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Nematic and chiral superconductivity induced by odd-parity fluctuations

Fengcheng Wu fengcheng.wu@anl.gov Materials Science Division, Argonne National Laboratory, Argonne, Illinois 60439, USA    Ivar Martin Materials Science Division, Argonne National Laboratory, Argonne, Illinois 60439, USA
(September 3, 2025)
Abstract

Recent experiments indicate that superconductivity in Bi2Se3 intercalated with Cu, Nb or Sr is nematic with rotational symmetry breaking. Motivated by this observation, we present a model study of nematic and chiral superconductivity induced by odd-parity fluctuations. We show that odd-parity fluctuations in the two-component EuE_{u} representation of D3dD_{3d} crystal point group can generate attractive interaction in both the even-parity ss-wave and odd-parity EuE_{u} pairing channels, but repulsive interaction in other odd-parity pairing channels. Coulomb repulsion can suppress ss-wave pairing relative to EuE_{u} pairing, and thus the latter can have a higher critical temperature. EuE_{u} pairing has two distinct phases: a nematic phase and a chiral phase, both of which can be realized in our model. When ss-wave and EuE_{u} pairings have similar instability temperature, we find an intermediate phase in which both types of pairing coexist.

I Introduction

The theoretical identification of time-reversal invariant topological insulatorsKane and Mele (2005); Fu et al. (2007) has sparked a great discovery of topological states in various forms of matter, including insulatorsHasan and Kane (2010); Qi and Zhang (2011), superconductorsQi and Zhang (2011) and semimetalsLiu et al. (2014); Xu et al. (2015). A topological superconductor is enriched by its intrinsic particle-hole symmetry, which protects zero-energy Majorana modes on boundaries and in vorticesQi and Zhang (2011). Topological superconductivity is being actively studied in both theoryFu and Kane (2008); Qi et al. (2009); Sau et al. (2010); Lutchyn et al. (2010) and experimentNadj-Perge et al. (2014); Albrecht et al. (2016).

Recent experiments have identified Bi2Se3 intercalated with Cu, Nb or Sr as a candidate system for topological superconductor. Many bulk properties in the superconducting state of doped Bi2Se3 display a uniaxial anisotropy in response to an in-plane magnetic field, which include Knight shiftMatano et al. (2016), upper critical fieldYonezawa et al. (2017); Pan et al. (2016), magnetic torqueAsaba et al. (2017) and specific heatYonezawa et al. (2017). Therefore, the superconducting state breaks the lattice discrete rotational symmetry, and can be termed as nematic. Specific heatKriener et al. (2011) and penetration depth measurementSmylie et al. (2016) have shown the absence of line nodes in the superconducting state. Given these experimental observations, the nematic state is most consistent with an EuE_{u} pairing channel that has two components and odd-parity symmetryFu (2014). Here EuE_{u} is one of the symmetry representations allowed by the D3dD_{3d} point group of Bi2Se3. The odd-parity nematic state can be a fully-gapped time-reversal-invariant topological superconductorFu (2014). So far, experimental evidence of surface Majorana states associated with topological superconductivity has been not conclusiveSasaki et al. (2011); Levy et al. (2013). On the theoretical side, different aspects of the nematic states have been explored, including bulk propertiesHashimoto et al. (2013); Nagai and Ota (2016); Venderbos et al. (2016a), surface statesYang et al. (2014), vortex statesWu and Martin (2017); Zyuzin et al. , and the interplay between EuE_{u} superconductivity and magnetismYuan et al. (2017); Chirolli et al. (2017).

The basic question, which remains largely openFu (2016); Behnia (2017), is the underlying microscopic mechanism for the odd-parity nematic superconductivity in doped Bi2Se3. In the pioneering work of Fu and Berg(Fu and Berg, 2010), they demonstrated that pairing instability in the odd-parity channels can be generated by a simple type of attractive interaction in doped Bi2Se3. However, the odd-parity A1uA_{1u} pairing channel has a higher critical temperature than the EuE_{u} pairing channel in their model.

Odd-parity pairing can be induced by magnetic fluctuations, as in the case of superfluid Helium-3Leggett (1975) and in strongly correlated materials like Sr2RuO4Rice and Sigrist (1995) and UPt3Nomoto and Ikeda (2016). It has recently been proposed that odd-parity pairing can also be induced by odd-parity fluctuations in a system with strong spin-orbit coupling, time reversal and inversion symmetriesKozii and Fu (2015); Wang et al. (2016); Ruhman et al. (2017). As doped Bi2Se3 is likely a weakly correlated material, we study superconductivity induced by odd-parity fluctuations in this paper.

In Ref. Kozii and Fu, 2015, Kozii and Fu have studied the most symmetric group O(3)O(3) in three dimensions, and found that odd-parity fluctuation in pseudoscalar and vector representations generate attractive interaction in both conventional even-parity ss-wave pairing channel and odd-parity pairing channels, while fluctuation in the multipolar channel only generates attractive interaction in the ss-wave channel. Our work builds upon Ref. Kozii and Fu, 2015. We apply a similar approach to doped Bi2Se3 which has a D3dD_{3d} point group symmetry. Symmetry classifications of odd-parity fluctuations for O(3)O(3) and D3dD_{3d} groups are different. Our main results can be summarized as follows. Odd-parity fluctuations in the EuE_{u} representation of the D3dD_{3d} point group can induce attractive interaction in both the ss-wave and odd-parity EuE_{u} pairing channels, but repulsive interaction in the other two odd-parity A1uA_{1u} and A2uA_{2u} pairing channels. The competition between ss-wave and EuE_{u} pairings can be further tuned by Coulomb repulsion, which has the strongest pair-breaking effect in the ss-wave channel.

The organization of this paper is the following. In Sec. II, we study odd-parity fluctuations and superconductivity. The fluctuations are possibly induced by electron-phonon interaction. We use an approach that closely follow that in Ref. Kozii and Fu, 2015. Essential details of the approach will be presented to make the discussion self-contained. We obtain a phase diagram (Fig. 1) as a function of phenomenological parameters γi\gamma_{i} (i=1,2,3) and UU. γi\gamma_{i}, introduced in Eq. (5), parametrize odd-parity particle-hole fluctuations in EuE_{u} representation. UU is the repulsive interaction in the ss-wave pairing channel, which can arise from Coulomb repulsion. There is a critical UcU_{c}, above which EuE_{u} pairing has a higher critical temperature compared to the ss-wave pairing. EuE_{u} superconductivity supports two distinct phasesVenderbos et al. (2016b): nematic and chiral, both of which can be realized in the parameter space of γi\gamma_{i}. In Sec. III, we study a phase in the vicinity of UcU_{c}, where even-parity ss-wave and odd-parity EuE_{u} pairing can coexist. The coexistence phase spontaneously breaks both time-reversal and lattice discrete rotational symmetries. The gap structures in different superconductivity phases are reviewed. In Sec. IV, we discuss our work in the context of previous studies. We present some related materials in the Appendixes. Appendix A shows that an on-site repulsion in Bi2Se3 generates repulsive interaction in both ss-wave and A2uA_{2u} pairing channels, but not in the EuE_{u} channel. In Appendixes B and C, we show that odd-parity fluctuations in A1uA_{1u} (A2uA_{2u}) representation can generate A1uA_{1u} (A2uA_{2u}) Cooper pairing besides the usual ss-wave pairing.

Before ending the Introduction section, we mention that odd-parity particle-hole fluctuations can become unstable and lead to spontaneous parity-breaking phasesFu (2015), which have been recently observed in Cd2Re2O7Harter et al. (2017).

II Two-component Odd-parity fluctuation and Superconductivity

Electronic bands in Bi2Se3 are doubly degenerate at every 𝒌\boldsymbol{k} point due to the presence of both time-reversal and inversion symmetries. When Bi2Se3 is intercalated with Cu, Nb or Sr, the chemical potential lies in the conduction bands. As attractive interaction induced by fluctuations typically occurs in a small energy window around chemical potential, we will only retain the lowest conduction bands in our theory. The Fermi surface of Bi2Se3 at low electron doping level is approximately sphericalWray et al. (2010); Lawson et al. (2012). Therefore, we approximate the conduction band by a parabolic dispersion:

H0=𝒌(𝒌22mμ)c𝒌c𝒌,H_{0}=\sum_{\boldsymbol{k}}(\frac{\hbar\boldsymbol{k}^{2}}{2m}-\mu)c_{\boldsymbol{k}}^{\dagger}c_{\boldsymbol{k}}, (1)

which is intended to describe physics near the chemical potential μ\mu. c𝒌c_{\boldsymbol{k}}^{\dagger} represents a two-component spinor (c𝒌,c𝒌)(c_{\boldsymbol{k}\uparrow}^{\dagger},c_{\boldsymbol{k}\downarrow}^{\dagger}), which is understood to be in the “manifestly covariant Bloch basis”(MCBB)Fu (2015). Here \uparrow and \downarrow represent pseudospin instead of real spin because of strong spin-orbit coupling. Nevertheless, the pseudospin in the MCBB transforms in the same way as the real spin of a free electron under symmetry operations. In particular, the transformations under time reversal (𝒯^\hat{\mathcal{T}}) and inversion (𝒫^\hat{\mathcal{P}}) operations are:

𝒯^c𝒌α𝒯^1=ϵαβc𝒌β,𝒫^c𝒌α𝒫^1=c𝒌α,\hat{\mathcal{T}}c_{\boldsymbol{k}\alpha}^{\dagger}\hat{\mathcal{T}}^{-1}=\epsilon_{\alpha\beta}c_{-\boldsymbol{k}\beta}^{\dagger},\,\,\,\,\hat{\mathcal{P}}c_{\boldsymbol{k}\alpha}^{\dagger}\hat{\mathcal{P}}^{-1}=c_{-\boldsymbol{k}\alpha}^{\dagger}, (2)

where ϵαβ\epsilon_{\alpha\beta} is the fully antisymmetric tensor with ϵ=1\epsilon_{\uparrow\downarrow}=1.

