relate them to quotients of birational models with (semi)ample linearizations. In our situation, we consider the birational model WW of E\mathbb{P}E with linearizations of the form

απ1η+βπ2(ψΛ).\alpha\pi_{1}^{*}\eta+\beta\pi_{2}^{*}(\psi_{\infty}^{*}\Lambda_{\infty}).

Note that for α,β0\alpha,\beta\geq 0, these linearizations are semiample on WW.

Notation 6.1.

Set L(t):=η+thL(t):=\eta+th (on E\mathbb{P}E) and Λ:=cψΛ\Lambda:=c\psi_{\infty}^{*}\Lambda_{\infty} (on Hilb4,1\operatorname{Hilb}_{4,1}), where cc is the constant in Proposition 5.3. Let M(t)=απ1L(0)+βπ2ΛM(t)=\alpha\pi_{1}^{*}L(0)+\beta\pi_{2}^{*}\Lambda (on WW), where α\alpha and β\beta are such that L(t)=αL(0)+βL(23)L(t)=\alpha L(0)+\beta L(\frac{2}{3}) (N.B. rankPic(E)=2\mathrm{rank}\operatorname{Pic}(\mathbb{P}E)=2). We will write Wss(t)W^{ss}(t) for the semistable locus on WW with respect to the linearization M(t)M(t), and Enss(t)\mathbb{P}E^{nss}(t) for the numerically semistable locus with respect to L(t)L(t).

We start by making the following observations on the behavior of GIT on WW.

Proposition 6.2.

Wss(t)π11(Enss(t))W^{ss}(t)\subseteq\pi_{1}^{-1}(\mathbb{P}E^{nss}(t)).

Proof.

First, suppose that yWy\in W is in the exceptional locus of the map π1\pi_{1}. Then π1(y)\pi_{1}(y) lies in the locus of pairs (q,f)(q,f) such that qq and ff share a common linear factor. Similarly, π2(y)\pi_{2}(y) is not a complete intersection of a quadric and a cubic. It follows from Proposition 4.6 that, for the 1-PS λ\lambda with weights (3,1,1,1)(-3,1,1,1), we have

μπ1L(0)(y,λ)\displaystyle\mu^{\pi_{1}^{*}L(0)}(y,\lambda) <\displaystyle< 0\displaystyle 0
μπ1L(23)(y,λ)\displaystyle\mu^{\pi_{1}^{*}L(\frac{2}{3})}(y,\lambda) <\displaystyle< 0.\displaystyle 0.

Moreover, it follows from Proposition 5.2 that

μπ2Λ(y,λ)<0.\mu^{\pi_{2}^{*}\Lambda}(y,\lambda)<0.

By the linearity of the Hilbert–Mumford index, yy is numerically unstable for all the line bundles in question. It follows that Wnss(t)W^{nss}(t) is contained in the ample locus of M(t)M(t), and thus Wnss(t)=Wss(t)W^{nss}(t)=W^{ss}(t).

Now suppose that yπ11(Enss(t))y\notin\pi_{1}^{-1}(\mathbb{P}E^{nss}(t)) is not in the exceptional locus of the map π1\pi_{1}. By Proposition 5.3 together with the linearity and functoriality of the Hilbert–Mumford index, there is a one-parameter subgroup λ\lambda such that

0>μαL(0)+βL(23)(y,λ)μαπ1L(0)+βπ2Λ(y,λ).0>\mu^{\alpha L(0)+\beta L(\frac{2}{3})}(y,\lambda)\geq\mu^{\alpha\pi_{1}^{*}L(0)+\beta\pi_{2}^{*}\Lambda}(y,\lambda).

It follows that yWss(t)y\notin W^{ss}(t). ∎

A consequence of Proposition 6.2 is that, for every tt in the range 0<t230<t\leq\frac{2}{3}, Wss(t)=Wnss(t)W^{ss}(t)=W^{nss}(t) is contained in the locus on which π2\pi_{2} restricts to an isomorphism. It follows that every invariant section of M(t)M(t) has affine non-vanishing locus, hence the usual results about GIT hold for the linearization M(t)M(t) despite the fact that it is only semi-ample, rather than ample. As another consequence, we may think of points in Wss(t)W^{ss}(t) as (2,3)(2,3)-complete intersections. Combining Proposition 6.2 with the results of §4.2, we can identify many tt-unstable points in WW. It remains to show that each curve that has not been explicitly destabilized thus far is in fact tt-semi-stable. We will prove this in Theorem 6.3. This type of argument is related in spirit to the potential stability argument used by Gieseker and Mumford for the GIT construction of M¯g\overline{M}_{g} (e.g. see [HM98, §4.C]).

Finally, we recall briefly the notion of the basin of attraction from [HL10b, Def. 4]. If the stabilizer of a curve CC^{\prime} contains a 1-PS λ\lambda, then the basin of attraction (of CC^{\prime} with respect to λ\lambda) is defined to be

Aλ(C):={C|C specializes to C under λ}.A_{\lambda}(C^{\prime}):=\{C\ |\ C\text{ specializes to }C^{\prime}\text{ under }\lambda\}.

If CC^{\prime} is strictly semi-stable with respect to λ\lambda, meaning that μ(C,λ)=0\mu(C^{\prime},\lambda)=0, then CC^{\prime} is semi-stable if and only if CC is semi-stable for every (equivalently, any) CAλ(C)C\in A_{\lambda}(C^{\prime}) (see [HH08, Lem. 4.3]).

