Introduction

Altermagnetism, distinct from ferromagnetism and antiferromagnetism, exhibits zero net magnetization with momentum-dependent collinear spin textures1,2,3,4,5,6,7,8,9,10,11,12,13. Analogous to unconventional superconductors, it establishes a profound connection between magnetism and topology, hosting nonzero Berry curvature for anomalous Hall transport2,14,15,16,17,18,19,20,21. The momentum-dependent spin splitting serves as a intrinsic platform for spin-current coupling22, enabling practical control in spin devices through the application of magnetic fields23,24, electrical currents1,25,26,27,28,29, strain30,31,32,33,34, torque35,36, and heat37,38. When coupled with superconductors, altermagnetism can induce intriguing phenomena39,40,41, such as the Fulde-Ferrell-Larkin-Ovchinnikov (FFLO) state42,43 and new platforms for enabling Majorana particles44.

As demonstrated through density functional theory (DFT)-based Hartree-Fock calculations3, the random phase approximation45, and analysis of Fermi surface Pomeranchuk instabilities3,46, altermagnetism is believed to be stabilized through strong on-site Coulomb interactions. Searches for this strong coupling instability form the basis for identifying new altermagnetic materials. In principle, in 2D, Van Hove singularities offer a weak coupling route towards stabilizing altermagnetism. Van Hove singularities are saddle points in the energy dispersion and induce a logarithmic divergence in the 2D density of states. Tuning the chemical potential across such singularities results in divergent susceptibilities, signaling an instability into a variety of possible competing orders that have been examined in cuprates, graphene, and Kagome metals47,48,49,50,51,52,53,54,55,56,57,58,59,60,61,62. However, in these applications, altermagnetism is not one of these competing orders, suggesting that this route is not viable for stabilizing this state. Indeed, the closest relative to altermagnetism that has been found is a non-collinear variant that appears only for fine-tuned higher-order Van Hove singularities62.

In contrast to the strong-coupling mechanisms typically examined with RPA-like approaches, here we identify a weak-coupling mechanism based on usual 2D logarithmic Van-Hove singularities that stabilize altermagnetism. Two ingredients are key to realizing this mechanism. The first is the existence of a pair of Van Hove singularities that are coincident in both energy and momentum. The second, which does not hold for all coincident Van Hove singularites, is a specific symmetry property of the Hamiltonian, which give rise to a new hopping interaction between these Van Hove singularities. This hopping interaction does not appear in Van Hove-based patch models for cuprates50,51,52,53 and graphene47,48,49,62 where it is forbidden by translation invariance. Both ingredients are a generic consequence of non-symmorphic symmetries that exist in nine 2D space groups, when spin-orbit coupling is neglected. Furthermore, unlike the Van Hove driven spin density wave transitions that occur in cuprate50,51,52,53, graphene47,48,49,62, and Kagome metal54 patch models, our altermagnetic mechanism does not require nesting or near-nesting of the bands. Instead, it is based on the BCS instability, which typically yields only a superconducting instability for the other Van Hove singularity scenarios. Our analysis also stabilizes other orders including interband d-wave superconductivity, nematicity, and orbital altermagnetism. To be concrete, we apply our analysis to the organic material κ-Cl where an altermagnetic state is believed to occur.

Results

Coincident Van Hove singularities

The phase diagram of the quasi-2D orthorhombic organic compound κ-(ET)2Cu[N(CN)2]Cl (κ-Cl, 2D layer group L25 (pba2)) shares similarities with cuprates63, exhibiting unconventional superconductivity adjacent to magnetism under pressure64,65,66 and anion substitution67,68,69,70,71,72,73,74. Previous theoretical studies, largely based on strong coupling RPA-like calculations, reveal superconducting and altermagetic states75,76,77. DFT calculations reveal a Van Hove singularity at the S = (ππ) point78. Recently, considerable hole-doping has been achieved in κ-Cl79. As the Van Hove singularity is approached, a substantial reduction in spectral weight is observed, revealing the importance of electronic correlations79. Here we show that this Van Hove singularity consists of a pair of Van Hove singularities that are coincident in both energy and momentum, and also satisfies the symmetry conditions that allow the new hopping interaction mentioned above. We also show that in the vicinity of the Van Hove singularity, interactions that fall outside of RPA-like approaches drive a weak-coupling instability to altermagnetism and other novel states.