To study electron-phonon interaction, we focus on phonons at the Brillouin zone center, which can be classified by the D3dD_{3d} point group of Bi2Se3. To be specific, we consider EuE_{u} phonons that are odd under inversion and have two degenerate modes. The coupling between electrons and EuE_{u} phonons can be expressed as:

Helph,0\displaystyle H_{el-ph,0} =ϕxQ^x+ϕyQ^y,\displaystyle=\phi_{x}\hat{Q}_{x}+\phi_{y}\hat{Q}_{y}, (3)
Q^a\displaystyle\hat{Q}_{a} =12𝒌c𝒌Γa(𝒌)c𝒌,\displaystyle=\frac{1}{2}\sum_{\boldsymbol{k}}c^{\dagger}_{\boldsymbol{k}}\Gamma_{a}(\boldsymbol{k})c_{\boldsymbol{k}},

where the Hermitian operators (ϕx,ϕy)(\phi_{x},\phi_{y}) represent the EuE_{u} phonons, and also take into account all coupling constants. Γx,y(𝒌)\Gamma_{x,y}(\boldsymbol{k}) are 2×22\times 2 matrices in the pseudospin space. As Helph,0H_{el-ph,0} should be invariant under all symmetries that the system has, the operators Q^x,y\hat{Q}_{x,y} are Hermitian, time reversal symmetric and form a two-component EuE_{u} representation. By Hermiticity, we can express Γx,y(𝒌)\Gamma_{x,y}(\boldsymbol{k}) using identity matrix s0s_{0} and Pauli matrices 𝒔\boldsymbol{s}:

Γa(𝒌)=D~a(𝒌)s0+𝑫a(𝒌)𝒔,\Gamma_{a}(\boldsymbol{k})=\tilde{D}_{a}(\boldsymbol{k})s_{0}+\boldsymbol{D}_{a}(\boldsymbol{k})\cdot\boldsymbol{s}, (4)

where both the scalar D~a\tilde{D}_{a} and the vector 𝑫a\boldsymbol{D}_{a} are real. By time reversal symmetry, we require D~a(𝒌)=D~a(𝒌)\tilde{D}_{a}(\boldsymbol{k})=\tilde{D}_{a}(-\boldsymbol{k}) and 𝑫a(𝒌)=𝑫a(𝒌)\boldsymbol{D}_{a}(\boldsymbol{k})=-\boldsymbol{D}_{a}(-\boldsymbol{k}). On the other hand, Q^a\hat{Q}_{a} is odd under inversion, which leads to Γa(𝒌)=Γa(𝒌)\Gamma_{a}(\boldsymbol{k})=-\Gamma_{a}(-\boldsymbol{k}). Therefore, D~a(𝒌)\tilde{D}_{a}(\boldsymbol{k}) must vanish. In our low-energy theory, odd-parity phonons couple to electron’s spin, which is possible due to the presence of strong spin-orbit coupling.

The form factors Γx,y(𝒌)\Gamma_{x,y}(\boldsymbol{k}) are further restricted by other point group symmetries. There are three basis functions separately for Γx\Gamma_{x} and Γy\Gamma_{y} to first order of 𝒌\boldsymbol{k} in the EuE_{u} representation, as listed in Table 1. In general, Γx,y(𝒌)\Gamma_{x,y}(\boldsymbol{k}) is a linear combination of these three basis functions:

Γa(𝒌)=γ1Γa(1)(𝒌)+γ2Γa(2(𝒌)+γ3Γa(3)(𝒌)\Gamma_{a}(\boldsymbol{k})=\gamma_{1}\Gamma_{a}^{(1)}(\boldsymbol{k})+\gamma_{2}\Gamma_{a}^{(2}(\boldsymbol{k})+\gamma_{3}\Gamma_{a}^{(3)}(\boldsymbol{k}) (5)

where γi\gamma_{i} are real parameters that are not fixed by symmetries. We will take γi\gamma_{i} as free parameters and study phase diagrams in this parameter space.

Table 1: Linear order expansion of odd-parity form factors in different symmetry representations of D3dD_{3d} point groupVenderbos et al. (2016b). A1uA_{1u} and EuE_{u} representations have multiple basis functions in lowest order expansion. k^i\hat{k}_{i} denotes ki/|𝒌|k_{i}/|\boldsymbol{k}|.
Symmetry Form factors
A1uA_{1u} Γ1(1)=12(k^xsx+k^ysy)\Gamma_{1}^{(1)}=\frac{1}{\sqrt{2}}(\hat{k}_{x}s_{x}+\hat{k}_{y}s_{y}), Γ1(2)=k^zsz\Gamma_{1}^{(2)}=\hat{k}_{z}s_{z}
A2uA_{2u} Γ2(1)=12(k^xsyk^ysx)\Gamma_{2}^{(1)}=\frac{1}{\sqrt{2}}(\hat{k}_{x}s_{y}-\hat{k}_{y}s_{x})
EuE_{u} Γx(1)=k^xsz,Γx(2)=k^zsx,Γx(3)=12(k^xsy+k^ysx)Γy(1)=k^ysz,Γy(2)=k^zsy,Γy(3)=12(k^xsxk^ysy)\begin{matrix}\Gamma_{x}^{(1)}=\hat{k}_{x}s_{z},\Gamma_{x}^{(2)}=\hat{k}_{z}s_{x},\Gamma_{x}^{(3)}=\frac{1}{\sqrt{2}}(\hat{k}_{x}s_{y}+\hat{k}_{y}s_{x})\\ \Gamma_{y}^{(1)}=\hat{k}_{y}s_{z},\Gamma_{y}^{(2)}=\hat{k}_{z}s_{y},\Gamma_{y}^{(3)}=\frac{1}{\sqrt{2}}(\hat{k}_{x}s_{x}-\hat{k}_{y}s_{y})\end{matrix}

Helph,0H_{el-ph,0} describes the coupling between electrons and zone-center phonon modes. We generalize the coupling to include phonon modes at finite momentum:

Helph\displaystyle H_{el-ph} =𝒒ϕx,𝒒Q^x(𝒒)+ϕy,𝒒Q^y(𝒒),\displaystyle=\sum_{\boldsymbol{q}}\phi_{x,\boldsymbol{q}}\hat{Q}_{x}(\boldsymbol{q})+\phi_{y,\boldsymbol{q}}\hat{Q}_{y}(\boldsymbol{q}), (6)
Q^a(𝒒)\displaystyle\hat{Q}_{a}(\boldsymbol{q}) =12𝒌c𝒌+𝒒[Γa(𝒌+𝒒)+Γa(𝒌)]c𝒌.\displaystyle=\frac{1}{2}\sum_{\boldsymbol{k}}c^{\dagger}_{\boldsymbol{k}+\boldsymbol{q}}[\Gamma_{a}(\boldsymbol{k}+\boldsymbol{q})+\Gamma_{a}(\boldsymbol{k})]c_{\boldsymbol{k}}.

In the generalization, we assume that the phonon modes vary smoothly in real space.

The electron-phonon coupling generates an effective electron-electron interaction:

Hint=1Ω𝒒V𝒒[Q^x(𝒒)Q^x(𝒒)+Q^y(𝒒)Q^y(𝒒)],H_{int}=\frac{1}{\Omega}\sum_{\boldsymbol{q}}V_{\boldsymbol{q}}[\hat{Q}_{x}(\boldsymbol{q})\hat{Q}_{x}(-\boldsymbol{q})+\hat{Q}_{y}(\boldsymbol{q})\hat{Q}_{y}(-\boldsymbol{q})], (7)

where Ω\Omega is the system size. By the definition in (6), we have Q^a(𝒒)=Q^a(𝒒)\hat{Q}_{a}(-\boldsymbol{q})=\hat{Q}_{a}^{\dagger}(\boldsymbol{q}).

In HintH_{int}, we neglect the frequency dependence of V𝒒V_{\boldsymbol{q}} for simplicity. The point group symmetries put constraints on the momentum dependence of V𝒒V_{\boldsymbol{q}}: (1) V𝒒V_{\boldsymbol{q}} is an even function of 𝒒\boldsymbol{q} and (2) it is invariant under a three-fold rotation of 𝒒\boldsymbol{q} along z^\hat{z} direction.

