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Kondo Lattice model for field induced triplet pairing in CeRh2_2As2_2

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Abstract

Spin triplet superconductors are of interest because of their topological properties, and their robustness to high magnetic fields. CeRh2_2As2_2 is a unique heavy fermion superconductor with both even-parity and candidate odd-parity superconducting phases with a special feature enabling a field induced phase transition between the two. The field induced transition which switches the parity of the Cooper pairs is enabled by a staggered antisymmetric spin orbit coupling (ASOC) interaction. However, the heavy fermion origins of the superconductivity in CeRh2_2As2_2 and the origin of the antisymmetric spin-orbit coupling are currently unexplored. Here, we develop a Kondo lattice model for CeRh2_2As2_2 and demonstrate how local hybridization between Cerium dd- and ff-orbitals, driven by the locally broken inversion symmetry, at the Cerium sites generates the ASOC. The resulting Kondo lattice model leads to nearly degenerate even and odd parity superconducting states that display a field induced parity transition between an even-parity state and an odd-parity pseudospin triplet state. We discuss the wider implications of our results extended to other heavy fermion systems like CeSiI.

Introduction

The possibility of superconductivity that survives strong magnetic fields has renewed interest in odd-parity and spin-triplet pairing, not least because some such states may possess nontrivial topological properties. In spin orbit coupled materials, however, the physical spin of a Cooper pair need not coincide with the pseudospin character of the gap projected onto the low energy quasiparticle bands. This distinction is especially important in multiband heavy fermion superconductors, where crystal symmetry and strong electronic correlations act together to determine the pairing state.

The heavy fermion compound CeRh2_2As2_2 exhibits a field-driven transition between two superconducting phases [1, 2]. For a magnetic field along the crystallographic cc axis, the low field SC1 phase gives way to a high field SC2 phase near 4 T, while superconductivity persists to an upper critical field of approximately 14 T, far above the conventional weak coupling Pauli scale for Tc≃0.3T_{\mathrm{c}} \simeq0.3 K. The pronounced contrast in field response motivates the interpretation of SC1 and SC2 as competing even and odd parity states, although the microscopic spin structure of the high field phase remains an active question [3].

A key feature of CeRh2_2As2_2 is that its crystal is globally inversion symmetric but the two Ce sites within a unit cell each lack a local inversion center. Inversion exchanges the Ce sublattices, allowing a staggered antisymmetric spin orbit coupling (ASOC) whose sign alternates between the layers. Symmetry based descriptions have shown how this structure can stabilize uniform even-parity and staggered odd parity superconducting states and allow a magnetic field to favor the latter [4, 5, 6]. The corresponding pairing patterns are illustrated in Figure 1.

Crystal structure of CeRh2As2 and uniform and staggered pairing possibilities

Figure 1. Left: the crystal structure of CeRh2_2As2_2 which crystallises in a tetragonal P4/nmmP4/nmm structure. The inversion center is represented by a red cross in between two distinct Ce atoms leading to a unit cell with two atoms. These are the Ce(A) and Ce(B) which are related to one another by inversion. There is the electric potential coming from the Rh atoms depicted by green arrows. Right: the two pairing possibilities stabilized by staggered ASOC interaction. The Δα0\Delta\alpha_0 is the uniform solution which has the same sign pairing gap and Δα3\Delta\alpha_3 is the staggered solution which has a modulated pairing gap on alternating layers. Here, Δ\Delta is the pairing gap magnitude and αm\alpha_m is the sublattice degree of freedom where m=0,3m = 0, 3 which are the Pauli matrices.

Several theoretical approaches have clarified the competition between superconducting states in locally non-centrosymmetric systems. Möckli and Ramires [7] analyzed both even to odd and odd to odd field driven transitions within a two sublattice description, while Cavanagh et al. [4] emphasized the role of nonsymmorphic symmetry and the associated momentum dependent spin orbit structure. Nogaki and Yanase [8] demonstrated that electronic correlations can enhance the parity transition field. Extending the description to vortex degrees of freedom, Minamim and Yanase [9, 10] investigated the parity transition and possible unconventional vortex textures.

Recent microscopic studies provide complementary perspectives on the pairing mechanism. Lee, Agterberg, and Brydon [11] found competing superconducting instabilities of opposite parity and spin density wave tendencies associated with type-II van Hove singularities. Nogaki and Yanase [12], using a multiorbital Dirac–Anderson model, identified leading B1uB_{1u} and B2gB_{2g} superconducting instabilities influenced by quantum geometry and correlations. The appearance of a B1uB_{1u} channel provides a useful symmetry level comparison with the leading projected gap discussed below, although the microscopic origins and orbital structures of the states need not coincide. Work on the coexistence of magnetic order and superconductivity [13] further underscores the importance of the nearby ordered phases.

More recently, Ishizuka et al. [14] investigated the superconducting symmetry and possible topological properties of CeRh2_2As2_2 using realistic electronic structure calculations and crystalline symmetry analysis. In particular, their classification accommodates staggered spin singlet pairing in an odd parity representation, including a dx2−y2d_{x^2-y^2}-type form factor in the BuB_u sector appropriate to a field along the cc axis. This provides a useful symmetry benchmark for a microscopic theory. The symmetry classification alone, however, does not determine how the staggered ASOC is generated in a heavy fermion Kondo lattice, or how the corresponding odd parity gap develops on the heavy quasiparticle Fermi surface.

These questions are sharpened by the strongly correlated normal state. The Curie–Weiss susceptibility, the onset of coherent transport on the Kondo scale, and the large superconducting specific heat anomaly indicate the importance of local moments and heavy quasiparticles [1, 2, 15]. Neutron measurements also reveal pronounced quasi-two-dimensional antiferromagnetic fluctuations [16], which naturally motivate predominantly intralayer dd-wave spin singlet pairing. The challenge is to understand how such pairing can develop in a Kondo lattice with antiferromagnetic interactions, while also giving rise to an odd parity pseudospin triplet gap in the high field phase.

Here we construct a minimal Kondo lattice description in which local inversion symmetry breaking permits an additional onsite hybridization channel. Interference between this channel and the conventional intersite hybridization generates a staggered ASOC for the heavy quasiparticles. We then study the competition between uniform and staggered intralayer pairing states in a magnetic field, determining their phase boundary by comparing the self-consistent free energies. The staggered physical spin singlet order parameter acquires an effective odd parity pseudospin triplet structure upon projection onto the heavy bands. Its leading momentum dependence is compatible with the BuB_u symmetry class discussed by Ishizuka et al., while our calculation identifies a microscopic route to that structure.

The paper is organized as follows. Section II introduces the crystal symmetries and the uniform and staggered pairing channels. Section III develops the local parity breaking hybridization and its symmetry allowed form factors. Section IV constructs the Kondo lattice model and mean-field formulation. Section V presents the emergent ASOC, the field dependent superconducting phase diagram, and the projected pseudospin gap. Section VI discusses the physical interpretation, limitations, and possible extensions to related heavy fermion materials. Technical details of the decoupling and charge conjugation conventions are given in the appendices.

Crystal Symmetry and Pairing

CeRh2_2As2_2 has a tetragonal P4/nmmP4/nmm space group with two Ce atoms per unit cell. Although there is global inversion symmetry, locally, inversion symmetry is broken at the Ce sites due to the alternating RhAs and AsRh layers along the cc axis. The two Ce atoms in the unit cell are related by inversion, as shown in Figure 1. This leads to an additional sublattice degree of freedom and allows a staggered antisymmetric spin orbit coupling (ASOC) interaction of the form:

HASOC=Λα3(sin⁡kyσ1−sin⁡kxσ2),(1)H_{\mathrm{ASOC}} = \Lambda\alpha_3(\sin k_y \sigma_1 - \sin k_x \sigma_2), \tag*{(1)}

where αi\alpha_i and σi\sigma_i are Pauli matrices in sublattice and spin space respectively. The sublattice α3\alpha_3 reverses sign under

sublattice exchange and together with the momentum inversion, preserves global inversion.

In conventional superconductors, the allowed pairing symmetry is determined from the combined parity of spin and momentum which must be antisymmetric. The electron pair wavefunction with fermionic statistics must be antisymmetric upon particle exchange:

Δ(1,2)=−Δ(2,1)(2)\Delta(1,2) = -\Delta(2,1) \tag*{(2)}

where 1={R1,α1,σ1}1 = \{\mathbf{R}_1, \alpha_1, \sigma_1\} and 2={R2,α2,σ2}2 = \{\mathbf{R}_2, \alpha_2, \sigma_2\} represents the position, sublattice, and spin of particle 1 and 2 respectively. Typically, in conventional superconductors with inversion symmetry, the allowed states are momentum even spin singlet or momentum odd spin triplet states. However, CeRh2_2As2_2 has an additional sublattice degree of freedom that enables a new combination of spin, momentum and sublattice. The quasi two dimensional nature of CeRh2_2As2_2 restricts to intralayer dominant pairing within the Ce layers. The symmetry allowed pairing states are given in Table I.

The two pairing solutions allowed by the sublattice is the uniform state which has the same pairing sign on all layers corresponding to an even parity state and the staggered state which has different pairing sign on alternating layers corresponding to an odd parity state. The two disTABLE I. The symmetry allowed pairing states in CeRh2_2As2_2. The total fermionic pair wavefunction must have odd parity upon particle exchange. The pairing wavefunction is given by Δs\Delta_s, where s=A,Bs = A, B which represent pairing within the layers which represent pairing between the same sublattice Ce atoms. The total parity is obtained by the product of the parities which include spin PσP_\sigma, momentum PlP_l, and sublattice PαP_\alpha parity.

SpinPσP_\sigmaMomentumPlP_lSublatticePαP_\alphaP\mathcal{P}Total Parity
Singlet(−)(-)fk=f−kf_{\mathbf{k}} = f_{-\mathbf{k}}(+)(+)ΔA=ΔB\Delta_A = \Delta_B(+)(+)(+)(+)Even
Singlet(−)(-)fk=f−kf_{\mathbf{k}} = f_{-\mathbf{k}}(+)(+)ΔA=−ΔB\Delta_A = -\Delta_B(−)(-)(−)(-)Odd
Triplet(+)(+)dk=−d−k\mathbf{d}_{\mathbf{k}} = -\mathbf{d}_{-\mathbf{k}}(−)(-)ΔA=ΔB\Delta_A = \Delta_B(+)(+)(−)(-)Odd
Triplet(+)(+)dk=−d−k\mathbf{d}_{\mathbf{k}} = -\mathbf{d}_{-\mathbf{k}}(−)(-)ΔA=−ΔB\Delta_A = -\Delta_B(−)(-)(+)(+)Even

tinct solutions are shown in Figure 1. These two states are nearly degenerate in energy and exhibit a field induced transition in the presence of a field applied perpendicular to the plane.

Parity breaking onsite hybridization

A simple model of Ce based heavy fermion systems treats the high energy physics via an Anderson model, describing ff electrons hybridized with a conduction band formed from delocalized dd electrons. The low energy physics is then obtained by carrying out a Schrieffer-Wolff transformation that encodes the physics of the hybridization as a Kondo exchange interaction between the local moments and the conduction sea. If we also include the nearest neighbor RKKY interactions, the resulting Hamiltonian is called a Kondo Heisenberg lattice.