For pedagogical purposes, we start with a tight-binding Hamiltonian. A general group theory analysis can be found later. κ-Cl has four ET molecules per unit cell, forming two molecule-dimers (Fig. 1) at positions: (r1r2) = {(0, 0), (1/2, 1/2)}. As a minimal model capturing the coincident Van Hove singularities, we consider one orbital on each dimer position. The Pauli matrices τi act in dimer (or sublattice) space and the Pauli matrices σi act in spin space. While spin-orbit coupling (SOC) is negligible1,78, the normal state tight-binding Hamiltonian is:

$$H= 2{t}_{1}\cos {k}_{x}+2{t}_{2}\cos {k}_{y}+4{t}_{3}\cos {k}_{x}\cos {k}_{y}\\ +4{t}_{4}\cos \frac{{k}_{x}}{2}\cos \frac{{k}_{y}}{2}{\tau }_{x}+{t}_{5}\sin {k}_{x}\sin {k}_{y}{\tau }_{z}-\mu .$$
(1)

Here, τx term describes inter-sublattice hopping (thick black arrows in Fig. 1). τz term captures the difference in intra-sublattice hopping between (1, 1) and (1, − 1) directions (solid/dashed red arrows in Fig. 1), which is opposite on the two sublattices. Each band is doubly degenerate, consisting of spin-up and down states. Due to the nonsymmorphic symmetries, the band without SOC is 4-fold degenerate at the entire Brillouin zone boundary kx = π and ky = π80. Near the Brillouin zone corner S=(ππ), where the coincident Van Hove singularities appear, we obtain the kp Hamiltonian:

$$H(\pi+{k}_{x},\pi+{k}_{y})={t}_{x}{k}_{x}^{2}+{t}_{y}{k}_{y}^{2}+{k}_{x}{k}_{y}({t}_{4}{\tau }_{x}+{t}_{5}{\tau }_{z})-\widetilde{\mu },$$
(2)

with \(\widetilde{\mu }=\mu+2{t}_{1}+2{t}_{2}-4{t}_{3}\), tx = (t1 − 2t3), and ty = (t2 − 2t3). This expansion reveals a central property of all the theories we examine here, both the operators τx and τz are multiplied by the momentum function kxky. Since the Hamiltonian must be invariant under all orthorhombic symmetries, this implies that both τx and τz share the same symmetry as kxky at the S point. A group theory analysis (given in detail later) applied to the momentum points and 2D and 3D space groups in Table 1 reveals that the kp-theory of Eq. (2) also appears in these cases and has the most general form allowed by symmetry (for the 3D groups, a term \({a}_{z}{k}_{z}^{2}\) is also allowed, and the physics discussed here occurs in the quasi-2D limit, where az is small relative to tx and ty). The other non-trivial sublattice operator τy is time-reversal odd, but invariant under all crystal symmetries. τy can only appear in a Hamiltonian multiplied by spin-1/2 operators80 as a SOC term. Here we ignore SOC and include a discussion of its effects in the appendix.

Fig. 1: Crystal structure.
Fig. 1: Crystal structure.
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a Hopping parameters. b Altermagnet where arrows represent spins. c Orbital altermagnet where arrows represent currents (even-parity current loop order). We name this state an orbital altermagnet since the local moments induced by the current loops form an altermagnet (which has the same symmetries as the altermagnet depicted in (b)).

Table 1 2D layer groups and 3D space groups87,88 hosting the kp Hamiltonian in Eq.(2) at quadratic level

The resulting dispersions of the two bands are

$${E}_{1,2}={t}_{x}{k}_{x}^{2}+{t}_{y}{k}_{y}^{2}\pm \sqrt{{t}_{4}^{2}+{t}_{5}^{2}}{k}_{x}{k}_{y}-\widetilde{\mu }.$$
(3)

The saddle point conditions for these two dispersions are the same: \({t}_{4}^{2}+{t}_{5}^{2}+{({t}_{x}-{t}_{y})}^{2} > {({t}_{x}+{t}_{y})}^{2}\). Consequently, each band hosts a Van Hove singularity at the band crossing point S = (ππ).

In the following, we work in the band basis for which the kp Hamiltonian, Eq. (2) is diagonal. To diagonalize the kp Hamiltonian, we take a k-independent unitary transformation \(u=\cos (\theta /2)I-i\sin (\theta /2){\tau }_{y}\) where \(\cos \theta={t}_{5}/\sqrt{{t}_{4}^{2}+{t}_{5}^{2}}\). In the band basis, \(\widetilde{{\tau }_{y}}\) is unchanged from τy in the sublattice basis. \(\widetilde{{\tau }_{x}}\) and \(\widetilde{{\tau }_{z}}\) in the band basis are linear combinations of τx and τz, with \(\widetilde{{\tau }_{x}}=\cos \theta {\tau }_{x}-\sin \theta {\tau }_{z}\) and \(\widetilde{{\tau }_{z}}=\sin \theta {\tau }_{x}+\cos \theta {\tau }_{z}\). Since τx,z have the same symmetry and θ is a constant, \(\widetilde{{\tau }_{x,z}}\) should remain the same symmetry as kxky. As interactions can be constructed from multiplying Fermionic bilinears with the same symmetry, this indicates the existence of a new interaction term with respect to kp theories in which τx and τz have different symmetries.

