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Floquet topological superconductivity induced by chiral many-body interaction


Non-equilibrium engineering is becoming a seminal way for realising novel quantum phases that are unimaginable in equilibrium. In particular, Floquet theory applied to quantum mechanics revealed that we can even control the band topology in semimetallic/insulating systems, while the straightforward application to topological superconductivity fails for typical superconductors because the supercondicting gap function does not couple to the electromagnetic field in a direct manner. Here we show that we can overcome this difficulty by taking account of correlation effects. Namely, we study how a d-wave superconductivity is changed when illuminated by circularly-polarised light (CPL) in the repulsive Hubbard model in the strong-coupling regime. We adopt the Floquet formalism for the Gutzwiller-projected effective Hamiltonian with the time-periodic Schrieffer-Wolff transformation. We find that CPL induces a topological superconductivity with a d + id pairing, which arises from the chiral spin coupling and the three-site term generated by the CPL. The latter term remains significant even for low frequencies and low intensities of the CPL. This is clearly reflected in the obtained phase diagram against the laser intensity and temperature for various frequencies red-detuned from the Hubbard U, with the transient dynamics also examined. The phenomenon revealed here can open a novel, dynamical way to induce a topological superconductivity.


It has become one of the key pursuits in the condensed-matter physics to design new quantum phases as exemplified by unconventional superconductivity and topological states. Conventionally, materials design is the accepted way, in which we tailor the crystal structures and consituent elements, as combined, if necessary, with carrier doping, pressure applications, etc. An entirely different avenue should be a “non-equilibrium design”, in which we envisage to realise interesting quantum phases by putting the systems out of equilibrium, typically by illuminating intense laser lights. This opens an in situ way to convert the system that would be unthinkable in equilibrium, and is also of fundamental interests as non-equilibrium physics. Ilya Prigogine, in his book From being to becoming1, once said that he would have liked to entitle the book as Time, the forgotten dimension, and we can indeed enlarge our horizon if we do not forget the temporal dimension.

One of the most important pathways is the Floquet physics, with which we can seek various novel quantum states arising from application of AC modulations to the system. This is based on Floquet’s theorem for time-periodic modulations, put forward by Gaston Floquet in 1883, which is much older than 1928 theorem by Bloch for spatially-periodic modulations. A prime application of Floquet physics is the “Floquet topological insulator” proposed by Takashi Oka and one of the present authors in 20092,3,4. Namely, by applying a circularly-polarised light to honeycomb systems such as graphene [see Fig. 1a], we can turn the system into a topological insulator in a dynamical manner. In other words, we are here talking about matter-light combined states, since the electron is converted into a superposition of the original, one-photon dressed, two-photon dressed, ..., electrons in the Floquet picture. The Floquet topological insulator with a topological gap exhibits a DC Hall effect despite the modulation being AC. The resulting state shows a kind of quantum anomalous Hall effect (i.e., quantum Hall effect in zero magnetic field) originally proposed for the static case by Duncan Haldane back in 19885. Indeed, the effective Hamiltonian for the irradiated system in the leading order in the Floquet formalism exactly coincides with Haldane’s model [Fig. 1b], as shown by Takuya Kitagawa et al.6. The year 2019 witnessed an experimental detection of the Floquet topological insulator in graphene by James McIver et al.7

Fig. 1: Various Floquet-induced quantum states.
figure 1

For Dirac fermions as in graphene, a illumination of a circularly-polarised light (CPL) induces the Floquet topological insulator, which arises from photon-assisted complex hopping (b), where colour shadings represent the piece-wise magnetic fluxes. c For magnetic phases in strongly-correlated systems, illumination of CPL induces a chiral spin coupling Jχ(Si × Sj) Sk with Si being the spin at site i, for which d illustrates a resonant behaviour in the coupling strength at ω/U = 1, 1/2, 1/3,    with ω being the driving frequency, and U the strength of the onsite repulsive interaction. e For superconductors (present work), illumination of CPL on a \({d}_{{x}^{2}-{y}^{2}}\)-wave superconductor produces pairing amplitudes \(\langle {\hat{c}}_{i\uparrow }{\hat{c}}_{j\downarrow }\rangle\) across nearest neighbours (red: positive; blue: negative) along with imaginary diagonal bonds (magenta and green), leading to an emergent complexified gap function F(k) in k space, and we have a photo-induced chiral \({d}_{{x}^{2}-{y}^{2}}+i{d}_{xy}\) superconductivity (f), where arrows schematically indicate the phase of the complex gap function.

Thus we have a surge of interests in Floquet topological phases, for many-body problems as well as one-body cases. Floquet physics has also been extended to explore superconductivity in AC-modulated situations. It is out of the scope of the present paper to review the whole field, but let us briefly mention that the spectrum of the many-body interests in Floquet physics covers a range of quantum phases as in Table 1. First, when a repulsive Hubbard model for correlated electrons is illuminated by laser, phase transitions arise between the Floquet topological insulator (FTI) and Mott’s insulator on a phase diagram against the AC modulation intensity and the repulsive electron-electron interaction8. Second, circularly-polarised laser lights can induce chiral spin interactions, \(({\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{i}\times {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{j})\cdot {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{k}\), and consequent spin liquids for the strongly-coupled systems with the repulsion U much greater than the electron hopping t0 [see Fig. 1c, d]9,10,11,12. There, we can realise that the Floquet-incuded chiral coupling becomes significant when the frequency ω of the laser is set close to the Hubbard U, with vastly different behaviours between the cases when ω is slightly red-detuned from U and blue-detuned.

Table 1 Examples of Floquet-induced quantum phases for topological and superconducting states.

Third, if we turn to superconductivity, Floquet physics can be used to even convert repulsive interactions into attractive ones by applying (linearly-polarised) laser13. Fourth, we can turn the usual pairing into an exotic η-pairing (condensation of pairs at Brillouin zone corners) by illuminating a superconductor with a (linearly-polarised) laser14. There, the Floquet effective pair-hopping is drastically modulated when ω is close to U, again with different behaviours between ω red-detuned or blue-detuned from U.

Now the purpose of the present paper is to encompass topological and superconducting properties to seek whether a “Floquet-induced topological superconductivity” can arise. While there have been various attempts at realising Floquet topological superconducting states15,16,17,18,19,20, an obstacle is the fact that the pairing symmetry is hard to be controlled in a direct manner, since the gap function does not couple to electromagnetic fields. Thus, usually, one has to modulate the one-body part in a nontrivial manner (with the gap function kept intact), which e.g. necessitates the Rashba spin-orbit coupling. Instead, the strategy of the present paper is to exploit the peculiar laser-induced interactions emergent in strongly-correlated systems. Namely, we illuminate a circularly-polarised light (CPL) to the repulsive Hubbard model in the strong-coupling regime to modulate the pairing interaction and the resultant gap function. We shall show that a \({d}_{{x}^{2}-{y}^{2}}\)-wave superconductor is indeed changed into a topological \({d}_{{x}^{2}-{y}^{2}}+i{d}_{xy}\) wave [Fig. 1f]. This will be shown in the Floquet formalism for the Gutzwiller-projected effective Hamiltonian with the time-periodic Schrieffer-Wolff transformation. The d + id pairing is shown to arise from the chiral spin coupling along with the three-site term caused by the CPL [Fig. 1e]. The latter term turns out to remain significant even for low frequencies and low intensities of the CPL. This will be reflected in a phase diagram against the laser intensity and temperature obtained here for various frequencies red-detuned from the Hubbard U, along with transient dynamics.


Low-energy effective Hamiltonian

We take in the present study the hole-doped Mott insulator on a square lattice, which is irradiated by an intense circularly-polarised light (CPL). This can be minimally modelled by the repulsive Hubbard model, with a Hamiltonian

$$\hat{H}(t)=-\mathop{\sum}\limits_{ij\sigma }{t}_{ij}{e}^{-i{{{{{{{\boldsymbol{A}}}}}}}}(t)\cdot {{{{{{{{\boldsymbol{R}}}}}}}}}_{ij}}{\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{j\sigma }+\frac{U}{2}\mathop{\sum}\limits_{i}{\hat{n}}_{i}({\hat{n}}_{i}-1),$$

where \({\hat{c}}_{j\sigma }\) annihilates an electron on the site j at Rj with spin σ = ,, and \({\hat{n}}_{i}={\sum }_{\sigma }{\hat{n}}_{i\sigma }={\sum }_{\sigma }{\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{i\sigma }\) is the density operator. For the hopping amplitude tij, here we consider the second-neighbour (\({t}_{0}^{\prime}\)) as well as the nearest-neighbour hopping (t0), as necessitated for realising a CPL-induced topological superconductivity [as we shall see below Eq. (17)]. The onsite repulsion is denoted as U (>0).

