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Lê numbers and Newton diagram

Christophe Eyral, Grzegorz Oleksik, Adam Różycki
Abstract.

We give an algorithm to compute the Lê numbers of (the germ of) a Newton non-degenerate complex analytic function f:(n,0)(,0)f\colon(\mathbf{\mathbb{C}}^{n},0)\rightarrow(\mathbf{\mathbb{C}},0) in terms of certain invariants attached to the Newton diagram of the function f+z1α1++zdαdf+z_{1}^{\alpha_{1}}+\cdots+z_{d}^{\alpha_{d}}, where dd is the dimension of the critical locus of ff and α1,,αd\alpha_{1},\ldots,\alpha_{d} are sufficiently large integers. This is a version for non-isolated singularities of a famous theorem of A. G. Kouchnirenko. As a corollary, we obtain that Newton non-degenerate functions with the same Newton diagram have the same Lê numbers.

Key words and phrases:
Non-isolated hypersurface singularity, Lê numbers, Newton diagram, Modified Newton numbers, Iomdine-Lê-Massey formula
2010 Mathematics Subject Classification:
32S25, 14J17, 14J70

1. Introduction

The most important numerical invariant attached to a complex analytic function f:(n,0)(,0)f\colon(\mathbf{\mathbb{C}}^{n},0)\rightarrow(\mathbf{\mathbb{C}},0) with an isolated singularity at 0 is its Milnor number at 0 (denoted by μf(0)\mu_{f}(0)). By a theorem of A. G. Kouchnirenko [7], we know that if ff is (Newton) non-degenerate and such that its Newton diagram meets each coordinate axis (so-called “convenient” function), then ff has an isolated singularity at 0 and μf(0)\mu_{f}(0) coincides with the Newton number ν(f)\nu(f) of ff — a numerical invariant attached to the Newton diagram of ff. Actually, if ff is a non-degenerate function with an isolated singularity at 0, then μf(0)=ν(f)\mu_{f}(0)=\nu(f) even if ff is not convenient (see [1]). This provides an elegant and easy way to compute the Milnor number of such functions.

For a function with a non-isolated singularity at 0, the Milnor number is no longer relevant. However, we can attach to such a function a series of polar invariants which plays a similar role to that of the Milnor number for an isolated singularity. These polar invariants are called Lê numbers. They were introduced by D. B. Massey in the 1990s (see [10, 11, 12]). Then we may wonder whether like for the Milnor number, the Lê numbers of a non-degenerate function ff with a non-isolated singularity at 0 can also be described with the help of invariants attached to a Newton diagram. In this paper, we positively answer this question. More precisely, we show that the Lê numbers of a non-degenerate function ff can be expressed in terms of certain invariants (which we shall call modified Newton numbers) attached to the Newton diagram of the function f+z1α1++zdαdf+z_{1}^{\alpha_{1}}+\ldots+z_{d}^{\alpha_{d}}, where dd is the dimension at 0 of the critical locus of ff and α1,,αd\alpha_{1},\ldots,\alpha_{d} are sufficiently large integers (see Theorem 4.1).

As an important corollary, we obtain that non-degenerate functions with the same Newton diagram have the same Lê numbers (see Corollary 5.1). In particular, any 11-parameter deformation family of non-degenerate functions with constant Newton diagram has constant Lê numbers. We recall that families with constant Lê numbers satisfy remarkable properties. For example, in [11], Massey proved that under appropriate conditions the diffeomorphism type of the Milnor fibrations associated to the members of such a family is constant. In [5], J. Fernández de Bobadilla showed that in the special case of families of 11-dimensional singularities, the constancy of Lê numbers implies the topological triviality of the family at least if n5n\geq 5.

The paper is organized as follows. In Section 2, we recall the definition of the Lê numbers. In Section 3, following Kouchnirenko’s definition of the Newton number, we introduce our modified Newton numbers. Our main result — the formulas for the Lê numbers of a non-degenerate function ff in terms of the modified Newton numbers of the function f+z1α1++zdαdf+z_{1}^{\alpha_{1}}+\cdots+z_{d}^{\alpha_{d}} — is given in Section 4. Corollaries of these formulas are given in Section 5. In Section 6, we discuss a complete example. Finally, in Sections 7 and 8, we give the proofs of our main result and main corollary respectively.

2. Lê numbers

Lê numbers are intersection numbers of certain analytic cycles — so-called Lê cycles — with certain affine subspaces. The Lê cycles are defined using the notion of gap sheaf. In this section, we briefly recall these definitions which are essential for the paper. We also recall the notion of “polar ratio” which is involved in so-called Iomdine-Lê-Massey formula. This formula plays a crucial role in the proof of our main theorem.

We follow the presentation given by Massey in [10, 11, 12].

2.1. Gap sheaves

Let (X,𝒪X)(X,\mathscr{O}_{X}) be a complex analytic space, WXW\subseteq X be an analytic subset of XX, and \mathscr{I} be a coherent sheaf of ideals in 𝒪X\mathscr{O}_{X}. As usual, we denote by V()V(\mathscr{I}) the analytic space defined by the vanishing of \mathscr{I}. At each point xV()x\in V(\mathscr{I}), we want to consider scheme-theoretically those components of V()V(\mathscr{I}) which are not contained in WW. For this purpose, we look at a minimal primary decomposition of the stalk x\mathscr{I}_{x} of \mathscr{I} in the local ring 𝒪X,x\mathscr{O}_{X,x}, and we consider the ideal x¬W\mathscr{I}_{x}\lnot W in 𝒪X,x\mathscr{O}_{X,x} consisting of the intersection of those (possibly embedded) primary components QQ of x\mathscr{I}_{x} such that V(Q)WV(Q)\nsubseteq W. This definition does not depend on the choice of the minimal primary decomposition of x\mathscr{I}_{x}. Now, if we perform the operation described above at the point xx simultaneously at all points of V()V(\mathscr{I}), then we obtain a coherent sheaf of ideals called a gap sheaf and denoted by ¬W\mathscr{I}\lnot W. Hereafter, we shall denote by V()¬WV(\mathscr{I})\lnot W the scheme (i.e., the complex analytic space) V(¬W)V(\mathscr{I}\lnot W) defined by the vanishing of the gap sheaf ¬W\mathscr{I}\lnot W.

2.2. Lê cycles and Lê numbers

Consider an analytic function f:(U,0)(,0)f\colon(U,0)\rightarrow(\mathbb{C},0), where UU is an open neighbourhood of 0 in n\mathbb{C}^{n}, and fix a system of linear coordinates z=(z1,,zn)z=(z_{1},\ldots,z_{n}) for n\mathbb{C}^{n}. Let Σf\Sigma f be the critical locus of ff. For 0kn10\leq k\leq n-1, the kkth (relative) polar variety of ff with respect to the coordinates zz is the scheme

Γf,zk:=V(fzk+1,,fzn)¬Σf.\Gamma_{f,z}^{k}:=V\bigg{(}\frac{\partial f}{\partial z_{k+1}},\ldots,\frac{\partial f}{\partial z_{n}}\bigg{)}\lnot\Sigma f.

The analytic cycle

[Λf,zk]:=[Γf,zk+1V(fzk+1)][Γf,zk][\Lambda^{k}_{f,z}]:=\bigg{[}\Gamma_{f,z}^{k+1}\cap V\bigg{(}\frac{\partial f}{\partial z_{k+1}}\bigg{)}\bigg{]}-\bigg{[}\Gamma_{f,z}^{k}\bigg{]}

is called the kkth Lê cycle of ff with respect to the coordinates zz. (We always use brackets [][\cdot] to denote analytic cycles.) The kkth Lê number λf,zk(0)\lambda^{k}_{f,z}(0) of ff at 0n0\in\mathbb{C}^{n} with respect to the coordinates zz is defined to be the intersection number

(2.1) λf,zk(0):=([Λf,zk][V(z1,,zk)])0\lambda^{k}_{f,z}(0):=\big{(}[\Lambda^{k}_{f,z}]\cdot[V(z_{1},\ldots,z_{k})]\big{)}_{0}

provided that this intersection is 0-dimensional or empty at 0; otherwise, we say that λf,zk(0)\lambda^{k}_{f,z}(0) is undefined.111As usual, [V(z1,,zk)][V(z_{1},\ldots,z_{k})] denotes the analytic cycle associated to the analytic space defined by z1==zk=0z_{1}=\cdots=z_{k}=0. The notation ([Λf,zk][V(z1,,zk)])0\big{(}[\Lambda^{k}_{f,z}]\cdot[V(z_{1},\ldots,z_{k})]\big{)}_{0} stands for the intersection number at 0 of the analytic cycles [Λf,zk][\Lambda^{k}_{f,z}] and [V(z1,,zk)][V(z_{1},\ldots,z_{k})]. For k=0k=0, the relation (2.1) means

λf,z0(0)=([Λf,z0]U)0=[Γf,z1V(fz1)]0.\lambda^{0}_{f,z}(0)=\big{(}[\Lambda^{0}_{f,z}]\cdot U\big{)}_{0}=\bigg{[}\Gamma_{f,z}^{1}\cap V\bigg{(}\frac{\partial f}{\partial z_{1}}\bigg{)}\bigg{]}_{0}.

For any dim0Σf<kn1\dim_{0}\Sigma f<k\leq n-1, the Lê number λf,zk(0)\lambda^{k}_{f,z}(0) is always defined and equal to zero. For this reason, we usually only consider the Lê numbers

λf,z0(0),,λf,zdim0Σf(0).\lambda^{0}_{f,z}(0),\ldots,\lambda^{\dim_{0}\Sigma f}_{f,z}(0).

Note that if 0 is an isolated singularity of ff, then λf,z0(0)\lambda^{0}_{f,z}(0) (which is the only possible non-zero Lê number) is equal to the Milnor number μf(0)\mu_{f}(0) of ff at 0.