We are now ready to prove the following key result describing the stability on the space WW which interpolates between E\mathbb{P}E and Hilb4,1\operatorname{Hilb}_{4,1}. The main advantages here are: (1) on WW we are in a standard GIT set-up (i.e. (semi-)ample linearizations, as opposed to the situation on E//tSL(4)\mathbb{P}E/\!\!/_{t}\mathrm{SL}(4) for t>12t>\frac{1}{2}), and (2) the natural spaces Hilb4,1m//SL(4)\operatorname{Hilb}^{m}_{4,1}/\!\!/\mathrm{SL}(4) are then easily described using W//tSL(4)W/\!\!/_{t}\mathrm{SL}(4).

Theorem 6.3.

Let CWss(t)C\in W^{ss}(t). Then CC is a complete intersection of a quadric and a cubic in 3\mathbb{P}^{3}, and:

  1. (1)

    CW(s)s(23)C\in W^{(s)s}(\frac{2}{3}) if and only if it is Chow (semi-)stable.

  2. (2)

    CW(s)s(t)C\in W^{(s)s}(t) for all t(611,23)t\in(\frac{6}{11},\frac{2}{3}) if and only if it is Chow (semi-)stable, but not a ribbon, an elliptic triborough, or a curve on a quadric cone with a tacnode at the vertex of the cone. The closed orbits of strictly tt-semi-stable points correspond to the maximally degenerate curve with A5A_{5} singularities (i.e. C2A5C_{2A_{5}} in the notation of §3) and the unions of three conics meeting in two D4D_{4} singularities (see Remark 3.7 (1) and (4)).

  3. (3)

    CWss(t)C\in W^{ss}(t) for all t(25,611)t\in(\frac{2}{5},\frac{6}{11}) if and only if

    1. (a)

      CWss(t)C\in W^{ss}(t) for t(611,23)t\in(\frac{6}{11},\frac{2}{3}) and is not an irreducible cuspidal curve with hyperelliptic normalization, or

    2. (b)

      CC contains a conic that meets the residual curve in a singularity of type A7A_{7}, but otherwise satisfies condition (2) of Theorem 3.1.

    The closed orbits of strictly tt-semi-stable points are the same as for t(611,23)t\in(\frac{6}{11},\frac{2}{3}).

  4. (4)

    CWss(t)C\in W^{ss}(t) for t(29,25)t\in(\frac{2}{9},\frac{2}{5}) if and only if

    1. (a)

      CWss(t)C\in W^{ss}(t) for t(25,611)t\in(\frac{2}{5},\frac{6}{11}) and is not an irreducible nodal curve with hyperelliptic normalization, or

    2. (b)

      CC has a triple-point singularity whose tangent cone is the union of a double conic and a conic meeting in two points, but otherwise satisfies condition (2) of Theorem 3.1.

    The closed orbits of strictly tt-semi-stable points correspond to the maximally degenerate curve with A5A_{5} singularities, the unions of three conics meeting in two D4D_{4} singularities, and the unions of a conic and a double conic meeting at two points (see Remark 3.7 (1), (3) and (4)).

  5. (5)

    CW(s)s(t)C\in W^{(s)s}(t) for t(0,29)t\in(0,\frac{2}{9}) if and only if it is contained in a smooth quadric and it is terminally (semi-)stable.

Proof.

As already mentioned, the strategy of the proof is to show that every curve that has not been explicitly destabilized by using the results of §4.2 and Proposition 6.2 is in fact tt-semi-stable. We start by proving items (1) and (5), which identify the quotients corresponding to the two end chambers of the VGIT on WW with the two GIT quotients discussed in §3. We then identify GIT walls using tt-semi-stable curves with positive dimensional stabilizer. We use the basin of attraction to determine tt-semi-stable curves at each wall. By general variation of GIT, each such curve that is contained in a smooth quadric is in fact tt-semi-stable for all smaller values of tt. In this way we identify the majority of tt-semi-stable curves. To establish the tt-semi-stability of the remaining curves, we use another basin of attraction argument.

Proof of (1). The isomorphism E//23SL(4)Chow4,1//SL(4)\mathbb{P}E/\!\!/_{\frac{2}{3}}\mathrm{SL}(4)\cong\operatorname{Chow}_{4,1}/\!\!/\mathrm{SL}(4) was established in [CMJL12]. Since M(23)=ΛM(\frac{2}{3})=\Lambda is semi-ample (it is the pull-back of the natural polarization 𝒪(1)\mathscr{O}(1) on Chow4,1\operatorname{Chow}_{4,1}), one obtains the identification ProjR(W,M(23))SL(4)=ProjR(Chow4,1,𝒪(1))SL(4)\operatorname{Proj}R\left(W,M(\frac{2}{3})\right)^{\mathrm{SL}(4)}=\operatorname{Proj}R(\operatorname{Chow}_{4,1},\mathscr{O}(1))^{\mathrm{SL}(4)}. In fact, although Λ\Lambda is only semi-ample, we have shown that Wss(M(t))=Wnss(M(t))W^{ss}(M(t))=W^{nss}(M(t)), and so one may also conclude that the (categorical) GIT quotients agree: W//M(23)SL(4)Chow4,1//SL(4)W/\!\!/_{M(\frac{2}{3})}\mathrm{SL}(4)\cong\operatorname{Chow}_{4,1}/\!\!/\mathrm{SL}(4). (QED (1))