The circularly-polarised laser field is introduced via the Peierls phase, which involves Rij ≡ Ri − Rj, and the vector potential,

$${{{{{{{\boldsymbol{A}}}}}}}}(t)=\frac{{{{{{{{\boldsymbol{E}}}}}}}}}{2i\omega }{e}^{-i\omega t}-\frac{{{{{{{{{\boldsymbol{E}}}}}}}}}^{* }}{2i\omega }{e}^{i\omega t},$$

for the right-circularly-polarised case; replace E with E* for the left circulation. We set  = e = 1 hereafter.

Since the laser electric field is time-periodic, \(\hat{H}(t+2\pi /\omega )=\hat{H}(t)\), we can employ the Floquet formalism21, where the eigenvalue, called quasienergy, of the discrete time translation plays a role of energy. Because the quasienergy spectrum is invariant under the time-periodic unitary transformation, \({e}^{-i\hat{{{\Lambda }}}(t)}\) with \(\hat{{{\Lambda }}}(t+2\pi /\omega )=\hat{{{\Lambda }}}(t)\), we can introduce an effective static Hamiltonian \({\hat{H}}_{{{{{{{{\rm{F}}}}}}}}}\) as

$${\hat{H}}_{{{{{{{{\rm{F}}}}}}}}}={e}^{i\hat{{{\Lambda }}}(t)}[\hat{H}(t)-i{\partial }_{t}]{e}^{-i\hat{{{\Lambda }}}(t)},$$

where \(\hat{{{\Lambda }}}(t)\) is determined such that \({\hat{H}}_{{{{{{{{\rm{F}}}}}}}}}\) becomes time-independent. With such a transformation, we can analyse the time-dependent original problem using various approaches that are designed for static Hamiltonians.

While it is difficult to determine \(\hat{{{\Lambda }}}(t)\) and \({\hat{H}}_{{{{{{{{\rm{F}}}}}}}}}\) in an exact manner, we can obtain their perturbative expansions in various situations. The high-frequency expansion8, 22, 23 is a seminal example of such perturbative methods, where the effective Hamiltonian \({\hat{H}}_{{{{{{{{\rm{F}}}}}}}}}\) is obtained as an asymptotic series in 1/ω, and widely used for describing the Floquet topological phase transition. However, since the onsite interaction U in Mott insulators is typically much greater than the photon energy ω, the high-frequency expansion is expected to be invalidated for the present case.

Still, in the present system in a strongly-correlated regime t0U, we can employ the Floquet extension of the strong-coupling expansion (Schrieffer-Wolff transformation)11, 12, 19, 24, 25, when the photon energy ω exceeds the band width ~ t0 of the doped holes (and chosen to be off-resonant with the Mott gap ~ U), i.e., t0ω < U. As we describe the detailed derivation in Methods, we can obtain \(\hat{{{\Lambda }}}(t)\) and \({\hat{H}}_{{{{{{{{\rm{F}}}}}}}}}\) in perturbative series in the hopping amplitudes \({t}_{0},{t}_{0}^{\prime}\). While the t0U assumption yields a low-energy effective model known in the undriven case as a tJ model26 which describes the dynamics of holes in the background of localised spins, an essential difference in the Floquet states under CPL is that extra terms emerge. Namely, the Hamiltonian of the irradiated case reads

$${\hat{H}}_{{{{{{{{\rm{F}}}}}}}}}= -\mathop{\sum}\limits_{ij\sigma }{\tilde{t}}_{ij}{\hat{P}}_{G}{\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{j\sigma }{\hat{P}}_{G}+\frac{1}{2}\mathop{\sum}\limits_{ij}{J}_{ij}\left({\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{i}\cdot {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{j}-\frac{1}{4}{\hat{n}}_{i}{\hat{n}}_{j}\right)\\ +\mathop{\sum}\limits_{ijk\sigma {\sigma }^{\prime}}{{{\Gamma }}}_{i,j;k}{\hat{P}}_{G}\left[({\hat{c}}_{i\sigma }^{{{{\dagger}}} }{{{{{{{{\boldsymbol{\sigma }}}}}}}}}_{\sigma {\sigma }^{\prime}}{\hat{c}}_{j{\sigma }^{\prime}})\cdot {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{k}-\frac{1}{2}{\delta }_{\sigma {\sigma }^{\prime}}{\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{j\sigma }{\hat{n}}_{k}\right]{\hat{P}}_{G}\\ +\frac{1}{6}\mathop{\sum}\limits_{ijk}{J}_{ijk}^{\chi }({\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{i}\times {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{j})\cdot {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{k},$$

where \({\hat{P}}_{G}={\prod }_{i}(1-{\hat{n}}_{i\uparrow }{\hat{n}}_{i\downarrow })\) projects out doubly-occupied configurations. Here, we have retained all the processes up to the second order (in the hopping amplitudes \({t}_{0},{t}_{0}^{\prime}\)), and additionally taken account of the fourth-order processes for the last line of the above equation. Thus the photon-modified exchange interaction, Jij, and the photon-induced correlated hopping, Γi,j; k, are of second order, while the photon-generated chiral spin coupling, \({J}_{ijk}^{\chi }\), is of fourth order.

Let us look at the effective model in the laser field term by term. First, the hopping amplitude of the holes is renormalised from tij into \({\tilde{t}}_{ij}={t}_{ij}{{{{{{{{\mathcal{J}}}}}}}}}_{0}({A}_{ij})\) due to the time-averaged Peierls phase27, 28, where Aij = ERij/ω and \({{{{{{{{\mathcal{J}}}}}}}}}_{m}\) is the m-th Bessel function. Then we come to the interactions. The spin–spin interaction has a coupling strength dramatically affected by the intense electric field, since it is mediated by kinetic motion of electrons. Namely, the static kinetic-exchange interaction J is modulated as24

$${J}_{ij}=\mathop{\sum }\limits_{m=-\infty }^{\infty }\frac{4{t}_{ij}^{2}{{{{{{{{\mathcal{J}}}}}}}}}_{m}{\left({A}_{ij}\right)}^{2}}{U-m\omega },$$

which is a sum over m-photon processes, and appears in the second term on the first line of Eq. (5).

While these modulations of t and J also occur for the case of linearly-polarised lasers (i.e., for time-reversal symmetric modulations), a notable feature of the CPL is the emergence of the time-reversal breaking many-body interactions specific to the strong correlation. In the one-body Floquet physics, the two-step hopping (i.e., a perturbative process with hopping twice) in CPL becomes imaginary (and thus breaks the time-reversal symmetry) already on the noninteracting level if we take a honeycomb lattice2, 6, 8, while such an imaginary hopping does not arise for the (noninteracting) square lattice due to a cancellation of contributions from different paths as depicted in Fig. 2a, which is why a honeycomb lattice fits with the FTI.

Fig. 2: Schematic picture for two-step hopping.
figure 2

a Photon-induced hopping processes in the noninteracting square lattice, where contributions from two different paths (red and blue dotted arrows) cancel with each other. b For a strongly-correlated model with an interaction U, the photon-induced hopping processes are sensitive to the charge and spin configurations on the path, which lifts the cancellation in general.

If we move on to correlated systems, on the other hand, the hopping process involves interactions for spinful electrons on the path, which lifts such cancellations, as exemplified in Fig. 2b. This implies that such a time-reversal breaking term is present in (interacting) square lattice as well. The two-step correlated hopping Γ appears in the second-order perturbation in the presence of holes [the second line of Eq. (5)], which involves three sites and sometimes referred to as the “three-site term”26. While the three-site term also appears in the undriven case with the amplitude Γi,j; k = Jij/4, this term involving the dynamics of holes (i.e., the change of holes’ positions) is usually neglected because its contribution is small in the low-doping regime [see the Gutzwiller factor in the next subsection, ~ g2δ in Eqs. (10), (11)]. In sharp contrast, when the system is driven by a CPL, Γi,j; k acquires an important three-site imaginary part as

$${{{{{{{\rm{Im}}}}}}}}\,{{{\Gamma }}}_{i,j;k}=\mathop{\sum }\limits_{m=1}^{\infty }\frac{2{t}_{ik}{t}_{kj}{{{{{{{{\mathcal{J}}}}}}}}}_{m}({A}_{ik}){{{{{{{{\mathcal{J}}}}}}}}}_{m}({A}_{kj})}{m\omega (1-{m}^{2}{\omega }^{2}/{U}^{2})}\sin m({\theta }_{jk}-{\theta }_{ik})$$

with θij defined as \({{{{{{{{\boldsymbol{R}}}}}}}}}_{ij}=| {{{{{{{{\boldsymbol{R}}}}}}}}}_{ij}| (\cos {\theta }_{ij},\sin {\theta }_{ij})\). The term triggers a topological superconductivity even when it is small, as we shall see.

In addition to the two-step correlated hopping Γ, another time-reversal breaking term arises if we go over to higher-order perturbations. In the previous studies of the half-filled case11, 12, an emergent three-spin interaction (i.e., the scalar spin chirality term Jχ) is shown to appear in the fourth-order perturbation. This appears on the last line in Eq. (5) with a coefficient \({J}_{ijk}^{\chi }\). While this term is basically much smaller than the second-order terms, it may become comparable with the contribution from \({{{{{{{\rm{Im}}}}}}}}\,{{\Gamma }}\), as the spin chirality term does not accompany the dynamics of holes and has a larger Gutzwiller factor [~g3 in Eqs. (10), (11). See also Fig. 3].