2.3. Polar ratios

As already mentioned above, a key ingredient in the proof of our main result is the Iomdine-Lê-Massey formula (see [12, Theorem 4.5]). Roughly, this formula says that if the Lê numbers of ff at 0 with respect to zz exist and if d:=dim0Σf1d:=\dim_{0}\Sigma f\geq 1, then for any integer α1\alpha_{1} large enough, dim0Σ(f+z1α1)=d1\dim_{0}\Sigma(f+z_{1}^{\alpha_{1}})=d-1 and the Lê numbers of f+z1α1f+z_{1}^{\alpha_{1}} at 0 with respect to the rotated coordinates z(1):=(z2,,zn,z1)z^{(1)}:=(z_{2},\ldots,z_{n},z_{1}) exist and they can be described in terms of the Lê numbers λf,zk(0)\lambda_{f,z}^{k}(0) of the original function ff. Moreover, the formula says that any α1>ρf,z(0)\alpha_{1}>\rho_{f,z}(0) is suitable, where ρf,z(0)\rho_{f,z}(0) is the maximum “polar ratio” of ff at 0 with respect to zz. In this section, we recall the definition of polar ratios (see [12, Definition 4.1]).

The notation is as in Section 2.2. Suppose that dim0Γf,z1=1\dim_{0}\Gamma^{1}_{f,z}=1. Let η\eta be an irreducible component of Γf,z1\Gamma^{1}_{f,z} (with its reduced structure) such that dim0(ηV(z1))=0\dim_{0}(\eta\cap V(z_{1}))=0. The polar ratio of η\eta at 0 is the number defined by

([η][V(f)])0([η][V(z1)])0=([η][V(fz1)])0([η][V(z1)])0+1.\frac{\bigl{(}[\eta]\cdot[V(f)]\bigr{)}_{0}}{\bigl{(}[\eta]\cdot[V(z_{1})]\bigr{)}_{0}}=\frac{\Bigl{(}\Bigl{[}\eta\Bigr{]}\cdot\Bigl{[}V\Bigl{(}\frac{\partial f}{\partial z_{1}}\Bigr{)}\Bigr{]}\Bigr{)}_{0}}{\bigl{(}[\eta]\cdot[V(z_{1})]\bigr{)}_{0}}+1.

If dim0(ηV(z1))0\dim_{0}(\eta\cap V(z_{1}))\not=0, then we say that the polar ratio of η\eta at 0 is equal to 11. A polar ratio for ff at 0 with respect to zz is any one of the polar ratios at 0 of any component of Γf,z1\Gamma^{1}_{f,z}.

For example, if ff is a homogeneous polynomial and if dim0Γf,z1=1\dim_{0}\Gamma^{1}_{f,z}=1, then each component of Γf,z1\Gamma^{1}_{f,z} is a line, and hence the polar ratios for ff at 0 with respect to zz are all equal to 11 or to the degree deg(f)\deg(f) of the polynomial ff (see [12, Remark 4.2]).

In [13, Section 3.2], M. Morgado and M. Saia gave an upper bound for the maximal polar ratio for a semi-weighted homogeneous arrangement.

3. Newton diagram and modified Newton numbers

Let z:=(z1,,zn)z:=(z_{1},\ldots,z_{n}) be a system of coordinates for n\mathbf{\mathbb{C}}^{n}, let UU be an open neighbourhood of the origin in n\mathbf{\mathbb{C}}^{n}, and let

f:(U,0)(,0),zf(z)=αcαzα,f\colon(U,0)\rightarrow(\mathbf{\mathbb{C}},0),\quad z\mapsto f(z)=\sum_{\alpha}c_{\alpha}z^{\alpha},

be an analytic function, where α:=(α1,,αn)+n\alpha:=(\alpha_{1},\ldots,\alpha_{n})\in\mathbb{Z}_{+}^{n}, cαc_{\alpha}\in\mathbb{C}, and zαz^{\alpha} is a notation for the monomial z1α1znαnz_{1}^{\alpha_{1}}\cdots z_{n}^{\alpha_{n}}.

3.1. Newton diagram

Here, the reference is Kouchnirenko [7]. The Newton polyhedron Γ+(f)\Gamma_{\!+}(f) of ff (at the origin and with respect to the coordinates z=(z1,,zn)z=(z_{1},\ldots,z_{n})) is the convex hull in +n\mathbb{R}_{+}^{n} of the set

cα0(α++n).\bigcup_{c_{\alpha}\not=0}(\alpha+\mathbb{R}_{+}^{n}).

For any v+n{0}v\in\mathbb{R}_{+}^{n}\setminus\{0\}, put

(v,Γ+(f)):=min{v,α;αΓ+(f)},\displaystyle\ell(v,\Gamma_{\!+}(f))=\min\{\langle v,\alpha\rangle\,;\,\alpha\in\Gamma_{\!+}(f)\},
Δ(v,Γ+(f)):={αΓ+(f);v,α=(v,Γ+(f))},\displaystyle\Delta(v,\Gamma_{\!+}(f))=\{\alpha\in\Gamma_{\!+}(f)\,;\,\langle v,\alpha\rangle=\ell(v,\Gamma_{\!+}(f))\},

where ,\langle\cdot\,,\cdot\rangle denotes the standard inner product in n\mathbb{R}^{n}. A subset ΔΓ+(f)\Delta\subseteq\Gamma_{\!+}(f) is called a face of Γ+(f)\Gamma_{\!+}(f) if there exists v+n{0}v\in\mathbb{R}_{+}^{n}\setminus\{0\} such that Δ=Δ(v,Γ+(f))\Delta=\Delta(v,\Gamma_{\!+}(f)). The dimension of a face Δ\Delta of Γ+(f)\Gamma_{\!+}(f) is the minimum of the dimensions of the affine subspaces of n\mathbb{R}^{n} containing Δ\Delta. The Newton diagram (also called Newton boundary) of ff is the union of the compact faces of Γ+(f)\Gamma_{\!+}(f). It is denoted by Γ(f)\Gamma(f). We say that ff is convenient if the intersection of Γ(f)\Gamma(f) with each coordinate axis of +n\mathbb{R}^{n}_{+} is non-empty (i.e., for any 1in1\leq i\leq n, the monomial ziαiz_{i}^{\alpha_{i}}, αi1\alpha_{i}\geq 1, appears in the expression αcαzα\sum_{\alpha}c_{\alpha}z^{\alpha} with a non-zero coefficient).

For any face ΔΓ(f)\Delta\subseteq\Gamma(f), define the face function fΔf_{\Delta} by

fΔ(z):=αΔcαzα.f_{\Delta}(z):=\sum_{\alpha\in\Delta}c_{\alpha}z^{\alpha}.

We say that ff is Newton non-degenerate (in short, non-degenerate) on the face Δ\Delta if the equations

fΔz1(z)==fΔzn(z)=0\frac{\partial f_{\Delta}}{\partial z_{1}}(z)=\cdots=\frac{\partial f_{\Delta}}{\partial z_{n}}(z)=0

have no common solution on ({0})n(\mathbf{\mathbb{C}}\setminus\{0\})^{n}. We say that ff is (Newton) non-degenerate if it is non-degenerate on every face Δ\Delta of Γ(f)\Gamma(f).

3.2. A bound for non-degeneracy of certain functions

Another important ingredient in the proof of our main theorem is Lemma 3.7 of [1]. This lemma asserts that if ff is a non-degenerate function with a singularity at 0, then there exists a constant m(f)m(f) such that for any αi>m(f)\alpha_{i}>m(f), the function f+ziαif+z_{i}^{\alpha_{i}} is non-degenerate too. Such a (non unique) number m(f)m(f) is defined as follows. For each face ΔΓ(f)\Delta\subseteq\Gamma(f) with maximal dimension (i.e., Δ\Delta is not contained in any other face), choose a vector vΔ+n{0}v_{\Delta}\in\mathbb{R}_{+}^{n}\setminus\{0\} such that Δ={αΓ+(f);vΔ,α=(vΔ,Γ+(f))}\Delta=\{\alpha\in\Gamma_{\!+}(f)\,;\,\langle v_{\Delta},\alpha\rangle=\ell(v_{\Delta},\Gamma_{\!+}(f))\}, and define

W:=ΔΓ(f)max dim{α+n;vΔ,α(vΔ,Γ+(f))},W:=\bigcup_{{\Delta\subseteq\Gamma(f)}\atop{\mbox{\tiny max dim}}}\{\alpha\in\mathbb{R}_{+}^{n}\,;\,\langle v_{\Delta},\alpha\rangle\leq\ell(v_{\Delta},\Gamma_{\!+}(f))\},

where the union is taken over all maximal dimensional faces ΔΓ(f)\Delta\subseteq\Gamma(f). Clearly, WW is a compact set and it intersects each coordinate axis of +n\mathbb{R}_{+}^{n} in a closed interval, say [0,wi][0,w_{i}] for some wiw_{i}. Then define

m(f):=max1inwi.m(f):=\max_{1\leq i\leq n}w_{i}.

Of course, m(f)m(f) depends on the choice of the vectors vΔv_{\Delta}. It is possible to define a “smallest” number m0(f)m_{0}(f) that also guarantees the non-degeneracy of the functions f+ziαif+z_{i}^{\alpha_{i}} with αi>m0(f)\alpha_{i}>m_{0}(f) (see [6, Section 2]). However, for our purpose, we shall not need it.

3.3. Newton number

Again, the reference for this section is [7]. Throughout the paper, for any subsets I{1,,n}I\subseteq\{1,\ldots,n\} and X+nX\subseteq\mathbb{R}^{n}_{+}, we shall use the following notation:

XI:={(x1,,xn)X;xi=0 if iI}.X^{I}:=\{(x_{1},\ldots,x_{n})\in X\,;\,x_{i}=0\text{ if }i\not\in I\}.

In particular, for any i{1,,n}i\in\{1,\ldots,n\}, the set X{i}X^{\{i\}} is nothing but the intersection of XX with the iith coordinate axis of +n\mathbb{R}^{n}_{+}.

Let Γ(f)\Gamma_{\!-}(f) denote the cone over Γ(f)\Gamma(f) with the origin as vertex. If ff is convenient, then the Newton number ν(f)\nu(f) of ff is defined by

(3.1) ν(f):=I{1,,n}(1)n|I||I|!Vol|I|(Γ(f)I),\nu(f):=\sum_{I\subseteq\{1,\ldots,n\}}(-1)^{n-|I|}|I|!\operatorname{Vol}_{|I|}(\Gamma_{\!-}(f)^{I}),

where |I||I| is the cardinality of II and Vol|I|(Γ(f)I)\operatorname{Vol}_{|I|}(\Gamma_{\!-}(f)^{I}) is the |I||I|-dimensional Euclidean volume of Γ(f)I\Gamma_{\!-}(f)^{I}. For I=I=\emptyset, the subset Γ(f)\Gamma_{\!-}(f)^{\emptyset} reduces to {0}\{0\}, and we set Vol0(Γ(f))=1\operatorname{Vol}_{0}(\Gamma_{\!-}(f)^{\emptyset})=1.