The hybridization between an ff-state and a dd-state is given by the overlap of the wavefunctions with the atomic potentials. The local hybridization is then

Vfd=∫−∞∞d3r ψfσ∗(r)V(r)ψdσ′(r),(3)V_{fd} = \int_{-\infty}^{\infty} d^3 r \, \psi^*_{f\sigma}(\mathbf{r}) V(\mathbf{r}) \psi_{d\sigma'}(\mathbf{r}), \tag*{(3)}

where V(r)V(\mathbf{r}) is the atomic potential at a Cerium site. In locally centrosymmetric systems, the ff-state is odd parity ψfσ(r)=−ψfσ(−r)\psi_{f\sigma}(\mathbf{r}) = -\psi_{f\sigma}(-\mathbf{r}) while the dd-state is even parity ψdσ(r)=+ψdσ(−r)\psi_{d\sigma}(\mathbf{r}) = +\psi_{d\sigma}(-\mathbf{r}), and since the electronic potential is inversion symmetric, V(r)=V(−r)V(\mathbf{r}) = V(-\mathbf{r}), Vfd=0V_{fd} = 0 vanishes. Thus in a centrosymmetric crystal, the f−df-d hybridization takes place between neighboring Cerium sites and when written in momentum space, must be odd under inversion, yet even under time reversal. A minimal model for the non local odd parity hybridization within the planes of Ce atoms, has the form

Vsin⁡k⊥⋅σ=V(sin⁡kxσx+sin⁡kyσy),(4)V \sin\mathbf{k}_{\perp} \cdot\boldsymbol{\sigma} = V(\sin k_x \sigma_x + \sin k_y \sigma_y), \tag*{(4)}

where VV is the intersite hybridization strength and k⊥\mathbf{k}_{\perp} is the in-plane wavevector. This model form is obtained in a Slater-Koster treatment of hybridizing ss- and pp-states and captures the essence of spin orbit coupled heavy fermion compounds allowing, for example, a simple description of topological Kondo insulators [17]. By contrast, CeRh2_2As2_2 has a locally noncentrosymmetric structure with inversion centers located in between the Cerium layers. In this case, the atomic potential contains a gradient along the cc-axis that alternates between neighboring Cerium layers. This time, the atomic potential is not necessarily inversion symmetric:

Vα(x,y,z)=V−α(−x,−y,−z)≠Vα(−x,−y,−z),(5)V_\alpha(x,y,z) = V_{-\alpha}(-x,-y,-z) \ne V_\alpha(-x,-y,-z), \tag*{(5)}

where α=±1\alpha= \pm1 is a layer index. In this situation, the ff- and dd-states now acquire a cc-axis dipole moment which alternates between layers, and they no longer a well defined parity. The resulting overlap between the ff and dd states at the same site given by (3) is then non-zero, leading to a local hybridization. A minimal model for the local parity breaking hybridization is given by:

iW~α3σ3,(6)i\widetilde{W}\alpha_{3}\sigma_{3}, \tag*{(6)}

where W~\widetilde{W} is the local parity breaking hybridization amplitude. The appearance of the α3\alpha_{3} term reflects the reversal of the cc-axis electric field on neighboring layers. The hybridization is invariant under inversion, which inverts both the spin and sublattice index. The imaginary prefactor also guarantees that the hybridization is invariant under time-reversal. A model calculation of such a local hybridization mechanism is obtained by calculating the Slater-Koster overlap integral between a j=1/2j=1/2 ss and pp-state (see: Figure 2). A more realistic model of the hybridization, involving the j=5/2j=5/2 overlap between a dd and ff state is expected to give rise to an even momentum dependence in the quantity WW which we neglect here. Combining the local (6) and intersite (4) terms, we can formulate a minimal model for the hybridization form factor

Depiction of orbitals overlapping on an atom

Figure 2. The depiction of orbitals overlapping on an atom. Here EzE_z is the electric field along the zz direction and W~\widetilde{W} is hybridization strength. In green and blue is the pp-orbital which has a node and in purple is the isotropic ss-orbital. a.) Inversion center is located at the atomic center which has an even atomic potential V(x)=V(−x)V(x) = V(-x). Orbitals have well defined parity. The spatial overlap integral between pp and ss orbitals is zero, W~=0\widetilde{W} = 0 due to the atomic potential is even. b.) Inversion is broken at the atomic sites, the local crystal fields distort the orbitals leading to an offset of the inversion center. The atomic potential is no longer even V(x)≠V(−x)V(x) \ne V(-x). The resulting overlap integral between pp and ss orbitals is finite W~≠0\widetilde{W} \ne0.

ϕk,σσ′=(sk⋅σ+iWα3σ3).(7)\phi_{\mathbf{k},\sigma\sigma'} = \left(\mathbf{s}_{\mathbf{k}}\cdot\boldsymbol{\sigma}+iW\alpha_{3}\sigma_{3}\right). \tag*{(7)}

where W=W~/VW=\widetilde{W}/V and sk=(sin⁡kx,sin⁡ky)\mathbf{s}_{\mathbf{k}}=(\sin k_x,\sin k_y). The dimensionless parameter WW is the ratio of the local hybridization amplitude W~\widetilde{W} to the intersite amplitude VV. For real WW and VV, the form factors obey the exact identity

ϕkϕk†=(sx2+sy2+W2)α0σ0+2Wα3(syσ1−sxσ2).(8)\phi_{\mathbf{k}}\phi_{\mathbf{k}}^{\dagger}=(s_x^2+s_y^2+W^2)\alpha_0\sigma_0+2W\alpha_3(s_y\sigma_1-s_x\sigma_2). \tag*{(8)}

The interference term is staggered in the layer index and has the antisymmetric spin-orbit structure. When an ff electron tunnels through the conduction band, the resulting tunneling amplitude will reflect an interference between the two terms in the hybridization. We can calculate this effect by integrating out the conduction electrons, to obtain an ff electron self-energy given by

Σf(k,iωn)∼V2iωn−ϵkϕkϕk†(9)\Sigma_f(\mathbf{k},i\omega_n)\sim\frac{V^2}{i\omega_n-\epsilon_{\mathbf{k}}}\phi_{\mathbf{k}}\phi_{\mathbf{k}}^{\dagger} \tag*{(9)}

where for simplicity we have approximated the conduction electrons by a single band of dispersion ϵk\epsilon_{\mathbf{k}}. The interference between the two channels creates a spin orbit cross term in this self-energy that has the form

Σf(k)∝VWα3(syσ1−sxσ2).(10)\Sigma_f(\mathbf{k})\propto VW\alpha_3(s_y\sigma_1-s_x\sigma_2). \tag*{(10)}

where we denote sx=sin⁡kxs_x=\sin k_x, sy=sin⁡kys_y=\sin k_y. This spin orbit term has the same momentum and spin dependence as the previous staggered ASOC interaction introduced from symmetry analysis. The Kondo lattice therefore demonstrates a mechanism of how the ASOC is generated through a local parity breaking hybridization induced by the locally broken inversion symmetry.

Model and Methods

Kondo lattice construction

We now formulate a minimal Kondo Heisenberg model for CeRh2_2As2_2, with the Hamiltonian H=Hc+HK+HHH=H_c+H_K+H_H where

Hc=∑kck,α,σ†(hk)αα′ck,α′,σ,(11)H_c=\sum_{\mathbf{k}}c_{\mathbf{k},\alpha,\sigma}^{\dagger}(h_{\mathbf{k}})_{\alpha\alpha'}c_{\mathbf{k},\alpha',\sigma}, \tag*{(11)}
HK=JK∑jc~j,σ†σσσ′c~j,σ′⋅Sj,(12)H_K=J_K\sum_j\widetilde{c}_{j,\sigma}^{\dagger}\sigma_{\sigma\sigma'}\widetilde{c}_{j,\sigma'}\cdot\mathbf{S}_j, \tag*{(12)}
HH=JH∑⟨i,j⟩Si⋅Sj,(13)H_H=J_H\sum_{\langle i,j\rangle}\mathbf{S}_i\cdot\mathbf{S}_j, \tag*{(13)}

where ck,α,σ†c_{\mathbf{k},\alpha,\sigma}^{\dagger} creates a conduction electron with momentum k\mathbf{k}, sublattice index α=±1\alpha=\pm1 and spin index σ=±1\sigma=\pm1, while Sj=(Sjx,Sjy,Sjz)\mathbf{S}_j=(S_j^x,S_j^y,S_j^z) is the three component spin-1/2 local moment operator for site jj. We use Pauli matrix normalization for the local moments, i.e. Tr⁡[SjσSjσ′]=2δσσ′\operatorname{Tr}[S_j^\sigma S_j^{\sigma'}]=2\delta_{\sigma\sigma'}. A summation convention is used for the sum over spin and sublattice indices α\alpha. The first term HcH_c describes the conduction electrons, with a dispersion obtained from a tight binding calculation on a tetragonal lattice

hk=ϵk,00α0+ϵk,10α1.(14)h_{\mathbf{k}}=\epsilon_{\mathbf{k},00}\alpha_0+\epsilon_{\mathbf{k},10}\alpha_1. \tag*{(14)}

Here the dispersion elements

ϵk,00=−2t(cos⁡(kx)+cos⁡(ky))−μ,\epsilon_{\mathbf{k},00}=-2t(\cos(k_x)+\cos(k_y))-\mu,
ϵk,10=−4tscos⁡(kx2)cos⁡(ky2)cos⁡(kz2)(15)\epsilon_{\mathbf{k},10}=-4t_s\cos\left(\frac{k_x}{2}\right)\cos\left(\frac{k_y}{2}\right)\cos\left(\frac{k_z}{2}\right) \tag*{(15)}

describe the intra, and inter-layer hopping processes. The normal state parameters are given by tt the intralayer hopping strength and μ\mu the chemical potential and ts=tu+tdt_s=t_u+t_d is the interlayer hopping strength, tut_u is hopping up and tdt_d is hopping down. To maintain a connectivity with earlier work, we have followed the notation used in [1, 4].

HKH_K is the local Kondo interaction between the conduction electrons and the local moments, where JKJ_K is the Kondo coupling strength and the site index j≡(Rj,α)j\equiv(\mathbf{R}_j,\alpha) is a proxy for the position of the unit cell and the sublattice index of the Cerium site. Following the discussion in the introduction, the operator c~j,σ\widetilde{c}_{j,\sigma} annihilates a conduction electron in a Wannier state localized at site jj:

c~j,α,σ=1Ns∑kϕ(k)α,α′,σ′,σ′ck,α′,σ′eik⋅Rj,(16)\widetilde{c}_{j,\alpha,\sigma}=\frac{1}{\sqrt{\mathcal{N}_s}}\sum_{\mathbf{k}}\phi(\mathbf{k})_{\alpha,\alpha',\sigma',\sigma'}c_{\mathbf{k},\alpha',\sigma'}e^{i\mathbf{k}\cdot\mathbf{R}_j}, \tag*{(16)}

where Ns\mathcal{N}_s is the number of unit-cells in the crystal. The form factor matrix ϕk=ϕ(k)\phi_{\mathbf{k}}=\phi(\mathbf{k}) describes a Wannier state which carries the symmetry of the hybridization inherited from an underlying Anderson model. We take this to have the sublattice diagonal form introduced in (7),

ϕk=(sk⋅σ+iWα3σ3).(17)\phi_{\mathbf{k}}=(\mathbf{s}_{\mathbf{k}}\cdot\boldsymbol{\sigma}+iW\alpha_3\sigma_3). \tag*{(17)}

where we use the short-hand sk=(sin⁡kx,sin⁡ky)\mathbf{s}_{\mathbf{k}}=(\sin k_x,\sin k_y). The dominant source of spin orbit coupling in a Kondo lattice derives from the hybridization with the ff electrons. In our minimal model spin orbit coupling only enters through these terms in the Kondo coupling, and for simplicity, all spin orbit coupling terms in the conduction sea have been dropped.

Lastly, the Heisenberg interaction in Eq. (13) describes the AFM superexchange interaction between neighbouring spins where JHJ_H is the coupling strength.

We employ a large-NN path integral approach to formulate the model as a field theory and then develop a mean-field description. In the large-NN limit, all quantities that are extensive in NN behave as semi-classical variables, whose fluctuations are suppressed by powers of 1/N1/N, causing the path integral to focus into a mean field configuration. In the limit N→∞N \to\infty, the mean field solution becomes exact, allowing the basis for a controlled mean-field expansion.