Fig. 3: Dependence of the coupling constants on the laser intensity for the driven model.
figure 3

a, b Two-step correlated hopping γ (a), and scalar spin-chirality term Jχ (b) are colour-coded against circularly-polarised-light amplitude E and driving frequency ω. Figure 1d corresponds to a cross section of b at E = 6t0/a. ce The renormalised hopping amplitude \(\tilde{t}\), exchange coupling J, along with the two-step correlated hopping γ [Eq. (18)] and the chiral spin-coupling Jχ [Eq. (19)], against E. The driving frequency is chosen as ω = 1.7t0 = 0.14U (c), ω = 5.4t0 = 0.45U (d), or ω = 10.5t0 = 0.88U (e) with t0: bare hopping amplitude, a: lattice constant. Note a difference in the horizontal scale between (c) and (d, e). We take here the bare second-neighbour hopping \({t}_{0}^{\prime}=-0.2{t}_{0}\), the onsite interaction U = 12t0, and a doping level δ = 0.2. Here, the infinite summations of Fourier components [∑m in Eq. (7) and ∑lmn in Eq. (39)] are truncated such that the Taylor series up to E20 is reproduced. This is accurate enough for ω > t0, while for the low-frequency regime ω < t0 an intricate resonant structure due to the ω = U/integer resonance (seen also for t0 < ω < 4t0) is not captured.

Mean-field decomposition under Gutzwiller ansatz

Let us investigate the fate of the d-wave superconductivity in the presence of the time-reversal breaking terms. To this end, we here adopt the Gutzwiller ansatz26, 29 for the ground-state wavefunction and perform a mean-field analysis, as elaborated in Methods. After the approximate evaluation of the Gutzwiller projection, the problem of determining the ground state is turned into an energy minimisation of Eq. (5) without the Gutzwiller factor \({\hat{P}}_{G}\) if we renormalise the parameters. The mean-field solution is then formulated as a diagonalisation of the Bogoliubov-de Gennes Hamiltonian in the momentum space,

$${\hat{H}}_{{{{{{{{\rm{F}}}}}}}}}=\mathop{\sum}\limits_{{{{{{{{\boldsymbol{k}}}}}}}}}{\left(\begin{array}{l}{\hat{c}}_{{{{{{{{\boldsymbol{k}}}}}}}}\uparrow }\\ {\hat{c}}_{-{{{{{{{\boldsymbol{k}}}}}}}}\downarrow }^{{{{\dagger}}} }\end{array}\right)}^{{{{\dagger}}} }\left(\begin{array}{l}\varepsilon ({{{{{{{\boldsymbol{k}}}}}}}})\,\,\,\quad F({{{{{{{\boldsymbol{k}}}}}}}})\\ F{({{{{{{{\boldsymbol{k}}}}}}}})}^{* }\,\,-\varepsilon (-{{{{{{{\boldsymbol{k}}}}}}}})\end{array}\right)\left(\begin{array}{l}{\hat{c}}_{{{{{{{{\boldsymbol{k}}}}}}}}\uparrow }\\ {\hat{c}}_{-{{{{{{{\boldsymbol{k}}}}}}}}\downarrow }^{{{{\dagger}}} }\end{array}\right)\hskip 2.5pc$$
$$\hskip 2pc=\mathop{\sum}\limits_{{{{{{{{\boldsymbol{k}}}}}}}}}{\left(\begin{array}{l}{\hat{c}}_{{{{{{{{\boldsymbol{k}}}}}}}}\uparrow }\\ {\hat{c}}_{-{{{{{{{\boldsymbol{k}}}}}}}}\downarrow }^{{{{\dagger}}} }\end{array}\right)}^{{{{\dagger}}} }\left[\mathop{\sum}\limits_{\tau }\left(\begin{array}{rc}{\varepsilon }_{\tau }&{F}_{\tau }\\ {F}_{\tau }^{* }&-{\varepsilon }_{\tau }\end{array}\right)\cos {{{{{{{\boldsymbol{k}}}}}}}}\cdot {{{{{{{{\boldsymbol{R}}}}}}}}}_{i,i+\tau }\right]\left(\begin{array}{l}{\hat{c}}_{{{{{{{{\boldsymbol{k}}}}}}}}\uparrow }\\ {\hat{c}}_{-{{{{{{{\boldsymbol{k}}}}}}}}\downarrow }^{{{{\dagger}}} }\end{array}\right).$$

Here we have

$${\varepsilon }_{\tau }= -g\delta {\tilde{t}}_{i,i+\tau }-{g}^{2}\frac{3-{\delta }^{2}}{8}{J}_{i,i+\tau }\,{\chi }_{\tau }\\ -{g}^{2}\delta \mathop{\sum}\limits_{{\tau }^{\prime}}{{{{{{{\rm{Re}}}}}}}}\left(\frac{1-{\delta }^{2}}{4}{{{\Gamma }}}_{i,i+\tau ;i+{\tau }^{\prime}}+\frac{3-\delta }{2}{{{\Gamma }}}_{i,i+\tau +{\tau }^{\prime};i+\tau }\,{\chi }_{{\tau }^{\prime}}\right)\\ -\frac{3}{16}{g}^{3}\mathop{\sum}\limits_{{\tau }^{\prime}}{J}_{i,i+\tau ,i+\tau +{\tau }^{\prime}}^{\chi }{{{{{{{\rm{Im}}}}}}}}({{{\Delta }}}_{\tau +{\tau }^{\prime}}^{* }{{{\Delta }}}_{{\tau }^{\prime}}),$$
$${F}_{\tau } = {\,}{g}^{2}\frac{3+{\delta }^{2}}{8}{J}_{i,i+\tau }{{{\Delta }}}_{\tau }+{g}^{2}\delta \frac{3+\delta }{2}\mathop{\sum}\limits_{{\tau }^{\prime}}{{{{{{{\rm{Re}}}}}}}}{{{\Gamma }}}_{i,i+\tau +{\tau }^{\prime};i+\tau }{{{\Delta }}}_{{\tau }^{\prime}}\\ +i{g}^{2}\mathop{\sum}\limits_{{\tau }^{\prime}}\left(\delta \frac{3+\delta }{2}{{{{{{{\rm{Im}}}}}}}}{{{\Gamma }}}_{i,i+\tau +{\tau }^{\prime};i+\tau }+\frac{3}{8}g{J}^{\chi}_{i,i+\tau ,i+\tau +{\tau }^{\prime}}\,{\chi }_{\tau +{\tau }^{\prime}}\right){{{\Delta }}}_{{\tau }^{\prime}},$$

where the expressions are independent of the site index i due to the spatial translational symmetry, and we have denoted the doping level as

$$\delta =1-\frac{1}{N}\mathop{\sum}\limits_{i}\langle {\hat{n}}_{i}\rangle$$

with N being the number of lattice sites. Here τ runs over τ = mx + ny with \(m,n\in {\mathbb{Z}}\), and the label i + τ represents the site at Ri+τ = Ri + (m, n) in units of the lattice constant. The dependence on δ and a factor g = 2/(1 + δ) appears as a result of the Gutzwiller projection, which suppresses the contribution from charge dynamics as represented by \(\tilde{t}\) and Γ in the small δ regime. For the detailed derivation, see Methods. Throughout the present study, we take δ = 0.2. The mean-field Hamiltonian is self-consistently determined for the bond order parameter χ and the pairing amplitude Δ as

$${\chi }_{\tau }=\frac{1}{N}\mathop{\sum}\limits_{i}\langle {\hat{c}}_{i\uparrow }^{{{{\dagger}}} }{\hat{c}}_{i+\tau \uparrow }+{\hat{c}}_{i\downarrow }^{{{{\dagger}}} }{\hat{c}}_{i+\tau \downarrow }\rangle ,$$
$${{{\Delta }}}_{\tau }=\frac{1}{N}\mathop{\sum}\limits_{i}\langle {\hat{c}}_{i\uparrow }{\hat{c}}_{i+\tau \downarrow }-{\hat{c}}_{i\downarrow }{\hat{c}}_{i+\tau \uparrow }\rangle .$$

In the absence of the external field, the system undergoes a phase transition from normal to the \({d}_{{x}^{2}-{y}^{2}}\)-wave superconductivity when the temperature is sufficiently low26. The corresponding order parameter is

$${{{\Delta }}}_{\pm x}=-{{{\Delta }}}_{\pm y}\equiv {{\Delta }},$$

for which the gap function F(k) becomes

$${F}^{{x}^{2}-{y}^{2}}({{{{{{{\boldsymbol{k}}}}}}}})=\frac{3}{4}{g}^{2}J{{\Delta }}(\cos {k}_{x}-\cos {k}_{y}),$$

as derived from the first term in Eq. (11) with τ = ± x, ± y. Here we have dropped a small correction due to δ. Without a loss of generality, we assume that Δ is real. The \({d}_{{x}^{2}-{y}^{2}}\) gap function has nodal lines along ky = ± kx, across which the gap function changes sign (see Fig. 4a–c below).