Patch model and interactions

The coincident Van Hove singularities provide a novel platform to study strongly interacting fermions and a natural mechanism for stabilizing 2D altermagnetism. To understand this, it is useful to consider a patch model50. Here, the density of states (DOS) of each band is approximated as a patch situated solely at the Van Hove point. With a Van Hove singularity on each band, we end up with two DOS patches located at the same point: (ππ), as shown in Fig. 2. This patch model has similarities with that examined for cuprates. For cuprates, there are also two Van Hove singularities, but these Van Hove singularities are not coincident and appear at the two distinct momenta (0, π) and (π, 0). The key difference between patch models for coincident Van Hove points and those for the cuprates is in the interactions allowed by symmetry. Both models contain the standard interactions g1, g2, g3, and g4. However, our coincident Van Hove patch model contains a new hopping interaction, g5, shown in Fig. 3

Fig. 2: Density of states is concentrated near the band crossing point (ππ), where the two bands are shown in different colors.
Fig. 2: Density of states is concentrated near the band crossing point (π, π), where the two bands are shown in different colors.
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In the patch model, states on the red band are replaced by a single point at (ππ), while states on the blue band are replaced by another point at (ππ). Here, we take t1 = t2 = t5 = 1, t3 = 0, t4 = 8, and μ = − 4. 20002 points are sampled, and states with energy (E < 0.1) are plotted.

Fig. 3: Allowed interactions for two coincident patches.
Fig. 3: Allowed interactions for two coincident patches.
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af The exchange interaction g1, inter-patch Hubbard interaction g2, pair-hopping interaction g3, intra-patch Hubbard interaction g4, and the new hopping interaction g5. Here, upper propagators are for spin-up, while lower ones are for spin-down. Solid& dashed lines label bands 1 and 2.

This g5-interaction involves a hopping between the two bands (DOS patches) which, due to momentum conservation, is permissible only when two patches coincide. The existence of coincident Van Hove singularities is not sufficient for the existence of the g5 interaction. Additionally, the Hamiltonian must satisfy the symmetry condition discussed just below Eq. 2 that \({\widetilde{\tau }}_{x}\) and \({\widetilde{\tau }}_{z}\) have the same symmetry. To demonstrate this, we use Cooper pair operators to derive the g5 interaction. Cooper pair operators are convenient since they automatically encode the Pauli exclusion principle. The interactions in Fig. 3 involve annihilating two electrons (a Cooper pair) from the left and then creating another Cooper pair with the same symmetry to the right. For g5, the corresponding Cooper pairs are \(\widetilde{{\tau }_{x}}i{\sigma }_{y}:{\Delta }_{xy,1}={c}_{2\downarrow }{c}_{1\uparrow }+{c}_{1\downarrow }{c}_{2\uparrow }\) and \(\widetilde{{\tau }_{z}}i{\sigma }_{y}:{\Delta }_{xy,2}={c}_{1\downarrow }{c}_{1\uparrow }-{c}_{2\downarrow }{c}_{2\uparrow }\) (here 1 and 2 in Fermionic operators label the bands). Since these two Cooper pairs share the same symmetry, the interaction \({g}_{5}{\Delta }_{xy,1}^{{{\dagger}} }{\Delta }_{xy,2}\) is symmetry allowed. If the \({\tilde{\tau }}_{x}\) and \({\tilde{\tau }}_{z}\) operators had different symmetries, this interaction would be symmetry forbidden. Expanding \({g}_{5}{\Delta }_{xy,1}^{{{\dagger}} }{\Delta }_{xy,2}\) yields

$${H}_{{g}_{5}}^{int}={{g}_{5}({c}_{2\downarrow }{c}_{1\uparrow }+{c}_{1\downarrow }{c}_{2\uparrow })}^{{{\dagger}} }({c}_{1\downarrow }{c}_{1\uparrow }-{c}_{2\downarrow }{c}_{2\uparrow })+h.c.$$
(4)

In the two g5 panels in Fig. 3, the two input electrons from the left annihilates the Cooper pair Δxy,2, and the two output electrons to the right creates the Cooper pair \({\Delta }_{xy,1}^{{{\dagger}} }\). The sign difference on the two bands in Δxy,2 results in the sign difference between the two  ± g5 panels.