An important aspect of our work is to use a large NN generalization of the SU(2) group to the symplectic group Sp(NN), where NN is even [18, 19, 20]. The first member of the Sp(NN) family is the SU(2) group, Sp(2) = SU(2), but at larger NN, Sp(NN) ∈\in SU(NN) is a subgroup of SU(NN) that preserves time reversal symmetry. Sp(NN) loosely corresponds to an N/2N/2-fold replication of the up and down spins, corresponding to N/2N/2 “up” and N/2N/2 “down” spin components:

σ∈(↑1, ↑2…↑N/2↓1, ↓2…↓N/2)≡(±1,±2…±N/2)(18)\sigma\in\left(\begin{matrix}\uparrow_1,\ \uparrow_2\ldots\uparrow_{N/2}\\ \downarrow_1,\ \downarrow_2\ldots\downarrow_{N/2}\end{matrix}\right)\equiv(\pm1,\pm2\ldots\pm N/2) \tag*{(18)}

where we identify the spin labels ↑σ≡σ\uparrow_\sigma\equiv\sigma and ↓σ≡−σ\downarrow_\sigma\equiv-\sigma, where σ=(1,2,…,N/2)\sigma=(1,2,\ldots,N/2) label the replicas [20]. The spin operators that connect up and down spins in the form factor (17) are diagonal in replica space which allows us to replicate the spins at each site to controlling the mean field theory without interfering with the SU(2) spin algebra which rotates between up and down spins in the original model. Our final results are expressed in terms of the properties per spin pair component, equivalent to formally setting N=2N=2 at the end of the calculation.

To formulate our model as a field theory, we use a fermionic representation

(Sj)λ=fjα†Sαβλfjβ,λ∈(1,N(N+1)2),(19)(S_j)^\lambda=f^\dagger_{j\alpha}S^\lambda_{\alpha\beta}f_{j\beta},\qquad\lambda\in\left(1,\frac{N(N+1)}{2}\right), \tag*{(19)}

for the components of the Hermitian Sp(NN) spin operators, where fα†f^\dagger_\alpha and fβf_\beta are fermionic creation and annihilation operators with spin component α∈(±1,…±N/2)\alpha\in(\pm1,\ldots\pm N/2). In passing to the large-NN theory we make the conventional rescaling JH→JH/NJ_H\to J_H/N and JK→JK/NJ_K\to J_K/N, so that the interaction energy remains extensive in NN and the N→∞N\to\infty limit is well defined. Using the corresponding Fierz decomposition (see appendix A for details), we rewrite the Kondo and Heisenberg interactions in the form:

cj,σ†σ⃗σσ′cj,σ′⋅Sj→(cj,σ†cj,σ′)Sσ′σ(j)c^\dagger_{j,\sigma} \vec{\sigma}_{\sigma\sigma'}c_{j,\sigma'}\cdot\mathbf{S}_j\to(c^\dagger_{j,\sigma}c_{j,\sigma'})S_{\sigma'\sigma}(j)
Si⋅Sj→Sσσ′(i)Sσ′σ(j)(20)\mathbf{S}_i\cdot\mathbf{S}_j\to S_{\sigma\sigma'(i)}S_{\sigma'\sigma(j)} \tag*{(20)}

where the

Sσσ′(j)=fj,σ†fj,σ′−σ~σ~′fj,−σ′†fj,−σ,(σ~≡sgn⁡(σ))(21)S_{\sigma\sigma'(j)}=f^\dagger_{j,\sigma}f_{j,\sigma'}-\widetilde{\sigma}\widetilde{\sigma}'f^\dagger_{j,-\sigma'}f_{j,-\sigma},\qquad(\widetilde{\sigma}\equiv\operatorname{sgn}(\sigma)) \tag*{(21)}

describe the matrix unit form of the spin operators. (These corresponds to an antisymmetrization of their SU(NN) spin counterpart SSU(N)=fα†fβ−(nf/N)δαβS^{\mathrm{SU}(N)}=f^\dagger_\alpha f_\beta-(n_f/N)\delta_{\alpha\beta} under time reversal). The parton decomposition of the local moments gives rise to a local SU(2) gauge invariance

fj,σ→{eiϕjfj,σ,cos⁡θjfj,σ+sin⁡θjfj,−σ†,(22)f_{j,\sigma}\to\left\{\begin{aligned} &e^{i\phi_j}f_{j,\sigma},\\ &\cos\theta_j f_{j,\sigma}+\sin\theta_j f^\dagger_{j,-\sigma}, \end{aligned}\right. \tag*{(22)}

which corresponds to rotations in particle-hole, or isospin space. We select amongst the various possible representations of the local moment by requiring that the ff parton state is an isospin singlet, requiring

∑σ>0fi,σ†fi,−σ†=∑σ>0fi,−σfi,σ=0,nf=N/2(23)\sum_{\sigma>0}f^\dagger_{i,\sigma}f^\dagger_{i,-\sigma}=\sum_{\sigma>0}f_{i,-\sigma}f_{i,\sigma}=0,\qquad n_f=N/2 \tag*{(23)}

corresponding to a half-filled ff state with local no ss-wave pairing. These are the “Gutzwiller constraints” of the Kondo lattice, which inside a path integral, are naturally imposed by fluctuations over the SU(2) gauge fields.

Path integral formulation

The SU(2) path integral is given by the partition function as Z=Tr⁡[e−βHPG]Z=\operatorname{Tr}[e^{-\beta H}P_G] where PGP_G imposes the Gutzwiller constraints (23). To develop the path integral, we adopt a Balian Werthammer notation,

Ck,α,σ=(ck,α,σck,α,−σ−c−k,α,−σ†c−k,α,σ†),Fj,σ=(fj,σfj,−σ−fj,−σ†fj,σ†),(σ>0),(24)C_{\mathbf{k},\alpha,\sigma}=\left(\begin{matrix}c_{\mathbf{k},\alpha,\sigma}\\c_{\mathbf{k},\alpha,-\sigma}\\-c^\dagger_{-\mathbf{k},\alpha,-\sigma}\\c^\dagger_{-\mathbf{k},\alpha,\sigma}\end{matrix}\right),\qquad F_{j,\sigma}=\left(\begin{matrix}f_{j,\sigma}\\f_{j,-\sigma}\\-f^\dagger_{j,-\sigma}\\f^\dagger_{j,\sigma}\end{matrix}\right),\qquad(\sigma>0), \tag*{(24)}

where the spin labels are purely positive. We will combine these Nambu spinors into a row, as follows

Ck,α=(Ck,α,1,Ck,α,2,…Ck,α,N/2)C_{\mathbf{k},\alpha}=(C_{\mathbf{k},\alpha,1},C_{\mathbf{k},\alpha,2},\ldots C_{\mathbf{k},\alpha,N/2})
Fj=(Fj,1,Fj,2,…Fj,N/2).(25)F_j=(F_{j,1},F_{j,2},\ldots F_{j,N/2}). \tag*{(25)}

In terms of these fields, the Gutzwiller constraints become Fj†τ⃗Fj=0F_j^\dagger\vec{\tau}F_j=0 where τ⃗=(τ1,τ2,τ3)\vec{\tau}=(\tau_1,\tau_2,\tau_3) are the isospin Pauli matrices, acting in particle-hole space. We can also form the conduction Wannier states as

Cj,α=1Ns∑k,α′ϕk,α′αCk,α′eik⋅Rj(26)C_{j,\alpha}=\frac{1}{\sqrt{N_s}}\sum_{\mathbf{k},\alpha'}\phi_{\mathbf{k},\alpha'\alpha}C_{\mathbf{k},\alpha'}e^{i\mathbf{k}\cdot\mathbf{R}_j} \tag*{(26)}

where the invariance of the form factor (17) under charge conjugation allows us to extend its usage to the Nambu formulation of the Wannier states. (See appendix B for details). In terms of this representation, the Gutzwiller constraint is simply that the isospin vanishes Fj†τ⃗Fj=0F_j^\dagger\vec{\tau} F_j = 0, where the τ⃗\vec{\tau} are the Pauli matrices in the particle-hole space of the Nambu spinors. In terms of this representation, the path integral has the form:

Z=∫D[ψˉ,ψ,w]exp⁡[−∫0βdτ(L0+H)].(27)Z=\int D[\bar{\psi},\psi,w]\exp\left[-\int_0^\beta d\tau(\mathcal{L}_0+H)\right]. \tag*{(27)}

where the Berry phase term

L0=∑k,α,σCk,α,σ†∂τCk,α,σ+∑j,σFj,σ†(∂τ+wj)Fj,σ.(28)\mathcal{L}_0=\sum_{k,\alpha,\sigma}C_{k,\alpha,\sigma}^\dagger\partial_\tau C_{k,\alpha,\sigma}+\sum_{j,\sigma}F_{j,\sigma}^\dagger(\partial_\tau+w_j)F_{j,\sigma}. \tag*{(28)}

The Fierz identities of the Sp(N) representation allow the Heisenberg and Kondo interactions to be rewritten in the form (see Appendix A for details)

HH=−JHN∑⟨i,j⟩[fi,σ†fi,σfj,σ′†fj,σ′+σ~σ~′fi,σ†fj,−σ†fj,−σ′fi,σ′].(29)H_H=-\frac{J_H}{N}\sum_{\langle i,j\rangle}\left[f_{i,\sigma}^\dagger f_{i,\sigma}f_{j,\sigma'}^\dagger f_{j,\sigma'}+\tilde{\sigma}\tilde{\sigma}'f_{i,\sigma}^\dagger f_{j,-\sigma}^\dagger f_{j,-\sigma'}f_{i,\sigma'}\right]. \tag*{(29)}
HK=−JKN∑j[c~j,σ†fj,σfj,σ′†c~j,σ′+σ~σ~′c~j,σ†fj,−σ†fj,−σ′c~j,σ′].(30)H_K=-\frac{J_K}{N}\sum_j\left[\tilde{c}_{j,\sigma}^\dagger f_{j,\sigma}f_{j,\sigma'}^\dagger\tilde{c}_{j,\sigma'}+\tilde{\sigma}\tilde{\sigma}'\tilde{c}_{j,\sigma}^\dagger f_{j,-\sigma}^\dagger f_{j,-\sigma'}\tilde{c}_{j,\sigma'}\right]. \tag*{(30)}

where the spin sums run over σ,σ′∈(±1,⋯±N/2)\sigma,\sigma'\in(\pm1,\cdots\pm N/2).