We now restrict the interaction to the Bardeen-Cooper-Schrieffer (BCS) channel:

HBCS=1Ω𝒌,𝒌Vαβγδ(𝒌,𝒌)c𝒌αc𝒌βc𝒌γc𝒌δ.H_{BCS}=\frac{1}{\Omega}\sum_{\boldsymbol{k},\boldsymbol{k}^{\prime}}V_{\alpha\beta\gamma\delta}(\boldsymbol{k},\boldsymbol{k}^{\prime})c^{\dagger}_{\boldsymbol{k}\alpha}c^{\dagger}_{-\boldsymbol{k}\beta}c_{-\boldsymbol{k}^{\prime}\gamma}c_{\boldsymbol{k}^{\prime}\delta}. (8)

The expression for the interaction vertex Vαβγδ(𝒌,𝒌)V_{\alpha\beta\gamma\delta}(\boldsymbol{k},\boldsymbol{k}^{\prime}) is given by:

Vαβγδ(𝒌,𝒌)\displaystyle V_{\alpha\beta\gamma\delta}(\boldsymbol{k},\boldsymbol{k}^{\prime}) (9)
=18a=x,y{\displaystyle=-\frac{1}{8}\sum_{a=x,y}\Big{\{} V𝒌𝒌[𝑫a+𝑫a]𝒔αδ[𝑫a+𝑫a]𝒔βγ\displaystyle V_{\boldsymbol{k}-\boldsymbol{k}^{\prime}}[\boldsymbol{D}_{a}+\boldsymbol{D}_{a}^{\prime}]\cdot\boldsymbol{s}_{\alpha\delta}[\boldsymbol{D}_{a}+\boldsymbol{D}_{a}^{\prime}]\cdot\boldsymbol{s}_{\beta\gamma}
\displaystyle- V𝒌+𝒌[𝑫a𝑫a]𝒔αγ[𝑫a𝑫a]𝒔βδ},\displaystyle V_{\boldsymbol{k}+\boldsymbol{k}^{\prime}}[\boldsymbol{D}_{a}-\boldsymbol{D}_{a}^{\prime}]\cdot\boldsymbol{s}_{\alpha\gamma}[\boldsymbol{D}_{a}-\boldsymbol{D}_{a}^{\prime}]\cdot\boldsymbol{s}_{\beta\delta}\Big{\}},

where 𝑫a\boldsymbol{D}_{a} and 𝑫a\boldsymbol{D}_{a}^{\prime} are respectively shorthand notations for 𝑫a(𝒌)\boldsymbol{D}_{a}(\boldsymbol{k}) and 𝑫a(𝒌)\boldsymbol{D}_{a}(\boldsymbol{k}^{\prime}). Here 𝑫a(𝒌)\boldsymbol{D}_{a}(\boldsymbol{k}) is the vector representation of Γa(𝒌)\Gamma_{a}(\boldsymbol{k}), as introduced in (4).

To minimize the number of parameters in our phenomenogical study, we further approximate V𝒒V_{\boldsymbol{q}} by its value at zero momentum V0V_{0}. Here V0<0V_{0}<0, representing attractive interaction induced by phonon fluctuations. Under this simplification, it is convenient to separate VαβγδV_{\alpha\beta\gamma\delta} to two parts: Vαβγδ=(Ve+Vo)αβγδV_{\alpha\beta\gamma\delta}=(V^{e}+V^{o})_{\alpha\beta\gamma\delta}. The expressions for Ve,oV^{e,o} are as follows:

Vαβγδe(𝒌,𝒌)\displaystyle V^{e}_{\alpha\beta\gamma\delta}(\boldsymbol{k},\boldsymbol{k}^{\prime}) (10)
\displaystyle\approx V08a=x,y{(𝑫a𝒔)αδ(𝑫a𝒔)βγ(𝑫a𝒔)αγ(𝑫a𝒔)βδ\displaystyle-\frac{V_{0}}{8}\sum_{a=x,y}\Big{\{}(\boldsymbol{D}_{a}\cdot\boldsymbol{s})_{\alpha\delta}(\boldsymbol{D}_{a}\cdot\boldsymbol{s})_{\beta\gamma}-(\boldsymbol{D}_{a}\cdot\boldsymbol{s})_{\alpha\gamma}(\boldsymbol{D}_{a}\cdot\boldsymbol{s})_{\beta\delta}
+\displaystyle+ (𝑫a𝒔)αδ(𝑫a𝒔)βγ(𝑫a𝒔)αγ(𝑫a𝒔)βδ}\displaystyle(\boldsymbol{D}_{a}^{\prime}\cdot\boldsymbol{s})_{\alpha\delta}(\boldsymbol{D}_{a}^{\prime}\cdot\boldsymbol{s})_{\beta\gamma}-(\boldsymbol{D}_{a}^{\prime}\cdot\boldsymbol{s})_{\alpha\gamma}(\boldsymbol{D}_{a}^{\prime}\cdot\boldsymbol{s})_{\beta\delta}\Big{\}}
=\displaystyle= V08a=x,y(|𝑫a|2+|𝑫a|2)ϵαβϵγδ,\displaystyle\frac{V_{0}}{8}\sum_{a=x,y}(|\boldsymbol{D}_{a}|^{2}+|\boldsymbol{D}_{a}^{\prime}|^{2})\epsilon_{\alpha\beta}\epsilon^{\dagger}_{\gamma\delta},
Vαβγδo(𝒌,𝒌)\displaystyle V^{o}_{\alpha\beta\gamma\delta}(\boldsymbol{k},\boldsymbol{k}^{\prime})
\displaystyle\approx V08a=x,y{(𝑫a𝒔)αδ(𝑫a𝒔)βγ+(𝑫a𝒔)αγ(𝑫a𝒔)βδ\displaystyle-\frac{V_{0}}{8}\sum_{a=x,y}\Big{\{}(\boldsymbol{D}_{a}\cdot\boldsymbol{s})_{\alpha\delta}(\boldsymbol{D}_{a}^{\prime}\cdot\boldsymbol{s})_{\beta\gamma}+(\boldsymbol{D}_{a}\cdot\boldsymbol{s})_{\alpha\gamma}(\boldsymbol{D}_{a}^{\prime}\cdot\boldsymbol{s})_{\beta\delta}
+(𝑫a𝒔)αδ(𝑫a𝒔)βγ+(𝑫a𝒔)αγ(𝑫a𝒔)βδ]}\displaystyle+(\boldsymbol{D}_{a}^{\prime}\cdot\boldsymbol{s})_{\alpha\delta}(\boldsymbol{D}_{a}\cdot\boldsymbol{s})_{\beta\gamma}+(\boldsymbol{D}_{a}^{\prime}\cdot\boldsymbol{s})_{\alpha\gamma}(\boldsymbol{D}_{a}\cdot\boldsymbol{s})_{\beta\delta}]\Big{\}}
=\displaystyle= V04a=x,y{[(𝑫a𝒔)ϵ]αβ[(𝑫a𝒔)ϵ]γδ\displaystyle\frac{V_{0}}{4}\sum_{a=x,y}\Big{\{}[(\boldsymbol{D}_{a}\cdot\boldsymbol{s})\epsilon]_{\alpha\beta}[(\boldsymbol{D}_{a}^{\prime}\cdot\boldsymbol{s})\epsilon]^{\dagger}_{\gamma\delta}
[(𝑫a×𝒔)ϵ]αβ[(𝑫a×𝒔)ϵ]γδ}.\displaystyle\quad\quad\quad\,\,-[(\boldsymbol{D}_{a}\times\boldsymbol{s})\epsilon]_{\alpha\beta}\cdot[(\boldsymbol{D}_{a}^{\prime}\times\boldsymbol{s})\epsilon]^{\dagger}_{\gamma\delta}\Big{\}}.

Here VeV^{e} and VoV^{o} are respectively even and odd functions of 𝒌\boldsymbol{k} and 𝒌\boldsymbol{k}^{\prime}, and, therefore, generate correspondingly even and odd parity pairings. In (10), the final expressions of Ve,oV^{e,o} are presented in a form that is suitable for BCS decomposition. In the following subsections II.1 and II.2, we study the pairing instabilities in even and odd parity channels separately and finally compare them.