The g5 interaction can be generated by an on-site Hubbard interaction after transforming to the band basis, so its magnitude can be large. In particular, for the interaction

$${H}_{{{{\rm{int}}}}}=U{\sum}_{m}{n}_{m\uparrow }{n}_{m\downarrow },$$
(5)

where m denotes the sublattice index, we find its components in the band basis (denoted by \({g}_{i}^{0}\)): \({g}_{1}^{0}={g}_{2}^{0}={g}_{3}^{0}=(U/2){\sin }^{2}\theta\), \({g}_{3}^{0}+{g}_{4}^{0}=U\), \({g}_{4}^{0}-{g}_{3}^{0}=U{\cos }^{2}\theta\), and \({g}_{5}^{0}=(U/2)\sin \theta \cos \theta\). Recall \(\cos \theta \equiv {t}_{5}/\sqrt{{t}_{4}^{2}+{t}_{5}^{2}}\), the existence of g5 thus requires both kxky(t4τx + t5τz) terms in the dispersion. In single-band cuprates, even if we fold the Brillouin zone such that the two Van Hove singularities coincide, g5 will still vanish as it corresponds to θ = π/2.

When the chemical potential is tuned close to the Van Hove singularity, the enhancement in the density of states results in substantial corrections to interaction strengths. These corrections originate through the intra- and inter-band particle-particle (\({\chi }_{pp}^{intra}\), \({\chi }_{pp}^{inter}\)) and particle-hole (\({\chi }_{ph}^{intra}\), \({\chi }_{ph}^{intra}\)) susceptibilities for the free fermions47,48,49,50,51,52,53,54,55,56,57,58,59,60,61. Here, these susceptibilities are

$$\begin{array}{rcl}&&{\chi }_{ph}^{intra}=-{\lim }_{{{{\bf{q}}}}\to 0}\frac{1}{N}{\sum }_{{{{\bf{k}}}}}\frac{f[{E}_{1}({{{\bf{k}}}})]-f[{E}_{1}({{{\bf{k+q}}}})]}{{E}_{1}({{{\bf{k}}}})-{E}_{1}({{{\bf{k+q}}}})}\\ &&{\chi }_{ph}^{inter}=-{\lim }_{{{{\bf{q}}}}\to 0}\frac{1}{N}{\sum }_{{{{\bf{k}}}}}\frac{f[{E}_{1}({{{\bf{k}}}})]-f[{E}_{2}({{{\bf{k+q}}}})]}{{E}_{1}({{{\bf{k}}}})-{E}_{2}({{{\bf{k+q}}}})}\\ &&{\chi }_{pp}^{intra}=-{\lim }_{{{{\bf{q}}}}\to 0}\frac{1}{N}{\sum }_{{{{\bf{k}}}}}\frac{f[{E}_{1}(-{{{\bf{k}}}}))-f(-{E}_{1}({{{\bf{k+q}}}})]}{{E}_{1}(-{{{\bf{k}}}})+{E}_{1}({{{\bf{k+q}}}})}\\ &&{\chi }_{pp}^{inter}=-{\lim }_{{{{\bf{q}}}}\to 0}\frac{1}{N}{\sum }_{{{{\bf{k}}}}}\frac{f[{E}_{1}(-{{{\bf{k}}}})]-f[-{E}_{2}({{{\bf{k+q}}}})]}{{E}_{1}(-{{{\bf{k}}}})+{E}_{2}({{{\bf{k+q}}}})},\end{array}$$
(6)

where f[E] is the Fermi Dirac distribution. The dominant corrections stem from \({\chi }_{pp}^{intra}\). This is because \({\chi }_{pp}^{intra}\) exhibits the conventional BCS logarithmic divergence multiplied by the logarithmic divergence in the density of states (\({\chi }_{pp}^{intra}\) diverges as \({\log }^{2}\Lambda /T\)) while other susceptibilities only exhibit the latter and hence diverge as \(\log \Lambda /T\). Keeping only the dominant interaction corrections, the one-loop BCS corrections to the interactions are:

$$\begin{array}{rcl}&&\Delta {g}_{1}=-2{\chi }_{pp}^{intra}{g}_{5}^{2}\\ &&\Delta {g}_{2}=-2{\chi }_{pp}^{intra}{g}_{5}^{2}\\ &&\Delta {g}_{3}=-2{\chi }_{pp}^{intra}{g}_{3}{g}_{4}\\ &&\Delta {g}_{4}=-{\chi }_{pp}^{intra}({g}_{3}^{2}+{g}_{4}^{2})\\ &&\Delta {g}_{5}=-{\chi }_{pp}^{intra}({g}_{4}-{g}_{3}){g}_{5}\\ \to &&\left[\begin{array}{c}\Delta ({g}_{4}+{g}_{3})=-{\chi }_{pp}^{intra}{({g}_{4}+{g}_{3})}^{2}\\ \Delta ({g}_{4}-{g}_{3})=-{\chi }_{pp}^{intra}{({g}_{4}-{g}_{3})}^{2}\end{array}\right].\end{array}$$
(7)

Let us start with g5 = 0, then these equations are the same as those found in cuprate patch models50,52. Hence, a bare attractive \({g}_{4}^{0}+{g}_{3}^{0}\) (or \({g}_{4}^{0}-{g}_{3}^{0}\)) enhances itself and gives an intra-band s-wave superconducting Δ = iσy (or d-wave superconducting \(\Delta=i\widetilde{{\tau }_{z}}{\sigma }_{y}\)) instability. For onsite Hubbard interactions and generic θ, we have \({g}_{4}^{0} > {g}_{3}^{0} > 0\), causing the BCS correction to suppress these two instabilities.

The g5-interaction introduces new one-loop BCS corrections to the exchange interaction g1, and the inter-band Hubbard interaction g2, as shown in Fig. 4. The first diagram in panel (a) illustrates a correction to the exchange interaction g1. This correction involves two g5 interactions. This diagram features two internal solid lines moving in the same direction, which are evaluated to be the negative BCS susceptibility, \(-{\chi }_{pp}^{intra}\), from the first band. Similarly, the second diagram has two  − g5 interaction lines and a negative BCS susceptibility from the second band. These two diagrams thus add up to \(\Delta {g}_{1}=-2{\chi }_{pp}^{intra}{g}_{5}^{2}\) in Eq.(7). The two diagrams in panel (b) add up to \(\Delta {g}_{2}=-2{\chi }_{pp}^{intra}{g}_{5}^{2}\). Within BCS corrections, g5 does not affect g3,4.

Fig. 4: g5-interaction leads to intra-band particle-particle corrections.
Fig. 4: g5-interaction leads to intra-band particle-particle corrections.
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(a) The correction to g1. (b) The correction to  g2.

Notably, these corrections are always negative, regardless of the signs of interactions. This can drive g1,2 < 0. In the appendix, we consider a patch renormalization group study including subleading corrections, which are important as g4 − g3 vanish81. We consider the small g3,4 sector and explicitly show that BCS corrections from g5 can push the RG flow to stable fixed points with divergent g1,2 < 0.

Competing instabilities

The above discussion reveals that negative g1 and g2 can become the dominant interactions, and so we may neglect other interactions. We find that g1 and g2 generically lead to competing instabilities in the intra-band particle–hole, inter-band particle-hole, and inter-band particle-particle channels (Table 2). These instabilities are obtained from self-consistent one-loop vertex corrections in the appendix, and here are illustrated from a mean-field perspective. Specifically, d-wave altermagnetism \(\widetilde{{\tau }_{z}}\sigma\) requires an antiferromagnetic interaction between the two bands, which is contributed by the attractive inter-band Hubbard interaction g2 (marked in blue below):

$${S}_{1z}{S}_{2z} =({n}_{1\uparrow }-{n}_{1\downarrow })({n}_{2\uparrow }-{n}_{2\downarrow })\\ =-({n}_{1\uparrow }{n}_{2\downarrow }+{n}_{2\uparrow }{n}_{1\downarrow })+{n}_{1\uparrow }{n}_{2\uparrow }+{n}_{1\downarrow }{n}_{2\downarrow }$$
(8)

The altermagnetism is in the intra-band particle-hole channel, so the instability criteria is \({\chi }_{ph}^{intra}| {g}_{2}| > 1\), as shown in Table 2. Other instabilities include inter-band dxy superconductivity, ϵxy nematicity, and orbital altermagnetic order. These order parameters inherit non-trivial symmetries through the band degrees of freedom \(\widetilde{{\tau }_{i}}\), even though the coincident Van Hove singularity is located at a single momentum point. The orbital altermagnetic order \(\widetilde{{\tau }_{y}}\) is a current-loop order breaking time-reversal symmetry while preserving all crystal reflection symmetries (Fig. 1). This state will induce an anomalous Hall effect under the application of an ϵxy strain, even without the presence of SOC (a detailed explanation is in the appendix). When SOC is present, this current loop order and the conventional d-wave spin altermagnetic order \(\widetilde{{\tau }_{z}}{\sigma }_{z}\) will coexist as these two orders share the same symmetry. It is notable that the d-wave superconductivity we find is inter-band, and cannot be stabilized through a conventional BCS mechanism.