Fig. 4: Gap functions.
figure 4

ac \({d}_{{x}^{2}-{y}^{2}}\)-wave superconductivity in the absence of driving field. di \({d}_{{x}^{2}-{y}^{2}}+i{d}_{xy}\)-wave superconductivity in the circularly-polarised laser. The driving frequency ω and the field amplitude E are chosen as ω = 10.5t0 = 0.88U, E = 16t0/a (df), or ω = 1.7t0 = 0.14U, E = 3.5t0/a (gi). a, d, g Colour-coded absolute values of the gap function, F(k); b, e, h phases, \(\arg F({{{{{{{\boldsymbol{k}}}}}}}})\). The dashed lines represent the Fermi surface at the critical temperature T = Tc. c, f, i Density of states against energy in units of the bare hopping amplitude t0. We take a parameter set: the bare second-neighbour hopping \({t}_{0}^{\prime}=-0.2{t}_{0}\), the onsite interaction U = 12t0, and a doping level δ = 0.2.

Now let us look into the possibility for the laser field converting this ground state into topological superconductivity from the time-reversal breaking terms [the second line in Eq. (11)]. The leading term should be those for \({\tau }^{\prime}=\pm x,\pm y\) (with \({{{\Delta }}}_{{\tau }^{\prime}}=\pm {{\Delta }}\)), which is nonzero even for the original \({d}_{{x}^{2}-{y}^{2}}\)-wave solution with no driving field and results in an imaginary gap function iΔ. In particular, gathering the terms with τ = ± (x + y), ± (x − y), we obtain the leading modulation to the gap function as

$${F}^{xy}({{{{{{{\boldsymbol{k}}}}}}}})\simeq 3i{g}^{2}\left[4\delta \gamma +g({J}_{\chi }\,{\chi }_{x}+{J}_{\chi }^{\prime}\,{\chi }_{2x+y})\right]{{\Delta }}\sin {k}_{x}\sin {k}_{y}$$

where we have defined

$$\gamma ={{{{{{{\rm{Im}}}}}}}}\,({{{\Gamma }}}_{i-x,i;i+y}-{{{\Gamma }}}_{i-x-y,i+x;i}),$$
$${J}_{\chi }={J}_{i,i+y,i+x}^{\chi }\,,\,\,{J}_{\chi }^{\prime}={J}_{i-x,i,i+x+y}^{\chi }.$$

Thus we are indeed led to an emergence of a topological (chiral) \({d}_{{x}^{2}-{y}^{2}}+i{d}_{xy}\) superconductivity with \(F({{{{{{{\boldsymbol{k}}}}}}}})\simeq {F}^{{x}^{2}-{y}^{2}}+i{F}^{xy}\) with a full gap. For the full expression of the modulated gap function, see Eq. (65) in “Methods”. The key interactions, γ and Jχ, take nonzero values when the original Hubbard Hamiltonian Eq. (1) has the second-neighbour hopping \({t}_{0}^{\prime}\): Since the two-step correlated hopping Γi,j; k is composed of two hoppings, k → i and j → k, we can see that the imaginary coefficient above has \(\gamma \propto {t}_{0}{t}_{0}^{\prime}\). The chiral spin-coupling \({J}_{\chi }\propto {({t}_{0}{t}_{0}^{\prime})}^{2}\) also necessitates the next-nearest-neighbour hopping, which can be deduced from Eq. (41) in “Methods”.

Having revealed the essential couplings for the chiral superconductivity, let us now explore how we can optimise the field amplitude and frequency for realising larger topological gaps. For this, we set here \({t}_{0}^{\prime}=-0.2{t}_{0}\) and U = 12t0 having cuprates with t0 0.4 eV in mind as a typical example.

We plot the essential γ and Jχ against the driving amplitude E and frequency ω in Fig. 3a, b. If we look at the overall picture, we can see that the dynamical time-reversal breaking is strongly enhanced along some characteristic frequencies in a resonant fashion at ω/U = 1/integer, which we can capture from the expressions for the coupling constants in the small-amplitude regime as follows.

The two-step correlated hopping γ is given, in the leading order in the amplitude, as

$$\gamma =\frac{2{t}_{0}{t}_{0}^{\prime}{{{{{{{{\mathcal{J}}}}}}}}}_{2}\left(\frac{Ea}{\omega }\right){{{{{{{{\mathcal{J}}}}}}}}}_{2}\left(\sqrt{2}\frac{Ea}{\omega }\right)}{\omega (1-4{\omega }^{2}/{U}^{2})}+O({E}^{12}).$$

This expression, as a function of E, takes the maximal value around E 2.45ω/a, while diverges for ω → 0 or ω → U/2 for each value of E, as seen from the energy denominator. The enhancement occurs even in the low-frequency regime, which should be advantageous for experimental feasibility, since the required field amplitude (E 2.4ω/a) can be small.

If we turn to the spin-chirality term, Jχ has a complicated form involving Bessel functions [see Eq. (41) below]. If we Taylor-expand it in E, we have

$${J}_{\chi } \sim \frac{2{(Ea)}^{4}{t}_{0}^{2}{t}_{0}^{^{\prime} 2}(2{U}^{6}+75{\omega }^{2}{U}^{4}-399{\omega }^{4}{U}^{2}-164{\omega }^{6})}{\omega {\left({U}^{2}-{\omega }^{2}\right)}^{3}{\left({U}^{2}-4{\omega }^{2}\right)}^{3}},$$

which takes large values around ω = U due to the energy denominator in the above expression, while γ is small in this regime. The expression reveals that a dynamical time-reversal breaking also occurs as a fourth-order nonlinear effect with respect to the field strength E.

We can see in Fig. 3c–e how Jχ, as well as the exchange interaction J and the renormalised nearest-neighbour hopping \(\tilde{t}\), vary with the CPL intensity for several representative frequencies for which the dynamical time-reversal breaking becomes prominent. The hopping amplitude \(\tilde{t}\) vanishes around the peak of γ (E 2.45ω/a), as seen in Fig. 3c, d. This involves a zero of the Bessel function (at E ~ 2.40ω/a), and known as the dynamical localisation27. In Fig. 3d, e, we can see a strong enhancement of J. Panel d has ω = 0.45U (slightly red-detuned from U/2), while panel e has ω = 0.88U (slightly red-detuned from U). If we go back to Eq. (6), the former has to do with the energy denominator for m = 2, while the latter for m = 1. While the driving frequency is set to be red-detuned from the resonance (which we can call “U − mω resonance”) in these results, the blue-detuned cases would give negative contributions from these terms, which will lead to a ferromagnetic exchange interaction, unfavouring the spin-singlet d-wave. With an optimal choice of the driving field, γ attains a significantly large value  0.04t0, which yields \({F}^{xy}({{{{{{{\boldsymbol{k}}}}}}}})\simeq 0.3{t}_{0}\times i{{\Delta }}\sin {k}_{x}\sin {k}_{y}\) (for δ = 0.2). This is remarkably large and comparable with the undriven \({F}^{{x}^{2}-{y}^{2}}({{{{{{{\boldsymbol{k}}}}}}}})\simeq 0.7{t}_{0}\times {{\Delta }}(\cos {k}_{x}-\cos {k}_{y})\), even though the coupling constant itself is much smaller than J. This is the first key result of the present work.

Phase diagram

Now we investigate the ground state of the effective static Bogoliubov-de Gennes Hamiltonian for several choices of the CPL parameters. Let us show the gap function and the density of states in Fig. 4. In the absence of the external field in Fig. 4a–c, the gap function has the \({d}_{{x}^{2}-{y}^{2}}\) symmetry with nodal lines that give the zero gap at the Fermi energy. We now switch on the CPL, with ω = 10.5t0 = 0.88U, E = 16t0/a for Fig. 4d–f, or with ω = 1.7t0 = 0.14U, E = 3.5t0/a for Fig. 4g–i. The former represents the case where Jχ is dominant (see Fig. 3e), while in the latter γ plays the central role. In both cases we have the \({d}_{{x}^{2}-{y}^{2}}+i{d}_{xy}\) pairing, where the nodal lines are gapped out due to the complex gap function. We can indeed see in Fig. 4f, i clear energy gaps in the density of states with a gap size comparable with the original \({d}_{{x}^{2}-{y}^{2}}\) superconducting gap (as measured by the energy spacing between the two peaks in the density of states). Note that the band width and the \({d}_{{x}^{2}-{y}^{2}}\) superconducting gap are renormalised there, due to the modified \(\tilde{t}\) and J.