The Newton number can also be defined even if ff is not convenient. More precisely, if II is the non-empty subset of {1,,n}\{1,\ldots,n\} such that Γ(f)\Gamma(f) meets the iith coordinate axis of +n\mathbb{R}^{n}_{+} if and only if iIi\notin I, then the Newton number ν(f)\nu(f) of ff is defined as

ν(f):=supm+ν(f+iIzim),\nu(f):=\sup_{m\in\mathbb{Z}_{+}}\nu\bigg{(}f+\sum_{i\in I}z_{i}^{m}\bigg{)},

where of course the Newton number of the (convenient) function f+iIzimf+\sum_{i\in I}z_{i}^{m} is given by (3.1).

3.4. Modified Newton numbers

Following Kouchnirenko’s definition of the Newton number, we now introduce our modified Newton numbers.

Let II be a non-empty subset of {1,,n}\{1,\ldots,n\} such that Γ(f)I\Gamma(f)^{I}\not=\emptyset. By [3, Theorem 1], choose a simplicial decomposition of Γ(f)I\Gamma(f)^{I} in which the vertices of a simplex are 0-dimensional faces of Γ(f)I\Gamma(f)^{I} (such a decomposition is not unique). The cones spanned by the origin 0n0\in\mathbb{R}^{n} and such simplexes give a simplicial decomposition

ΞI:={SI,r}1rrI\Xi_{I}:=\{S_{I,r}\}_{1\leq r\leq r_{I}}

of Γ(f)I\Gamma_{\!-}(f)^{I}. Note that

(3.2) Vol|I|(Γ(f)I)=SI,rΞI,dimSI,r=|I|Vol|I|(SI,r).\operatorname{Vol}_{|I|}(\Gamma_{\!-}(f)^{I})=\sum_{S_{I,r}\in\Xi_{I},\,\dim S_{I,r}=|I|}\operatorname{Vol}_{|I|}(S_{I,r}).

Clearly, each simplex SI,r(+n)IS_{I,r}\subseteq(\mathbb{R}^{n}_{+})^{I} may be identified to a simplex (still denoted by SI,rS_{I,r}) of |I|\mathbb{R}^{|I|}, and with such an identification, the volume Vol|I|(SI,r)\operatorname{Vol}_{|I|}(S_{I,r}) of a simplex SI,rS_{I,r} with maximal dimension (i.e., with dimension |I||I|) is given by

(3.3) Vol|I|(SI,r)=±1|I|!det(0SI,r;1SI,r;|I|111),\operatorname{Vol}_{|I|}(S_{I,r})=\pm\frac{1}{|I|!}\det\left(\begin{matrix}0&S_{I,r;1}&\cdots&S_{I,r;|I|}\\ 1&1&\cdots&1\end{matrix}\right),

where 0,SI,r;1,,SI,r;|I|0,S_{I,r;1},\ldots,S_{I,r;|I|} are the column vectors representing the coordinates of the vertices of the simplex SI,r|I|S_{I,r}\subseteq\mathbb{R}^{|I|}. Note that each such column vector has |I||I| components, so that the matrix in (3.3) has dimension (|I|+1)×(|I|+1)(|I|+1)\times(|I|+1).

Let JJ be another subset of {1,,n}\{1,\ldots,n\}. We suppose that for any iJi\in J the Newton boundary Γ(f)\Gamma(f) meets the iith coordinate axis of +n\mathbb{R}^{n}_{+}. Then to each i0{1,,n}i_{0}\in\{1,\ldots,n\}, we associate a subset ΞI,J,i0\Xi_{I,J,i_{0}} of ΞI\Xi_{I} (depending on II, JJ and i0i_{0}) as follows. If i0IJi_{0}\in I\cap J, then we define ΞI,J,i0\Xi_{I,J,i_{0}} as the set of all simplexes SI,rΞIS_{I,r}\in\Xi_{I} (as simplexes in (+n)I(\mathbb{R}^{n}_{+})^{I}) with maximal dimension |I||I| such that for any iJi\in J the following property holds true:

SI,r{i}=SI,rΓ(f){i} is an edge of SI,ri=i0.S_{I,r}^{\{i\}}=S_{I,r}\cap\Gamma_{\!-}(f)^{\{i\}}\mbox{ is an edge of }S_{I,r}\Leftrightarrow i=i_{0}.

(As usual, by an “edge” of a simplex we mean a 11-dimensional face.) If i0Ji_{0}\notin J (in particular if J=J=\emptyset) or if i0Ii_{0}\notin I, then we set ΞI,J,i0:=\Xi_{I,J,i_{0}}:=\emptyset.

By definition, if SI,rS_{I,r} is a simplex of ΞI,J,i0\Xi_{I,J,i_{0}}, then it has maximal dimension and possesses a vertex with coordinates of the form (0,,0,αi0,0,,0)n(0,\ldots,0,\alpha_{i_{0}},0,\ldots,0)\in\mathbb{R}^{n} (for some αi0\alpha_{i_{0}} located at the i0i_{0}th place). To each such a simplex SI,rΞI,J,i0S_{I,r}\in\Xi_{I,J,i_{0}}, we associate a (unique) “reduced” simplex S~I,r\widetilde{S}_{I,r} defined by the same vertices as those of SI,rS_{I,r} with the exception of the vertex (0,,0,αi0,0,,0)(0,\ldots,0,\alpha_{i_{0}},0,\ldots,0) which we replace by (0,,0,1,0,,0)(0,\ldots,0,1,0,\ldots,0). We denote by Ξ~I,J,i0\widetilde{\Xi}_{I,J,i_{0}} the set of such reduced simplexes.

By convention, for the next definition and all the statements hereafter, we agree that if II is a non-empty subset of {1,,n}\{1,\ldots,n\} such that Γ(f)I\Gamma(f)^{I} is empty, then the corresponding “simplicial decomposition” ΞI\Xi_{I} is the empty set.

Definition 3.1.

For each JJ, i0i_{0}, and each collection Ξ:={ΞI}I{1,,n},I\Xi:=\{\Xi_{I}\}_{I\subseteq\{1,\ldots,n\},\,I\not=\emptyset} as above, we define a modified Newton number ν~Ξ,J,i0(f)\widetilde{\nu}_{\Xi,J,i_{0}}(f) for the function ff by

ν~Ξ,J,i0(f):=I{1,,n},Ii0(S~I,rΞ~I,J,i0(1)n|I||I|!Vol|I|(S~I,r)).\widetilde{\nu}_{\Xi,J,i_{0}}(f):=\sum_{I\subseteq\{1,\ldots,n\},\,I\ni i_{0}}\Bigg{(}\sum_{\widetilde{S}_{I,r}\in\widetilde{\Xi}_{I,J,i_{0}}}(-1)^{n-|I|}|I|!\operatorname{Vol}_{|I|}(\widetilde{S}_{I,r})\Bigg{)}.

(If ΞI=\Xi_{I}=\emptyset or if i0Ji_{0}\notin J, then ΞI,J,i0=Ξ~I,J,i0=\Xi_{I,J,i_{0}}=\widetilde{\Xi}_{I,J,i_{0}}=\emptyset, and the corresponding term in the above sum is zero by convention.)

Similarly, we introduce the subset ΞI,J,0\Xi_{I,J,0} of ΞI\Xi_{I} consisting of those simplexes SI,rΞIS_{I,r}\in\Xi_{I} with maximal dimension and such that for any iJi\in J the intersection SI,r{i}=SI,rΓ(f){i}S_{I,r}^{\{i\}}=S_{I,r}\cap\Gamma_{\!-}(f)^{\{i\}} is not an edge of SI,rS_{I,r}.

Definition 3.2.

For each JJ and each Ξ:={ΞI}I{1,,n},I\Xi:=\{\Xi_{I}\}_{I\subseteq\{1,\ldots,n\},\,I\not=\emptyset} as above, we define a special modified Newton number νΞ,J,0(f){\nu}_{\Xi,J,0}(f) for the function ff by

νΞ,J,0(f):=I{1,,n},I(SI,rΞI,J,0(1)n|I||I|!Vol|I|(SI,r)).{\nu}_{\Xi,J,0}(f):=\sum_{I\subseteq\{1,\ldots,n\},\,I\not=\emptyset}\Bigg{(}\sum_{{S}_{I,r}\in{\Xi}_{I,J,0}}(-1)^{n-|I|}|I|!\operatorname{Vol}_{|I|}({S}_{I,r})\Bigg{)}.

Let us emphasize the fact that the simplexes involved in the definition of the modified Newton number ν~Ξ,J,i0(f)\widetilde{\nu}_{\Xi,J,i_{0}}(f) are reduced simplexes, while those used to define the special modified Newton number νΞ,J,0(f){\nu}_{\Xi,J,0}(f) are not reduced.

4. Formulas for the Lê numbers of a non-degenerate function

Let z:=(z1,,zn)z:=(z_{1},\ldots,z_{n}) be a system of linear coordinates for n\mathbf{\mathbb{C}}^{n}, let UU be an open neighbourhood of the origin in n\mathbf{\mathbb{C}}^{n}, and let f:(U,0)(,0)f\colon(U,0)\rightarrow(\mathbf{\mathbb{C}},0) be a non-degenerate analytic function. We denote by Σf\Sigma f the critical locus of ff, and we suppose that d:=dim0Σf1d:=\dim_{0}\Sigma f\geq 1. We also assume that the Lê numbers

λf,z0(0),,λf,zd(0)\lambda^{0}_{f,z}(0),\ldots,\lambda^{d}_{f,z}(0)

of ff at 0 with respect to the coordinates z=(z1,,zn)z=(z_{1},\ldots,z_{n}) are defined. For example, if the coordinates are “prepolar” for ff (see [12, Definition 1.26]), then the corresponding Lê numbers do exist. In particular, this is the case if ff has an “aligned” singularity at 0 (e.g., a line singularity) and the coordinates are “aligning” for ff at 0 (see [12, Definition 7.1]).