Table 2 Orders stabilized by coincident Van Hove points and corresponding symmetries and eigenvalues

While the one-loop correction for the interaction comes from the dominant intra-band particle-particle (BCS) channel, the one-loop correction for the vertices all belong to the three subleading channels. The ultimate leading instability can be determined by the magnitude of the three eigenvalues \({\chi }_{pp}^{inter}| {g}_{1}+{g}_{2}|\), \({\chi }_{ph}^{inter}| {g}_{1}|\) and \({\chi }_{ph}^{intra}| {g}_{2}|\). The three susceptibilities share the same scaling: \(\chi \propto \log {\Lambda }_{i}/T\), generically with different energy cutoff Λi. To examine what parameter range enables the different instabilities, we set the cutoffs in all three susceptibilities the same and consider the limit g1 = g2. This limit occurs when only BCS corrections from on-site Coulomb interactions are included but generally g1 ≠ g2. The results then depend upon the kp dispersion in Eq.(3). Figure 5 reveals that all instability channels are stable for some choice of \(a\equiv \frac{\sqrt{{t}_{4}^{2}+{t}_{5}^{2}}}{2{t}_{x}}\) (Van Hove dispersion requires a > 1). We note that once g1 > g2 (or g1 < g2), the inter-band (or intra-band) altermagnetic phase will expand.

Fig. 5: Susceptibilities \({\chi }_{pp}^{inter}\), \({\chi }_{ph}^{inter}\) and \({\chi }_{ph}^{intra}\), normalized with respect to \({\chi }_{ph}^{intra}\), with tx = ty and \(a\equiv \frac{\sqrt{{t}_{4}^{2}+{t}_{5}^{2}}}{2{t}_{x}}\).
Fig. 5: Susceptibilities 
                        
                          
                        
                        $${\chi }_{pp}^{inter}$$
                        
                          
                            
                              χ
                            
                            
                              p
                              p
                            
                            
                              i
                              n
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                      , 
                        
                          
                        
                        $${\chi }_{ph}^{inter}$$
                        
                          
                            
                              χ
                            
                            
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                              n
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                              e
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                       and 
                        
                          
                        
                        $${\chi }_{ph}^{intra}$$
                        
                          
                            
                              χ
                            
                            
                              p
                              h
                            
                            
                              i
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                              a
                            
                          
                        
                      , normalized with respect to 
                        
                          
                        
                        $${\chi }_{ph}^{intra}$$
                        
                          
                            
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                              p
                              h
                            
                            
                              i
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                              r
                              a
                            
                          
                        
                      , with tx = ty and 
                        
                          
                        
                        $$a\equiv \frac{\sqrt{{t}_{4}^{2}+{t}_{5}^{2}}}{2{t}_{x}}$$
                        
                          a
                          ≡
                          
                            
                              
                                
                                  
                                    
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                                  +
                                  
                                    
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                                      5
                                    
                                    
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                                  x
                                
                              
                            
                          
                        
                      .
Full size image

\(2{\chi }_{pp}^{inter}\) is plotted as the SC vertex is contributed by both g1 and g2. N = 20002 points are sampled, for kx,y [ − 5, 5]. Temperature T/tx = 0.01 is taken. q = (10−4, 0) is used in \({\chi }_{ph}^{intra}\). q = (0, 0) is used in \({\chi }_{ph}^{inter}\) and \({\chi }_{pp}^{inter}\).

It is worth noting that the above results are not captured by the standard random phase approximation (RPA). The RPA diagram is shown in panel (a) in Fig. 6. It gives the usual instability criteria \(| {g}_{2}| {\chi }_{ph}^{intra} > 1\) (topleft) and \(| {g}_{1}| {\chi }_{ph}^{inter} > 1\) (topright). The BCS instability for altermagnetism is equivalent to a two-loop correction described by panel (b). This diagram is derived from panel (a) by substituting the g2 interaction with its g5-correction in Fig. 4. The instability criteria is thus \(| \Delta {g}_{2}| {\chi }_{ph}^{intra}=2| {g}_{5}{| }^{2}{\chi }_{pp}^{intra}{\chi }_{ph}^{intra} > 1\). Since \({\chi }_{pp}^{intra}\gg {\chi }_{ph}^{intra},{\chi }_{ph}^{inter}\) at low temperature, the BCS correction from g5 describes a stronger weak-coupling instability. Since the g5 contributions exceed the RPA-based contributions in the weak-coupling limit, it is reasonable to include them beyond the conventional RPA-based contributions when addressing intermediate and strong coupling problems in future studies.