Proof of (5). Suppose now that 0<t<290<t<\frac{2}{9} (in particular, L(t)L(t) is ample on E\mathbb{P}E) and note that by Prop. 6.2 and Lem. 4.18, Wss(t)π11(Enss(t))=π11(Ess(t))W^{ss}(t)\subseteq\pi_{1}^{-1}(\mathbb{P}E^{nss}(t))=\pi_{1}^{-1}(\mathbb{P}E^{ss}(t)) is contained in the open set VV consisting of pairs (q,f)(q,f) where qq is smooth. Since π1\pi_{1} restricts to an isomorphism on the open set VV and M(t)|V=L(t)|VM(t)|_{V}=L(t)|_{V}, (5) follows from Lemmas 4.17 and 4.18. (QED (5))

We now turn to the intermediate chambers. By general variation of GIT, we know that if CWss(ϵ)Wss(23)C\in W^{ss}(\epsilon)\cap W^{ss}(\frac{2}{3}), then CWss(t)C\in W^{ss}(t) for all tt in the range ϵ<t<23\epsilon<t<\frac{2}{3}. On the other hand, suppose that CC is neither Chow semi-stable nor terminally semi-stable. It follows that one of the following must be true:

  1. (1)

    CC contains a line LL such that LC\L¯L\cap\overline{C\backslash L} is a singular point of the residual curve;

  2. (2)

    CC has a singularity of multiplicity greater than three;

  3. (3)

    CC is contained in a quadric of rank 1 or 2;

  4. (4)

    CC is contained in a quadric cone and has a singularity of type other than A2A_{2}, A3A_{3} or A4A_{4} at the singular point of the cone;

  5. (5)

    CC is contained in a quadric cone and has a separating A7A_{7} singularity, or

  6. (6)

    CC is contained in a quadric cone and has a triple-point singularity of type other than D4D_{4}.

By Proposition 6.2 and the results of §4.2, any of the first four possibilities imply that CWss(t)C\notin W^{ss}(t) for any t<23t<\frac{2}{3}. The fifth case can only be tt-semi-stable for t[29,611]t\in[\frac{2}{9},\frac{6}{11}]. In the last case, CC specializes to its “tangent cone” under the one-parameter subgroup described in §2.2. By the proof of Proposition 4.11, this one-parameter subgroup has weight zero on CC, and hence if CC is tt-semi-stable then its tangent cone is tt-semi-stable as well. Since the singularity is not of type D4D_{4}, the tangent cone is non-reduced. It cannot be a triple conic unless t=29t=\frac{2}{9}, because by Proposition 4.16 a triple conic and a curve on a singular quadric cannot be simultaneously semi-stable except at this critical value. It therefore must be the union of a conic and a double conic on a quadric cone, which can only be tt-semi-stable for t[29,25]t\in[\frac{2}{9},\frac{2}{5}].

Having destabilized the necessary curves, we now turn our attention to showing that various curves are (semi-)stable for particular values of tt.

Proof of (2). We consider first the tt-interval (611,23)(\frac{6}{11},\frac{2}{3}). By the above, every tt-semi-stable point for t(611,23)t\in(\frac{6}{11},\frac{2}{3}) is either terminally semi-stable or Chow semi-stable. The only terminally polystable curves that are not Chow semi-stable are the triple conic, the double conics, and the curves with separating A7A_{7} singularities (§3.1, §3.2), and none of these can be tt-semi-stable for t>611t>\frac{6}{11}4.2). It follows that Wss(t)Wss(23)W^{ss}(t)\subset W^{ss}(\frac{2}{3}) for all tt in this interval. As a consequence, since a wall t0t_{0} of this GIT chamber is characterized by Wss(t0)Wss(23)W^{ss}(t_{0})\nsubseteq W^{ss}(\frac{2}{3}), the wall must lie outside the open tt-interval (611,23)(\frac{6}{11},\frac{2}{3}). By general variation of GIT, we therefore have that Ws(23)Wss(t)W^{s}(\frac{2}{3})\subset W^{ss}(t) for tt in this interval, and Wss(23)Wss(ϵ)Wss(t)W^{ss}(\frac{2}{3})\cap W^{ss}(\epsilon)\subset W^{ss}(t) for all 0<ϵ<t0<\epsilon<t (and in particular for 0<ϵ<290<\epsilon<\frac{2}{9}) as well.

Thus it remains to determine the tt-semi-stability of the remaining strictly Chow semi-stable points that are not terminally semi-stable. These all lie on the quadric cone. Considering the possibilities from Theorem 3.1, we see that the only such curves that have not already been destabilized are the curves on the quadric cone with AkA_{k} (k5k\geq 5) singularities (that do not have an AnA_{n} (n3n\geq 3) singularity at the vertex of the cone) and the curves on the quadric cone with D4D_{4} singularities.