For any 1qd1\leq q\leq d, we consider the function

(4.1) fq(z):=f(z)+z1α1++zqαq,f_{q}(z):=f(z)+z_{1}^{\alpha_{1}}+\dots+z_{q}^{\alpha_{q}},

where α1,,αq{\alpha_{1}},\ldots,{\alpha_{q}} are integers such that, for any 1pq1\leq p\leq q,

αp>max{2,ρfp1,z(p1)(0),m(fp1)}.\alpha_{p}>\max\{2,\rho_{f_{p-1},z^{(p-1)}}(0),m(f_{p-1})\}.

Here, ρfp1,z(p1)(0)\rho_{f_{p-1},z^{(p-1)}}(0) is the maximum polar ratio for fp1f_{p-1} at 0 with respect to the rotated coordinates

z(p1):=(zp,,zn,z1,,zp1),z^{(p-1)}:=(z_{p},\ldots,z_{n},z_{1},\ldots,z_{p-1}),

and m(fp1)m(f_{p-1}) is a bound which guarantees the non-degeneracy of the function fpf_{p} (see Sections 2.3 and 3.2). (By f0f_{0} and z(0)z^{(0)} we mean ff and zz respectively.) For example, if ff is a homogeneous polynomial such that d:=dim0Σf=1d:=\dim_{0}\Sigma f=1, then we can take fd(z)=f1(z):=f(z)+z1α1f_{d}(z)=f_{1}(z):=f(z)+z_{1}^{\alpha_{1}}, where α1>max{2,deg(f)}\alpha_{1}>\mbox{max}\{2,\deg(f)\}.

Hereafter, we are mainly interested in the modified Newton numbers of the function fdf_{d}. For each non-empty subset I{1,,n}I\subseteq\{1,\ldots,n\}, we choose a simplicial decomposition

ΞI:={SI,r}1rrI\Xi_{I}:=\{S_{I,r}\}_{1\leq r\leq r_{I}}

of Γ(fd)I\Gamma_{\!-}(f_{d})^{I} as in Section 3.4 (again, if Γ(fd)I=\Gamma(f_{d})^{I}=\emptyset, then ΞI=\Xi_{I}=\emptyset), and we write Ξ:={ΞI}I{1,,n},I\Xi:=\{\Xi_{I}\}_{I\subseteq\{1,\ldots,n\},\,I\not=\emptyset}. Since throughout this section we shall only consider modified Newton numbers of the form

νΞ,{1,,d},0(fd)andν~Ξ,{1,,d},k(fd){\nu}_{\Xi,\{1,\ldots,d\},0}(f_{d})\quad\mbox{and}\quad\widetilde{\nu}_{\Xi,\{1,\ldots,d\},k}(f_{d})

(1kd1\leq k\leq d) where dd is the dimension at 0 of the critical locus Σf\Sigma f, we may simplify the notation as follows:

νΞ,0(fd):=νΞ,{1,,d},0(fd)andν~Ξ,k(fd):=ν~Ξ,{1,,d},k(fd).{\nu}_{\Xi,0}(f_{d}):={\nu}_{\Xi,\{1,\ldots,d\},0}(f_{d})\quad\mbox{and}\quad\widetilde{\nu}_{\Xi,k}(f_{d}):=\widetilde{\nu}_{\Xi,\{1,\ldots,d\},k}(f_{d}).

Here is our main result.

Theorem 4.1.

Suppose that ff is non-degenerate, d:=dim0Σf1d:=\dim_{0}\Sigma f\geq 1 and the Lê numbers λf,zk(0)\lambda^{k}_{f,z}(0) of ff at 0 with respect to the coordinates z=(z1,,zn)z=(z_{1},\ldots,z_{n}) are defined for any 0kd0\leq k\leq d. Then the following two assertions hold true.

  1. (1)

    The modified Newton numbers νΞ,0(fd){\nu}_{\Xi,0}(f_{d}) and ν~Ξ,k(fd)\widetilde{\nu}_{\Xi,k}(f_{d}) of the function fdf_{d} do not depend on the choice of Ξ:={ΞI}I{1,,n},I\Xi:=\{\Xi_{I}\}_{I\subseteq\{1,\ldots,n\},\,I\not=\emptyset}. Therefore, we may further simplify the notation as follows:

    ν0(fd):=νΞ,0(fd)andν~k(fd):=ν~Ξ,k(fd).{\nu}_{0}(f_{d}):={\nu}_{\Xi,0}(f_{d})\quad\mbox{and}\quad\widetilde{\nu}_{k}(f_{d}):=\widetilde{\nu}_{\Xi,k}(f_{d}).
  2. (2)

    The Lê numbers λf,z0(0),,λf,zd(0)\lambda^{0}_{f,z}(0),\ldots,\lambda^{d}_{f,z}(0) are given by the following formulas:

    1. \cdot

      λf,z0(0)=(1)n+ν0(fd)+ν~1(fd)\lambda^{0}_{f,z}(0)=(-1)^{n}+\nu_{0}(f_{d})+\widetilde{\nu}_{1}(f_{d});

    2. \cdot

      λf,zk(0)=(1)k1(ν~k(fd)ν~k+1(fd))\lambda^{k}_{f,z}(0)=(-1)^{k-1}(\widetilde{\nu}_{k}(f_{d})-\widetilde{\nu}_{k+1}(f_{d})) for 1kd11\leq k\leq d-1 (if d2d\geq\penalty 100002);

    3. \cdot

      λf,zd(0)=(1)d1ν~d(fd)\lambda^{d}_{f,z}(0)=(-1)^{d-1}\widetilde{\nu}_{d}(f_{d}).

Theorem 4.1 is a version for non-isolated singularities of the Kouchnirenko theorem mentioned in the introduction. It will be proved in Section 7. The formulas given in item (2) reduce the calculation of the Lê numbers of a non-degenerate function to a simple computation of volumes of simplexes. Certainly, these formulas are well suited for computer algebra programs.

5. Corollaries

Let z=(z1,,zn)z=(z_{1},\ldots,z_{n}) be linear coordinates for n\mathbb{C}^{n}. The first important corollary of Theorem 4.1 is the invariance of the Lê numbers within the class of non-degenerate functions with fixed Newton diagram. More precisely we have the following statement.

Corollary 5.1.

Let f,g:(U,0)(,0)f,g\colon(U,0)\rightarrow(\mathbf{\mathbb{C}},0) be two non-degenerate analytic functions, where UU is an open neighbourhood of the origin of n\mathbb{C}^{n}. Suppose that the dimensions at 0 of the critical loci Σf\Sigma f and Σg\Sigma g of ff and gg, respectively, are greater than or equal to 11. If furthermore Γ(f)=Γ(g)\Gamma(f)=\Gamma(g) and the Lê numbers of ff and gg at 0 with respect to the coordinates z=(z1,,zn)z=(z_{1},\ldots,z_{n}) exist, then dim0Σf=dim0Σg\dim_{0}\Sigma f=\dim_{0}\Sigma g, and for any 0kn10\leq k\leq n-1, we have

λf,zk(0)=λg,zk(0).\lambda^{k}_{f,z}(0)=\lambda^{k}_{g,z}(0).

Corollary 5.1 will be proved in Section 8. In particular, it implies that any 11-parameter deformation family of non-degenerate functions with constant Newton diagram has constant Lê numbers, provided that these numbers exist. Here is a more precise statement.

Corollary 5.2.

Let {ft}\{f_{t}\} be a 11-parameter deformation family of analytic functions ftf_{t} defined in an open neighbourhood of 0n0\in\mathbb{C}^{n} and depending analytically on the parameter tt\in\mathbb{C}. If for any sufficiently small tt (say |t|ε|t|\leq\varepsilon for some ε>0\varepsilon>0), the function ftf_{t} is non-degenerate, Γ(ft)=Γ(f0)\Gamma(f_{t})=\Gamma(f_{0}) and all the Lê numbers λft,zk(0)\lambda_{f_{t},z}^{k}(0) are defined, then dim0Σft=dim0Σf0\dim_{0}\Sigma f_{t}=\dim_{0}\Sigma f_{0} and λft,zk(0)=λf0,zk(0)\lambda^{k}_{f_{t},z}(0)=\lambda^{k}_{f_{0},z}(0) for all small tt.

By combining Corollary 5.2 with [12, Theorem 9.4] and [5, Theorem 42], we obtain a new proof of the following result, which is a special case of a much more general theorem of J. Damon [2].

Corollary 5.3 (Damon).

Let {ft}\{f_{t}\} be a family as in Corollary 5.2, that is, such that for any sufficiently small tt, the function ftf_{t} is non-degenerate, Γ(ft)=Γ(f0)\Gamma(f_{t})=\Gamma(f_{0}) and all the Lê numbers λft,zk(0)\lambda_{f_{t},z}^{k}(0) are defined. Under these assumptions, the following two assertions hold true.

  1. (1)

    If for all small tt, the coordinates z=(z1,,zn)z=(z_{1},\ldots,z_{n}) are prepolar for ftf_{t} and dim0Σftn4\dim_{0}\Sigma f_{t}\leq n-4, then the diffeomorphism type of the Milnor fibration of ftf_{t} at 0 is independent of tt for all small tt.

  2. (2)

    If n5n\geq 5 and dim0Σft=1\dim_{0}\Sigma f_{t}=1 for all small tt, then the family {ft}\{f_{t}\} is topologically trivial.

Indeed, by Corollary 5.2, the family {ft}\{f_{t}\} has constant Lê numbers with respect to the coordinates z=(z1,,zn)z=(z_{1},\ldots,z_{n}). Item (1) then follows from [12, Theorem 9.4] while item (2) is a consequence of [5, Theorem 42].

In fact, in [2], Damon obtains the topological triviality without the restrictions n5n\geq 5 or dim0Σft=1\dim_{0}\Sigma f_{t}=1. A third proof (based on so-called “uniform stable radius”) of item (2) for line singularities is also given in [4].

Finally, combined with [12, Theorem 3.3], Theorem 4.1 has the following corollary about the Euler characteristic of the Milnor fibre associated to a non-degenerate function.

Corollary 5.4.