II.1 Even-parity instability

Even-parity pairing, or typically named as ss-wave pairing, is induced by VeV^{e}. As we will discuss in the subsection II.2, the effective interaction HintH_{int} (7) always generates a larger instability in ss-wave channel compared to odd-parity channels. To study competition between even and odd parity pairings, we add a repulsive interaction to VeV^{e}:

He=\displaystyle H_{e}= 1Ω𝒌,𝒌[Vαβγδe(𝒌,𝒌)+U|V0|4ϵαβϵγδ]c𝒌αc𝒌βc𝒌γc𝒌δ\displaystyle\frac{1}{\Omega}\sum_{\boldsymbol{k},\boldsymbol{k}^{\prime}}[V^{e}_{\alpha\beta\gamma\delta}(\boldsymbol{k},\boldsymbol{k}^{\prime})+\frac{U|V_{0}|}{4}\epsilon_{\alpha\beta}\epsilon^{\dagger}_{\gamma\delta}]c^{\dagger}_{\boldsymbol{k}\alpha}c^{\dagger}_{-\boldsymbol{k}\beta}c_{-\boldsymbol{k}^{\prime}\gamma}c_{\boldsymbol{k}^{\prime}\delta} (11)
=\displaystyle= V0Ω𝒌,𝒌[g0(𝒌)+g0(𝒌)][12ϵαβc𝒌αc𝒌β][12ϵγδc𝒌γc𝒌δ],\displaystyle\frac{V_{0}}{\Omega}\sum_{\boldsymbol{k},\boldsymbol{k}^{\prime}}[g_{0}(\boldsymbol{k})+g_{0}(\boldsymbol{k}^{\prime})][\frac{1}{2}\epsilon_{\alpha\beta}c^{\dagger}_{\boldsymbol{k}\alpha}c^{\dagger}_{-\boldsymbol{k}\beta}][\frac{1}{2}\epsilon^{\dagger}_{\gamma\delta}c_{-\boldsymbol{k}^{\prime}\gamma}c_{\boldsymbol{k}^{\prime}\delta}],

where U>0U>0 characterizes the repulsive interaction and g0(𝒌)=(|𝑫x(𝒌)|2+|𝑫y(𝒌)|2U)/2g_{0}(\boldsymbol{k})=(|\boldsymbol{D}_{x}(\boldsymbol{k})|^{2}+|\boldsymbol{D}_{y}(\boldsymbol{k})|^{2}-U)/2. For reasons to become clear shortly, we make the following transformation:

g0(𝒌)+g0(𝒌)\displaystyle g_{0}(\boldsymbol{k})+g_{0}(\boldsymbol{k}^{\prime}) =12κ[g+(𝒌)g+(𝒌)g(𝒌)g(𝒌)],\displaystyle=\frac{1}{2\kappa}[g_{+}(\boldsymbol{k})g_{+}(\boldsymbol{k}^{\prime})-g_{-}(\boldsymbol{k})g_{-}(\boldsymbol{k}^{\prime})], (12)
g±(𝒌)\displaystyle g_{\pm}(\boldsymbol{k}) =g0(𝒌)±κ,\displaystyle=g_{0}(\boldsymbol{k})\pm\kappa,

where κ\kappa is a positive parameter. We choose κ\kappa such that:

g+(𝒌)g(𝒌)=0,\langle g_{+}(\boldsymbol{k})g_{-}(\boldsymbol{k})\rangle=0, (13)

where \langle...\rangle denotes an average over Fermi surface, normalized so 1=1\langle 1\rangle=1. Using (12), HeH_{e} can be decomposed into two channels:

He=\displaystyle H_{e}= V02κΩ(S+S+SS),\displaystyle\frac{V_{0}}{2\kappa\Omega}(S_{+}^{\dagger}S_{+}-S_{-}^{\dagger}S_{-}), (14)
S±=\displaystyle S_{\pm}^{\dagger}= 12𝒌αβg±(𝒌)ϵαβc𝒌αc𝒌β.\displaystyle\frac{1}{2}\sum_{\boldsymbol{k}\alpha\beta}g_{\pm}(\boldsymbol{k})\epsilon_{\alpha\beta}c^{\dagger}_{\boldsymbol{k}\alpha}c^{\dagger}_{-\boldsymbol{k}\beta}.

Because g+(𝒌)g_{+}(\boldsymbol{k}) and g(𝒌)g_{-}(\boldsymbol{k}) are orthogonal over the Fermi surface as required by (13), the attractive and repulsive channels respectively represented by S+S_{+}^{\dagger} and SS_{-}^{\dagger} are decoupled in the linearized gap equation. Therefore, we only consider S+S_{+}^{\dagger} in the following. The critical temperature Tc,sT_{c,s} for S+S_{+}^{\dagger} channel is determined by its linearized gap equation:

|V0|χs(Tc,s)=1,\displaystyle|V_{0}|\chi_{s}(T_{c,s})=1, (15)
χs(T)=12κ12Tr[g+(𝒌)s0]2χ0(T).\displaystyle\chi_{s}(T)=\frac{1}{2\kappa}\langle\frac{1}{2}\text{Tr}[g_{+}(\boldsymbol{k})s_{0}]^{2}\rangle\chi_{0}(T).

Here χ0\chi_{0} is the standard superconductivity susceptibility: χ0(T)=N(0)ωDωD𝑑εtanh[ε/(2T)]/(2ε)\chi_{0}(T)=N(0)\int_{-\omega_{D}}^{\omega_{D}}d\varepsilon\text{tanh}[\varepsilon/(2T)]/(2\varepsilon), where N(0)N(0) is the density of states at the Fermi energy, ωD\omega_{D} is the cut off energy for attractive interaction, and TT is the temperature.

II.2 Odd-parity instability

Refer to caption
Figure 1: (a) χp(T)/χs(T)\chi_{p}(T)/\chi_{s}(T) at U=0U=0 as a function of γ1\gamma_{1} and γ2\gamma_{2}. (b) The surface with rainbow color represents UcU_{c} at which χp(T)=χs(T)\chi_{p}(T)=\chi_{s}(T). The odd-parity EuE_{u} superconductivity supports two different phases: nematic and chiral, which are separated by the gray boundaries. In (a) and (b), we used the normalization γ12+γ22+γ32=1\gamma_{1}^{2}+\gamma_{2}^{2}+\gamma_{3}^{2}=1 without loss of generality. Therefore, γ12+γ221\gamma_{1}^{2}+\gamma_{2}^{2}\leq 1.

We turn to the VoV^{o} interaction:

Ho=1Ω𝒌,𝒌Vαβγδo(𝒌,𝒌)c𝒌αc𝒌βc𝒌γc𝒌δ.\displaystyle H_{o}=\frac{1}{\Omega}\sum_{\boldsymbol{k},\boldsymbol{k}^{\prime}}V^{o}_{\alpha\beta\gamma\delta}(\boldsymbol{k},\boldsymbol{k}^{\prime})c^{\dagger}_{\boldsymbol{k}\alpha}c^{\dagger}_{-\boldsymbol{k}\beta}c_{-\boldsymbol{k}^{\prime}\gamma}c_{\boldsymbol{k}^{\prime}\delta}. (16)

We will decompose HoH_{o} into different odd-parity pairing channels, which are classified into different representation of the point group and generally take the form:

F^a(i)=12𝒌,αβc𝒌α[Γa(i)(𝒌)ϵ]αβc𝒌β.\hat{F}_{a}^{(i)\dagger}=\frac{1}{2}\sum_{\boldsymbol{k},\alpha\beta}c^{\dagger}_{\boldsymbol{k}\alpha}[\Gamma_{a}^{(i)}(\boldsymbol{k})\epsilon]_{\alpha\beta}c^{\dagger}_{-\boldsymbol{k}\beta}. (17)

The form factor Γa\Gamma_{a} can be classified in the same way as those used in the particle-hole channel, which are listed in Table 1. We use subscript a=1a=1 and 22 to stand for A1uA_{1u} and A2uA_{2u} representation respectively, and a=xa=x and yy to denote the two components in EuE_{u} representation. The superscript ii enumerates different basis functions within the same representation.

HoH_{o} decomposed in terms of F^a(i)\hat{F}_{a}^{(i)\dagger} has the form:

Ho=\displaystyle H_{o}= V0Ω{(γ1F^1(1)2γ2F^1(2))(γ1F^1(1)2γ2F^1(2))\displaystyle\frac{V_{0}}{\Omega}\Big{\{}-(\gamma_{1}\hat{F}_{1}^{(1)}-\sqrt{2}\gamma_{2}\hat{F}_{1}^{(2)})^{\dagger}(\gamma_{1}\hat{F}_{1}^{(1)}-\sqrt{2}\gamma_{2}\hat{F}_{1}^{(2)}) (18)
γ12F^2(1)F^2(1)+a=x,yi,jF^a(i)𝒲ijF^a(j)},\displaystyle-\gamma_{1}^{2}\hat{F}_{2}^{(1)\dagger}\hat{F}_{2}^{(1)}+\sum_{a=x,y}\sum_{i,j}\hat{F}_{a}^{(i)\dagger}\mathcal{W}_{ij}\hat{F}_{a}^{(j)}\Big{\}},

where the coefficient matrix 𝒲\mathcal{W} is symmetric and real:

𝒲=(γ12γ32γ1γ22γ1γ3γ1γ202γ2γ32γ1γ32γ2γ3γ12).\mathcal{W}=\begin{pmatrix}\gamma_{1}^{2}-\gamma_{3}^{2}&\gamma_{1}\gamma_{2}&2\gamma_{1}\gamma_{3}\\ \gamma_{1}\gamma_{2}&0&2\gamma_{2}\gamma_{3}\\ 2\gamma_{1}\gamma_{3}&2\gamma_{2}\gamma_{3}&-\gamma_{1}^{2}\end{pmatrix}. (19)

Because V0<0V_{0}<0, the interaction is repulsive for A1uA_{1u} and A2uA_{2u} pairing channels in HoH_{o} so there is no superconductivity instability in these two channels.