To examine the robustness of the d + id superconductivity, we calculate Δ and \({{{\Delta }}}^{\prime}\equiv -i{{{\Delta }}}_{\pm (x+y)}=i{{{\Delta }}}_{\pm (x-y)}\) at finite temperatures, which gives a phase diagram against T and field amplitude E in Fig. 5. We can see that the critical temperature Tc, as delineated by the region for Δ ≠ 0, increases significantly as the laser intensity E is increased. The enhanced Tc originates from the fact that J [and \({{{{{{{\rm{Re}}}}}}}}\,{{\Gamma }}\); see Eq. (38) below] are enhanced when the laser is applied, as we have seen in Fig. 3c–e. The time-reversal breaking order parameter \({{{\Delta }}}^{\prime}\) emerges below Tc down to T = 0, with the field dependence emerging from those of γ and Jχ.

Fig. 5: Finite-temperature phase diagram.
figure 5

For the driving frequency ω = 10.5t0 = 0.88U (a, b) or ω = 1.7t0 = 0.14U (c, d), the superconducting order parameter Δ (a, c) and the time-reversal breaking order parameter \({{{\Delta }}}^{\prime}\equiv -i{{{\Delta }}}_{\pm (x+y)}=i{{{\Delta }}}_{\pm (x-y)}\) (b, d) are colour-coded against the field amplitude E and temperature T. Dotted lines represent the effective temperature of the Floquet Hamiltonian when the system is quenched from E = 0 at a temperature that is the leftmost starting point of each dotted line. We take the same bare second-neighbour hopping \({t}_{0}^{\prime}=-0.2{t}_{0}\), onsite interaction U = 12t0, and doping level δ = 0.2 as in Fig. 4.

Transient dynamics

So far, we have investigated static properties of the effective Hamiltonian \({\hat{H}}_{{{{{{{{\rm{F}}}}}}}}}\). While the results clearly show the presence of Floquet topological superconductivity in a wide parameter region, an important question from a dynamical viewpoint is whether we can achieve the Floquet topological superconductivity within a short enough time scale, over which the description with the effective Hamiltonian Eq. (5) is valid (i.e., over which we can neglect the coupling to phonons, the heating process due to higher-order perturbations, etc.).

Thus let us study the dynamics of the superconducting gap, by solving a quench problem formulated as follows. We first prepare the initial state as the mean-field ground state of the equilibrium tJ model [i.e., Eq. (5) with E = 0], and then look at the transient dynamics when the CPL electric field is suddenly switched on, by changing the Hamiltonian at t = 0 to the effective Hamiltonian \({\hat{H}}_{{{{{{{{\rm{F}}}}}}}}}\) (Eq. 5) with E ≠ 0. In such a treatment, \(\langle {\hat{H}}_{{{{{{{{\rm{F}}}}}}}}}\rangle\) is a conserved quantity for t > 0, and the driven state is expected to thermalise to the equilibrium state of \({\hat{H}}_{{{{{{{{\rm{F}}}}}}}}}\) having a temperature that corresponds to the internal energy \(\langle {\hat{H}}_{{{{{{{{\rm{F}}}}}}}}}\rangle\) (which we call an effective temperature). Note that here we implicitly neglect the fact that \({\hat{H}}_{{{{{{{{\rm{F}}}}}}}}}\)s for E = 0 and E ≠ 0 are on different frames [specified by \(\hat{{{\Lambda }}}(t)\)].

Before exploring the dynamics, it is important to check whether the expected steady state of the quench problem remains superconducting. We can do this by looking at the above-defined effective temperature on the phase diagram as indicated by dotted lines in Fig. 5. While the effective temperature rises as we increase the field strength E when we start from temperatures below Tc, we can see that the effective temperature does not exceed Tc in a wide parameter region, which implies that the Floquet topological superconductivity should indeed appear as a steady state of the quench dynamics. A sudden increase of temperature around E ~ 4t0/a in Fig. 5c, d is due to the band flipping (sign change of \(\tilde{t}\)), which makes the kinetic energy of the initial state quite large. As we further increase the field strength, the effective temperature eventually reaches infinity and will even become negative13.

Now, the question is whether the equilibration (known as the Floquet prethermalisation) occurs fast enough (e.g., faster than the neglected heating processes, within the experimentally accessible pulse duration, etc.). We compute the time evolution of the superconducting order parameter in the time-dependent mean-field approximation (with the Gutzwiller ansatz), and plot the time evolution of Δ and \(| {{{\Delta }}}^{\prime}|\) in Fig. 6a, b, where we set the initial temperature at kBTinitial = 0 with E = 7t0/a, ω = 10.5t0 = 0.88U. Here, the unit of time /t0 corresponds to ~1 fs for t0 0.4 eV. We can see that Δ rapidly evolves with an overshooting behaviour, and converges to a certain value with a damped oscillation. Similar behaviour can be found in a previous study of the quench problem for the d-wave (but within the \({d}_{{x}^{2}-{y}^{2}}\) pairing) superconductor30. The time-reversal breaking order parameter \(| {{{\Delta }}}^{\prime}|\) also quickly converges to a nonzero value. This is the second key result in the present work. We note that the obtained steady state slightly deviates from the equilibrium state with respect to \({\hat{H}}_{{{{{{{{\rm{F}}}}}}}}}\), where the deviation arises because the pair-breaking scattering30 is lacking in the mean-field treatment of the dynamics.

Fig. 6: Quench dynamics of the order parameters.
figure 6

Time evolution of Δ = cici+x, and \(| {{{\Delta }}}^{\prime}| =| \langle {c}_{i\uparrow }{c}_{i+x+y,\downarrow }\rangle |\) after a sudden quench of the field amplitude from E = 0 to E = 7t0/a with an initial temperature kBTinitial = 0 (a, b), or to E = 16t0/a with an initial kBTinitial = 0.2t0 (c, d). The latter corresponds to the case in which the superconductivity appears even when we start from an initial temperature above Tc. Δ (a, c) represents the conventional \({d}_{{x}^{2}-{y}^{2}}\)-wave component, while \(| {{{\Delta }}}^{\prime}|\) (b, d) represents the time-reversal breaking idxy-wave component. Horizontal lines indicate the equilibrium value at the effective temperature. The driving frequency is set to ω = 10.5t0 = 0.88U with t0 being the bare hopping amplitude.

The curious oscillation in the amplitude of the gap function can be interpreted as an excitation of the Higgs modes in superconductors31,32,33, and thus the typical time scale for the oscillation (and the emergence of \({{{\Delta }}}^{\prime}\)) can be roughly estimated as the inverse of the superconducting gap (~1/2F(k) with an appropriate k-average). This should be much faster than the time scale for heating, although its nonempirical evaluation would be difficult. We can analyse the present quench dynamics in a linearised form34 if the change in the coupling constant is small, which reveals that the appearance of \({{{\Delta }}}^{\prime}\) is described as the A2g Higgs mode in the d-wave sector with an amplitude proportional to E4.

If we have a closer look at the effective temperature in Fig. 5, we find an intriguing phenomenon: the superconducting state can appear even when we start from an initial temperature that is above the Tc before laser illumination. Namely, some dotted lines that start from T above Tc at E = 0 do plunge into the superconducting region as E is increased. We show the time evolution of the order parameter for this “nonequilibrium-induced superconductivity” in Fig. 6c, d, where we set kBTinitial = 0.2t0 as an initial temperature, and choose E = 16t0/a, ω = 10.5t0. Since the homogeneous mean-field ansatz without fluctuations cannot describe the spontaneous symmetry breaking, we instead inspect the growth of a tiny (homogeneous) perturbation Δ = 10−4 on the initial state. After the quench, both of the gap functions Δ and \({{\Delta }}^{\prime}\) grow exponentially and converge respectively to nonzero values, although the damped oscillation is slower than the previous case, and the converged values are far below those (Δ 0.18 and \(| {{{\Delta }}}^{\prime}| \simeq 0.03\)) expected for equilibrium with the effective temperature.


In the present paper, we reveal that Floquet-induced interactions do indeed give rise to a novel way for creating topological superconductivity. Let us recapitulate advantages of the present proposal for the Floquet topological superconductivity. In the previous study of Floquet topological superconductivity in cuprates17, the topological transition is triggered by the modulation of the kinetic part of the Hamiltonian [diagonal components in Eq. (8)], with the pairing symmetry of the gap function remaining the same. The nontrivial structure of the kinetic part necessitates the presence of a strong Rashba spin-orbit coupling, which would limit the applicable class of materials. In the present approach, by contrast, we exploit the correlation effects themselves, with which we can directly modulate the pairing symmetry to obtain the topological superconductivity. Our approach does not require tailored structures in the one-body part, either, and thus a simple square-lattice Hubbard model suffices for inducing the topological transition. The present approach is also advantageous in achieving a large topological gap. Namely, the topological gap we conceive is comparable with kBTc (since the \({F}^{{x}^{2}-{y}^{2}}({{{{{{{\boldsymbol{k}}}}}}}})\) and Fxy(k) components have the same order of magnitude), while in the previous studies the size of the topological gap is bounded, e.g. by the Rashba spin-orbit coupling and estimated to be ~1 K.