Again, assume that ff is non-degenerate, d:=dim0Σf1d:=\dim_{0}\Sigma f\geq 1 and the Lê numbers λf,zk(0)\lambda^{k}_{f,z}(0) of ff at 0 with respect to the coordinates z=(z1,,zn)z=(z_{1},\ldots,z_{n}) are defined for any 0kd0\leq k\leq d. If furthermore the coordinates z=(z1,,zn)z=(z_{1},\ldots,z_{n}) are prepolar for ff, then the reduced Euler characteristic χ~(Ff,0)\widetilde{\chi}(F_{f,0}) of the Milnor fibre Ff,0F_{f,0} of ff at 0 is given by

χ~(Ff,0)=(1)n1(ν0(fd)+(1)n),\widetilde{\chi}(F_{f,0})=(-1)^{n-1}(\nu_{0}(f_{d})+(-1)^{n}),

where fdf_{d} is defined by (4.1).

Indeed, by [12, Theorem 3.3], we have

χ~(Ff,0)=k=0d(1)n1kλf,zk(0).\widetilde{\chi}(F_{f,0})=\sum_{k=0}^{d}(-1)^{n-1-k}\lambda^{k}_{f,z}(0).

Thus, to get the formula in Corollary 5.4, it suffices to replace λf,zk(0)\lambda^{k}_{f,z}(0) by its expression in terms of the modified Newton numbers given in Theorem 4.1.

6. Example

Consider the homogeneous polynomial function

f(z1,z2,z3):=z12z22+z24+z34.f(z_{1},z_{2},z_{3}):=z_{1}^{2}z_{2}^{2}+z_{2}^{4}+z_{3}^{4}.

The Newton diagram Γ(f)\Gamma(f) of ff is nothing but the triangle in +3\mathbb{R}^{3}_{+} (with coordinates (x1,x2,x3)(x_{1},x_{2},x_{3})) defined by the vertices A=(2,2,0)A=(2,2,0), B=(0,4,0)B=(0,4,0) and C=(0,0,4)C=(0,0,4) (see Figure 1). We easily check that ff is non-degenerate. The critical locus Σf\Sigma f of ff is given by the z1z_{1}-axis, and the restriction of ff to the hyperplane V(z1)V(z_{1}) defined by z1=0z_{1}=0 has an isolated singularity at 0. In other words, ff has a line singularity at 0 in the sense of [9, §4]. Then, by [12, Remark 1.29], the partition of V(f):=f1(0)V(f):=f^{-1}(0) given by

𝒮:={V(f)Σf,Σf{0},{0}}\mathscr{S}:=\{V(f)\setminus\Sigma f,\Sigma f\setminus\{0\},\{0\}\}

is a “good stratification” for ff in a neighbourhood of 0, and the hyperplane V(z1)V(z_{1}) is a “prepolar slice” for ff at 0 with respect to 𝒮\mathscr{S} (see [12, Definitions 1.24 and 1.26]). In other words, the coordinates z=(z1,z2,z3)z=(z_{1},z_{2},z_{3}) are prepolar for ff. In particular, combined with [12, Proposition 1.23], this implies that the Lê numbers λf,z0(0)\lambda^{0}_{f,z}(0) and λf,z1(0)\lambda^{1}_{f,z}(0) are defined. We can compute these numbers either using the definition or by applying Theorem 4.1.

Refer to caption
Figure 1. Newton diagrams of ff and f1f_{1}

6.1. Calculation using the definition

We need to compute the polar varieties Γf,z2\Gamma^{2}_{f,z} and Γf,z1\Gamma^{1}_{f,z} and the Lê cycles [Λf,z1][\Lambda^{1}_{f,z}] and [Λf,z0][\Lambda^{0}_{f,z}]. By definition,

Γf,z2=V(fz3)¬V(z2,z3)=V(z33)¬V(z2,z3)=V(z33),\displaystyle\qquad\Gamma^{2}_{f,z}=V\bigg{(}\frac{\partial f}{\partial z_{3}}\bigg{)}\lnot V(z_{2},z_{3})=V(z_{3}^{3})\lnot V(z_{2},z_{3})=V(z_{3}^{3}),

while

Γf,z1\displaystyle\qquad\Gamma^{1}_{f,z} =V(fz2,fz3)¬V(z2,z3)\displaystyle=V\bigg{(}\frac{\partial f}{\partial z_{2}},\frac{\partial f}{\partial z_{3}}\bigg{)}\lnot V(z_{2},z_{3})
=V(z2(2z12+4z22),z33)¬V(z2,z3)=V(2z12+4z22,z33).\displaystyle=V(z_{2}(2z_{1}^{2}+4z_{2}^{2}),z_{3}^{3})\lnot V(z_{2},z_{3})=V(2z_{1}^{2}+4z_{2}^{2},z_{3}^{3}).

It follows that the Lê cycles are given by

[Λf,z1]\displaystyle\qquad[\Lambda^{1}_{f,z}] =[Γf,z2V(fz2)][Γf,z1]\displaystyle=\bigg{[}\Gamma^{2}_{f,z}\cap V\bigg{(}\frac{\partial f}{\partial z_{2}}\bigg{)}\bigg{]}-\bigg{[}\Gamma^{1}_{f,z}\bigg{]}
=[V(z33)V(z2(2z12+4z22))][V(2z12+4z22,z33)]\displaystyle=[V(z_{3}^{3})\cap V(z_{2}(2z_{1}^{2}+4z_{2}^{2}))]-[V(2z_{1}^{2}+4z_{2}^{2},z_{3}^{3})]
=[V(z2,z33)]\displaystyle=[V(z_{2},z_{3}^{3})]

and

[Λf,z0]\displaystyle\qquad[\Lambda^{0}_{f,z}] =[Γf,z1V(fz1)]\displaystyle=\bigg{[}\Gamma^{1}_{f,z}\cap V\bigg{(}\frac{\partial f}{\partial z_{1}}\bigg{)}\bigg{]}
=[V(2z12+4z22,z33)V(z1z22)]\displaystyle=[V(2z_{1}^{2}+4z_{2}^{2},z_{3}^{3})\cap V(z_{1}z_{2}^{2})]
=[V(z1,z22,z33)]+[V(z12,z22,z33)].\displaystyle=[V(z_{1},z_{2}^{2},z_{3}^{3})]+[V(z_{1}^{2},z_{2}^{2},z_{3}^{3})].

Finally the Lê numbers are given by

λf,z1\displaystyle\qquad\lambda^{1}_{f,z} =([Λf,z1][V(z1)])0=[V(z1,z2,z33)]0=3;\displaystyle=([\Lambda^{1}_{f,z}]\cdot[V(z_{1})])_{0}=[V(z_{1},z_{2},z_{3}^{3})]_{0}=3;
λf,z0\displaystyle\qquad\lambda^{0}_{f,z} =([Λf,z0]3)0=6+12=18.\displaystyle=([\Lambda^{0}_{f,z}]\cdot\mathbb{C}^{3})_{0}=6+12=18.

6.2. Calculation using Theorem 4.1

Consider a polynomial function

f1(z1,z2,z3):=f(z1,z2,z3)+z1α1f_{1}(z_{1},z_{2},z_{3}):=f(z_{1},z_{2},z_{3})+z_{1}^{\alpha_{1}}

such that α1>max{2,ρf,z(0),m(f)}\alpha_{1}>\max\{2,\rho_{f,z}(0),m(f)\}. Since ff is a homogeneous polynomial of degree 44, the maximum polar ratio ρf,z(0)\rho_{f,z}(0) for ff at 0 with respect to the coordinates zz is 44 (see Section 2.3), and clearly, we can take m(f)=4m(f)=4. So, let us take for instance α1=5\alpha_{1}=5. Clearly, Γ(f1)\Gamma_{\!-}(f_{1}) is the union of two tetrahedra {O,A,C,E}\{O,A,C,E\} and {O,A,B,C}\{O,A,B,C\}. For each subset I{1,2,3}I\subseteq\{1,2,3\}, take the “natural” simplicial decomposition ΞI\Xi_{I} of Γ(f1)I\Gamma_{\!-}(f_{1})^{I} generated by the vertices of the set {O,A,B,C,E}(+n)I\{O,A,B,C,E\}\cap(\mathbb{R}^{n}_{+})^{I} as suggested in Figure 1 (at this level, we ignore the point DD mentioned in the figure). For example, Ξ{1,2}\Xi_{\{1,2\}} is defined by the simplexes {O,A,E}\{O,A,E\} and {O,A,B}\{O,A,B\}. By Theorem 4.1,

λf,z0(0)=(1)3+ν0(f1)+ν~1(f1)andλf,z1(0)=(1)0ν~1(f1).\lambda^{0}_{f,z}(0)=(-1)^{3}+\nu_{0}(f_{1})+\widetilde{\nu}_{1}(f_{1})\quad\mbox{and}\quad\lambda^{1}_{f,z}(0)=(-1)^{0}\widetilde{\nu}_{1}(f_{1}).

The data to compute the modified Newton numbers ν0(f1)\nu_{0}(f_{1}) and ν~1(f1)\widetilde{\nu}_{1}(f_{1}) are given in Table 1. In this table, O=(0,0,0)O=(0,0,0), D=(1,0,0)D=(1,0,0), and AA, BB, CC are as above. Each pair in the third and fourth columns of the table consists of a simplex together with its volume. For example, in the first row of the third column, the pair ({O,D};1)(\{O,D\};1) consists of the simplex {O,D}Ξ~{1},{1},1\{O,D\}\in\widetilde{\Xi}_{\{1\},\{1\},1} and its volume Vol1({O,D})=1\operatorname{Vol}_{1}(\{O,D\})=1. The calculation shows that ν0(f1)=16\nu_{0}(f_{1})=16 and ν~1(f1)=3\widetilde{\nu}_{1}(f_{1})=3, and therefore the Lê numbers are given by

λf,z0(0)=18andλf,z1(0)=3.\lambda^{0}_{f,z}(0)=18\quad\mbox{and}\quad\lambda^{1}_{f,z}(0)=3.