Fig. 6: Comparison of conventional and the g5 bubbles to magnetism.
Fig. 6: Comparison of conventional and the g5 bubbles to magnetism.
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a Conventional Stoner bubbles from g1,2, for intra-band and inter-band particle-hole channel. b Contribution through intra-band particle-particle channel from the g5 interaction. The two pairs of vertical propagators can be from both patches.

Our coincident Van Hove mechanism relies on the existence of a g5 hopping interaction and exclusively yields d-wave altermagnetic states. Given the discovery of g-wave altermagnetism82,83, it is interesting to ask if there exists a weak-coupling Van Hove scenario that stabilizes such a g-wave state. In the appendix we show that this is indeed possible for a different coincident Van Hove scenario that also applies to many of the space groups examined here. In this case, a momentum-dependent spin-splitting of the form \({k}_{x}{k}_{y}({k}_{x}^{2}-{k}_{y}^{2})\) is generated from coincident Van Hove singularities with a symmetry that forbid the existence of the g5 interaction. This Van Hove scenario can be mapped onto the patch model for the cuprates59 and this mapping reveals that the Neel spin density wave state found for the cuprate case maps to the g-wave altermagnetic state. In contrast to the d-wave altermagnetic that appears when g5 ≠ 0, the g-wave altermagnetic state requires nesting to become stable.

Group theory arguments

We now explicitly derive the symmetry requirements that underlie the kp Hamiltonian in Eq.(2). Key to this argument are non-symmorphic 2-fold symmetries. For these symmetries, we adopt the notation \(\widetilde{O}=\{O| {{{\bf{t}}}}\}\) to describe a reflection symmetry O followed by a half-translation vector t. We also denote a pure translation as {txty}. The first requirement for Eq.(2) is a 2-fold sublattice degeneracy, which appears independently of 2-fold spin degeneracy. This degeneracy is ensured by the product of spinless time-reversal symmetry T (here T is represented by the complex conjugation operator) and a non-symmorphic symmetry. For example in κ-Cl, reflection symmetry \(\widetilde{{M}_{x}}=\{{M}_{x}| 1/2,1/2\}\) takes the position (xy) to ( − x + 1/2, y + 1/2). We have \({(T\widetilde{{M}_{x}})}^{2}=-1\), which follows for T2 = 1 and \({(\widetilde{{M}_{x}})}^{2}=\{0,1\}=\exp (i{k}_{y})\) when the momentum of the Bloch state has ky = π. The TRIM point thus exhibits 2-fold sublattice degeneracy. In this work, we do not consider TRIM points with higher sublattice degeneracies.

As the T invariant operators τx and τz both share the same non-trivial transformation properties as kxky, this places the second constraint on possible allowed little co-groups (the group of crystal symmetries that keep the relevant momentum point unchanged up to a reciprocal lattice vector). Specifically, the little co-group must have a specific irreducible representation that transforms as kxky. This representation should not mix in other quadratic terms, such as \({k}_{x}^{2}\), because that would lead to terms like \({k}_{x}^{2}{\tau }_{x}\) in the kp Hamiltonian. Notably, linear terms like kxτx are already excluded from the kp Hamiltonian by T.

Now suppose τx,z already transform as kxky. Since τy is proportional to the product of τx and τz, it must transform trivially under all crystal symmetries, and belong to the trivial representation. The trivial representation should not mix in linear terms like kx, because that would lead to terms like kxτy in the Hamiltonian.

Let us check the above requirements of little co-groups on κ-Cl, which has mirror symmetries \(\widetilde{{M}_{x}}=\{{M}_{x}| 1/2,1/2\}\), \(\widetilde{{M}_{y}}=\{{M}_{y}| 1/2,1/2\}\), and their product C2z. These three symmetries keep the TRIM point (ππ) invariant. At this TRIM point, these symmetries form the 2mm point group. In this point group, the A2 representation only hosts kxky at quadratic level. The trivial A1 representation does not contain k-odd terms in (kxky). The above requirement of little co-groups are thus satisfied.