Suppose first that C=V(q,f)C=V(q,f) is a 23\frac{2}{3}-semi-stable curve on the quadric cone that has an AkA_{k} (k5k\geq 5) singularity at a smooth point of the cone, but does not have an AnA_{n} (n3n\geq 3) singularity at the vertex of the cone. We argue by contradiction that CC is also tt-semi-stable. Suppose that λ\lambda is a one-parameter subgroup such that μt((q,f),λ)<0\mu^{t}((q,f),\lambda)<0. By standard facts from variation of GIT, one can assume that μ23((q,f),λ)=0\mu^{\frac{2}{3}}((q,f),\lambda)=0 (see e.g. [Laz11, §4.1.2 ]). Now let C=V(q,f)C^{\prime}=V(q^{\prime},f^{\prime}) be the specialization of CC under λ\lambda. Since λ\lambda fixes CC^{\prime}, it follows from the basin of attraction argument that CC^{\prime} is 23\frac{2}{3}-semi-stable as well. The only 23\frac{2}{3}-semi-stable curve in the orbit closure of CC, however, is a curve of the form

C=CA,B=V(x22x1x3,Ax13+Bx0x1x2+x02x3),C^{\prime}=C_{A,B}=V(x_{2}^{2}-x_{1}x_{3},Ax_{1}^{3}+Bx_{0}x_{1}x_{2}+x_{0}^{2}x_{3}),

whose stabilizer in the given coordinates is the \mathbb{C}^{*} with weights ±(3,1,1,3)\pm(3,1,-1,-3). All of the curves that specialize to CA,BC_{A,B} under the 11-PS with weights (3,1,1,3)(3,1,-1,-3) have an AnA_{n} (n3n\geq 3) singularity at the vertex of the cone. Consequently, λ\lambda must be the 11-PS with weights (3,1,1,3)(-3,-1,1,3). This gives μ(q,λ)=2\mu(q^{\prime},\lambda)=2 and μ(f,λ)=3\mu(f^{\prime},\lambda)=-3, so that μt((q,f),λ)>0\mu^{t}((q^{\prime},f^{\prime}),\lambda)>0 (any other representative of ff^{\prime} will have weight 3\geq-3). Now since (q,f)(q^{\prime},f^{\prime}) is the limit of (q,f)(q,f) under λ\lambda, we have μt((q,f),λ)=μt((q,f),λ)>0\mu^{t}((q,f),\lambda)=\mu^{t}((q^{\prime},f^{\prime}),\lambda)>0, a contradiction.

Similarly, if CC has a D4D_{4} singularity, then CC specializes to its tangent cone under the one-parameter subgroup described in §2.2, and this one-parameter subgroup has weight zero on CC by Proposition 4.11. Hence CC is tt-semi-stable if and only if its tangent cone is tt-semi-stable as well. Now, suppose that there is a one-parameter subgroup λ\lambda such that μt((q,f),λ)<0\mu^{t}((q,f),\lambda)<0. As in the previous case, we see that λ\lambda must be contained in the stabilizer of the 23\frac{2}{3}-polystable limit of CC, which is CD=V(x0x3,x13+x23)C_{D}=V(x_{0}x_{3},x_{1}^{3}+x_{2}^{3}). The stabilizer of CDC_{D} is the 2-dimensional torus consisting of one-parameter subgroups with weights of the form ±(a,1,1,2a)\pm(a,-1,-1,2-a). Since CC specializes to CDC_{D} under λ\lambda and CC is not contained in a reducible quadric, we see that λ\lambda has weights of the form (a,1,1,2a)(a,-1,-1,2-a). But then μ(x0x3,λ)=2\mu(x_{0}x_{3},\lambda)=2 and μ(x13+x23,λ)=3\mu(x_{1}^{3}+x_{2}^{3},\lambda)=-3, so as above, μt((q,f),λ)>0\mu^{t}((q,f),\lambda)>0, a contradiction. (QED (2))

The proofs of the remaining parts are similar. We include the details for the convenience of the reader.

Proof of (3). We next consider the tt-interval (25,611)(\frac{2}{5},\frac{6}{11}). For t<611t<\frac{6}{11}, cuspidal curves with hyperelliptic normalization can no longer be tt-semi-stable, so there must be a GIT wall at t=611t=\frac{6}{11}. This implies that there is a 611\frac{6}{11}-semi-stable curve with positive dimensional stabilizer that is not tt-semi-stable for t=611+ϵt=\frac{6}{11}+\epsilon. Reviewing the possibilities, we see that there is only one possible such curve, namely

C=V(x12+x0x2,x22x3+x0x32),C^{\prime}=V(x_{1}^{2}+x_{0}x_{2},x_{2}^{2}x_{3}+x_{0}x_{3}^{2}),

which has both a separating A7A_{7} singularity and a cusp at the vertex of the quadric cone on which it lies. If CWss(611+ϵ)C\in W^{ss}(\frac{6}{11}+\epsilon) is not in Wss(611ϵ)W^{ss}(\frac{6}{11}-\epsilon), then the orbit of CC under the \mathbb{C}^{*} that stabilizes CC^{\prime} must contain CC^{\prime} in its closure. It follows that, up to change of coordinates, CC must be of the form:

C=V(x12+x0x2+αx02+βx0x1,x22x3+x0x32+f(x0,x1,x2)),C=V(x_{1}^{2}+x_{0}x_{2}+\alpha x_{0}^{2}+\beta x_{0}x_{1},x_{2}^{2}x_{3}+x_{0}x_{3}^{2}+f(x_{0},x_{1},x_{2})),

where α,β\alpha,\beta are constants and ff is a cubic. In other words, CC must be contained in a singular quadric and have a cusp at the vertex. We therefore see that every (611+ϵ)(\frac{6}{11}+\epsilon)-semi-stable curve that is not of this form is (611ϵ)(\frac{6}{11}-\epsilon)-semi-stable as well.