II (1)3|I||I|!(-1)^{3-|I|}|I|! (SΞ~I,{1},1;Vol|I|(S))(S\in\widetilde{\Xi}_{I,\{1\},1};\mbox{Vol}_{|I|}(S)) (SΞI,{1},0;Vol|I|(S))(S\in\Xi_{I,\{1\},0};\mbox{Vol}_{|I|}(S))
{1}\{1\} 11 ({O,D};1)(\{O,D\};1) (;0)(\emptyset;0)
{2}\{2\} 11 (;0)(\emptyset;0) ({O,B};4)(\{O,B\};4)
{3}\{3\} 11 (;0)(\emptyset;0) ({O,C};4)(\{O,C\};4)
{1,2}\{1,2\} 2-2 ({O,A,D};1)(\{O,A,D\};1) ({O,A,B};4)(\{O,A,B\};4)
{1,3}\{1,3\} 2-2 ({O,C,D};2)(\{O,C,D\};2) (;0)(\emptyset;0)
{2,3}\{2,3\} 2-2 (;0)(\emptyset;0) ({O,B,C};8)(\{O,B,C\};8)
{1,2,3}\{1,2,3\} 66 ({O,A,C,D};43)(\{O,A,C,D\};\frac{4}{3}) ({O,A,B,C};163)(\{O,A,B,C\};\frac{16}{3})
Table 1. Data to compute ν0(f1)\nu_{0}(f_{1}) and ν~1(f1)\widetilde{\nu}_{1}(f_{1})

6.3. Euler characteristic

Since the coordinates z=(z1,z2,z3)z=(z_{1},z_{2},z_{3}) are prepolar for ff, Corollary 5.4 says that to calculate the reduced Euler characteristic χ~(Ff,0)\widetilde{\chi}(F_{f,0}) of the Milnor fibre Ff,0F_{f,0} of ff at 0, it suffices to compute the special modified Newton number ν0(f1)\nu_{0}(f_{1}). Precisely, χ~(Ff,0)\widetilde{\chi}(F_{f,0}) is given by

χ~(Ff,0)=(1)2(ν0(f1)+(1)3)=15.\widetilde{\chi}(F_{f,0})=(-1)^{2}(\nu_{0}(f_{1})+(-1)^{3})=15.

7. Proof of Theorem 4.1

Applying the Iomdine-Lê-Massey formula (see [12, Theorem 4.5]) successively to f,f1,,fd1f,f_{1},\ldots,f_{d-1} shows that for any 0qd10\leq q\leq d-1:

  1. (1)

    Σfq+1=ΣfV(z1,,zq+1)\Sigma f_{q+1}=\Sigma f\cap V(z_{1},\ldots,z_{q+1}) in a neighbourhood of the origin;

  2. (2)

    dim0Σfq+1=d(q+1)\dim_{0}\Sigma f_{q+1}=d-(q+1);

  3. (3)

    the Lê numbers λfq+1,z(q+1)k(0)\lambda^{k}_{f_{q+1},z^{(q+1)}}(0) of fq+1f_{q+1} at 0 with respect to the rotated coordinates

    z(q+1)=(zq+2,,zn,z1,,zq+1)\displaystyle z^{(q+1)}=(z_{q+2},\ldots,z_{n},z_{1},\ldots,z_{q+1})

    exist for all 0kd(q+1)0\leq k\leq d-(q+1) and are given by

    {λfq+1,z(q+1)0(0)=λfq,z(q)0(0)+(αq+11)λfq,z(q)1(0);λfq+1,z(q+1)k(0)=(αq+11)λfq,z(q)k+1(0)for1kd(q+1);\displaystyle\begin{cases}\lambda^{0}_{f_{q+1},z^{(q+1)}}(0)=\lambda^{0}_{f_{q},z^{(q)}}(0)+(\alpha_{q+1}-1)\lambda^{1}_{f_{q},z^{(q)}}(0);\\ \lambda^{k}_{f_{q+1},z^{(q+1)}}(0)=(\alpha_{q+1}-1)\lambda^{k+1}_{f_{q},z^{(q)}}(0)\quad\mbox{for}\quad 1\leq k\leq d-(q+1);\end{cases}

where λfq,z(q)k(0)\lambda^{k}_{f_{q},z^{(q)}}(0) is the kkth Lê number of fqf_{q} at 0 with respect to the rotated coordinates

z(q)=(zq+1,,zn,z1,,zq),z^{(q)}=(z_{q+1},\ldots,z_{n},z_{1},\ldots,z_{q}),

and where αq+1\alpha_{q+1} is an integer satisfying

αq+1>max{2,ρfq,z(q)(0),m(fq)}.\alpha_{q+1}>\max\{2,\rho_{f_{q},z^{(q)}}(0),m(f_{q})\}.

In particular (see [12, Corollary 4.6]) fdf_{d} has an isolated singularity at 0 and its Milnor number μfd(0)\mu_{f_{d}}(0) (which, in this case, coincides with its 0th Lê number λfd,z(d)0(0)\lambda^{0}_{f_{d},z^{(d)}}(0)) is given by

(7.1) μfd(0)=λf,z0(0)+k=1d(q=1k(αq1))λf,zk(0).\mu_{f_{d}}(0)=\lambda^{0}_{f,z}(0)+\sum_{k=1}^{d}\left(\prod_{q=1}^{k}(\alpha_{q}-1)\right)\lambda^{k}_{f,z}(0).

Let {i1,,ip}\{i_{1},\ldots,i_{p}\} be the subset of {1,,n}{1,,d}\{1,\ldots,n\}\setminus\{1,\ldots,d\} consisting of all indices ii for which Γ(fd)\Gamma(f_{d}) does not meet the iith coordinate axis of +n\mathbb{R}^{n}_{+}. Then, by [1, Lemmas 3.6–3.8 and Corollary 3.11] and [7, Théorème I], for any 0α1αdαi1αip0\ll\alpha_{1}\ll\cdots\ll\alpha_{d}\ll\alpha_{i_{1}}\ll\cdots\ll\alpha_{i_{p}} sufficiently large, the function

fd(z)\displaystyle f^{\prime}_{d}(z) :=f(z)+z1α1++zdαdfd(z)+zi1αi1++zipαip\displaystyle:=\underbrace{f(z)+z_{1}^{\alpha_{1}}+\cdots+z_{d}^{\alpha_{d}}}_{f_{d}(z)}+z_{i_{1}}^{\alpha_{i_{1}}}+\cdots+z_{i_{p}}^{\alpha_{i_{p}}}

is non-degenerate, convenient, and the following equalities hold true:

(7.2) μfd(0)=μfd(0)=ν(fd)=ν(fd).\mu_{f_{d}}(0)=\mu_{f^{\prime}_{d}}(0)=\nu(f^{\prime}_{d})=\nu(f_{d}).

The expression (7.1) for the Milnor number μfd(0)\mu_{f_{d}}(0) can be viewed as a polynomial in the variables α1,,αd\alpha_{1},\ldots,\alpha_{d}. Its linear part is given by

(7.3) k=0d(1)kλf,zk(0)+i=1d(αik=id(1)k1λf,zk(0)).\sum_{k=0}^{d}(-1)^{k}\lambda^{k}_{f,z}(0)+\sum_{i=1}^{d}\bigg{(}\alpha_{i}\sum_{k=i}^{d}(-1)^{k-1}\lambda^{k}_{f,z}(0)\bigg{)}.

Now we need the following lemma.

Lemma 7.1.

The function ff has no term of the form c1z1a1,,cdzdadc_{1}z_{1}^{a_{1}},\ldots,c_{d}z_{d}^{a_{d}}, where ci{0}c_{i}\in\mathbb{C}\setminus\{0\}, ai>0a_{i}\in\mathbb{Z}_{>0}.

We postpone the proof of this lemma to the end of this section, and we first complete the proof of Theorem 4.1.

Since ff has no term of the form c1z1a1,,cdzdadc_{1}z_{1}^{a_{1}},\ldots,c_{d}z_{d}^{a_{d}}, the Newton number ν(fd)\nu(f^{\prime}_{d}) can be viewed as a polynomial in the variables α1,,αd\alpha_{1},\ldots,\alpha_{d} and αi1,,αip\alpha_{i_{1}},\ldots,\alpha_{i_{p}}. Its linear part with respect to α1,,αd\alpha_{1},\ldots,\alpha_{d} has the form

(7.4) P0(αi1,,αip)+α1P1(αi1,,αip)++αdPd(αi1,,αip),P_{0}(\alpha_{i_{1}},\ldots,\alpha_{i_{p}})+\alpha_{1}\,P_{1}(\alpha_{i_{1}},\ldots,\alpha_{i_{p}})+\cdots+\alpha_{d}\,P_{d}(\alpha_{i_{1}},\ldots,\alpha_{i_{p}}),

where Pi(αi1,,αip)P_{i}(\alpha_{i_{1}},\ldots,\alpha_{i_{p}}) are polynomials in αi1,,αip\alpha_{i_{1}},\ldots,\alpha_{i_{p}}. Taking the difference μfd(0)ν(fd)\mu_{f_{d}}(0)-\nu(f^{\prime}_{d}) gives a polynomial

Q(α1,,αd,αi1,,αip):=μfd(0)ν(fd)Q(\alpha_{1},\ldots,\alpha_{d},\alpha_{i_{1}},\ldots,\alpha_{i_{p}}):=\mu_{f_{d}}(0)-\nu(f^{\prime}_{d})

in the variables α1,,αd,αi1,,αip\alpha_{1},\ldots,\alpha_{d},\alpha_{i_{1}},\ldots,\alpha_{i_{p}}. Then it follows from (7.2) that for any 0α1αdαi1αip0\ll\alpha_{1}\ll\cdots\ll\alpha_{d}\ll\alpha_{i_{1}}\ll\cdots\ll\alpha_{i_{p}} sufficiently large (equivalently, for any (α1,,αd,αi1,,αip)(\alpha_{1},\ldots,\alpha_{d},\alpha_{i_{1}},\ldots,\alpha_{i_{p}}) in the set Z(d+p)Z(d+p) which appears in Lemma A.1 of the appendix, with the appropriate coefficients c1c_{1} and c(α1,,α1)c_{\ell}(\alpha_{1},\ldots,\alpha_{\ell-1}) for 2d+p2\leq\ell\leq d+p), we have

Q(α1,,αd,αi1,,αip)=0.Q(\alpha_{1},\ldots,\alpha_{d},\alpha_{i_{1}},\ldots,\alpha_{i_{p}})=0.