The third requirement is on the symmetry operators. Because T commutes with all crystal symmetries, these symmetries are represented by real 2 × 2 matrices. Since τy is invariant under all crystal symmetries, these matrices should commute with τy. Hence, they are either  ± τ0(identity) or  ± iτy. This implies that all the symmetry operators at the TRIM point should commute with each other.

If a symmetry preserves τx,z ~ kxky, then τx,z should commute with the symmetry matrix. The symmetry operator is then  ± τ0. Such symmetries are thus squared to  + 1. If a symmetry flips kxky, then τx,z should anticommute with the symmetry matrix. The symmetry matrix is then  ± iτy. Such symmetries are thus squared to -1.

We can now deduce the remaining symmetry requirements for the kp Hamiltonian in Eq.(2): (1) All the symmetry operators at the TRIM point commute with each other. (2) Symmetries preserving kxky are squared to  + 1 while symmetries flipping kxky are squared to  − 1. As shown below, these requirements can be checked without explicitly introducing matrix representations for the symmetries.

Let us check the above requirements for the symmetries on κ-Cl. Firstly, \(\widetilde{{M}_{x}}\) and \(\widetilde{{M}_{y}}\) commute as:

$$\begin{array}{rcl}&&\{{M}_{x}| {t}_{x}^{x},{t}_{x}^{y}\}\{{M}_{y}| {t}_{y}^{x},{t}_{y}^{y}\}\\ &&=\{-2{t}_{y}^{x},2{t}_{x}^{y}\}\{{M}_{y}| {t}_{y}^{x},{t}_{y}^{y}\}\{{M}_{x}| {t}_{x}^{x},{t}_{x}^{y}\}\\ &&=\{-1,1\}\{{M}_{y}| {t}_{y}^{x},{t}_{y}^{y}\}\{{M}_{x}| {t}_{x}^{x},{t}_{x}^{y}\}\end{array}$$
(9)

In real space, the commutator is evaluated into a translation operation { − 1, 1}, which is equal to  + 1 at the (kxky) = (ππ) point. Symmetries \(\widetilde{{M}_{x}}\), \(\widetilde{{M}_{y}}\), and their product C2z thus commute with each other.

Note that kxky is odd under \(\widetilde{{M}_{x}}\) and \(\widetilde{{M}_{y}}\), but even under their product C2z. Consequently, we require \({\widetilde{{M}_{x}}}^{2}={\widetilde{{M}_{y}}}^{2}=-1\), and \({C}_{2z}^{2}=+ 1\). To check this:

$$ {\widetilde{{M}_{x}}}^{2}=\{0,1\}=\exp (i{k}_{y})=-1\\ {\widetilde{{M}_{y}}}^{2}=\{1,0\}=\exp (i{k}_{x})=-1\\ {C}_{2z}^{2}=\{0,0\}=1.$$
(10)

The symmetry conditions are thus satisfied in κ-Cl. Table 1 is obtained by checking the above three requirements for TRIM points in all 2D layer groups and 3D space groups.

Discussion

Here we have identified coincident Van Hove singularities as a platform to realize 2D altermagnetic states and other novel electronic states. These states are stabilized due to a new interaction term, g5, through a weak-coupling BCS mechanism that leads to altermagnetism, nematic, d-wave superconducting, and orbital altermagnetic orders. Our results apply to nine 2D space groups and we have chosen a specific application in κ-Cl, where altermagnetism with the same symmetry found here is observed in κ-Cl84 and d-wave superconductivity is reported under pressure64,65 and anion substitution67,68,69,70,71,72,73,74. Another relevant 2D material is monolayer RuF4 in layer group L17(p21/b11). It has the same kp Hamiltonian as κ-Cl at the (ππ) point, and recent DFT calculation85 reveals an altermagnetic instability within an RPA-like approach.

Although our study focuses on 2D systems, the same coincident Van Hove singularities exist at high symmetry momenta in the 3D space groups listed in Table 1. Strictly speaking, in 3D, there is no divergence in the density of states near the Van Hove singularity. However, the density of states can still be large near the Van Hove momentum in the quasi-2D limit. In this case, the BCS weak-coupling instability will still aid in stabilizing the altermagnetic states. Among these 3D space groups, 55(Pbam), 58(Pnnm), 62(Pnma), 136(P42/mnm), and 138(P42/ncm) are known to host multiple altermagnetic candidates, according to the search on MAGNDATA database86. In these 3D materials, the contribution of the coincident Van Hove singularity to the ordering instability can be revealed by studying the doping dependence of the altermagnetic transition temperature.