These interactions are now decoupled using the Hubbard Stratonovich transformations. The Kondo interaction becomes

HK→∑j[Cj†Vj†Fj+Fj†VjCj+NTr⁡[Vj†Vj]2JK].(31)H_K\to\sum_j\left[C_j^\dagger\mathcal{V}_j^\dagger F_j+F_j^\dagger\mathcal{V}_j C_j+N\frac{\operatorname{Tr}[\mathcal{V}_j^\dagger\mathcal{V}_j]}{2J_K}\right]. \tag*{(31)}

where the matrix

Vj=(Vjνj∗νj−Vj∗).(32)\mathcal{V}_j=\begin{pmatrix}V_j&\nu_j^*\\ \nu_j&-V_j^*\end{pmatrix}. \tag*{(32)}

describes hybridization (VjV_j) and pairing (νj\nu_j) between the conduction and ff parton fields. Similarly, a Hubbard Stratonovich decoupling of the Heisenberg term gives

HH→∑⟨i,j⟩[Fi†UijFj+Fj†Uij†Fi+NTr⁡[Uij†Uij]2JH].(33)H_H\to\sum_{\langle i,j\rangle}\left[F_i^\dagger U_{ij}F_j+F_j^\dagger U_{ij}^\dagger F_i+N\frac{\operatorname{Tr}[U_{ij}^\dagger U_{ij}]}{2J_H}\right]. \tag*{(33)}

where

Uij=(tijfΔij∗Δij−tijf∗),Uji=(tijf∗Δij∗Δij−tijf).(34)U_{ij}=\begin{pmatrix}t_{ij}^f&\Delta_{ij}^*\\ \Delta_{ij}&-t_{ij}^{f*}\end{pmatrix},\quad U_{ji}=\begin{pmatrix}t_{ij}^{f*}&\Delta_{ij}^*\\ \Delta_{ij}&-t_{ij}^f\end{pmatrix}. \tag*{(34)}

Here, the tijft_{ij}^f and Δij\Delta_{ij} are the ff electron hopping and RVB pairing fields, respectively. Notice also that Uji=Uij†U_{ji}=U_{ij}^\dagger. The notation ⟨i,j⟩\langle i,j\rangle denotes nearest neighbours within a given layer. Note that the nearest neighbour pairing Δij≡ΔRi,α;Rj,α\Delta_{ij}\equiv\Delta_{R_i,\alpha;R_j,\alpha} can depend on the layers. With these transformations, the Lagrangian in the path integral now takes the form

L0=∑k,αCk,α†∂τCk,α+∑jFj†(∂τ+wj)Fj+H.(35)\mathcal{L}_0=\sum_{k,\alpha}C_{k,\alpha}^\dagger\partial_\tau C_{k,\alpha}+\sum_jF_j^\dagger(\partial_\tau+w_j)F_j+H. \tag*{(35)}

Here wj=w⃗j⋅τ⃗w_j=\vec{w}_j\cdot\vec{\tau}, where w⃗j=(wj1,wj2,λj)\vec{w}_j=(w_j^1,w_j^2,\lambda_j) are three SU(2) gauge potentials whose fluctuation along the imaginary axis impose the Gutzwiller constraints (23).

The Fierz identities of the Sp(N) representation allow the Heisenberg and Kondo interactions to be rewritten in the form (see Appendix A for details)

Here H=Hc+HK+HHH=H_c+H_K+H_H, while HKH_K take the expanded forms shown in (31) and (33), respectively. The SU(2) gauge invariance (22) now includes the gauge fields,

Fj→gjFj,Vj→gjVj,wj→gjwjgj†+gj∂τgj†,Uij→giUijgj†.(36)\begin{aligned} F_j&\to g_jF_j,\\ \mathcal{V}_j&\to g_j\mathcal{V}_j,\\ w_j&\to g_jw_jg_j^\dagger+g_j\partial_\tau g_j^\dagger,\\ U_{ij}&\to g_iU_{ij}g_j^\dagger. \tag*{(36)} \end{aligned}

where gjg_j are members of the SU(2) group. We use this gauge degree of freedom to fix the gauge by writing Vj=gj∣Vj∣τ3\mathcal{V}_j=g_j|V_j|\tau_3, absorbing the gjg_j by the above gauge transformation. In this “radial gauge”, Vj=∣Vj∣τ3\mathcal{V}_j=|V_j|\tau_3 describes a pure, real hybridization. The pure Kondo model, without the Heisenberg terms describes a Fermi liquid with an expanded Fermi surface volume which accommodates the hybridized ff electrons, according to Oshikawa’s theorem[21, 22]. In this phase, the difference between the internal SU(2) gauge field and the external electromagnetic field is Higgsed[23], in a fashion reminiscent of electroweak symmetry breaking. The finite mass of the difference field locks the internal gauge field to the external electromagnetic field, endowing the previously neutral ff partons with physical charge, thus converting them into heavy electrons. Once the Heisenberg coupling is restored, there are now further low temperature instabilities of the heavy Fermi liquid.

Mean field Theory

To develop a mean field theory we examine static, translationally invariant solutions. In the normal state, Vj=V\mathcal{V}_j=V and λj=λ\lambda_j=\lambda, and tijf=−tft_{ij}^f=-t_f are real, while the pairing order parameter variables Δij=0\Delta_{ij}=0 are zero. We restrict our study of instabilities of the Fermi liquid to superconductivity, in which the nearest neighbour Heisenberg couplings develop an expectation value that can depend on the sublattice variable α\alpha. Within a layer, energetics favours a dd-wave pairing state, i.e. Δx=−Δy=Δ\Delta_x=-\Delta_y=\Delta. The dd-wave order parameter within the layers guarantees there is no ss-wave pairing at the ff sites, which allows us to set the pairing components of the constraint fields to zero, i.e. w⃗=(w1,w2,λ)=(0,0,λ)\vec{w}=(w^1,w^2,\lambda)=(0,0,\lambda).

Now since the inversion centers lie between the layers, this allows for the possibility of both uniform and staggered pairing solutions in which the pairing develops a layer dependence. These two classes of solution are respectively, even and odd-parity under inversion.

Δk(α)=2Δ(cos⁡kx−cos⁡ky)×{1even parityαodd-parity(37)\Delta_{\mathbf{k}}^{(\alpha)}=2\Delta(\cos k_x-\cos k_y)\times \begin{cases} 1 & \text{even parity}\\ \alpha& \text{odd-parity} \end{cases} \tag*{(37)}

where α=±1\alpha=\pm1 is the sublattice label. We will show that under the influence of the hybridization, these two states correspond to singlet and triplet pairing states, as originally reasoned by Yoshida, Sigrist and Yanase[24]. To accomodate a magnetic field, we introduce a Zeeman term into the Hamiltonian H→H−σzB\mathcal{H}\rightarrow\mathcal{H}-\sigma_zB. We will show that while the uniform state has a higher TcT_c, the staggered odd parity triplet state is able to accomodate a Zeeman polarization, stabilizing it in a magnetic field.

Putting this all together, the resulting mean-field Hamiltonian takes the form

HMF=∑kΨk†H(k)Ψk+2NNs[∣V∣2JK+2(∣Δ∣2+tf2)JH](38)H_{\mathrm{MF}}=\sum_{\mathbf{k}}\Psi_{\mathbf{k}}^\dagger\mathcal{H}(\mathbf{k})\Psi_{\mathbf{k}}+2NN_s\left[\frac{|V|^2}{J_K}+\frac{2(|\Delta|^2+t_f^2)}{J_H}\right] \tag*{(38)}

where the superconducting Hamiltonian is given by

H(k)=(hkτ3−σzBVk†Vkhkfτ3−σzB+Δk(α)τ1)(39)\mathcal{H}(\mathbf{k})= \begin{pmatrix} h_{\mathbf{k}}\tau_3-\sigma_zB & V_{\mathbf{k}}^\dagger\\ V_{\mathbf{k}} & h_{\mathbf{k}}^f\tau_3-\sigma_zB+\Delta_{\mathbf{k}}^{(\alpha)}\tau_1 \end{pmatrix} \tag*{(39)}

and

Ψk=(Ck+Ck−Fk+Fk−)(40)\Psi_{\mathbf{k}}= \begin{pmatrix} C_{\mathbf{k}+}\\ C_{\mathbf{k}-}\\ F_{\mathbf{k}+}\\ F_{\mathbf{k}-} \end{pmatrix} \tag*{(40)}

combines the conduction and ff Nambu spinors on the two layers. Here α=±\alpha=\pm are the layer indices of Ck,αC_{\mathbf{k},\alpha} and Fk,αF_{\mathbf{k},\alpha}. The off diagonal hybridization terms are given by Vk=Vϕkτ3V_{\mathbf{k}}=V\phi_{\mathbf{k}}\tau_3. The ff electron dispersion is

hkf=−2tf(cos⁡(kx)+cos⁡(ky))+λ.(41)h_{\mathbf{k}}^f=-2t_f(\cos(k_x)+\cos(k_y))+\lambda. \tag*{(41)}

In a compact notation define hkf=tfγk+λh_{\mathbf{k}}^f=t_f\gamma_{\mathbf{k}}+\lambda, where γk=−2(cos⁡(kx)+cos⁡(ky))\gamma_{\mathbf{k}}=-2(\cos(k_x)+\cos(k_y)). Note that the factor of 2NNs2NN_s in the mean-field term derives from the NN spin components and the 2Ns2N_s sites.

The mean field solutions are obtained by finding the stationary points of the free energy. Integrating out the fermionic fields leads to the free energy F=−T∑k,nln⁡(det⁡(−Gk−1(iωn)))F=-T\sum_{\mathbf{k},n}\ln(\det(-\mathcal{G}_{\mathbf{k}}^{-1}(i\omega_n))) where Gk−1(iωn)=[iωn−H(k)]\mathcal{G}_{\mathbf{k}}^{-1}(i\omega_n)=[i\omega_n-\mathcal{H}(\mathbf{k})] is the Greens function in imaginary time where iωnβ=iπ(2n+1)i\omega_n\beta=i\pi(2n+1) represents the fermionic Matsubara frequencies that runs over nn discrete frequencies. The mean field Hamiltonian is diagonalised by integrating out the ff electrons. With the energy eigenvalues ξkn\xi_{\mathbf{k}n}, using the identity ln⁡(det⁡(A))=Tr⁡[ln⁡(A)]\ln(\det(A))=\operatorname{Tr}[\ln(A)] and computing the Matsubara sum leads to the mean field free energy

FN=12∑k,n=1,8[−2Tln⁡(2cosh⁡(ξkn2T))](42)\frac{F}{N}=\frac{1}{2}\sum_{\mathbf{k},n=1,8}\left[-2T\ln\left(2\cosh\left(\frac{\xi_{\mathbf{k}n}}{2T}\right)\right)\right] \tag*{(42)}
+2Ns(∣V∣2JK+2(tf2+∣Δ∣2)JH),(43)+2N_s\left(\frac{|V|^2}{J_K}+\frac{2(t_f^2+|\Delta|^2)}{J_H}\right), \tag*{(43)}

where ±ξkn\pm\xi_{\mathbf{k}n} are the eigenvalues of the mean-field Hamiltonian, η∈(1,8)\eta\in(1,8) is the eigenvalue index and NsN_s the number of unit cells in the lattice[25]. The saddle point approximation is obtained by seeking the stationary points of the effective action ∂Seff/∂x=∂F/∂x=0\partial S_{\mathrm{eff}}/\partial x=\partial F/\partial x=0, where x=V,tf,λ,Δx=V,t_f,\lambda,\Delta. In practice, we impose these conditions on our numerical calculations, thereby imposing four self-consistency conditions:

12NNs∑k,α,σγk⟨fk,α,σ†fk,α,σ⟩+4tfJH=0,(44)\frac{1}{2NN_s}\sum_{\mathbf{k},\alpha,\sigma}\gamma_{\mathbf{k}}\langle f_{\mathbf{k},\alpha,\sigma}^{\dagger}f_{\mathbf{k},\alpha,\sigma}\rangle+\frac{4t_f}{J_H}=0, \tag*{(44)}
12NNs∑k,α,σ2(cx−cy)⟨f~−k,α,−σfk,α,σ⟩+4ΔJH=0,(45)\frac{1}{2NN_s}\sum_{\mathbf{k},\alpha,\sigma}2(c_x-c_y)\langle\tilde{f}_{-\mathbf{k},\alpha,-\sigma}f_{\mathbf{k},\alpha,\sigma}\rangle+\frac{4\Delta}{J_H}=0, \tag*{(45)}
12NNs∑k,α,σ,σ′⟨ck,α,σ†ϕ(k)fk,α,σ′⟩+VJK=0,(46)\frac{1}{2NN_s}\sum_{\mathbf{k},\alpha,\sigma,\sigma'}\langle c_{\mathbf{k},\alpha,\sigma}^{\dagger}\phi(\mathbf{k})f_{\mathbf{k},\alpha,\sigma'}\rangle+\frac{V}{J_K}=0, \tag*{(46)}
12NNs∑k,α,σ⟨fk,α,σ†fk,α,σ⟩=12,(47)\frac{1}{2NN_s}\sum_{\mathbf{k},\alpha,\sigma}\langle f_{\mathbf{k},\alpha,\sigma}^{\dagger}f_{\mathbf{k},\alpha,\sigma}\rangle=\frac{1}{2}, \tag*{(47)}

where the normalizing prefactors derive from the 2Ns2N_s ff sites and the NN spin components. The last condition is the constraint of a half-filled ff band, ⟨F†τ3F⟩=0\langle F^\dagger\tau_3F\rangle=0. In general, once a finite hybridization VV develops in the normal state, this gives rise to a finite hybridization between ff electrons at different sites, which by (44) induces a finite tft_f.