Thus applying Lemma A.1 shows that QQ identically vanishes. In particular, comparing the coefficients of the linear parts (7.3) and (7.4) of μfd(0)\mu_{f_{d}}(0) and ν(fd)\nu(f^{\prime}_{d}), respectively, shows that the polynomials Pi:=Pi(αi1,,αip)P_{i}:=P_{i}(\alpha_{i_{1}},\ldots,\alpha_{i_{p}}) are independent of αi1,,αip\alpha_{i_{1}},\ldots,\alpha_{i_{p}} (i.e., PiP_{i} is constant) and are given by

{P0=k=0d(1)kλf,zk(0);Pi=k=id(1)k1λf,zk(0)for1id.\left\{\begin{aligned} P_{0}&=\sum_{k=0}^{d}(-1)^{k}\lambda^{k}_{f,z}(0);\\ P_{i}&=\sum_{k=i}^{d}(-1)^{k-1}\lambda^{k}_{f,z}(0)\quad\mbox{for}\quad 1\leq i\leq d.\\ \end{aligned}\right.

Theorem 4.1 is now an immediate consequence of the following lemma.

Lemma 7.2.

For each non-empty subset I{1,,n}I\subseteq\{1,\ldots,n\}, choose a simplicial decomposition

ΞI:={SI,r}1rrI{\Xi}^{\prime}_{I}:=\{{S}^{\prime}_{I,r}\}_{1\leq r\leq r^{\prime}_{I}}

of Γ(fd)I\Gamma_{\!-}({f}^{\prime}_{d})^{I} as in Section 3.4 such that its restriction to Γ(fd)I\Gamma_{\!-}(f_{d})^{I} coincides with the simplicial decomposition ΞI\Xi_{I}. (We can always achieve this condition by taking αi1,,αip\alpha_{i_{1}},\ldots,\alpha_{i_{p}} sufficiently large.) Write Ξ:={ΞI}I{1,,n},I\Xi^{\prime}:=\{{\Xi}^{\prime}_{I}\}_{I\subseteq\{1,\ldots,n\},\,I\not=\emptyset} and set J:={1,,d,i1,,ip}J:=\{1,\ldots,d,i_{1},\ldots,i_{p}\}. Then the following equalities hold true:

{Pi0=ν~Ξ,J,i0(fd)=ν~i0(fd) for 1i0d;P0=νΞ,J,0(fd)+(1)n=ν0(fd)+(1)n.\left\{\begin{aligned} &P_{i_{0}}=\widetilde{\nu}_{\Xi^{\prime},J,i_{0}}(f^{\prime}_{d})=\widetilde{\nu}_{i_{0}}(f_{d})\mbox{ for }1\leq i_{0}\leq d;\\ &P_{0}=\nu_{\Xi^{\prime},J,0}(f^{\prime}_{d})+(-1)^{n}=\nu_{0}(f_{d})+(-1)^{n}.\\ \end{aligned}\right.

To complete the proof of Theorem 4.1, it remains to prove Lemmas 7.1 and 7.2. We start with the proof of Lemma 7.2.

Proof of Lemma 7.2.

By (3.1) and (3.2), the Newton number ν(fd)\nu(f^{\prime}_{d}) is (up to coefficients of the form (1)n|I||I|!(-1)^{n-|I|}\,|I|!) a sum of volumes of the form Vol|I|(SI,r)\operatorname{Vol}_{|I|}({S}^{\prime}_{I,r}), where I{1,,n}\emptyset\not=I\subseteq\{1,\ldots,n\} and SI,r{S}^{\prime}_{I,r} is a simplex of ΞI{\Xi}^{\prime}_{I} with maximal dimension |I||I|, plus the number

(1)n||||!Vol||(Γ(fd))=(1)n,(-1)^{n-|\emptyset|}|\emptyset|!\,\mbox{Vol}_{|\emptyset|}(\Gamma_{\!-}(f_{d}^{\prime})^{\emptyset})=(-1)^{n},

which corresponds to I=I=\emptyset in the definition of ν(fd)\nu(f^{\prime}_{d}) (see Section 3.3). If for any 1i0d1\leq i_{0}\leq d the matrix used to compute the volume Vol|I|(SI,r)\operatorname{Vol}_{|I|}({S}^{\prime}_{I,r}) (see (3.3)) does not have any column of the form

(β1βi01αi0βi0+1β|I|1)T,\left(\begin{matrix}\beta_{1}&\cdots&\beta_{i_{0}-1}&\alpha_{i_{0}}&\beta_{i_{0}+1}&\cdots&\beta_{|I|}&1\end{matrix}\right)^{T},

then Vol|I|(SI,r)\operatorname{Vol}_{|I|}({S}^{\prime}_{I,r}) contributes to the term P0P_{0} which appears in (7.4). (Here, the letter “TT” stands for the transposed matrix.) On the other hand, if it contains such a column for some i0{1,,d}i_{0}\in\{1,\ldots,d\}, then necessarily the βi\beta_{i}’s are zero, and the column is of the form

Ci0:=(00αi0001)TC_{i_{0}}:=\left(\begin{matrix}0&\cdots&0&\alpha_{i_{0}}&0&\cdots&0&1\end{matrix}\right)^{T}

(because Γ(fd)\Gamma(f_{d}^{\prime}) intersects the i0i_{0}th coordinate axis of +n\mathbb{R}^{n}_{+} precisely at the point (0,,0,αi0,0,,0)(0,\ldots,0,\alpha_{i_{0}},0,\ldots,0) by Lemma 7.1). If the matrix has two columns Ci0C_{i_{0}} and Ci0C_{i_{0}^{\prime}} of the above form, with i0,i0{1,,d}i_{0},i_{0}^{\prime}\in\{1,\ldots,d\} and i0i0i_{0}\not=i_{0}^{\prime}, then Vol|I|(SI,r)\operatorname{Vol}_{|I|}({S}^{\prime}_{I,r}) is not involved in the linear part (7.4) of ν(fd)\nu(f_{d}^{\prime}). Now, if it has one column Ci0C_{i_{0}} for some i0{1,,d}i_{0}\in\{1,\ldots,d\} and no any other column Ci0C_{i_{0}^{\prime}} for i0{1,,d}{i0}i_{0}^{\prime}\in\{1,\ldots,d\}\setminus\{i_{0}\}, then Vol|I|(SI,r)\operatorname{Vol}_{|I|}({S}^{\prime}_{I,r}) contributes to the term αi0Pi0\alpha_{i_{0}}P_{i_{0}} which appears in (7.4). Note that in the latter case, the matrix cannot have any column of the form CijC_{i_{j}} with ij{i1,,ip}i_{j}\in\{i_{1},\ldots,i_{p}\} (as otherwise the constant polynomial Pi0P_{i_{0}} would depend on αij\alpha_{i_{j}}). Altogether, for any 1i0d1\leq i_{0}\leq d, the volume Vol|I|(SI,r)\operatorname{Vol}_{|I|}({S}^{\prime}_{I,r}) contributes to the term αi0Pi0\alpha_{i_{0}}P_{i_{0}} if and only if the corresponding matrix has a column of the form Ci0C_{i_{0}} and no column of the form Ci0C_{i_{0}^{\prime}} for any other i0{1,,d,i1,,ip}{i0}=J{i0}i_{0}^{\prime}\in\{1,\ldots,d,i_{1},\ldots,i_{p}\}\setminus\{i_{0}\}=J\setminus\{i_{0}\}. In other words, Vol|I|(SI,r)\operatorname{Vol}_{|I|}({S}^{\prime}_{I,r}) contributes to the term αi0Pi0\alpha_{i_{0}}P_{i_{0}} if and only if SI,rΞI,J,i0{S}^{\prime}_{I,r}\in\Xi^{\prime}_{I,J,i_{0}}. Thus,

αi0Pi0\displaystyle\alpha_{i_{0}}P_{i_{0}} =I{1,,n},Ii0(SI,rΞI,J,i0(1)n|I||I|!Vol|I|(SI,r))\displaystyle=\sum_{I\subseteq\{1,\ldots,n\},\,I\ni i_{0}}\Bigg{(}\sum_{{S}^{\prime}_{I,r}\in{\Xi}^{\prime}_{I,J,i_{0}}}(-1)^{n-|I|}|I|!\operatorname{Vol}_{|I|}({S}^{\prime}_{I,r})\Bigg{)}
=I{1,,n},Ii0αi0(S~I,rΞ~I,J,i0(1)n|I||I|!Vol|I|(S~I,r))\displaystyle=\sum_{I\subseteq\{1,\ldots,n\},\,I\ni i_{0}}\alpha_{i_{0}}\Bigg{(}\sum_{\widetilde{S}^{\prime}_{I,r}\in\widetilde{\Xi}^{\prime}_{I,J,i_{0}}}(-1)^{n-|I|}|I|!\operatorname{Vol}_{|I|}(\widetilde{S}^{\prime}_{I,r})\Bigg{)}
=αi0ν~Ξ,J,i0(fd),\displaystyle=\alpha_{i_{0}}\widetilde{\nu}_{\Xi^{\prime},J,i_{0}}(f^{\prime}_{d}),

where S~I,r\widetilde{S}^{\prime}_{I,r} denotes the reduced simplex associated to SI,rS^{\prime}_{I,r} (see Section 3.4). Since Γ(fd)\Gamma(f_{d}^{\prime}) is obtained from Γ(fd)\Gamma(f_{d}) only by “adding” the vertices

vij:=(0,,0,αij,0,,0)\displaystyle v_{i_{j}}:=(0,\ldots,0,\alpha_{i_{j}},0,\ldots,0)

(with αij\alpha_{i_{j}} at the iji_{j}th place) for large αij\alpha_{i_{j}} (1jp1\leq j\leq p), if a simplex SI,r{S}^{\prime}_{I,r} of ΞI{\Xi}^{\prime}_{I} with maximal dimension is not a simplex of ΞI{\Xi}_{I} (in particular this is the case if ΞI=\Xi_{I}=\emptyset), then necessarily it intersects the iji_{j}th coordinate axis of +n\mathbb{R}^{n}_{+} for some jj (1jp1\leq j\leq p). It follows that

ΞI,{1,,d},i0=ΞI,J,i0,\displaystyle\Xi_{I,\{1,\ldots,d\},i_{0}}=\Xi^{\prime}_{I,J,i_{0}},

and hence,

ν~Ξ,i0(fd):=ν~Ξ,{1,,d},i0(fd)=ν~Ξ,J,i0(fd)=Pi0.\displaystyle\widetilde{\nu}_{\Xi,i_{0}}(f_{d}):=\widetilde{\nu}_{\Xi,\{1,\ldots,d\},i_{0}}(f_{d})=\widetilde{\nu}_{\Xi^{\prime},J,i_{0}}(f^{\prime}_{d})=P_{i_{0}}.