While we have evaluated the increase of the effective temperature upon a sudden change in the field amplitude (which might be evaded by adiabatic ramping of the field), there is also a many-body heating process that is dropped in the present formulation. In isolated, nonintegrable many-body systems in general, the exact eigenstates of \({\hat{H}}_{{{{{{{{\rm{F}}}}}}}}}\) in the thermodynamic limit at long times are believed to represent a featureless, infinite-temperature state (sometimes called the Floquet eigenstate thermalisation hypothesis35,36,37,38,39,40). Thus, the present strong-coupling expansion for the nontrivial structure should be interpreted as an asymptotic expansion (with a vanishing radius of convergence) of this featureless Hamiltonian. The expanded Hamiltonian truncated at an optimal order accurately describes dynamics towards a long-lived state (dubbed as Floquet prethermalisation40,41,42,43), while the inevitable small truncation error separately describes a slow heating process towards the infinite temperature.

Specifically, the present expansion is characterised by the energy denominators of the form (nU − mω) with integers n, m, in which the enhancement of γ and Jχ grows as the resonance is approached. We have to note, however, that the accuracy of the asymptotic expansion becomes degraded, i.e., the time scale over which the effective Hamiltonian remains valid shrinks (with heating becoming faster) as we come closer to the resonance with vanishing denominators. Thus, we will have to examine whether the time scale t ~ 10/t0 for the emergence of \({{{\Delta }}}^{\prime}\) (see Fig. 6b) lies within the validity of the Floquet tJ description, with more sophisticated methods including direct analyses of a time-dependent problem, in future works. While the emergence of the topological superconductivity is verified here with a numerically economical approach, we do obtain in the present paper the effective Hamiltonian with the crucial time-reversal breaking by fully taking account of the noncommutative nature of the Gutzwiller projector \({\hat{P}}_{{{{{{{{\rm{G}}}}}}}}}\) (whereas the usual hopping terms are commutative). It should be thus important to retain such correlation effects in performing sophisticated calculations.

As for “nonequilibrium-induced superconductivity” (i.e., laser illumination making a system superconducting even when we start from T above Tc) discussed in the present paper, there is existing literature that reports laser-induced phenomena44 along with related theories45,46,47,48, although the time scale and proposed mechanism are quite different from the present paper. Whether the present theory has some possible relevance will be a future problem.

Let us turn to the required field amplitude and frequency for experimental feasibility. Specifically, if we want to employ the enhancement of time-reversal breaking around ω = U/2 or ω = U, the required field intensity is E ~ 10t0/a, which corresponds to E ~ 102 MV/cm for the typical cuprates with t0 0.4 eV, a 3 Å. One reason why the strong intensities are required derives from the fact that the time-reversal breaking terms evoked here are of fourth order in E, while usually the time-reversal breaking terms can be of second order11, 12. This comes from the cancellation similar to Fig. 2a for the present square lattice [see Eq. (44) for details], and can be evaded in e.g. honeycomb and kagome lattices. So the application of the present mechanism for the Floquet topological superconductivity to a wider class of materials with various lattice structures and/or multi-orbitals may be an interesting strategy. More trivially, going to low frequencies is another practical route for the enhanced γ, since the required intensity scales with the frequency ω. A possibility of chiral superconductivity triggered by the same interaction but with a different mechanism (such as proposed for the doped spin liquid on triangular lattice49) is also of interest.

We can further raise an intriguing possibility that, since the emergence of the topological superconductivity is intimately related to the excitation of Higgs modes as stressed above, the topological signature might be enhanced by resonantly exciting the Higgs modes, which provides another future problem.


Time-periodic Schrieffer-Wolff transformation

To obtain the effective low-energy Hamiltonian in the presence of the laser electric field, we employ the time-periodic Schrieffer-Wolff transformation (a canonical transformation). Following a previous study11 (but extending it for the case where holes exist; see also ref. 19), we decompose the Hubbard Hamiltonian as

$$\hat{H}(t)=-\lambda \mathop{\sum }\limits_{m=-\infty }^{\infty }({\hat{T}}_{-1,m}+{\hat{T}}_{0,m}+{\hat{T}}_{+1,m}){e}^{-im\omega t}+U\hat{D},$$

where λ is a bookkeeping parameter bridging the atomic limit λ = 0 to the system of interest at λ = 1, and \(\hat{D}\equiv {\sum }_{i}{\hat{n}}_{i\uparrow }{\hat{n}}_{i\downarrow }\) counts the number of doubly-occupied sites. The hopping operator \({\hat{T}}_{d,m}\) describes the process that increases the number of doubly-occupied sites by d, as given by

$${\hat{T}}_{0,m}=\mathop{\sum}\limits_{ij\sigma }{t}_{ij}^{(m)}\left[{\hat{n}}_{i\bar{\sigma }}{\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{j\sigma }{\hat{n}}_{j\bar{\sigma }}+(1-{\hat{n}}_{i\bar{\sigma }}){\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{j\sigma }(1-{\hat{n}}_{j\bar{\sigma }})\right],$$
$${\hat{T}}_{+1,m}=\mathop{\sum}\limits_{ij\sigma }{t}_{ij}^{(m)}{\hat{n}}_{i\bar{\sigma }}{\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{j\sigma }(1-{\hat{n}}_{j\bar{\sigma }})={\hat{T}}_{-1,-m}^{{{{\dagger}}} },$$
$${t}_{ij}^{(m)}={t}_{ij}\frac{\omega }{2\pi }\int\nolimits_{0}^{2\pi /\omega }dt{e}^{-i{{{{{{{\boldsymbol{A}}}}}}}}(t)\cdot {{{{{{{{\boldsymbol{R}}}}}}}}}_{ij}+im\omega t}$$
$$={t}_{ij}{{{{{{{{\mathcal{J}}}}}}}}}_{m}({A}_{ij}){(-1)}^{m}{e}^{im{\theta }_{ij}},$$

where \(\bar{\sigma }\equiv -\sigma\). We also decompose the generator \(\hat{{{\Lambda }}}(t)\) in Eq. (4) into \({e}^{i\hat{{{\Lambda }}}(t)}={e}^{i{\hat{{{\Lambda }}}}_{{{{{{{{\rm{h}}}}}}}}}(t)}{e}^{i{\hat{{{\Lambda }}}}_{{{{{{{{\rm{c}}}}}}}}}(t)}\), where \({\hat{{{\Lambda }}}}_{{{{{{{{\rm{c}}}}}}}}}\) eliminates the charge excitations (doubly-occupied sites) from the transformed Hamiltonian, while \({\hat{{{\Lambda }}}}_{{{{{{{{\rm{h}}}}}}}}}\) makes the Hamiltonian static.

We first consider \({\hat{H}}_{{{{{{{{\rm{c}}}}}}}}}(t):= {\hat{P}}_{G}{e}^{i{\hat{{{\Lambda }}}}_{{{{{{{{\rm{c}}}}}}}}}(t)}(\hat{H}(t)-i{\partial }_{t}){e}^{-i{\hat{{{\Lambda }}}}_{{{{{{{{\rm{c}}}}}}}}}(t)}{\hat{P}}_{G}\). Let us introduce a series solution,

$${\hat{{{\Lambda }}}}_{{{{{{{{\rm{c}}}}}}}}}(t)=\mathop{\sum }\limits_{n=1}^{\infty }\mathop{\sum}\limits_{d\ne 0}\mathop{\sum }\limits_{m=-\infty }^{\infty }{\lambda }^{n}{\hat{{{\Lambda }}}}_{+d,m}^{(n)}{e}^{-im\omega t}$$

with \([\hat{D},{\hat{{{\Lambda }}}}_{+d,m}^{(n)}]=d{\hat{{{\Lambda }}}}_{+d,m}^{(n)}\), which eliminates the charge excitation from \({\hat{H}}_{{{{{{{{\rm{c}}}}}}}}}(t)\), i.e., \([\hat{D},{e}^{i{\hat{{{\Lambda }}}}_{{{{{{{{\rm{c}}}}}}}}}(t)}(\hat{H}(t)-i{\partial }_{t}){e}^{-i{\hat{{{\Lambda }}}}_{{{{{{{{\rm{c}}}}}}}}}(t)}]=0\). The form of \({\hat{{{\Lambda }}}}_{+d,m}^{(n)}\) can be uniquely determined order by order, and we arrive at

$${\hat{H}}_{{{{{{{{\rm{c}}}}}}}}} = -\lambda \mathop{\sum }\limits_{m=-\infty }^{\infty }{\hat{P}}_{G}{\hat{T}}_{0,m}{\hat{P}}_{G}{e}^{-im\omega t}\\ +{\lambda }^{2}\mathop{\sum }\limits_{n,m=-\infty }^{\infty }\frac{{\hat{P}}_{G}\left[{\hat{T}}_{+1,n},{\hat{T}}_{-1,m-n}\right]{\hat{P}}_{G}}{2(U-n\omega )}{e}^{-im\omega t}+{{{{{{{\rm{H.c.}}}}}}}}+O({\lambda }^{3}).$$