Results

Normal state: Emergent Spin-Orbit Coupling

We begin with a discussion of the normal state. Here, the key point is that the absence of local inversion symmetry at the Cerium sites modifies the electrostatic environment of the atoms. This polarizes the atomic orbitals, giving them an ill defined parity which opens up previously forbidden mixing between even and odd parity states. We will see how this modifies the spin orbit coupling (SOC). To elucidate this effect, we examine the $f propagator obtained after integrating out the conduction electrons. This takes the form:

Gf(k,iωn)=[iωn−hkτ3−Σf(k,iωn)]−1.(48)G_f(\mathbf{k},i\omega_n)=\left[i\omega_n-h_{\mathbf{k}}\tau_3-\Sigma_f(\mathbf{k},i\omega_n)\right]^{-1}. \tag*{(48)}

The ff electron self-energy Σf(k,iωn)\Sigma_f(\mathbf{k},i\omega_n) is represented by the following diagram

Σf(k,iωn)=Vk1iωn−hkτ3Vk†.(49)\Sigma_f(\mathbf{k},i\omega_n)=\mathcal{V}_{\mathbf{k}}\frac{1}{i\omega_n-h_{\mathbf{k}}\tau_3}\mathcal{V}_{\mathbf{k}}^\dagger. \tag*{(49)}

where Vk=Vϕ(k)τ3\mathcal{V}_{\mathbf{k}}=V\phi(\mathbf{k})\tau_3. Let us now examine the spin orbit coupling generated by this process. The conduction electron dispersion hkh_{\mathbf{k}} can be divided into sublattice independent and dependent parts, hk=hk0+hk1α1h_{\mathbf{k}}=h_{\mathbf{k}}^0+h_{\mathbf{k}}^1\alpha_1. Now since τ3\tau_3 and α1\alpha_1 are commuting operators, which can be simultaneously diagonalized, we can rewrite the conduction electron propagator in the form

1iωn−hkτ3=(iωn−hk0τ3)+hk1α1τ3(iωn−hk0τ3)2−(hk1)2(50)\frac{1}{i\omega_n-h_{\mathbf{k}}\tau_3}= \frac{(i\omega_n-h_{\mathbf{k}}^0\tau_3)+h_{\mathbf{k}}^1\alpha_1\tau_3}{(i\omega_n-h_{\mathbf{k}}^0\tau_3)^2-(h_{\mathbf{k}}^1)^2} \tag*{(50)}

Reinstating α1\alpha_1 and τ3\tau_3 as operators, the self-energy takes the form

Σf(k,iωn)=V2(sk⋅σ+iWα3σ3)[(iωn−hk0τ3)+hk1α1τ3(iωn−hk0τ3)2−(hk1)2](sk⋅σ−iWα3σ3).(51)\Sigma_f(\mathbf{k},i\omega_n)=V^2(\mathbf{s}_{\mathbf{k}}\cdot\boldsymbol{\sigma}+iW\alpha_3\sigma_3)\left[\frac{(i\omega_n-h_{\mathbf{k}}^0\tau_3)+h_{\mathbf{k}}^1\alpha_1\tau_3}{(i\omega_n-h_{\mathbf{k}}^0\tau_3)^2-(h_{\mathbf{k}}^1)^2}\right](\mathbf{s}_{\mathbf{k}}\cdot\boldsymbol{\sigma}-iW\alpha_3\sigma_3). \tag*{(51)}
=V2τ3(iωn−hk0τ3)2−(hk1)2((iωnτ3−hk0)[(sk2+W2)−2Wα3(z^×sk)⋅σ]+hk1α1(sk2−W2)).(52)=\frac{V^2\tau_3}{(i\omega_n-h_{\mathbf{k}}^0\tau_3)^2-(h_{\mathbf{k}}^1)^2}\left((i\omega_n\tau_3-h_{\mathbf{k}}^0)\left[\left(s_{\mathbf{k}}^2+W^2\right)-2W\alpha_3(\hat{\mathbf{z}}\times\mathbf{s}_{\mathbf{k}})\cdot\boldsymbol{\sigma}\right]+h_{\mathbf{k}}^1\alpha_1\left(s_{\mathbf{k}}^2-W^2\right)\right). \tag*{(52)}

where sk=(sin⁡kx,sin⁡ky)\mathbf{s}_{\mathbf{k}}=(\sin k_x,\sin k_y) and sk2=sin⁡2kx+sin⁡2kys_{\mathbf{k}}^2=\sin^2 k_x+\sin^2 k_y. We see that the interference between the two terms in the hybridization generates staggered spin orbit coupling with a cross product structure between momentum and spin. At low energies,

ΣfSOC(k,iωn)=2VW~α3τ3(iωn−hk0τ3)2−(hk1)2(syσ1−sxσ2),(53)\Sigma_f^{\mathrm{SOC}}(\mathbf{k},i\omega_n)=\frac{2V\widetilde{W}\alpha_3\tau_3}{(i\omega_n-h_{\mathbf{k}}^0\tau_3)^2-(h_{\mathbf{k}}^1)^2}(s_y\sigma_1-s_x\sigma_2), \tag*{(53)}

where W=W~/VW=\widetilde{W}/V demonstrating that the self-energy of the ff electron in (53) develops a frequency dependent form of the ASOC interaction deduced from symmetry analysis. Unlike previous models which added the ASOC interaction as a phenomenological term in the normal state, here the essential physics is produced from an interplay between the local parity breaking hybridization and the intersite sk⋅σ=sin⁡k⊥⋅σ\mathbf{s}_{\mathbf{k}}\cdot\boldsymbol{\sigma}=\sin\mathbf{k}_{\perp}\cdot\boldsymbol{\sigma} hybridization that carries the strong SOC effects of the ff-states. The new local parity breaking term iα3Wσ3i\alpha_3W\sigma_3 in the hybridization form factor ϕk=(sk⋅σ+iWα3σ3)\phi_{\mathbf{k}}=(\mathbf{s}_{\mathbf{k}}\cdot\boldsymbol{\sigma}+iW\alpha_3\sigma_3) provides the spin flip necessary to swap the spin components of the intersite hybridization sin⁡k⊥⋅σ\sin\mathbf{k}_{\perp}\cdot\boldsymbol{\sigma} generating an antisymmetric SOC. The frequency dependent prefactor encodes the virtual processes of the ff electrons fluctuating into the conduction sea and returning having acquired the necessary spin and momentum symmetry required to induce the ASOC interaction. In otherwords, Kondo screening in a noncentrosymmetric environment creates a heavy Fermi liquid with the necessary ingredients for a triplet superconducting state. The normal state properties can be seen in how the dispersion and Fermi surfaces change across the Brillouin zone.

The dispersion plot of the normal state is shown in Figure 3. The dispersion plotted along the path given by the high symmetry points Γ=(0,0,0)\Gamma=(0,0,0), X=(π,0,0)X=(\pi,0,0), M=(π,π,0)M=(\pi,\pi,0), Z=(0,0,π)Z=(0,0,\pi), R=(π,0,π)R=(\pi,0,\pi), A=(π,π,π)A=(\pi,\pi,\pi). The 3D fermi surfaces of the normal state are shown in Figure 4.

Normal state bandstructure plotted along the high symmetry points

Figure 3. The normal state bandstructure plotted along the high symmetry points. The intralayer hopping is given by t=5t=5, the interlayer hopping ts=1.5t_s=1.5 and the ff electron hopping is tf=0.5t_f=0.5, the chemical potential μ=−1\mu=-1 and the ff electron constraint λ=−1.7\lambda=-1.7. The hybridization strengths are V=3V=3 and W=2W=2. The doubly degenerate bands are ensured by Kramer's degeneracy.

The 3D Fermi surface of the normal state

Figure 4. The 3D Fermi surface of the normal state, the surfaces are doubly degenerate. The parameters for the normal state are given by the intralayer hopping t=5t=5, the chemical potential μ=−1\mu=-1, the interlayer hopping ts=1.5t_s=1.5 and the ff electron hopping tf=0.5t_f=0.5, and the ff electron chemical potential λ=−1.7\lambda=-1.7, the hybridization strengths are V=3V=3 and W=2W=2. Top: the top view. Bottom: the side view.

Superconducting State

We now examine the superconductor, and the effect of a magnetic field in stabilizing an odd-parity condensate. In the absence of a magnetic field, the even parity solution with its lower kinetic energy, is expected to be more stable, exhibiting a higher TcT_c than its odd parity counterpart. Interestingly, in the limit where the hybridization is a constant, Vk=V0V_{\mathbf{k}}=V_0, there is no staggered solution. The only solution is the uniform pairing which leads to the conventional dd-wave singlet pairing within the layers commonly seen in the 115 heavy fermion superconductors [26, 27]. In CeRh2_2As2_2, neutron scattering does indeed detect a peak at the dynamic structure factor at Q=(π,π)\mathbf{Q}=(\pi,\pi), a hallmark for AFM fluctuations [16].

To investigate the effect of the applied field on the superconducting state, we now switch on a Zeeman field as defined in (39). Although CeRh2_2As2_2 is a type II superconductor which develops a vortex lattice in a field, the effect of spatial modulation is assumed to be negligible for the low temperature and high field regime where Pauli limiting dominates, as described in (39).

Application of a Zeeman field affects the critical temperature TcT_c which can be computed from the pair susceptibility χP\chi_P. Generally, in the normal state, the pair susceptibility enters into the Landau free energy functional via the quadratic term F[Δ]=∣Δ∣2(χP(Bz)−2/JH)+β∣Δ∣4F[\Delta]=|\Delta|^2(\chi_P(B_z)-2/J_H)+\beta|\Delta|^4 calculated by taking the second derivative w.r.t the pairing field Δ\Delta. At TcT_c, the ∂2F/∂Δ2∣Δ=0=0\partial^2F/\partial\Delta^2|_{\Delta=0}=0 giving the well known criteria for TcT_c:

χP(Bz,Tc)−2JH=0.(54)\chi_P(B_z,T_c)-\frac{2}{J_H}=0. \tag*{(54)}

In our calculations, the pair susceptibility was obtained by evaluating the second derivative of the Free energy, χP(Bz,Tc)−2/JH=−∂2F(Bz,Tc)/∂Δ2\chi_P(B_z,T_c)-2/J_H=-\partial^2F(B_z,T_c)/\partial\Delta^2 for a range of magnetic field strengths for both uniform and staggered solutions. The corresponding phase boundaries for the uniform Δk(0)\Delta_{\mathbf{k}}^{(0)} and staggered Δk(3)\Delta_{\mathbf{k}}^{(3)} solutions are shown in Figure 5. The first order SC1 to SC2 boundary was determined by comparing the fully evaluated mean-field free energies of the self-consistent uniform and staggered superconducting solutions at the same (Bz,T)(B_z,T). The transition occurs where these two free energy branches cross; the pair susceptibility criterion in Eq. (54) determines the normal state instability lines, not the first order boundary. The uniform state (SC1) has a higher condensation energy than the staggered state since staggering the phase of the pairing field Δ\Delta requires a higher kinetic energy [24], and this results in a higher TcT_c at zero field. However, the condensation energy of the singlet SC1 phase is more strongly susceptible to a Zeeman splitting, ultimately raising its energy above the staggered, triplet SC2 phase. Once a magnetic field is applied, there is a first order phase transition to the staggered state. There is a thus field induced parity switching between the uniform even parity state to the staggered odd parity state providing a concrete Kondo lattice demonstration of the field induced parity switching behavior observed in experiments.