Since the choice of Ξ\Xi is arbitrary and Pi0P_{i_{0}} is a constant independent of Ξ\Xi, it follows that the modified Newton number ν~Ξ,i0(fd)\widetilde{\nu}_{\Xi,i_{0}}(f_{d}) is also independent of Ξ\Xi. The notation ν~i0(fd):=ν~Ξ,i0(fd)\widetilde{\nu}_{i_{0}}(f_{d}):=\widetilde{\nu}_{\Xi,i_{0}}(f_{d}) is therefore quite relevant.

Since the volume Vol|I|(SI,r)\operatorname{Vol}_{|I|}({S}^{\prime}_{I,r}) contributes to the term P0P_{0} if and only if the simplex SI,r{S}^{\prime}_{I,r} belongs to ΞI,J,0\Xi^{\prime}_{I,J,0} (we recall that P0P_{0} is constant, independent of αi1,,αip\alpha_{i_{1}},\ldots,\alpha_{i_{p}}), a similar argument shows that

ν0(fd)+(1)n=νΞ,J,0(fd)+(1)n=P0.\nu_{0}(f_{d})+(-1)^{n}=\nu_{\Xi^{\prime},J,0}(f^{\prime}_{d})+(-1)^{n}=P_{0}.\qed

Now we prove Lemma 7.1.

Proof of Lemma 7.1.

We argue by contradiction. Suppose that ff has a term of the form ciziaic_{i}z_{i}^{a_{i}} for some ii (1id1\leq i\leq d). To simplify, without loss of generality, we may assume i=1i=1 (the other cases are similar). By the Iomdine-Lê-Massey formula again and by Lemmas 3.7 and 3.8 of [1], for any 0b1bd0\ll b_{1}\ll\cdots\ll b_{d} sufficiently large (in particular so that a1<b1a_{1}<b_{1}), the function

g(z):=f(z)+z1b1++zdbdg(z):=f(z)+z_{1}^{b_{1}}+\cdots+z_{d}^{b_{d}}

is non-degenerate and has an isolated singularity at 0. Then, by [1, Corollary 2.9], its support (denoted by suppg\operatorname{supp}g) satisfies so-called Kouchnirenko condition (see [8] or Section 2 of [1] for the definition; see also Section 3 of [14] and the references mentioned therein for equivalent formulations and historical comments). Now, since a1<b1a_{1}<b_{1}, the Newton diagrams of gg and of the function

g(z):=g(z)z1b1g^{\prime}(z):=g(z)-z_{1}^{b_{1}}

coincide. It follows that gg^{\prime} is also non-degenerate and such that its support suppg\operatorname{supp}g^{\prime} satisfies the Kouchnirenko condition. Theorem 3.1 of [1] then implies that gg^{\prime} has an isolated singularity at 0. If d:=dim0Σf=1d:=\dim_{0}\Sigma f=1, then this is already a contradiction, because in this case g=fg^{\prime}=f. If d>1d>1, then define

Zg\displaystyle Z_{g^{\prime}} :={zn;gzi(z)=0 for all i{1,d+1,,n}}.\displaystyle:=\left\{z\in\mathbf{\mathbb{C}}^{n}\,;\,\frac{\partial g^{\prime}}{\partial z_{i}}(z)=0\mbox{ for all }i\in\{1,d+1,\ldots,n\}\right\}.

Define ZfZ_{f} similarly (replacing gg^{\prime} by ff). Clearly, Zg=ZfZ_{g^{\prime}}=Z_{f}. Therefore, we have d:=dim0Σfdim0Zf=dim0Zgd:=\dim_{0}\Sigma f\leq\dim_{0}Z_{f}=\dim_{0}Z_{g^{\prime}}, but since gg^{\prime} has an isolated singularity at 0, we must also have dim0Zg=d1\dim_{0}Z_{g^{\prime}}=d-1, a new contradiction. ∎

8. Proof of Corollary 5.1

First, we show that dim0Σf=dim0Σg\dim_{0}\Sigma f=\dim_{0}\Sigma g. The argument is similar to that given in the proof of Lemma 7.1. We argue by contradiction. Put d:=dim0Σfd:=\dim_{0}\Sigma f and s:=dim0Σgs:=\dim_{0}\Sigma g, and suppose for instance d<sd<s. By the Iomdine-Lê-Massey formula and by Lemmas 3.7 and 3.8 of [1], for any integers 0α1αd0\ll\alpha_{1}\ll\cdots\ll\alpha_{d} sufficiently large222Precisely, αp>max{2,ρfp1,z(p1)(0),ρgp1,z(p1)(0),m(fp1),m(gp1)}\alpha_{p}>\max\{2,\rho_{f_{p-1},z^{(p-1)}}(0),\rho_{g_{p-1},z^{(p-1)}}(0),m(f_{p-1}),m(g_{p-1})\}., the functions

fd(z):=f(z)+z1α1++zdαdandgd(z):=g(z)+z1α1++zdαdf_{d}(z):=f(z)+z_{1}^{\alpha_{1}}+\cdots+z_{d}^{\alpha_{d}}\quad\mbox{and}\quad g_{d}(z):=g(z)+z_{1}^{\alpha_{1}}+\cdots+z_{d}^{\alpha_{d}}

are non-degenerate, fdf_{d} has an isolated singularity at 0, and dim0Σgd=sd>0\dim_{0}\Sigma g_{d}=s-d>0. Then, by [1, Corollary 2.9], the support of fdf_{d} satisfies the Kouchnirenko condition. Since ff and gg have the same Newton diagram, it follows that Γ(fd)=Γ(gd)\Gamma(f_{d})=\Gamma(g_{d}) too. Thus the support of gdg_{d} also satisfies the Kouchnirenko condition, and by [1, Theorem 3.1], the function gdg_{d} must have an isolated singularity at 0 — a contradiction.

Now, to show that the Lê numbers of ff and gg at 0 with respect to the coordinates z=(z1,,zn)z=(z_{1},\ldots,z_{n}) are equal, we apply Theorem 4.1. By this theorem, these Lê numbers are described in terms of the modified (and special modified) Newton numbers of the functions fdf_{d} and gdg_{d}. Then the result follows immediately from the equality Γ(fd)=Γ(gd)\Gamma(f_{d})=\Gamma(g_{d}).

Appendix A

For completeness, in this appendix, we give a proof of a useful elementary lemma which we have used in the proof of Theorem 4.1.

Let dd be a positive integer. Consider the following system 𝒮\mathscr{S} of dd integral inequalities with dd variables α1,,αd\alpha_{1},\ldots,\alpha_{d}:

{α1c1,α2c2(α1),α3c3(α1,α2),αdcd(α1,,αd1).\begin{cases}\alpha_{1}\geq c_{1},\\ \alpha_{2}\geq c_{2}(\alpha_{1}),\\ \alpha_{3}\geq c_{3}(\alpha_{1},\alpha_{2}),\\ \cdots\\ \alpha_{d}\geq c_{d}(\alpha_{1},\ldots,\alpha_{d-1}).\end{cases}

Here, c1c_{1} is a constant, and for 2d2\leq\ell\leq d, c(α1,,α1)c_{\ell}(\alpha_{1},\ldots,\alpha_{\ell-1}) is a number depending on α1,,α1\alpha_{1},\ldots,\alpha_{\ell-1}. For each 1rd1\leq r\leq d, let 𝒮(r)\mathscr{S}(r) be the system consisting only of the first rr inequalities of the system 𝒮\mathscr{S}. Finally, let Z(r)rZ(r)\subseteq\mathbf{\mathbb{Z}}^{r} be the set of (integral) solutions of the system 𝒮(r)\mathscr{S}(r).

Lemma A.1.

For any 1rd1\leq r\leq d, if P(x1,,xr)P(x_{1},\ldots,x_{r}) is a polynomial function that vanishes on Z(r)Z(r), then it is identically zero.

Proof.

By induction on rr. For r=1r=1, the lemma immediately follows from the fundamental theorem of algebra. Now suppose the lemma holds true for some integer r1r-1 (with r2r\geq 2), and let us show that it also holds true for the integer rr. So, let P(x1,,xr)P(x_{1},\ldots,x_{r}) be a polynomial function such that P(α1,,αr)=0P(\alpha_{1},\ldots,\alpha_{r})=0 for any (α1,,αr)Z(r)(\alpha_{1},\ldots,\alpha_{r})\in Z(r). Note that (α1,,αr)Z(r)(\alpha_{1},\ldots,\alpha_{r})\in Z(r) implies (α1,,αr1)Z(r1)(\alpha_{1},\ldots,\alpha_{r-1})\in Z(r-1). Expand PP with respect to the variable xrx_{r}:

P(x1,,xr)=k=0δPk(x1,,xr1)xrk.P(x_{1},\ldots,x_{r})=\sum_{k=0}^{\delta}P_{k}(x_{1},\ldots,x_{r-1})\,x_{r}^{k}.

(Here, δ\delta denotes the degree of PP.) Then for all (α1,,αr)Z(r)(\alpha_{1},\ldots,\alpha_{r})\in Z(r),

k=0δPk(α1,,αr1)αrk=0.\sum_{k=0}^{\delta}P_{k}(\alpha_{1},\ldots,\alpha_{r-1})\,\alpha_{r}^{k}=0.

By the fundamental theorem of algebra, it follows that for each 0kδ0\leq k\leq\delta,

Pk(α1,,αr1)=0P_{k}(\alpha_{1},\ldots,\alpha_{r-1})=0

for every fixed (α1,,αr1)Z(r1)(\alpha_{1},\ldots,\alpha_{r-1})\in Z(r-1). Now, by the induction hypothesis, this implies that the polynomial PkP_{k} identically vanishes. ∎

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    E-mail: ch.eyral@impan.pl  Grzegorz Oleksik
    Faculty of Mathematics and Computer Science, University of Łódź
    S. Banacha 22, 90-238 Łódź, Poland
    E-mail: oleksig@math.uni.lodz.pl  Adam Różycki
    Faculty of Mathematics and Computer Science, University of Łódź
    S. Banacha 22, 90-238 Łódź, Poland
    E-mail: rozycki@math.uni.lodz.pl