We diagonalize the matrix 𝒲\mathcal{W} to decompose the EuE_{u} channels:

i,jF^a(i)𝒲ijF^a(j)=ν=13wν[iλi(ν)F^a(i)][jλj(ν)F^a(j)],\displaystyle\sum_{i,j}\hat{F}_{a}^{(i)\dagger}\mathcal{W}_{ij}\hat{F}_{a}^{(j)}=\sum_{\nu=1}^{3}w_{\nu}\big{[}\sum_{i}\lambda_{i}^{(\nu)}\hat{F}_{a}^{(i)}\big{]}^{\dagger}\big{[}\sum_{j}\lambda_{j}^{(\nu)}\hat{F}_{a}^{(j)}\big{]}, (20)

where wνw_{\nu} represents the ν\nuth largest eigenvalue of 𝒲\mathcal{W} and (λ1(ν),λ2(ν),λ3(ν))(\lambda_{1}^{(\nu)},\lambda_{2}^{(\nu)},\lambda_{3}^{(\nu)}) is the corresponding normalized eigenvector. We find that w10w_{1}\geq 0 and w2,30w_{2,3}\leq 0. w1w_{1} is generically positive, and it is zero only when γ1,2=0\gamma_{1,2}=0 or γ1,3=0\gamma_{1,3}=0. Therefore, there is generally one attractive EuE_{u} pairing channel and two repulsive EuE_{u} channels. Furthermore, the three EuE_{u} channels are decoupled in the linearized gap equation because (1) different eigenvectors of 𝒲\mathcal{W} are orthogonal and (2) different form factors are orthogonal over the Fermi surface and have the same normalization for the Fermi surface average:

12Tr[Γa(i)(𝒌)Γa(i)(𝒌)]=13δaaδii.\langle\frac{1}{2}\text{Tr}[\Gamma_{a}^{(i)}(\boldsymbol{k})\Gamma_{a^{\prime}}^{(i^{\prime})}(\boldsymbol{k})]\rangle=\frac{1}{3}\delta_{aa^{\prime}}\delta_{ii^{\prime}}. (21)

We focus on the attractive EuE_{u} channel as summarized in the following:

H~o\displaystyle\tilde{H}_{o} =w1V0Ω(ΛxΛx+ΛyΛy),\displaystyle=\frac{w_{1}V_{0}}{\Omega}(\Lambda_{x}^{\dagger}\Lambda_{x}+\Lambda_{y}^{\dagger}\Lambda_{y}), (22)
Λa\displaystyle\Lambda_{a}^{\dagger} =iλi(1)F^a(i)=12𝒌,αβc𝒌α[ga(𝒌)ϵ]αβc𝒌β,\displaystyle=\sum_{i}\lambda_{i}^{(1)}\hat{F}_{a}^{(i)\dagger}=\frac{1}{2}\sum_{\boldsymbol{k},\alpha\beta}c^{\dagger}_{\boldsymbol{k}\alpha}[g_{a}(\boldsymbol{k})\epsilon]_{\alpha\beta}c^{\dagger}_{-\boldsymbol{k}\beta},

where we have introduced matrices gx,yg_{x,y} that are defined as ga(𝒌)=iλi(1)Γa(i)g_{a}(\boldsymbol{k})=\sum_{i}\lambda_{i}^{(1)}\Gamma_{a}^{(i)}. The corresponding linearized gap equation is:

|V0|χp(Tc,p)=1,\displaystyle|V_{0}|\chi_{p}(T_{c,p})=1, (23)
χp(T)=w112Tr[gx(𝒌)]2χ0(T)=w13χ0(T),\displaystyle\chi_{p}(T)=w_{1}\langle\frac{1}{2}\text{Tr}[g_{x}(\boldsymbol{k})]^{2}\rangle\chi_{0}(T)=\frac{w_{1}}{3}\chi_{0}(T),

where Tc,pT_{c,p} is the critical temperature for the EuE_{u} channel. χp(T)\chi_{p}(T) remains the same if gx(𝒌)g_{x}(\boldsymbol{k}) is replaced by gy(𝒌)g_{y}(\boldsymbol{k}) in its expression, which is a result of the discrete lattice rotational symmetry.

As a summary, the EuE_{u} phonon generates superconductivity instability in both ss-wave channel and EuE_{u} channel. We find that χp(T)\chi_{p}(T) is always weaker compared to χs(T)\chi_{s}(T) when U=0U=0 (Fig. 1(a)), which means ss-wave has higher critical temperature in this case. Nevertheless, χp(T)\chi_{p}(T) can reach about 0.5χs(T)0.5\chi_{s}(T) in a large parameter space of γi\gamma_{i}, indicating that the EuE_{u} pairing instability can be strong. As UU increases, χs(T)\chi_{s}(T) decreases while χp(T)\chi_{p}(T) does not change. We can define a critical UcU_{c} at which χp(T)=χs(T)\chi_{p}(T)=\chi_{s}(T). The ss-wave and odd-parity EuE_{u} superconductivity have larger instability temperature below and above UcU_{c}, respectively. The phase diagram as a function of UU and γi\gamma_{i} is summarized in Fig. 1(b).

We note that other phonon modes, which are not included in our model, generally produce attractive interaction in ss-wave channel, but not necessarily in EuE_{u} channel. Some particular phonon modes, for example A2uA_{2u} modes discussed in Appendix C, can even have pair-breaking effects for EuE_{u} channel. Therefore, the value of UcU_{c} obtained from our model should be viewed as a lower bound of the critical repulsive interaction.

Assuming U>UcU>U_{c}, the EuE_{u} superconductivity pairing is realized below Tc,pT_{c,p}. As a two-component superconductivity, EuE_{u} pairing generally has two forms: nematic and chiral. To determine which one is realized, we study the Ginzburg-Landau free energy up to fourth order in the EuE_{u} pairing order parameter (ηx,ηy)(\eta_{x},\eta_{y}):

p=\displaystyle\mathcal{F}_{p}= r1(|ηx|2+|ηy|2)+b1(|ηx|2+|ηy|2)2\displaystyle\,\,\,\,\,\,\,r_{1}(|\eta_{x}|^{2}+|\eta_{y}|^{2})+b_{1}(|\eta_{x}|^{2}+|\eta_{y}|^{2})^{2} (24)
+b2|ηx2+ηy2|2,\displaystyle+b_{2}|\eta_{x}^{2}+\eta_{y}^{2}|^{2},

where the parameters r1r_{1} and b1,2b_{1,2} can be fully determined by the interaction H~o\tilde{H}_{o} under the weak-coupling analysis:

r1\displaystyle r_{1} =1w1|V0|(1|V0|χp),\displaystyle=\frac{1}{w_{1}|V_{0}|}(1-|V_{0}|\chi_{p}), (25)
b1\displaystyle b_{1} =Tr[gx2(𝒌)gy2(𝒌)]β0,\displaystyle=\langle\text{Tr}[g_{x}^{2}(\boldsymbol{k})g_{y}^{2}(\boldsymbol{k})]\rangle\beta_{0},
b2\displaystyle b_{2} =12Tr[gx(𝒌)gy(𝒌)]2β0,\displaystyle=\frac{1}{2}\langle\text{Tr}[g_{x}(\boldsymbol{k})g_{y}(\boldsymbol{k})]^{2}\rangle\beta_{0},

where β0=7ζ(3)N(0)/(16π2T2)\beta_{0}=7\zeta(3)N(0)/(16\pi^{2}T^{2}) and ζ(x)\zeta(x) is the Riemann zeta function. Here b1b_{1} is always positive, but the sign of b2b_{2} can vary as a function of γi\gamma_{i}. When b2<0b_{2}<0, a nematic state with real order parameter (ηx,ηy)(cosθ,sinθ)(\eta_{x},\eta_{y})\propto(\cos\theta,\sin\theta) is favored. Here the angle θ\theta characterizes the nematic direction, and its value is arbitrary for the free energy p\mathcal{F}_{p} that only includes terms up to fourth order. For the case of b2>0b_{2}>0, a chiral state with complex order parameter (ηx,ηy)(1,±i)(\eta_{x},\eta_{y})\propto(1,\pm i) is favored. The nematic and chiral states respectively break the lattice rotational symmetry and time reversal symmetry. The phase boundary (b2=0b_{2}=0) between the nematic and chiral states is shown in Fig. 1(b), indicating a large parameter space in which nematic state is more favorable. It is intriguing that phononic mechanism can induce time-reversal-breaking chiral superconductivity. The competition between nematic and chiral states has been studied as a function of λi(1)\lambda_{i}^{(1)} in Ref. Venderbos et al., 2016b. Our work reveals that λi(1)\lambda_{i}^{(1)} can be derived from parameters γi\gamma_{i}, the latter of which could be extracted from ab inito study of electron-phonon interactions.