To identify the remaining 611\frac{6}{11}-semi-stable curves, we use the basin of attraction of CC^{\prime}. Namely, since the curve CC^{\prime} is 611\frac{6}{11}-semi-stable, we see that every curve in the basin of attraction of CC^{\prime} is also 611\frac{6}{11}-semistable. By Proposition 4.12, we see that this includes every curve with a separating A7A_{7} singularity apart from those that we have explicitly destabilized already. If such a curve CC is contained in a smooth quadric, then CWss(611)Wss(0)C\in W^{ss}(\frac{6}{11})\cap W^{ss}(0), so CWss(t)C\in W^{ss}(t) for all t[0,611]t\in[0,\frac{6}{11}].

It remains to show that the curves contained in a quadric cone with a separating A7A_{7} singularity are in fact (611ϵ)(\frac{6}{11}-\epsilon)-semi-stable. So let C=V(q,f)C=V(q,f) be such a curve. To show CC is tt-semi-stable, we argue as above, noting that if λ\lambda is a 1-PS such that μt((q,f),λ)<0\mu^{t}((q,f),\lambda)<0, then λ\lambda must be contained in the stabilizer of the 611\frac{6}{11}-polystable limit of this curve, which is the curve CC^{\prime} above. The stabilizer of CC^{\prime} is a one-dimensional torus, so this determines the 1-PS λ\lambda uniquely. Indeed, in these coordinates, λ\lambda must be the 1-PS with weights (7,3,1,9)(7,3,-1,-9). Then μ(x12+x0x2,λ)=6\mu(x_{1}^{2}+x_{0}x_{2},\lambda)=6 and μ(x22x3+x0x32,λ)=11\mu(x_{2}^{2}x_{3}+x_{0}x_{3}^{2},\lambda)=-11, so as above μt((q,f),λ)>0\mu^{t}((q,f),\lambda)>0, a contradiction.

To complete this part of the proof, we note that by the above we obtain the inclusion Wss(t)Wss(611ϵ)W^{ss}(t)\subset W^{ss}(\frac{6}{11}-\epsilon) for all t(25,611)t\in(\frac{2}{5},\frac{6}{11}), and hence this interval is contained in a single GIT chamber. (QED (3))

Proof of (4). By arguments nearly identical to the previous case, we identify a GIT wall at t=25t=\frac{2}{5} corresponding to the curve C=V(x0x2x12,x1x32)C^{\prime}=V(x_{0}x_{2}-x_{1}^{2},x_{1}x_{3}^{2}), which is the union of a double conic and two rulings of a quadric cone. As before, if CWss(25+ϵ)C\in W^{ss}(\frac{2}{5}+\epsilon) is not in Wss(25ϵ)W^{ss}(\frac{2}{5}-\epsilon), then the orbit of CC under the stabilizer of CC^{\prime} must contain CC^{\prime} in its closure. It follows that, up to change of coordinates, CC must be of the form C=V(q(x0,x1,x2),f(x0,x1,x2,x3))C=V(q(x_{0},x_{1},x_{2}),f(x_{0},x_{1},x_{2},x_{3})), where ff is a cubic containing the vertex (0,0,0,1)(0,0,0,1). In other words, CC must be contained in a singular quadric and have a node at the vertex. We therefore see that every (25+ϵ)(\frac{2}{5}+\epsilon)-semi-stable curve that is not of this form is (25ϵ)(\frac{2}{5}-\epsilon)-semi-stable as well.

As in the previous case, we see that every curve with a double conic component, apart from those we have explicitly destabilized, is 25\frac{2}{5}-semi-stable, as such curves are in the basin of attraction of CC^{\prime}. Specifically, if a curve CC contains a double conic component that is contained in the plane x0=0x_{0}=0, then CC specializes to CC^{\prime} under the 1-PS with weights (3,1,1,1)(-3,1,1,1), which is contained in the stabilizer of CC^{\prime}. Furthermore, if such a curve is contained in a smooth quadric then it is contained in Wss(25)Wss(0)W^{ss}(\frac{2}{5})\cap W^{ss}(0), and hence it is tt-semi-stable for all t25t\leq\frac{2}{5}.

It remains to show that the double conics contained in a quadric cone are (25ϵ)(\frac{2}{5}-\epsilon)-semi-stable as well. For this, we argue as above, noting that if λ\lambda is a 1-PS such that μt((q,f),λ)<0\mu^{t}((q,f),\lambda)<0 for such a curve C=V(q,f)C=V(q,f), then λ\lambda must be contained in the stabilizer of the 25\frac{2}{5}-polystable limit of this curve, which is the curve CC^{\prime} above. The stabilizer of CC^{\prime} is the two-dimensional torus consisting of one parameter subgroups with weights ±(a,1,2a,3)\pm(a,1,2-a,-3). All the curves that specialize to CC under a 1-PS with weights (a,1,a2,3)(-a,-1,a-2,3) pass through the vertex of the cone, so λ\lambda must have weights (a,1,2a,3)(a,1,2-a,-3). But then μ(x0x2x12,λ)=2\mu(x_{0}x_{2}-x_{1}^{2},\lambda)=2 and μ(x1x32,λ)=5\mu(x_{1}x_{3}^{2},\lambda)=-5, so as above, μt((q,f),λ)>0\mu^{t}((q,f),\lambda)>0, a contradiction. The fact that the entire tt-interval (29,25)(\frac{2}{9},\frac{2}{5}) is contained in a GIT chamber follows exactly as above. (QED (4)). ∎

Remark 6.4.