The superconducting phase diagram

Figure 5. The superconducting phase diagram of applied field BzB_z along the zz-axis w.r.t TT for uniform Δkα0\Delta_{\mathbf{k}\alpha0} and staggered Δkα3\Delta_{\mathbf{k}\alpha3} phases. The SC1 phase is given by the uniform state which is Pauli limited and the high field SC2 phase is given by the staggered state. The TcT_c was calculated by computing the pair susceptibility χP(Bz,Tc)\chi_P(B_z,T_c) obtained from taking the second derivative w.r.t pairing field Δ\Delta. The first order phase transition line is shown in purple which separates the two second order phase transitions.

For further investigation, a self consistent calculation was performed to analyze the uniform and staggered pairing states. The heavy Fermi liquid phase has already been developed and frozen with the Kondo hybridization parameters V=3V=3 and W=2W=2 which are the intersite and onsite hybridization respectively and the Kondo and Heisenberg coupling strengths are set to JK=0.3J_K=0.3 and JH=0.15J_H=0.15 respectively. The intralayer and interlayer hopping strengths are given by t=5t=5 and ts=1.5t_s=1.5 respectively and the chemical potential was set to μ=−1\mu=-1. The hopping scales are consistent with a quasi-2D structure. The ff electron hopping strength is set to tf=0.5t_f=0.5 with tf≪tt_f\ll t and the chemical potential for the ff electron was set to λ=−1.7\lambda=-1.7 with a q=1/3q=1/3 charge. The qualitative results do not depend on the microscopic details of the band structure as long as keeping the ratio of t/ts>1t/t_s>1 for the interlayer to intralayer coupling and VW/ts>1V W/t_s>1 for the interlayer to hybridization strength. With these parameters, a Newton Raphson method was used to find the saddle point of the pairing field by minimizing the Free energy w.r.t the pairing field Δ\Delta for the uniform and staggered solutions. The resulting phase diagram of the pairing gap Δ\Delta vs temperature in the presence of magnetic field is given by Figure 6.

Phase diagram of the pairing gap versus temperature for uniform and staggered phases

Figure 6. The phase diagram of the pairing gap vs temperature for both uniform Δkα0\Delta_{\mathbf{k}\alpha_0} and staggered Δkα3\Delta_{\mathbf{k}\alpha_3} phases for different magnetic field strengths BzB_z. The calculation of the gap magnitude Δ\Delta was determined self consistently. Top: Bz=0B_z=0 dominated by uniform pairing Δkα0\Delta_{\mathbf{k}\alpha_0} state. Bottom: Bz=0.8B_z=0.8 is dominated by staggered Δkα3\Delta_{\mathbf{k}\alpha_3} state.

The zero field behaviour of the uniform and staggered states is shown in the top plot of Figure 6 which shows the pairing field and TcT_c for the two states are nearly degenerate. The uniform state has a higher TcT_c emphasising the dominance of the even parity singlet state at zero field. However, once a magnetic field of Bz=0.8B_z=0.8 is applied, as shown in the lower plot Figure 6, the even parity state is suppressed by Pauli limiting effect. When the TcT_c of the staggered odd parity state starts to overcome the uniform even parity state, a field induced transition takes place. The staggered odd parity state is more weakly susceptible to Pauli limiting effects. The upper critical field of the staggered state is Bc2≈3.2B_{c2}\approx3.2 for which the uniform state completely vanishes. To understand how a spin singlet pairing in the layers staggered could realise a triplet odd parity state, the pairing gap will be projected onto the low energy pseudospin basis.

Projection of the Gap onto pseudospin basis

To understand the nature of the gap structure, the gap must be projected onto the Fermi surface. The procedure requires the gap operator originally in the high energy sublattice and spin subspace to be evaluated within the Kramers pair of energy eigenstates in a given band [4]

Δ(k)σσ′=2Δ(cx−cy)[ξknσ†(τ1αmPf)ξknσ′].(55)\Delta(\mathbf{k})_{\sigma\sigma'}=2\Delta(c_x-c_y)\left[\xi_{\mathbf{k}n}^{\sigma\dagger}(\tau_1\alpha_mP_f)\xi_{\mathbf{k}n}^{\sigma'}\right]. \tag*{(55)}

Here ξkn(σ)\xi_{\mathbf{k}n}^{(\sigma)}, (σ∈(↑,↓))(\sigma\in(\uparrow,\downarrow)) denotes the Kramers doublet of eigenstates of the superconducting mean field Hamiltonian at momentum k\mathbf{k} in the nn-th band and PfP_f projects onto the ff sector. The sublattice matrices can take either αm=α0\alpha_m=\alpha_0 or α3\alpha_3 which denotes the sublattice for the uniform, and staggered gap functions respectively.

To consistently calculate this quantity, we need to consistently fix the phase relationship between the pseudospin up and down eigenstates. We calculate the up eigenstate by applying a small field to split the Kramers degeneracy, selecting it as the “up” state as the lowest energy member of the doublet. We then apply time-reversal and parity inversion to the up state to generate its down-spin partner, ξkn↓=iα1σ2(ξkn↑)∗\xi_{\mathbf{k}n}^{\downarrow}=i\alpha_1\sigma_2(\xi_{\mathbf{k}n}^{\uparrow})^*.

The Fermi surface projection of the uniform gap Δkα0\Delta_{\mathbf{k}\alpha_0} is shown in Figure 7. As expected from (55), the gap has zeros along the kx=kyk_x=k_y derived from the in-plane dd-wave gap structure. The colors show the sign of the gap sgn⁡(Δ)\operatorname{sgn}(\Delta) where the ++ and −- signs are denoted by pink and blue respectively. Thus the projected gap structure of the uniform gap on the Fermi surface is an even parity dd-wave spin singlet Δkn(0)\Delta^{(0)}_{\mathbf{k}n} where nn represents the band index

Uniform gap projected onto the normal state basis

Figure 7. Uniform gap Δk(0)\Delta^{(0)}_{\mathbf{k}} projected onto the normal state basis which reflects a diagonal projection where the gap is given by ψ0(k)\psi_0(\mathbf{k}). The Fermi surface contour is shown by the green. The diagonal lines in light purple are the zeros of the projected gap function Δk(0)=0\Delta^{(0)}_{\mathbf{k}}=0 which represent a B1gB_{1g}, dx2−y2d_{x^2-y^2} nodal structure. The pink and blue shaded regions show the sign of the pairing gap corresponding to positive Δk(0)>0\Delta^{(0)}_{\mathbf{k}}>0 and negative Δk(0)<0\Delta^{(0)}_{\mathbf{k}}<0 gaps respectively. The purple contour is the angular dependence of the projected gap showing vanishing gap near the nodes.

Δk(s)=(ψ0(k)00ψ0(k)).(56)\Delta^{(s)}_{\mathbf{k}}= \begin{pmatrix} \psi_0(\mathbf{k}) & 0\\ 0 & \psi_0(\mathbf{k}) \end{pmatrix}. \tag*{(56)}

Here ψ0(k)\psi_0(\mathbf{k}) is an even, generally signed gap function. Throughout this subsection, Δk\Delta_{\mathbf{k}} denotes the reduced gap matrix, while the full anomalous gap matrix is Δ^k=Δk(iσ2)\hat{\Delta}_{\mathbf{k}}=\Delta_{\mathbf{k}}(i\sigma_2) in the pseudospin basis.

The Symmetry of the singlet and pseudo-spin triplet states

Symmetry of the gap

We now discuss the symmetry and physical origin of the spin-orbit generated pseudospin triplet state. The projection of the staggered gap Δk(t)\Delta^{(t)}_{\mathbf{k}} is shown in Figure 8. The key result is that even though the in plane pairing is singlet, the staggered pair potential on alternating layers transforms it into an odd parity triplet state on

Plots displaying the B1u triplet gap function

Figure 8. Plots displaying the B1uB_{1u} triplet gap function, showing its product structure, Δ↓↓(k)=dx(k)+idy(k)∝cos⁡(2θ)e−iθ\Delta_{\downarrow\downarrow}(\mathbf{k})=d_x(\mathbf{k})+id_y(\mathbf{k})\propto\cos(2\theta)e^{-i\theta} which vanishes along the diagonals and is a mixture of ff and pp wave pairing. a. The plot of the projected staggered gap Δk(t)\Delta^{(t)}_{\mathbf{k}} onto the normal state basis. To more clearly display the dd-wave form factor, the Rashba dd-vector has been rotated anticlockwise by 90∘90^\circ, corresponding to a gauge transformation Δ→−iΔ\Delta\to-i\Delta. The Fermi surface is shown by a green contour. b. the d⃗k\vec{d}_{\mathbf{k}} vector across the Brillouin zone.

the Fermi surface. The projected odd-parity pseudospin-triplet gap, with the universal factor iσ2i\sigma_2 suppressed, has the structure

Δk(t)=d⃗k⋅σ⃗=(0d−(k)d+(k)0)(57)\Delta^{(t)}_{\mathbf{k}}=\vec{d}_{\mathbf{k}}\cdot\vec{\sigma}= \begin{pmatrix} 0 & d_-(\mathbf{k})\\ d_+(\mathbf{k}) & 0 \end{pmatrix} \tag*{(57)}

where d±(k)=dx(k)±idy(k)d_{\pm}(\mathbf{k})=d_x(\mathbf{k})\pm id_y(\mathbf{k}), If we rewrite the pairing Hamiltonian in terms of the quasiparticle creation operators, ak,σ†a^\dagger_{\mathbf{k},\sigma},

ak,σ†[d⃗k⋅σ⃗(iσ2)]σ,σ′a−k,σ′†=a^\dagger_{\mathbf{k},\sigma}\left[\vec{d}_{\mathbf{k}}\cdot\vec{\sigma}(i\sigma_2)\right]_{\sigma,\sigma'}a^\dagger_{-\mathbf{k},\sigma'}=
(d+(k)ak,↑†a−k,↓†−d−(k)ak,↑†a−k,↑†)(58)\left(d_{+}(\mathbf{k})a^\dagger_{\mathbf{k},\uparrow}a^\dagger_{-\mathbf{k},\downarrow}-d_{-}(\mathbf{k})a^\dagger_{\mathbf{k},\uparrow}a^\dagger_{-\mathbf{k},\uparrow}\right) \tag*{(58)}