III Coexistence of even and odd parity superconductivity

Refer to caption
Figure 2: Schematic phase diagram as a function of repulsive interaction UU (ss-wave channel) and temperature TT. In the vicinity of UcU_{c} where ss-wave and nematic superconductivity have the same instability temperature, there is a phase where both types of superconductivity coexist with a relative phase difference ±π/2\pm\pi/2.

At U=UcU=U_{c}, the ss-wave and EuE_{u} channel have the same critical temperature Tc,s=Tc,p=TcT_{c,s}=T_{c,p}=T_{c}^{*}. To pin down the nature of the superconductivity below TcT_{c}^{*}, we study the Ginzburg-Landau free energy that includes both ss-wave and EuE_{u} pairing order parameters:

=\displaystyle\mathcal{F}= s+p+sp\displaystyle\mathcal{F}_{s}+\mathcal{F}_{p}+\mathcal{F}_{sp} (26)
s=\displaystyle\mathcal{F}_{s}= r0|ηs|2+b0|ηs|4\displaystyle r_{0}|\eta_{s}|^{2}+b_{0}|\eta_{s}|^{4}
sp=\displaystyle\mathcal{F}_{sp}= b3{4(|ηx|2+|ηy|2)|ηs|2\displaystyle b_{3}\big{\{}4(|\eta_{x}|^{2}+|\eta_{y}|^{2})|\eta_{s}|^{2}
+[(ηx2+ηy2)ηs2+c.c.]},\displaystyle\quad+[(\eta_{x}^{2}+\eta_{y}^{2})\eta_{s}^{*2}+c.c.]\big{\}},

where s\mathcal{F}_{s} is the free energy for ss-wave pairing characterized by the order parameter ηs\eta_{s}, p\mathcal{F}_{p} is give in (24) and sp\mathcal{F}_{sp} describes the coupling between ss-wave and EuE_{u} pairings. Parameters in the free energy are again obtained using weak-coupling analysis: r0=2κ(1|V0|χs)/|V0|r_{0}=2\kappa(1-|V_{0}|\chi_{s})/|V_{0}|, b0=12Tr[g0(𝒌)s0]4β0b_{0}=\frac{1}{2}\langle\text{Tr}[g_{0}(\boldsymbol{k})s_{0}]^{4}\rangle\beta_{0} and b3=12Tr[gx2(𝒌)g02(𝒌)]β0b_{3}=\frac{1}{2}\langle\text{Tr}[g_{x}^{2}(\boldsymbol{k})g_{0}^{2}(\boldsymbol{k})]\rangle\beta_{0}. Here b0b_{0} and b3b_{3} are always positive.

To minimize \mathcal{F} below TcT_{c}^{*} at U=UcU=U_{c}, it is most instructive to consider the case b2<0b_{2}<0. \mathcal{F} is then minimized by a state where the ss-wave and nematic superconductivity coexist and have a relative phase difference ±π/2\pm\pi/2, i.e. ηs=±i|ηs|\eta_{s}=\pm i|\eta_{s}| and (ηx,ηy)=|ηp|(cosθ,sinθ)(\eta_{x},\eta_{y})=|\eta_{p}|(\cos\theta,\sin\theta). |ηs||\eta_{s}| and |ηp||\eta_{p}| are given by:

|ηs|2\displaystyle|\eta_{s}|^{2} =r0(b1+b2)+r1b32[b0(b1+b2)b32],\displaystyle=\frac{-r_{0}(b_{1}+b_{2})+r_{1}b_{3}}{2[b_{0}(b_{1}+b_{2})-b_{3}^{2}]}, (27)
|ηp|2\displaystyle|\eta_{p}|^{2} =r1b0+r0b32[b0(b1+b2)b32].\displaystyle=\frac{-r_{1}b_{0}+r_{0}b_{3}}{2[b_{0}(b_{1}+b_{2})-b_{3}^{2}]}.

The coexistence of the two superconductivity order parameters requires the expressions for |ηs|2|\eta_{s}|^{2} and |ηp|2|\eta_{p}|^{2} in (27) to be positive, which we find to be generally satisfied in the γi\gamma_{i} parameter space.

When UU is away from UcU_{c}, the coexistence state can still develop, but at a temperature lower than Tc,sT_{c,s} when U<UcU<U_{c} or Tc,pT_{c,p} when U>UcU>U_{c}. The schematic phase diagram as a function of UU and TT is shown in Fig. 2. This coexistence phase not only breaks lattice discrete rotational symmetry because of the presence of nematic order parameter, but also breaks time reversal symmetry because of the relative phase difference ±π/2\pm\pi/2 between the even and odd parity order parameters.

In the case of b2>0b_{2}>0, there can also be an intermediate phase between ss-wave and chiral phases in the vicinity of UcU_{c}. This intermediate phase is characterized by non-zero order parameters (ηs,η+,η)(\eta_{s},\eta_{+},\eta_{-}), where η±=ηx±iηy\eta_{\pm}=\eta_{x}\pm i\eta_{y}. |η+||\eta_{+}| and |η||\eta_{-}| are generally unequal so both time reversal and discrete rotational symmetries are also broken.

We now discuss gap structures in different phases. In the ss-wave phase, the superconductivity gap is proportional to g+(𝒌)g_{+}(\boldsymbol{k}) on the Fermi surface, which is fully gapped for weak repulsion UU.

To study gap structure in the nematic phase, we express ga(𝒌)g_{a}(\boldsymbol{k}) for a=xa=x and yy in terms of a vector:

ga(𝒌)=𝒅a(𝒌)𝒔.g_{a}(\boldsymbol{k})=\boldsymbol{d}_{a}(\boldsymbol{k})\cdot\boldsymbol{s}. (28)

For order parameter (ηx,ηy)(\eta_{x},\eta_{y}) given by |ηp|(cosθ,sinθ)|\eta_{p}|(\cos\theta,\sin\theta), the gap is proportional to |𝒅||\boldsymbol{d}| on the Fermi surface, where the vector 𝒅\boldsymbol{d} is defined as cosθ𝒅x+sinθ𝒅y\cos\theta\boldsymbol{d}_{x}+\sin\theta\boldsymbol{d}_{y}. |𝒅||\boldsymbol{d}| is finite everywhere on the Fermi surface unless θ=nπ/3\theta=n\pi/3 (integer nn takes value from 0 to 5). The nematic phase realizes a fully gapped topological superconductor when θnπ/3\theta\neq n\pi/3, as it has odd parity pairing and the Fermi surface encloses only one time reversal invariant momentumFu and Berg (2010). A hallmark of a time-reversal invariant topological superconductor is that it supports Majorana modes bound to surfaces and time-reversal-invariant vortex defectsQi et al. (2009); Wu and Martin (2017). When θ=nπ/3\theta=n\pi/3, the nematic pairing preserves one of the mirror symmetries and the gap vanishes at two opposite momenta located on the corresponding mirror-invariant plane in the Brillouin zoneFu (2014). Therefore, the nematic phase with θ=nπ/3\theta=n\pi/3 realizes a topological Dirac superconductor with Dirac point nodes in the bulk and Majorana arcs on certain surfacesYang et al. (2014).

In the coexistence phase where ss-wave and nematic order parameter has a phase difference ±π/2\pm\pi/2, the Bogoliubov-de Gennes Hamiltonian is:

(𝒌)=ε0(𝒌)τz+|ηp|[𝒅(𝒌)𝒔]τx+|ηs|g+(𝒌)τy,\mathcal{H}(\boldsymbol{k})=\varepsilon_{0}(\boldsymbol{k})\tau_{z}+|\eta_{p}|[\boldsymbol{d}(\boldsymbol{k})\cdot\boldsymbol{s}]\tau_{x}+|\eta_{s}|g_{+}(\boldsymbol{k})\tau_{y}, (29)

which is expressed in the basis (c𝒌,c𝒌,c𝒌,c𝒌)(c_{\boldsymbol{k}\uparrow}^{\dagger},c_{\boldsymbol{k}\downarrow}^{\dagger},c_{-\boldsymbol{k}\downarrow},-c_{-\boldsymbol{k}\uparrow}). ε0(𝒌)=2𝒌2/(2m)μ\varepsilon_{0}(\boldsymbol{k})=\hbar^{2}\boldsymbol{k}^{2}/(2m)-\mu, and τx,y,z\tau_{x,y,z} are Pauli matrices in the Nambu space. Here |ηp||\eta_{p}| and |ηs||\eta_{s}| are respectively coupled to τx\tau_{x} and τy\tau_{y}, reflecting the π/2\pi/2 phase difference. The energy spectrum of (𝒌)\mathcal{H}(\boldsymbol{k}) is ±ε0(𝒌)2+|ηp|2|𝒅(𝒌)|2+|ηs|2g+(𝒌)2\pm\sqrt{\varepsilon_{0}(\boldsymbol{k})^{2}+|\eta_{p}|^{2}|\boldsymbol{d}(\boldsymbol{k})|^{2}+|\eta_{s}|^{2}g_{+}(\boldsymbol{k})^{2}}, which is fully gapped for any value of θ\theta. The surface Majorana zero modes presented in the nematic phase also become gapped in the coexistence phase because of broken time reversal symmetry. Such a state represents a superconducting analog of an axion insulatorQi et al. (2008), and can have thermal Hall effect on the surface. Similar phase with coexistence of even and odd parity pairing have been studied in Ref. Goswami and Roy, 2014 and recently in Ref. Wang and Fu, . A distinct feature of the coexistence phase that we obtain is that it spontaneously breaks discrete rotational symmetry besides time reversal symmetry. We also note an additional symmetry breaking in the coexistence phase. In (29), (𝒌)\mathcal{H}(\boldsymbol{k}) satisfies an inversion symmetry (𝒌)=(𝒌)\mathcal{H}(\boldsymbol{k})=\mathcal{H}(-\boldsymbol{k}) when |ηp|=0|\eta_{p}|=0, or an inversion-gauge symmetry τz(𝒌)τz=(𝒌)\tau_{z}\mathcal{H}(\boldsymbol{k})\tau_{z}=\mathcal{H}(-\boldsymbol{k}) when |ηs|=0|\eta_{s}|=0. In the coexistence phase, neither the inversion nor inversion-gauge symmetry remains.