Note that in the theorem, points that are strictly semi-stable on a wall may become stable in the adjacent chamber. For instance, for t=23t=\frac{2}{3}, the ribbon is semi-stable, and the strictly semi-stable points corresponding to curves with A8,A9A_{8},A_{9} singularities degenerate to this curve. For 611<t<23\frac{6}{11}<t<\frac{2}{3}, the ribbon is unstable, but the curves with A8,A9A_{8},A_{9} singularities become stable (not just semi-stable).

Remark 6.5.

The argument above also determines semi-stability conditions at the GIT walls.

  1. (1)

    At t=611t=\frac{6}{11}, both irreducible cuspidal curves with hyperelliptic normalization and curves with a separating A7A_{7} singularity are strictly semi-stable. The orbit closure of either type of curve contains the point

    x12+x0x2=x22x3+x0x32=0.x_{1}^{2}+x_{0}x_{2}=x_{2}^{2}x_{3}+x_{0}x_{3}^{2}=0.
  2. (2)

    At t=25t=\frac{2}{5}, both irreducible nodal curves with hyperelliptic normalization and double conics are strictly semi-stable. The orbit closure of either type of curve contains the union of a double conic and two rulings on the quadric cone, given by

    q(x0,x1,x2)=x0x32=0.q(x_{0},x_{1},x_{2})=x_{0}x_{3}^{2}=0.
  3. (3)

    At t=29t=\frac{2}{9}, both curves contained in a quadric cone and triple conics are strictly semi-stable. The orbit closure of either type of curve contains the triple conic on a quadric cone.

6.2. Comparing the GIT quotients

We set

W//tSL(4):=W//M(t)SL(4)=ProjR(W,M(t))SL(4),W/\!\!/_{t}\mathrm{SL}(4):=W/\!\!/_{M(t)}\mathrm{SL}(4)=\operatorname{Proj}R(W,M(t))^{\mathrm{SL}(4)},

where recall W//M(t)SL(4)W/\!\!/_{M(t)}\mathrm{SL}(4) is the categorical quotient of the semi-stable locus, and the equality on the right holds because Wnss(t)W^{nss}(t) is contained in the ample locus of M(t)M(t).

As discussed in Section 4, the GIT quotient E//tSL(4)\mathbb{P}E/\!\!/_{t}\mathrm{SL}(4) makes sense as a categorical quotient for all tt. However, for non-ample linearizations (i.e. t12t\geq\frac{1}{2}), it is not a priori clear how to describe it in terms of the numerically (semi-)stable points (e.g. Rem. 4.4). Here we note that Proposition 6.2 and Theorem 6.3 allows us to interpret our numerical results from the previous section as honest GIT results on the resolution WW, and then the expected properties of E//tSL(4)\mathbb{P}E/\!\!/_{t}\mathrm{SL}(4) follow (as well as the connection between numerical stability and stability).

Corollary 6.6.

For t[0,23]t\in[0,\frac{2}{3}], E//L(t)SL(4)=W//M(t)SL(4)\mathbb{P}E/\!\!/_{L(t)}\mathrm{SL}(4)=W/\!\!/_{M(t)}\mathrm{SL}(4) and for both spaces, numerical (semi-)stablility agrees with Mumford (semi-)stability. Moreover, the ring of invariant sections R(E,L(t))SL(4)R(\mathbb{P}E,L(t))^{\mathrm{SL}(4)} is finitely generated and

E//L(t)SL(4)=ProjR(E,L(t))SL(4).\mathbb{P}E/\!\!/_{L(t)}\mathrm{SL}(4)=\operatorname{Proj}R(\mathbb{P}E,L(t))^{\mathrm{SL}(4)}.
Proof.

The boundary cases t=0t=0 and t=23t=\frac{2}{3} have been proven already. For t(0,23)t\in(0,\frac{2}{3}), Wss(M(t))π11(Enss(L(t)))W^{ss}(M(t))\subseteq\pi_{1}^{-1}(\mathbb{P}E^{nss}(L(t))) by Prop 6.2. On the other hand, in Theorem 6.3 we showed that every curve that is not explicitly destabilized in §4.2 is in fact semi-stable in WW, so π11(Enss(L(t)))Wss(M(t))\pi_{1}^{-1}(\mathbb{P}E^{nss}(L(t)))\subseteq W^{ss}(M(t)). By Prop. 4.6, we see that π11(Enss(L(t)))\pi_{1}^{-1}(\mathbb{P}E^{nss}(L(t))) is contained in the locus where π1\pi_{1} restricts to an isomorphism identifying Enss(L(t))\mathbb{P}E^{nss}(L(t)) and π11(Enss(L(t)))\pi_{1}^{-1}(\mathbb{P}E^{nss}(L(t))). Thus the categorical quotient of Enss(L(t))\mathbb{P}E^{nss}(L(t)) agrees with the categorical quotient W//M(t)SL(4)W/\!\!/_{M(t)}\mathrm{SL}(4), which equals ProjR(M(t))SL(4)\operatorname{Proj}R(M(t))^{\mathrm{SL}(4)}.