Thus the off-diagonal structure of the reduced gap matrix corresponds, after multiplication by iσ2i\sigma_{2}, to diagonal equal pseudospin pairing amplitudes Δ^↑↑=−d−\hat{\Delta}_{\uparrow\uparrow}=-d_{-} and Δ^↓↓=d+\hat{\Delta}_{\downarrow\downarrow}=d_{+}. These are pseudospin labels, not necessarily the physical electron spin quantum numbers. Fig. 8 shows the variation of d⃗k\vec{d}_{\mathbf{k}} around the Fermi surface. To a good approximation Δ↓↓(k)=dx(k)+idy(k)∝icos⁡(2θ)e−iθ\Delta_{\downarrow\downarrow}(\mathbf{k})=d_{x}(\mathbf{k})+id_{y}(\mathbf{k})\propto i\cos(2\theta)e^{-i\theta} is a product of a dd-wave and pp-wave gap function. We can decompose this into Δ↓↓(k)∝(eiθ+e−3iθ)\Delta_{\downarrow\downarrow}(\mathbf{k})\propto(e^{i\theta}+e^{-3i\theta}), corresponding to angular harmonics of winding numbers +1+1 and −3-3 (often described as pp- and ff-wave components); the crystalline representation is determined by the full tetragonal symmetry. In the tetragonal point group approximation, the uniform intralayer gap cos⁡kx−cos⁡ky\cos k_{x}-\cos k_{y} belongs to B1gB_{1g} of D4hD_{4h}. For the projected staggered state, the approximate form d⃗k∝(cos⁡kx−cos⁡ky)(sin⁡ky,−sin⁡kx,0)\vec{d}_{\mathbf{k}}\propto(\cos k_{x}-\cos k_{y})(\sin k_{y},-\sin k_{x},0) is odd under inversion, changes sign under a fourfold rotation, and is even under a vertical mirror when the axial vector transformation of d⃗\vec{d} is included. It therefore transforms as B1uB_{1u} in this pseudospin convention. This identification is for the displayed leading harmonic; a complete space group classification must also account for the nonsymmorphic sublattice representation and the momentum dependent pseudospin gauge. The interesting feature of the d⃗k\vec{d}_{\mathbf{k}} vector is that it lies in the basal plane, and this makes the resulting triplet state robust against fields along the zz-axis. This projected symmetry is consistent with the analysis of Ishizuka et al. [14], who classified candidate superconducting gaps in CeRh2_2As2_2 using electronic structure calculations and crystalline symmetry. For a magnetic field along the cc axis, the relevant point group classification is reduced to C4hC_{4h}; the leading B1uB_{1u} gap identified above belongs to its BuB_{u} sector. In particular, their staggered spin singlet BuB_{u} basis includes kx2−ky2k_{x}^{2}-k_{y}^{2}, the long wavelength limit of our cos⁡kx−cos⁡ky\cos k_{x}-\cos k_{y} form factor. Our projected gap d⃗k∝(cos⁡kx−cos⁡ky)(sin⁡ky,−sin⁡kx,0)\vec{d}_{\mathbf{k}}\propto(\cos k_{x}-\cos k_{y})(\sin k_{y},-\sin k_{x},0) provides a higher harmonic realization of the same BuB_{u} symmetry class. The diagonal zeros of this leading form factor need not be enforced for every gap in that representation. The approaches are complementary: their work establishes crystalline symmetry constraints and possible topological properties, whereas our Kondo lattice calculation provides a microscopic mechanism for the emergence of the projected pseudospin triplet structure. This agreement at the point group level does not replace a full nonsymmorphic analysis of our heavy band gap.

Physical origin of the triplet gap

The origin of this pseudospin triplet structure can be understood physically by considering the bonding and antibonding combinations of ff states on neighboring Ce layers. In the absence of staggered spin orbit coupling, the heavy quasiparticle bands are approximately eigenstates of the interlayer hopping matrix α1\alpha_{1}, with eigenvalues ±1\pm1. Since {α1,α3}=0\{\alpha_{1},\alpha_{3}\}=0, the staggered pairing and staggered spin-orbit coupling, both proportional to α3\alpha_{3}, are off-diagonal in this approximate band basis.

Virtual transitions between the low energy Fermi surface and higher energy quasiparticle bands then generate an effective intraband pairing interaction. To leading order, this contribution has the symmetry of the product of the staggered dd-wave pairing and the staggered Rashba spin orbit coupling:

Δeff(k)∼WVΔδEk(cx−cy)(syσx−sxσy),(59)\Delta_{\mathrm{eff}}(\mathbf{k})\sim\frac{WV\Delta}{\delta E_{\mathbf{k}}}(c_{x}-c_{y})(s_{y}\sigma_{x}-s_{x}\sigma_{y}), \tag*{(59)}

where δEk\delta E_{\mathbf{k}} denotes the characteristic energy separation between the bands. The two staggered factors combine through α32=1\alpha_{3}^{2}=1, producing a sublattice even, momentum odd pseudospin triplet gap.

This mechanism illustrates how an odd-parity pseudospin triplet superconducting state can emerge from staggered spin singlet pairing in the presence of locally broken inversion symmetry. More generally, analogous processes may occur in multi sublattice superconductors where staggered pairing interacts with staggered spin orbit coupling.

Conclusion

In this work we have developed a Kondo lattice framework for the field induced parity transition for the heavy fermion superconductor CeRh2_2As2_2. Our central result combines the Kondo hybridization and local inversion symmetry breaking which provides a microscopic mechanism by which the two sublattice structure of CeRh2_2As2_2 can generate nearly competing superconducting states of opposite parity. Local inversion symmetry breaking at the Ce sites generates a new onsite spin flip hybridization which combines with the non local odd parity hybridization to generate a staggered antisymmetric spin orbit coupling (ASOC). For pairing driven by antiferromagnetic exchange interaction within the Ce layers, the uniform and staggered solutions are then determined by how they transform under inversion, which are even and odd respectively. In this model, the uniform intralayer dd-wave pairing produces the low field, even parity state, while the staggered intralayer dd-wave pairing with opposite signs of the pairing gap between the two Ce sublattices produces the high field, odd-parity pseudospin-triplet state after projection onto the heavy quasiparticle bands. A magnetic field along the cc axis suppresses the uniform phase much more strongly than the staggered phase leading to the field induced phase transition between the two superconducting phases.

Projection onto the normal state describing the heavy Fermi surface further shows an important consequence of the two pairing states. Although the underlying interaction was decoupled through an intralayer spin singlet dd-wave pairing, the staggered state projected onto the Fermi surface reveals odd parity pseudospin triplet gap structure with an in-plane d⃗k\vec{d}_k vector. The resulting odd parity state is not affected by the cc-axis magnetic field as the d⃗k⊥Bz\vec{d}_k \perp B_z. More generally, this illustrates that in a locally noncentrosymmetric Kondo lattice system, the spin, sublattice and parity structure of the microscopic pairing mechanism cannot be thought of independently. The interplay between the Kondo hybridization and ASOC can modify the structure of superconducting gap function when it is projected onto the normal state heavy quasiparticle basis. The key physics here is not to identify the particular dd- or pp-wave pairing interaction within the layers, but rather a mechanism by which the locally broken inversion symmetry with the two sublattice structure leads to a closely competing superconducting states with opposite global parity.

This distinction is particularly important because the microscopic pairing symmetry of CeRh2_2As2_2 has not yet been established experimentally. We have assumed that antiferromagnetic exchange favours an in-plane dd-wave singlet pairing, but an intrinsic spin triplet pairing interaction is also possible. Indeed, a Hund’s–Kondo mechanism has been proposed in which valence fluctuations into high spin configurations generate triplet correlations, with the two sublattice structural motif allowing these correlations to acquire an odd parity form factor on the heavy Fermi surface [28]. Starting from an intralayer triplet pairing rather than a singlet state would alter the correspondence between the uniform/staggered sublattice structure and the parity of the superconducting state, while retaining the central importance of the locally noncentrosymmetric environment. It is therefore an important open problem to repeat the present microscopic analysis allowing singlet and triplet pairing channels to compete on an equal footing. Measurements capable of determining the spin susceptibility and gap anisotropy in the two superconducting phases would be especially valuable in distinguishing the different possibilities.

A second direction is suggested by the recently discovered van der Waals heavy fermion material CeSiI. CeSiI provides a striking two dimensional realization of a Kondo lattice. Within a single van der Waals layer, two triangular Ce layers surround a conducting silicene layer, and heavy fermion coherence and magnetic order persist into the ultrathin limit [29, 30]. More recently, pressure has been shown to suppress the antiferromagnetic state and produce a superconducting dome, establishing CeSiI as a two dimensional heavy fermion superconductor [31]. Its two Cerium layer structure that naturally leads to the question whether a sublattice dependent Kondo hybridization can generate an analogous relation between local symmetry, ASOC and superconducting parity. Unlike CeRh2_2As2_2, however, the Ce ions form triangular layers surrounding a conducting silicene layer, so the microscopic hybridization form factors and crystal symmetry are distinct. Extending the current Kondo lattice framework to the actual symmetry and electronic structure of CeSiI would therefore test which aspects of the parity switching mechanism are generic to a two sublattice Kondo lattice system and which are specific to a noncentrosymmetric CeRh2_2As2_2. The ability to exfoliate, gate and assemble CeSiI into van der Waals heterostructure additionally raises the prospect of controlling the relative Kondo coupling of the two Ce layers and hence tuning the balance between competing superconducting states.

An equally revealing comparison is provided by β\beta-CeNi2_2As2_2. Recent work has established superconductivity in the CaBe2_2Ge2_2 isomorph of CeNi2_2As2_2, which is a structural analogue of CeRh2_2As2_2 and possesses the same essential locally noncentrosymmetric two sublattice structural motif [32]. Yet β\beta-CeNi2_2As2_2 does not display the characteristic field induced high field phase observed in CeRh2_2As2_2. This comparison to CeRh2_2As2_2 is important. It shows that the locally noncentrosymmetric crystal structure by itself is not sufficient to a field induced parity transition. Within the framework developed here, the occurrence of such a transition also depends on quantitative microscopic ingredients. These are the strength and momentum dependence of the Kondo hybridization, the resulting staggered ASOC, the interlayer coupling, the structure of the heavy Fermi surface, the pairing interaction, and the degree of nearly degenerate uniform and staggered superconducting states. A microscopic comparison of CeRh2_2As2_2 and β\beta-CeNi2_2As2_2 could provide a stringent test of the mechanism proposed here. Rather than asking only why CeRh2_2As2_2 has the high field phase, one can ask which microscopic ingredient present in CeRh2_2As2_2, but absent or weaker in β\beta-CeNi2_2As2_2, is responsible for the high field phase.

A further challenge is to establish the superconducting symmetry classification at the full nonsymmorphic space group level. The assignments discussed here are based on the tetragonal point-group transformation properties of the leading gap form factors and their projected pseudospin structure. A complete analysis for P4/nmmP4/nmm must additionally track the fractional translations, the sublattice dependent Bloch phases, and the momentum dependent symmetry sewing matrices of the heavy quasiparticle bands, especially near Brillouin zone boundaries. Such a treatment would test the robustness of the proposed irreducible representation assignments and clarify any symmetry enforced constraints on the gap nodes.

There remain further unresolved questions within CeRh2_2As2_2 itself. The superconductivity develops in close proximity to an additional ordered phase, Phase I whose microscopic origin remains uncertain, and antiferromagnetic order has also been reported at temperatures below TcT_c [3, 15, 33, 34]. Understanding how these orders couple to the two superconducting phases may be important for a quantitative theory of the phase diagram. Similarly, the anomalous normal state transport and indications of a non Fermi liquid behavior suggests that the superconductivity develops from a strongly correlated normal state close to quantum criticality [35]. These effects lie beyond the static mean field treatment used here and motivate extensions in which the Kondo coherence, magnetic fluctuations and superconducting instability are treated on an equal footing.

Our results suggest a broader perspective for locally noncentrosymmetric heavy fermion superconductors. The essential ingredient identified here is the interplay between Kondo hybridization with the crystal structure where the inversion exchanges two locally noncentrosymmetric magnetic atoms. This structure allows local parity breaking to become encapsulated as a staggered ASOC of the heavy quasiparticles and provides a natural route to competing superconducting states of opposite global parity. CeSiI and β\beta-CeNi2_2As2_2 now provide complementary tests of this idea. CeSiI extends the problem toward a tunable two dimensional Kondo lattice, while the β\beta-CeNi2_2As2_2 enables an isostructural superconducting control system in which the high field phase is absent. Together with a systematic treatment of intrinsic triplet as well as singlet pairing, these materials should help determine whether the mechanism presented here is peculiar to CeRh2_2As2_2 or forms part of a more general organizing principle for unconventional superconductivity in two sublattice Kondo lattices.