The chiral phase characterized by (ηx,ηy)(1,±i)(\eta_{x},\eta_{y})\propto(1,\pm i) realizes a topological Weyl superconductor with bulk Weyl point nodes. The nodal structure has been extensively discussed in Refs. Venderbos et al., 2016b and Kozii et al., 2016. When there is some mixing between ss-wave and chiral superconductivity near UcU_{c}, the Weyl points remain robust unless two Weyl points with opposite chiralities meet and annihilate each other.

IV Discussion

We discuss connections between our work and previous studies. Reference Brydon et al., 2014 reached a general conclusion that pure electron-phonon interaction in a system with time-reversal and inversion symmetries can generate odd-parity superconductivity, but its instability temperature can not be larger than that of the ss-wave superconductivity. Our results are consistent with this general statement, and we also show that local Coulomb repulsion can tip the balance in favor of odd-parity pairing. In Ref. Wan and Savrasov, 2014, Wan and Savrasov presented a first principle study of phonon mediated superconductivity in Cu doped Bi2Se3. Encouragingly, they found that pure electron-phonon interaction does generate odd-parity pairings in both EuE_{u} and A2uA_{2u} channels besides the usual even-parity channel. Their calculation indicated that the phonon-mediated instability is stronger in A2uA_{2u} channel compared to EuE_{u} channel. In Appendix A, we show that an on-site repulsive interaction in Bi2Se3 generates repulsion in both the ss-wave channel and A2uA_{2u} channel, but not in EuE_{u} channel. In general a finite-range repulsive interaction could also suppress EuE_{u} pairingFu and Berg (2010). However, the on-site interaction presumably leads to the most dominant repulsion, which could make EuE_{u} pairing more favorable compared to ss-wave and A2uA_{2u} pairings. It is interesting to reexamine electron-phonon interaction in metal doped Bi2Se3 using ab initio calculation. In particular, parameters γi\gamma_{i}, which determine whether nematic or chiral superconductivity is realized in our theory, could be extracted from such a study. In our work, we do not attempt to determine the critical temperature of EuE_{u} superconductivity. Such a task requires a detailed knowledge about electron-phonon interaction, which we leave for ab initio calculation. The study of Wan and SavrasovWan and Savrasov (2014) has shown that the electron-phonon interaction is capable of producing a critical temperature of 353\sim 5 K in the A2uA_{2u} channel.

In summary, we studied odd-parity fluctuations as a possible mechanism for the nematic superconductivity observed in doped Bi2Se3.

V Acknowledgment

F.W. thanks J.W.F. Venderbos for stimulating discussion. We acknowledge support from Department of Energy, Office of Basic Energy Science, Materials Science and Engineering Division.

Appendix A Onsite repulsion in Bi2Se3\text{Bi}_{2}\text{Se}_{3}

In this appendix, we show that an on-site repulsive interaction in Bi2Se3 generates repulsive interaction in ss-wave and A2uA_{2u} pairing channels. We start from a two-orbital kpk\cdot p model of Bi2Se3:

0(𝒌)=Mσx+v(kxs~ykys~x)σz+vzkzσyμ~,\mathcal{H}_{0}(\boldsymbol{k})=M\sigma_{x}+v(k_{x}\tilde{s}_{y}-k_{y}\tilde{s}_{x})\sigma_{z}+v_{z}k_{z}\sigma_{y}-\tilde{\mu}, (30)

where σa\sigma_{a} and s~a\tilde{s}_{a} are Pauli matrices respectively in the orbital and spin spaces. Here μ~\tilde{\mu} and the chemical potential μ\mu in (1) are related by μ~=μ+M\tilde{\mu}=\mu+M. 0(𝒌)\mathcal{H}_{0}(\boldsymbol{k}) is expressed in the basis d𝒌=(d𝒌,1+,d𝒌,1,d𝒌,2+,d𝒌,2)Td_{\boldsymbol{k}}=(d_{\boldsymbol{k},1+},d_{\boldsymbol{k},1-},d_{\boldsymbol{k},2+},d_{\boldsymbol{k},2-})^{\text{T}}, where the subscript 1 and 2 label the two orbitals, and ±\pm are the spin indices. Here the two orbitals are mainly derived from Se pzp_{z} orbitals localized on top and bottom layers of the Bi2Se3 unit cellZhang et al. (2009). The two orbitals are interchanged under inversion operation. 0(𝒌)\mathcal{H}_{0}(\boldsymbol{k}) has four bands, corresponding to the two-fold generate valence bands and another two-fold degenerate conduction bands near the band gap.

We consider an on-site repulsive interaction within each orbital:

HU=2U~Ω𝒑𝒌𝒌σ=1,2d𝒑+𝒌,σ+d𝒑𝒌,σd𝒑𝒌,σd𝒑+𝒌,σ+,H_{U}=\frac{2\tilde{U}}{\Omega}\sum_{\boldsymbol{p}\boldsymbol{k}\boldsymbol{k}^{\prime}}\sum_{\sigma=1,2}d_{\boldsymbol{p}+\boldsymbol{k},\sigma+}^{\dagger}d_{\boldsymbol{p}-\boldsymbol{k},\sigma-}^{\dagger}d_{\boldsymbol{p}-\boldsymbol{k}^{\prime},\sigma-}d_{\boldsymbol{p}+\boldsymbol{k}^{\prime},\sigma+}, (31)

Here U~\tilde{U} is positive for repulsive interaction. We decompose HUH_{U} into BCS channels:

HUU~Ω𝒌,𝒌{[σd𝒌,σd𝒌,σ][σd𝒌,σd𝒌,σ]\displaystyle H_{U}\approx\frac{\tilde{U}}{\Omega}\sum_{\boldsymbol{k},\boldsymbol{k}^{\prime}}\Big{\{}[\sum_{\sigma}d_{\boldsymbol{k},\sigma\uparrow}^{\dagger}d_{-\boldsymbol{k},\sigma\downarrow}^{\dagger}][\sum_{\sigma^{\prime}}d_{-\boldsymbol{k}^{\prime},\sigma^{\prime}\downarrow}d_{\boldsymbol{k}^{\prime},\sigma^{\prime}\uparrow}] (32)
+[σσz(σσ)d𝒌,σd𝒌,σ][σσz(σσ)d𝒌,σd𝒌,σ]},\displaystyle+[\sum_{\sigma}\sigma_{z}^{(\sigma\sigma)}d_{\boldsymbol{k},\sigma\uparrow}^{\dagger}d_{-\boldsymbol{k},\sigma\downarrow}^{\dagger}][\sum_{\sigma^{\prime}}\sigma_{z}^{(\sigma^{\prime}\sigma^{\prime})}d_{-\boldsymbol{k}^{\prime},\sigma^{\prime}\downarrow}d_{\boldsymbol{k}^{\prime},\sigma^{\prime}\uparrow}]\Big{\}},

where the first and second line respectively represent even and odd parity pairing channels. Finally we project them to the conduction bandsVenderbos et al. (2016b)

𝒌,σd𝒌,1d𝒌,1+d𝒌,2d𝒌,2\displaystyle\sum_{\boldsymbol{k},\sigma}d_{\boldsymbol{k},1\uparrow}^{\dagger}d_{-\boldsymbol{k},1\downarrow}^{\dagger}+d_{\boldsymbol{k},2\uparrow}^{\dagger}d_{-\boldsymbol{k},2\downarrow}^{\dagger} (33)
\displaystyle\approx 12𝒌αβc𝒌αϵαβc𝒌β,\displaystyle\frac{1}{2}\sum_{\boldsymbol{k}}\sum_{\alpha\beta}c_{\boldsymbol{k}\alpha}^{\dagger}\epsilon_{\alpha\beta}c_{-\boldsymbol{k}\beta}^{\dagger},
𝒌,σd𝒌,1d𝒌,1d𝒌,2d𝒌,2\displaystyle\sum_{\boldsymbol{k},\sigma}d_{\boldsymbol{k},1\uparrow}^{\dagger}d_{-\boldsymbol{k},1\downarrow}^{\dagger}-d_{\boldsymbol{k},2\uparrow}^{\dagger}d_{-\boldsymbol{k},2\downarrow}^{\dagger}
\displaystyle\approx 12𝒌αβc𝒌α[vμ~(kxsykysx)ϵ]αβc𝒌β.\displaystyle\frac{1}{2}\sum_{\boldsymbol{k}}\sum_{\alpha\beta}c_{\boldsymbol{k}\alpha}^{\dagger}[\frac{v}{\tilde{\mu}}(k_{x}s_{y}-k_{y}s_{x})\epsilon]_{\alpha\beta}c_{-\boldsymbol{k}\beta}^{\dagger}.