Now consider the injective restriction maps:

H0(W,M(t))SL(4)H0(Wss,M(t)|Wss)SL(4)H^{0}(W,M(t))^{\mathrm{SL}(4)}\to H^{0}(W^{ss},M(t)|_{W^{ss}})^{\mathrm{SL}(4)}
H0(E,L(t))SL(4)H0(Enss,L(t)|Enss)SL(4).H^{0}(\mathbb{P}E,L(t))^{\mathrm{SL}(4)}\to H^{0}(\mathbb{P}E^{nss},L(t)|_{\mathbb{P}E^{nss}})^{\mathrm{SL}(4)}.

The map on the top is in fact surjective (up to possibly taking a higher tensor power of M(t)M(t)) by Lemma 4.17. The map on the bottom is surjective as well. This follows for t29t\leq\frac{2}{9} by Lemma 4.17, and for 29<t23\frac{2}{9}<t\leq\frac{2}{3} since the complement of Enss\mathbb{P}E^{nss} has codimension at least two. Since Enss\mathbb{P}E^{nss} is identified with WssW^{ss}, and M(t)|WssL(t)|EnssM(t)|_{W^{ss}}\cong L(t)|_{\mathbb{P}E^{nss}}, we get the equality we need.

It follows immediately that R(E,L(t))SL(4)R(\mathbb{P}E,L(t))^{\mathrm{SL}(4)} is finitely generated, and gives the same projective variety as R(W,M(t))SL(4)R(W,M(t))^{\mathrm{SL}(4)}. It is also elementary to check from this equality of invariant sections, that Mumford stability and numerical stability then agree on E\mathbb{P}E, since this holds on WW. Thus we have

E//L(t)SL(4)=W//M(t)SL(4)=ProjR(M(t))SL(4)=ProjR(L(t))SL(4).\mathbb{P}E/\!\!/_{L(t)}\mathrm{SL}(4)=W/\!\!/_{M(t)}\mathrm{SL}(4)=\operatorname{Proj}R(M(t))^{\mathrm{SL}(4)}=\operatorname{Proj}R(L(t))^{\mathrm{SL}(4)}.

We now compare the GIT quotients of WW to those of the Hilbert scheme.

Theorem 6.7.

We have the following isomorphisms of GIT quotients:

  1. (1)

    Chow4,1//SL(4)W//M(23)SL(4).\operatorname{Chow}_{4,1}/\!\!/\mathrm{SL}(4)\cong W/\!\!/_{M(\frac{2}{3})}\mathrm{SL}(4).

  2. (2)

    Hilb4,1m//SL(4)W//M(t)SL(4)\operatorname{Hilb}^{m}_{4,1}/\!\!/\mathrm{SL}(4)\cong W/\!\!/_{M(t)}\mathrm{SL}(4), where t=m2m+1t=\frac{m-2}{m+1} for 2m42\leq m\leq 4 and t=2(m2)23m29m+8t=\frac{2(m-2)^{2}}{3m^{2}-9m+8} m5\forall m\geq 5.

Proof.

(1) was established in the proof of Theorem 6.3. (2) Let UEU\subset\mathbb{P}E be the open set parameterizing complete intersections (see Rem. 1.4) and UmHilb4,1mU_{m}\subset\operatorname{Hilb}^{m}_{4,1} be the corresponding open subset of Hilb4,1m\operatorname{Hilb}^{m}_{4,1}. By Proposition 5.2, Hilb4,1m,ssUm\operatorname{Hilb}^{m,ss}_{4,1}\subset U_{m}, hence Hilb4,1m//ΛmSL(4)Um//Λm|UmSL(4)\operatorname{Hilb}^{m}_{4,1}/\!\!/_{\Lambda_{m}}\mathrm{SL}(4)\cong U_{m}/\!\!/_{\Lambda_{m}|_{U_{m}}}\mathrm{SL}(4) by Lemma 4.17. The rational map φm:EHilb4,1m\varphi_{m}:\mathbb{P}E\dashrightarrow\operatorname{Hilb}^{m}_{4,1} restricts to an isomorphism φm|U:UUm\varphi_{m}|_{U}:U\to U_{m}, and φm|UΛm=L(t)|U\varphi_{m}|_{U}^{*}\Lambda_{m}=L(t)|_{U}, where tt is given by the formula above. It follows from Lem. 4.17 and Cor. 6.6 that Hilb4,1m//SL(4)Um//Λm|UmSL(4)U//L(t)|USL(4)E//tSL(4)\operatorname{Hilb}^{m}_{4,1}/\!\!/\mathrm{SL}(4)\cong U_{m}/\!\!/_{\Lambda_{m}|_{U_{m}}}\mathrm{SL}(4)\cong U/\!\!/_{L(t)|_{U}}\mathrm{SL}(4)\cong\mathbb{P}E/\!\!/_{t}\mathrm{SL}(4). ∎

7. Hassett–Keel Program

So far, we have described the GIT quotients E//tSL(4)\mathbb{P}E/\!\!/_{t}\mathrm{SL}(4) parameterizing (2,3)(2,3)-complete intersections in 3\mathbb{P}^{3}, as well as the birational transformations among them as the linearization varies. To complete the proof of the Main Theorem stated in the introduction, we only need to relate these GIT quotients to the Hassett–Keel spaces M¯4(α)\overline{M}_{4}(\alpha). In fact, by [CMJL12] and [Fed12], this is already known for the extremal values of the slope tt (see (3.4) and (3.8)). Now, using the GIT computation of the previous sections, we will obtain in Theorem 7.1 the relationship for the intermediate cases.