While this Hamiltonian projected onto the spin subspace is evaluated in a previous study11, here we need to consider the expression for nonzero numbers of holes. We then obtain

$${\hat{P}}_{G}\left[{\hat{T}}_{+1,n},{\hat{T}}_{-1,m-n}\right]{\hat{P}}_{G} {\hskip 6pt}=-\mathop{\sum}\limits_{ijk\sigma {\sigma }^{\prime}}{\hat{P}}_{G}({t}_{ij}^{(m-n)}{\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{j\sigma }){\hat{n}}_{j\bar{\sigma }}({t}_{jk}^{(n)}{\hat{c}}_{j{\sigma }^{\prime}}^{{{{\dagger}}} }{\hat{c}}_{k{\sigma }^{\prime}}){\hat{P}}_{G}$$
$$=\mathop{\sum}\limits_{ijk\sigma {\sigma }^{\prime}}{t}_{ij}^{(m-n)}{t}_{jk}^{(n)}{\hat{P}}_{G}\left[({\hat{c}}_{i\sigma }^{{{{\dagger}}} }{{{{{{{{\boldsymbol{\sigma }}}}}}}}}_{\sigma {\sigma }^{\prime}}{\hat{c}}_{k{\sigma }^{\prime}})\cdot {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{j}-\frac{1}{2}{\delta }_{\sigma {\sigma }^{\prime}}{\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{k\sigma }{\hat{n}}_{j}\right]{\hat{P}}_{G}.$$

Note that, while we recover the Heisenberg spin–spin interaction for k = i, the so-called three-site terms with k ≠ i arise as well. The final static Hamiltonian \({\hat{H}}_{{{{{{{{\rm{F}}}}}}}}}={e}^{i{\hat{{{\Lambda }}}}_{{{{{{{{\rm{h}}}}}}}}}(t)}({\hat{H}}_{{{{{{{{\rm{c}}}}}}}}}-i{\partial }_{t}){e}^{-i{\hat{{{\Lambda }}}}_{{{{{{{{\rm{h}}}}}}}}}(t)}\) is obtained by using the formula8, 11, 22

$${\hat{H}}_{{{{{{{{\rm{F}}}}}}}}}={\hat{H}}_{{{{{{{{\rm{c}}}}}}}},0}+\mathop{\sum}\limits_{m\ne 0}\frac{\left[{\hat{H}}_{{{{{{{{\rm{c}}}}}}}},-m},{\hat{H}}_{{{{{{{{\rm{c}}}}}}}},m}\right]}{2m\omega }+O({\omega }^{-2}),$$

where \({\hat{H}}_{{{{{{{{\rm{c}}}}}}}},m}\equiv (\omega /2\pi )\int\nolimits_{0}^{2\pi /\omega }dt{\hat{H}}_{{{{{{{{\rm{c}}}}}}}}}{e}^{im\omega t}\). The second term is calculated up to λ2 as

$$\mathop{\sum}\limits_{m\ne 0}\frac{\left[{\hat{H}}_{{{{{{{{\rm{c}}}}}}}},-m},{\hat{H}}_{{{{{{{{\rm{c}}}}}}}},m}\right]}{2m\omega } ={\lambda }^{2}\mathop{\sum}\limits_{m\ne 0}\frac{{\hat{P}}_{G}\left[{\hat{T}}_{0,-m},{\hat{T}}_{0,m}\right]{\hat{P}}_{G}}{2m\omega }\hskip 11pc$$
$$\hskip 6.4pc={\lambda }^{2}\mathop{\sum}\limits_{ijk\sigma {\sigma }^{\prime}}\mathop{\sum}\limits_{m\ne 0}\frac{{t}_{ij}^{(-m)}{t}_{jk}^{(m)}}{m\omega } {\hat{P}}_{G}\left[({\hat{c}}_{i\sigma }^{{{{\dagger}}} }{{{{{{{{\boldsymbol{\sigma }}}}}}}}}_{\sigma {\sigma }^{\prime}}{\hat{c}}_{k{\sigma }^{\prime}})\cdot {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{j}+{\delta }_{\sigma {\sigma }^{\prime}}{\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{k\sigma }\frac{2-{\hat{n}}_{j}}{2}\right]{\hat{P}}_{G},$$

where we have used \(\{{\hat{c}}_{i\sigma }(1-{\hat{n}}_{i\bar{\sigma }}),(1-{\hat{n}}_{j{\bar{\sigma }}^{\prime}}){\hat{c}}_{j{\sigma }^{\prime}}^{{{{\dagger}}} }\}={\delta }_{ij}[{\delta }_{\sigma {\sigma }^{\prime}}(1-{\hat{n}}_{i}/2)+{{{{{{{{\boldsymbol{\sigma }}}}}}}}}_{\sigma {\sigma }^{\prime}}\cdot {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{i}]\), \(\{(1-{\hat{n}}_{i\bar{\sigma }}){\hat{c}}_{i\sigma }^{{{{\dagger}}} },(1-{\hat{n}}_{j{\bar{\sigma }}^{\prime}}){\hat{c}}_{j{\sigma }^{\prime}}^{{{{\dagger}}} }\}=0\).

The effective Hamiltonian Eq. (4) is obtained up to the second order as

$${\hat{H}}_{{{{{{{{\rm{F}}}}}}}}} = -\mathop{\sum}\limits_{ij\sigma }{\tilde{t}}_{ij}{\hat{P}}_{G}{\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{j\sigma }{\hat{P}}_{G}+\frac{1}{2}\mathop{\sum}\limits_{ij}{J}_{ij}\left({\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{i}\cdot {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{j}-\frac{1}{4}{\hat{n}}_{i}{\hat{n}}_{j}\right)\\ +\mathop{\sum}\limits_{ijk\sigma {\sigma }^{\prime}}{{{\Gamma }}}_{i,j;k}{\hat{P}}_{G}\left[({\hat{c}}_{i\sigma }^{{{{\dagger}}} }{{{{{{{{\boldsymbol{\sigma }}}}}}}}}_{\sigma {\sigma }^{\prime}}{\hat{c}}_{j{\sigma }^{\prime}})\cdot {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{k}-\frac{1}{2}{\delta }_{\sigma {\sigma }^{\prime}}{\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{j\sigma }{\hat{n}}_{k}\right]{\hat{P}}_{G},$$


$${\tilde{t}}_{ij}={t}_{ij}^{(0)}-\mathop{\sum}\limits_{k}\mathop{\sum}\limits_{m\ne 0}\frac{{t}_{ik}^{(-m)}{t}_{kj}^{(m)}}{m\omega },$$
$${J}_{ij}=\mathop{\sum }\limits_{m=-\infty }^{\infty }\frac{4U| {t}_{ij}^{(m)}{| }^{2}}{{U}^{2}-{m}^{2}{\omega }^{2}},$$
$${{{\Gamma }}}_{i,j;k}=\left[\frac{{t}_{ik}^{(0)}{t}_{kj}^{(0)}}{U}+\mathop{\sum}\limits_{m\ne 0}\frac{{t}_{ik}^{(-m)}{t}_{kj}^{(m)}}{m\omega (1-m\omega /U)}\right](1-{\delta }_{ij}).$$

Note that the second term in the hopping \({\tilde{t}}_{ij}\) describing the two-step hopping vanishes for the square lattice [see Fig. 2a], and the renormalised hopping is given as \({\tilde{t}}_{ij}={t}_{ij}^{(0)}={t}_{ij}{{{{{{{{\mathcal{J}}}}}}}}}_{0}({A}_{ij})\) if we put m = 0 in Eq. (26). For the Heisenberg term Jij we end up with Eq. (6) in the main text. The two-step correlated hopping is much more intricate, and reads

$${{{\Gamma }}}_{i,j;k} = \frac{{t}_{ik}{t}_{kj}{{{{{{{{\mathcal{J}}}}}}}}}_{0}({A}_{ik}){{{{{{{{\mathcal{J}}}}}}}}}_{0}({A}_{kj})}{U}+\mathop{\sum}\limits_{m\ne 0}\frac{{t}_{ik}{t}_{kj}{{{{{{{{\mathcal{J}}}}}}}}}_{m}({A}_{ik}){{{{{{{{\mathcal{J}}}}}}}}}_{m}({A}_{kj})}{m\omega (1-m\omega /U)}{e}^{im({\theta }_{jk}-{\theta }_{ik})}.$$