By looking up Table 1, it is clear that the odd-parity pairing in (33) belongs to A2uA_{2u} representation.

Appendix B Odd-parity fluctuation in A1uA_{1u} representation

In Bi2Se3, there is no Brillouin-zone-center phonon mode in A1uA_{1u} representationWang and Zhang (2012). Nevertheless, we can still theoretically study superconductivity induced by odd-parity particle-hole fluctuation in A1uA_{1u} representation. The procedure is parallel to that presented in Sec. II. The main difference is the form factor:

Γ1(𝒌)=γ1Γ1(1)(𝒌)+γ2Γ1(2)(𝒌),\Gamma_{1}(\boldsymbol{k})=\gamma_{1}\Gamma_{1}^{(1)}(\boldsymbol{k})+\gamma_{2}\Gamma_{1}^{(2)}(\boldsymbol{k}), (34)

where Γ1(1)(𝒌)\Gamma_{1}^{(1)}(\boldsymbol{k}) and Γ1(2)(𝒌)\Gamma_{1}^{(2)}(\boldsymbol{k}), given in Table 1, are two basis functions in A1uA_{1u} representation up to first order in 𝒌\boldsymbol{k}.

The effective interaction induced by A1uA_{1u} fluctuation can again be decomposed into even and odd parity pairing channels:

He=\displaystyle H_{e}= V0Ω𝒌,𝒌[g0(𝒌)+g0(𝒌)][12ϵαβc𝒌αc𝒌β][12ϵγδc𝒌γc𝒌δ],\displaystyle\frac{V_{0}}{\Omega}\sum_{\boldsymbol{k},\boldsymbol{k}^{\prime}}[g_{0}(\boldsymbol{k})+g_{0}(\boldsymbol{k}^{\prime})][\frac{1}{2}\epsilon_{\alpha\beta}c^{\dagger}_{\boldsymbol{k}\alpha}c^{\dagger}_{-\boldsymbol{k}\beta}][\frac{1}{2}\epsilon^{\dagger}_{\gamma\delta}c_{-\boldsymbol{k}^{\prime}\gamma}c_{\boldsymbol{k}^{\prime}\delta}], (35)
Ho=\displaystyle H_{o}= V0Ω{(γ1F^1(1)+γ2F^1(2))(γ1F^1(1)+γ2F^1(2))\displaystyle\frac{V_{0}}{\Omega}\Big{\{}(\gamma_{1}\hat{F}_{1}^{(1)}+\gamma_{2}\hat{F}_{1}^{(2)})^{\dagger}(\gamma_{1}\hat{F}_{1}^{(1)}+\gamma_{2}\hat{F}_{1}^{(2)})
\displaystyle- γ12F^2(1)F^2(1)\displaystyle\gamma_{1}^{2}\hat{F}_{2}^{(1)\dagger}\hat{F}_{2}^{(1)}
\displaystyle- a=x,y(γ12F^a(1)γ2F^a(2))(γ12F^a(1)γ2F^a(2))},\displaystyle\sum_{a=x,y}(\frac{\gamma_{1}}{\sqrt{2}}\hat{F}_{a}^{(1)}-\gamma_{2}\hat{F}_{a}^{(2)})^{\dagger}(\frac{\gamma_{1}}{\sqrt{2}}\hat{F}_{a}^{(1)}-\gamma_{2}\hat{F}_{a}^{(2)})\Big{\}},

where HeH_{e} describes attractive interaction in even-parity channel, and the form factor is g0(𝒌)=γ12(k^x2+k^y2)/4+γ22k^z2g_{0}(\boldsymbol{k})=\gamma_{1}^{2}(\hat{k}_{x}^{2}+\hat{k}_{y}^{2})/4+\gamma_{2}^{2}\hat{k}_{z}^{2}/2, which does not include repulsive interaction in the ss-wave channel. In HoH_{o} of Eq. (35), A1uA_{1u} pairing channel has attractive interaction, while the other two odd-parity channels are repulsive.

The critical temperature in the even-parity and odd-parity A1uA_{1u} channels are separately given by the corresponding linearized gap equations:

|V0|χs(Tc,s)=1,|V0|χp(Tc,p)=1,\displaystyle|V_{0}|\chi_{s}(T_{c,s})=1,\quad\quad|V_{0}|\chi_{p}(T_{c,p})=1, (36)
χs(T)χ0(T)=γ12+γ226+160(2γ14+2γ12γ22+3γ24),\displaystyle\frac{\chi_{s}(T)}{\chi_{0}(T)}=\frac{\gamma_{1}^{2}+\gamma_{2}^{2}}{6}+\sqrt{\frac{1}{60}(2\gamma_{1}^{4}+2\gamma_{1}^{2}\gamma_{2}^{2}+3\gamma_{2}^{4})},
χp(T)χ0(T)=γ12+γ223.\displaystyle\frac{\chi_{p}(T)}{\chi_{0}(T)}=\frac{\gamma_{1}^{2}+\gamma_{2}^{2}}{3}.

The ratio χp/χs\chi_{p}/\chi_{s} takes its minimum value 0.85 when γ1=0\gamma_{1}=0, and its maximum value 1 when γ1/γ2=2\gamma_{1}/\gamma_{2}=\sqrt{2}. Therefore, ss-wave and A1uA_{1u} pairings can have the same critical temperature even without considering the repulsive interaction in the ss-wave channelKozii and Fu (2015); Wang et al. (2016); Wang and Fu .

Appendix C Odd-parity fluctuation in A2uA_{2u} representation

There are A2uA_{2u} phonon modes at the Brillouin zone center in Bi2Se3. The corresponding form factor has only one basis function to linear order in 𝒌\boldsymbol{k}:

Γ2(𝒌)=γ1Γ2(1)(𝒌)=γ12(k^xsyk^ysx).\Gamma_{2}(\boldsymbol{k})=\gamma_{1}\Gamma_{2}^{(1)}(\boldsymbol{k})=\frac{\gamma_{1}}{\sqrt{2}}(\hat{k}_{x}s_{y}-\hat{k}_{y}s_{x}). (37)

In the effective interaction, the even-parity part HeH_{e} takes similar form as that in (35), but the form factor go(𝒌)g_{o}(\boldsymbol{k}) is replaced by γ12(k^x2+k^y2)/4\gamma_{1}^{2}(\hat{k}_{x}^{2}+\hat{k}_{y}^{2})/4. The odd-parity part HoH_{o} is given by:

Ho=γ12V0Ω{\displaystyle H_{o}=\frac{\gamma_{1}^{2}V_{0}}{\Omega}\Big{\{} F^1(1)F^1(1)+F^2(1)F^2(1)\displaystyle-\hat{F}_{1}^{(1)\dagger}\hat{F}_{1}^{(1)}+\hat{F}_{2}^{(1)\dagger}\hat{F}_{2}^{(1)} (38)
12a=x,yF^a(1)F^a(1)},\displaystyle-\frac{1}{2}\sum_{a=x,y}\hat{F}_{a}^{(1)\dagger}\hat{F}_{a}^{(1)}\Big{\}},

where only the A2uA_{2u} pairing channel has an attractive interaction.

The linearized gap equations for even-parity and A2uA_{2u} channels are respectively expressed as:

γ12|V0|χs(Tc,s)=1,γ12|V0|χp(Tc,p)=1,\displaystyle\gamma_{1}^{2}|V_{0}|\chi_{s}(T_{c,s})=1,\quad\quad\gamma_{1}^{2}|V_{0}|\chi_{p}(T_{c,p})=1, (39)
χs(T)χ0(T)=16+130,χp(T)χ0(T)=13.\displaystyle\frac{\chi_{s}(T)}{\chi_{0}(T)}=\frac{1}{6}+\sqrt{\frac{1}{30}},\quad\frac{\chi_{p}(T)}{\chi_{0}(T)}=\frac{1}{3}.

Here the ratio χp/χs\chi_{p}/\chi_{s} is about 0.95, indicating that the critical temperature for the two channels can be comparable. For simplicity, the gap equations in (39) do not include the repulsive interaction discussed in Appendix A.

References