To prove the theorem, we will use some elementary properties of birational contractions (e.g. [HK00, §1]). Let f:XYf:X\dashrightarrow Y be a birational map between normal projective varieties with XX \mathbb{Q}-factorial. Let (π1,π2):WX×Y(\pi_{1},\pi_{2}):W\to X\times Y be a resolution of ff, with WW projective (and π1\pi_{1} birational). We call ff a birational contraction if every π1\pi_{1}-exceptional divisor is also a π2\pi_{2}-exceptional divisor. In this case, for a \mathbb{Q}-Cartier divisor DD on YY, we define fDf^{*}D to be (π1)(π2D)(\pi_{1})_{*}(\pi_{2}^{*}D) and one can check that H0(Y,D)=H0(X,fD)H^{0}(Y,D)=H^{0}(X,f^{*}D). These definitions are independent of the choice of resolution.

Theorem 7.1.

Each of the log minimal models M¯4(α)\overline{M}_{4}(\alpha) for α59\alpha\leq\frac{5}{9} is isomorphic to one of the GIT quotients constructed above. Namely, we have

M¯4(α)E//tSL(4)\overline{M}_{4}(\alpha)\cong\mathbb{P}E/\!\!/_{t}\mathrm{SL}(4)

where t=34α1633α14t=\frac{34\alpha-16}{33\alpha-14} α[817,59]\forall\alpha\in[\frac{8}{17},\frac{5}{9}].

Proof.

We argue similarly to the case α=59\alpha=\frac{5}{9}, which is Theorem 3.4 in [CMJL12]. First, by the description of the GIT stability, we get that the natural map

φ:M¯4E//tSL(4)\varphi:\overline{M}_{4}\dashrightarrow\mathbb{P}E/\!\!/_{t}\mathrm{SL}(4)

is a birational contraction for all t(0,23]t\in\left(0,\frac{2}{3}\right]. We then write

φ(4sη+4h)=aλb0δ0b1δ1b2δ2.\varphi^{*}(4s\eta+4h)=a\lambda-b_{0}\delta_{0}-b_{1}\delta_{1}-b_{2}\delta_{2}.

(using s=1ts=\frac{1}{t} and the scalar 44 to make the formulas more attractive). The computations in §1.2.1 tell us that a=34s33a=34s-33 and b0=4s4b_{0}=4s-4. To compute the coefficients b1b_{1} and b2b_{2}, we proceed exactly as in [CMJL12]. In particular, let ZM¯4Z\subset\overline{M}_{4} be the curve obtained by gluing a fixed non-hyperelliptic curve CC of genus 3 to a varying elliptic tail. By the results of §1.3 of [CMJL12], the map φ\varphi is regular and constant along ZZ, so b1=14s15b_{1}=14s-15. Specifically, we see that the image of ZZ is the point corresponding to the cuspidal curve with normalization CC, which is tt-stable for all t(0,23]t\in(0,\frac{2}{3}]. Similarly, we see that if j:M¯2,1M¯4j:\overline{M}_{2,1}\to\overline{M}_{4} is the standard gluing map, then jφ(4sη+4h)j^{*}\varphi^{*}(4s\eta+4h) is supported along the union of δ1\delta_{1} and the Weierstrass divisor, and hence b2=18s21b_{2}=18s-21. In short, we obtain

φ(4sη+4h)=(34s33)λ(4s4)δ0(14s15)δ1(18s21)δ2.\varphi^{*}(4s\eta+4h)=(34s-33)\lambda-(4s-4)\delta_{0}-(14s-15)\delta_{1}-(18s-21)\delta_{2}.

Now, since δ1\delta_{1} and δ2\delta_{2} are φ\varphi-exceptional and t23<1417t\leq\frac{2}{3}<\frac{14}{17}, we have

H0(M¯4,nφ(4sη+4h))H^{0}(\overline{M}_{4},n\varphi^{*}(4s\eta+4h))
\displaystyle\cong H0(M¯4,nφ(4sη+4h)+(10s11)δ1+(14s17)δ2))\displaystyle H^{0}(\overline{M}_{4},n\varphi^{*}(4s\eta+4h)+(10s-11)\delta_{1}+(14s-17)\delta_{2}))
=\displaystyle= H0(M¯4,n((34s33)λ(4s4)(δ0+δ1+δ2))).\displaystyle H^{0}(\overline{M}_{4},n((34s-33)\lambda-(4s-4)(\delta_{0}+\delta_{1}+\delta_{2}))).

Thus, for s=33α1434α16s=\frac{33\alpha-14}{34\alpha-16},

E//tSL(4)\displaystyle\mathbb{P}E/\!\!/_{t}\mathrm{SL}(4) =\displaystyle= ProjnH0(E//tSL(4),n(4sη+4h))\displaystyle\operatorname{Proj}\bigoplus_{n}H^{0}(\mathbb{P}E/\!\!/_{t}\mathrm{SL}(4),n(4s\eta+4h))
=\displaystyle= ProjnH0(M¯4,nφ(4sη+4h))\displaystyle\operatorname{Proj}\bigoplus_{n}H^{0}(\overline{M}_{4},n\varphi^{*}(4s\eta+4h))
\displaystyle\cong ProjnH0(M¯4,n(KM¯4+αδ))\displaystyle\operatorname{Proj}\bigoplus_{n}H^{0}\left(\overline{M}_{4},n\left(K_{\overline{M}_{4}}+\alpha\delta\right)\right)
=\displaystyle= M¯4(α).\displaystyle\overline{M}_{4}\left(\alpha\right).

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