Acknowledgments

We gratefully acknowledge discussions David Vanderbilt, Kevin Lucht, Andreas Gleis, Po-Jui Chen, Liam Lau, Elena Hassinger, Joerg Schmalian, Daniel Schultz and particularly, Philip Brydon. The early part of the work in this paper was completed under the support from the Division of Materials Research, US National Science Foundation grant DMR-1830707(PC). We acknowledge support from the US National Science Foundation (NSF) Grant Number 2201516 under the Accelnet program of Office of International Science and Engineering (OISE)

Symplectic decoupling of the Heisenberg interaction

Here we derive the dot product of the spins in the Heisenberg interaction. More specifically, the fermionic form of the Heisenberg interaction used in Eq. (29) will be obtained. The main framework for the symplectic NN construction comes from the work [20]. For an even NN, the spin can have NN number of components:

σ=±1,…,±N/2,(60)\sigma= \pm1,\ldots,\pm N/2, \tag*{(60)}

and the antisymmetric tensor which time-reverses the spins is

ϵσσ′=σ~δσ,−σ′,σ~≡sgn⁡(σ).(61)\epsilon_{\sigma\sigma'} = \widetilde{\sigma}\delta_{\sigma,-\sigma'},\qquad\widetilde{\sigma} \equiv\operatorname{sgn}(\sigma). \tag*{(61)}

There are N(N+1)/2N(N+1)/2 components of Hermitian spin generators SaS^a in the Sp⁡(N)\operatorname{Sp}(N) subgroup. These symplectic spin generators are odd under time reversal operation:

Sa=−ϵ(Sa)TϵT,(62)S^a = -\epsilon(S^a)^T \epsilon^T, \tag*{(62)}

The normalization condition of the symplectic spin generators are defined as:

Tr⁡(SaSb)=2δab.(63)\operatorname{Tr}\left(S^aS^b\right)=2\delta^{ab}. \tag*{(63)}

The spin in terms of the fermionic operator and symplectic spin generator is given by:

S^ia=fiα†Sαβafiβ,(64)\widehat{S}_i^a=f_{i\alpha}^{\dagger}S_{\alpha\beta}^a f_{i\beta}, \tag*{(64)}

In this convention, there is no additional factor of 1/2. For completeness, we now derive the Fierz identity used for decoupling the spin. An arbitrary N×NN\times N matrix AA can be decomposed into parts that are odd and even under time reversal as A=AS+AAA=A_S+A_A, where

AS=−ϵASTϵT,AA=+ϵAATϵT.(65)A_S=-\epsilon A_S^T\epsilon^T,\qquad A_A=+\epsilon A_A^T\epsilon^T. \tag*{(65)}

The projector onto the symplectic subspace which has the property that inverts under time reversal is therefore

PSA=12(A−ϵATϵT).(66)P_SA=\frac{1}{2}\left(A-\epsilon A^T\epsilon^T\right). \tag*{(66)}

Here PSP_S represents the projector onto the symplectic subgroup. Writing this relation in component form,

(PSA)αβ=PγδαβAγδ,(67)(P_SA)^{\alpha\beta}=P_{\gamma\delta}^{\alpha\beta}A^{\gamma\delta}, \tag*{(67)}

then it follows from (A7) that

(PS)γδαβ=12(δαδδβγ−ϵαγϵβδ).(68)(P_S)_{\gamma\delta}^{\alpha\beta}=\frac{1}{2}\left(\delta_{\alpha\delta}\delta_{\beta\gamma}-\epsilon_{\alpha\gamma}\epsilon_{\beta\delta}\right). \tag*{(68)}

The same projector PGP_G can be expanded in terms of the symplectic part consisting of the complete set of Symplectic NN generators,

AS=∑acaSa.(69)A_S=\sum_a c_aS^a. \tag*{(69)}

Using the normalisation Tr⁡(SaSb)=2δab\operatorname{Tr}(S^aS^b)=2\delta_{ab} leads to

ca=12Tr⁡(ASSa)=12Tr⁡(ASa),(70)c_a=\frac{1}{2}\operatorname{Tr}(A_SS^a)=\frac{1}{2}\operatorname{Tr}(AS^a), \tag*{(70)}

where the second equality comes from the fact that the symplectic and antisymplectic subgroups are orthogonal to each other. Then using the definition of the prefactors the projection onto the symplectic subgroup in terms of components:

(PSA)γδαβ=12∑aSαβaTr⁡(ASa)(71)(P_SA)_{\gamma\delta}^{\alpha\beta}=\frac{1}{2}\sum_a S_{\alpha\beta}^{a} \operatorname{Tr}(AS^a) \tag*{(71)}
=12∑aSαβaSγδa.(72)=\frac{1}{2}\sum_a S_{\alpha\beta}^{a}S_{\gamma\delta}^{a}. \tag*{(72)}

Then the projector PGP_G in terms of the spin generator representation has the form:

(PS)γδαβ=12∑aSαβaSγδa.(73)(P_S)_{\gamma\delta}^{\alpha\beta} = \frac{1}{2}\sum_a S_{\alpha\beta}^{a}S_{\gamma\delta}^{a}. \tag*{(73)}

Combining both the definition of the projector in Eq. (68) and Eq. (73) leads to the symplectic completeness relation:

∑a=1N(N+1)/2SαβaSγδa=δαδδβγ−ϵαγϵβδ.(74)\sum_{a=1}^{N(N+1)/2}S_{\alpha\beta}^{a}S_{\gamma\delta}^{a}=\delta_{\alpha\delta}\delta_{\beta\gamma}-\epsilon_{\alpha\gamma}\epsilon_{\beta\delta}. \tag*{(74)}

This is the Fierz identity for the SP(NN) generators. The second term imposes the inversion of spins under the time reversal operation.

In the main text which uses the large-NN treatment, the Heisenberg interaction with the rescaled interaction has the explicit form:

HH=JHN∑⟨ij⟩∑aS^iaS^ja.(75)H_H=\frac{J_H}{N}\sum_{\langle ij\rangle}\sum_a \hat{S}_{i}^{a}\hat{S}_{j}^{a}. \tag*{(75)}

Using the completeness relation in Eq. (74), and normal ordering fermions on the two different sites leads to:

HH=−JHN∑⟨ij⟩,σσ′[fjσ†fiσfiσ′†fjσ′+σ~σ′~fiσ†fj,−σfj,−σ′†fiσ′].(76)H_H=-\frac{J_H}{N}\sum_{\langle ij\rangle,\sigma\sigma'}\left[f_{j\sigma}^{\dagger}f_{i\sigma}f_{i\sigma'}^{\dagger}f_{j\sigma'}+\widetilde{\sigma}\widetilde{\sigma'}f_{i\sigma}^{\dagger}f_{j,-\sigma}f_{j,-\sigma'}^{\dagger}f_{i\sigma'}\right]. \tag*{(76)}

where σ,σ′=±1,…,±N/2\sigma,\sigma'=\pm1,\ldots,\pm N/2 which are the spin components. This is the decoupled Heisenberg interaction in Eq. (29) of the main text. Physically, the two terms in Eq. (76) are the particle hole and particle particle channels respectively. It is useful to introduce the bond orientation operators:

Dji=∑σfjσ†fiσ,Pji=∑σσ~fj,−σfiσ.(77)D_{ji}=\sum_{\sigma}f_{j\sigma}^{\dagger}f_{i\sigma},\qquad P_{ji}=\sum_{\sigma}\widetilde{\sigma}f_{j,-\sigma}f_{i\sigma}. \tag*{(77)}

Since this is Hermitian construction, their Hermitian conjugates are given by:

Dji†=∑σfiσ†fjσ,Pji†=∑σσ~fiσ†fj,−σ†.(78)D_{ji}^{\dagger}=\sum_{\sigma}f_{i\sigma}^{\dagger}f_{j\sigma},\qquad P_{ji}^{\dagger}=\sum_{\sigma}\widetilde{\sigma}f_{i\sigma}^{\dagger}f_{j,-\sigma}^{\dagger}. \tag*{(78)}

Rewriting the Heisenberg interaction in terms of the bond operators leads to the simple form:

HH=−JHN∑⟨ij⟩(Dij†Dij+Pij†Pij).(79)H_H=-\frac{J_H}{N}\sum_{\langle ij\rangle}\left(D_{ij}^{\dagger}D_{ij}+P_{ij}^{\dagger}P_{ij}\right). \tag*{(79)}

Equation (A20) gives the explicit form of the SU(2) isospin structure of the symplectic-NN representation. The antiferromagnetic exchange interaction generates degenerate particle hole and particle particle singlet decoupling channels. Using a Hubbard Stratonovich decoupling of the two channels leads to the ff electron hopping and pairing fields used in the main text.

Charge conjugation transformation

We now show explicitly develop the Balian-Werthammer (BW) isospin structure used in the main text. The definitions of the fermionic operators used in the path integral formulation in the main text are:

Ck,α,σ=(ck,α,σck,α,−σ−c−k,α,−σ†c−k,α,σ†),Fk,α,σ=(fk,α,σfk,α,−σ−f−k,α,−σ†f−k,α,σ†),(80)C_{k,\alpha,\sigma}= \begin{pmatrix} c_{k,\alpha,\sigma}\\ c_{k,\alpha,-\sigma}\\ -c_{-k,\alpha,-\sigma}^{\dagger}\\ c_{-k,\alpha,\sigma}^{\dagger} \end{pmatrix}, \qquad F_{k,\alpha,\sigma}= \begin{pmatrix} f_{k,\alpha,\sigma}\\ f_{k,\alpha,-\sigma}\\ -f_{-k,\alpha,-\sigma}^{\dagger}\\ f_{-k,\alpha,\sigma}^{\dagger} \end{pmatrix}, \tag*{(80)}

with σ>0\sigma>0. The Pauli matrices τi\tau_i act in this particle hole also known as the isospin space. Combining the sublattice and the conduction and ff electron sectors leads to the spinor used in the mean field Hamiltonian,

Ψk=(Ck+Ck−Fk+Fk−).(81)\Psi_k= \begin{pmatrix} C_{k+}\\ C_{k-}\\ F_{k+}\\ F_{k-} \end{pmatrix}. \tag*{(81)}

To transform normal state bilinears of the form ak†A(k)aka_k^\dagger A(k)a_k into the Balian Werthammer form, we combine it with the corresponding hole component, obtained by charge conjugation. The Balian Werthammer representation of this operator then becomes:

A(k)⟶A(k)12(1+τ3)−σ2AT(−k)σ212(1−τ3).(82)A(k)\longrightarrow A(k)\frac{1}{2}(1+\tau_3)-\sigma_2A^{T}(-k)\sigma_2\frac{1}{2}(1-\tau_3). \tag*{(82)}

Now in general, operators are either even, or odd under time-reversal, so that

σ2AT(−k)σ2={+A(k)even,−A(k)odd,(83)\sigma_2A^{T}(-k)\sigma_2= \begin{cases} +A(k)&\text{even},\\ -A(k)&\text{odd}, \end{cases} \tag*{(83)}

then the corresponding operators in the Balian-Werthammer representation take the form

A(k)⟶{A(k)τ3even,A(k)odd.(84)A(k)\longrightarrow \begin{cases} A(k)\tau_3&\text{even},\\ A(k)&\text{odd}. \end{cases} \tag*{(84)}

For example, in the normal state the Hamiltonian contains a dispersion and a Zeeman term H(k)=HN(k)−σzBz\mathcal{H}(k)=H_N(k)-\sigma_zB_z. Since the first term is even under time-reversal, while the second is odd under time reversal, in the Balian Werthammer notation,

H(k)⟶HN(k)τ3−σzBz.(85)\mathcal{H}(k)\longrightarrow H_N(k)\tau_3-\sigma_zB_z. \tag*{(85)}

Thus, in the BW formulation, the normal-state Hamiltonian takes the form

H(k)=(hkτ3−σzBVϕ†(k)Vϕ(k)hkfτ3−σzB)(86)\mathcal{H}(k)= \begin{pmatrix} h_k\tau_3-\sigma_zB & V\phi^{\dagger}(k)\\ V\phi(k) & h_k^f\tau_3-\sigma_zB \end{pmatrix} \tag*{(86)}

which accounts for the form used in (39) of the main text.

References

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