In the main text, we have also considered the scalar spin-chirality term \({J}_{ijk}^{\chi }\), which appears in the fourth-order perturbation. While the perturbative processes involving three sites are considered in previous studies11, 12, we need to evaluate the processes involving four sites as well for the present case of the square lattice as we see in Eq. (44) below. By dropping the density-dependent part, \({\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{i}\cdot ({\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{j}\times {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{k})(1-{\hat{n}}_{h}) \sim O(\delta )\), we obtain

$${J}_{ijk}^{\chi }=2{{{{{{{\rm{Im}}}}}}}}\mathop{\sum }\limits_{lmn=-\infty }^{\infty }({K}_{ijk}^{lmn}+{K}_{jki}^{lmn}+{K}_{kij}^{lmn}-{K}_{jik}^{lmn}-{K}_{kji}^{lmn}-{K}_{ikj}^{lmn}),$$


$${K}_{ijk}^{lmn}= \frac{2{t}_{ij}^{(-l-m)}{t}_{ji}^{(l-m)}{t}_{jk}^{(m-n)}{t}_{kj}^{(n+m)}(1-{\delta }_{m,0})}{m\omega [U+(l-m)\omega ][U-(n+m)\omega ]}\hfill\\ -\frac{2{t}_{ij}^{(m-n)}{t}_{ji}^{(l)}{t}_{jk}^{(n)}{t}_{kj}^{(-l-m)}}{(U+l\omega )(U-m\omega )(U-n\omega )}\hfill\\ -\mathop{\sum}\limits_{h\ne ijk}\frac{{t}_{ij}^{(-l-m)}{t}_{jk}^{(l)}{t}_{kh}^{(m-n)}{t}_{hi}^{(n)}+{t}_{ij}^{(m-n)}{t}_{jk}^{(n)}{t}_{kh}^{(-l-m)}{t}_{hi}^{(l)}}{(U+l\omega )(U+n\omega )[U+(n-m)\omega ]}\hfill\\ -2\mathop{\sum}\limits_{h\ne ijk}\frac{\left[({t}_{ij}^{(l)}{t}_{jk}^{(-l-m)}+{t}_{ij}^{(-l-m)}{t}_{jk}^{(l)}){t}_{kh}^{(m-n)}+{t}_{ij}^{(m-n)}{t}_{jk}^{(l)}{t}_{kh}^{(-l-m)}\right]{t}_{hi}^{(n)}}{(U+l\omega )(U+n\omega )(U+m\omega )}\hfill\\ +\mathop{\sum}\limits_{h\ne ijk}\frac{{t}_{ij}^{(m-n)}{t}_{jk}^{(-l-m)}{t}_{kh}^{(l)}{t}_{hi}^{(n)}+{t}_{ij}^{(n)}{t}_{jk}^{(l)}{t}_{kh}^{(-l-m)}{t}_{hi}^{(m-n)}}{(U+l\omega )(U-n\omega )(U-m\omega )}.$$

The above expression is derived under an assumption \({t}_{ji}^{(n)}={t}_{ij}^{(n)}{(-1)}^{n}\), which holds for monochromatic laser lights. In particular, the chiral coupling of crucial interest reads, for the present square lattice with second-neighbour hopping,

$${J}_{i,i+y,i+x}^{\chi }={J}_{\chi }=2{J}_{\chi }^{\prime}+2{J}_{\chi }^{^{\prime\prime} },$$
$${J}_{i-x,i,i+x+y}^{\chi }=\, {J}_{\chi }^{\prime}= \,4{t}_{0}^{2}{t}_{0}^{^{\prime} 2}\mathop{\sum}\limits_{lmn}\sin \frac{m\pi }{2}\hfill\\ \times \left[\frac{{D}_{m-l}}{m\omega }+({D}_{m-l}+2{D}_{n-l}){D}_{n-m}\right]{D}_{n+m}\hfill\\ \times \left[{{{{{{{{\mathcal{J}}}}}}}}}_{l+m}(\sqrt{2}A){{{{{{{{\mathcal{J}}}}}}}}}_{l-m}(\sqrt{2}A){{{{{{{{\mathcal{J}}}}}}}}}_{n+m}(A){{{{{{{{\mathcal{J}}}}}}}}}_{n-m}(A)\right.\\ +\left.{{{{{{{{\mathcal{J}}}}}}}}}_{n+m}(\sqrt{2}A){{{{{{{{\mathcal{J}}}}}}}}}_{n-m}(\sqrt{2}A){{{{{{{{\mathcal{J}}}}}}}}}_{l+m}(A){{{{{{{{\mathcal{J}}}}}}}}}_{l-m}(A)\right],$$
$${J}_{i-x,i-y,i+x}^{\chi }={J}_{\chi }^{^{\prime\prime} }=\; 4{t}_{0}^{2}{t}_{0}^{^{\prime} 2}\mathop{\sum}\limits_{lmn}\sin \frac{(3m+2n)\pi }{4}\hfill\\ \times \left[{D}_{l}{D}_{n}{D}_{n-m}+({D}_{l}{D}_{-n}+{D}_{-n}{D}_{-n+m}){D}_{l+m-n}\right]\\ \times \left[{{{{{{{{\mathcal{J}}}}}}}}}_{-l-m}(A){{{{{{{{\mathcal{J}}}}}}}}}_{l}(A){{{{{{{{\mathcal{J}}}}}}}}}_{m-n}(\sqrt{2}A){{{{{{{{\mathcal{J}}}}}}}}}_{n}(\sqrt{2}A)\right.\hfill\\ +\,\left.\,{{{{{{{{\mathcal{J}}}}}}}}}_{m-n}(A){{{{{{{{\mathcal{J}}}}}}}}}_{n}(A){{{{{{{{\mathcal{J}}}}}}}}}_{-l-m}(\sqrt{2}A){{{{{{{{\mathcal{J}}}}}}}}}_{l}(\sqrt{2}A)\right],$$

where Dn = (U + nω)−1 and A = Ea/ω with a being the lattice constant.

In the “Discussion” section, we mentioned that the time-reversal breaking terms are of fourth order in E due to a cancellation similar to Fig. 2a. Let us here elaborate on that, which marks the importance of the perturbative processes involving four sites. If we expand Eq. (40) up to E2, we can find

$$\begin{array}{l}{{{{{{{\rm{Im}}}}}}}}\mathop{\sum }\limits_{lmn=-\infty }^{\infty }({K}_{ijk}^{lmn}-{K}_{kji}^{lmn})\propto i({{{{{{{{\boldsymbol{E}}}}}}}}}^{* }\times {{{{{{{\boldsymbol{E}}}}}}}})\cdot \left({t}_{kj}{t}_{ji}{{{{{{{{\boldsymbol{R}}}}}}}}}_{ij}\times {{{{{{{{\boldsymbol{R}}}}}}}}}_{jk}+\mathop{\sum}\limits_{h\ne ijk}{t}_{kh}{t}_{hi}{{{{{{{{\boldsymbol{R}}}}}}}}}_{ih}\times {{{{{{{{\boldsymbol{R}}}}}}}}}_{hk}\right){t}_{ij}{t}_{jk}.\end{array}$$

The first term on the second line (three-site term) coincides with the result in a previous study11. While the second term (four-site term) is absent for e.g. honeycomb and kagome lattices with no candidates for the fourth site h, square lattice accommodates this additional contribution. Then we can note that we have a combination of blue and red paths as depicted in Fig. 2a, which was invoked for the three-site term but also applies to the four-site term involving tkjtji and tkhthi. There, due to the factor R × R, the first and second terms cancel with each other for the square lattice (even if we consider many-body effects). The square lattice model does have a nonzero coefficient, however, if we go over to E4 in the presence of the next-nearest-neighbour hopping, as we have seen Eq. (21).

Gutzwiller projection

Here we analyse the ground-state property of the system using the mean-field approximation with the Gutzwiller ansatz26, 29. Namely, we consider an ansatz for the wavefunction,

$$\left|{{\Psi }}\right\rangle ={\hat{P}}_{G}\left|{{{\Psi }}}_{0}\right\rangle ,$$
$$\left|{{{\Psi }}}_{0}\right\rangle ={\mathop{\prod}\limits_{{{{{{{{\boldsymbol{k}}}}}}}}}}\left({u}_{{{{{{{{\boldsymbol{k}}}}}}}}}+{v}_{{{{{{{{\boldsymbol{k}}}}}}}}}{\hat{c}}_{{{{{{{{\boldsymbol{k}}}}}}}}\uparrow }^{{{{\dagger}}} }{\hat{c}}_{-{{{{{{{\boldsymbol{k}}}}}}}}\downarrow }^{{{{\dagger}}} }\right)\left|0\right\rangle ,$$

with \({\hat{P}}_{G}={\prod }_{i}(1-{\hat{n}}_{i\uparrow }{\hat{n}}_{i\downarrow })\) being the Gutzwiller projection. Here, \({\hat{c}}_{{{{{{{{\boldsymbol{k}}}}}}}}\sigma }={N}^{-1/2}\mathop{\sum}\nolimits_{i}{\hat{c}}_{i\sigma }{e}^{-i{{{{{{{\boldsymbol{k}}}}}}}}\cdot {{{{{{{{\boldsymbol{R}}}}}}}}}_{i}}\) with N being the number of lattice sites. The ground state within this ansatz can be obtained by minimising the expectation value,

$${E}_{0}=\frac{\langle {{\Psi }}| {\hat{H}}_{{{{{{{{\rm{F}}}}}}}}}| {{\Psi }}\rangle }{\langle {{\Psi }}| {{\Psi }}\rangle }=\frac{{\langle {\hat{P}}_{G}{\hat{H}}_{{{{{{{{\rm{F}}}}}}}}}{\hat{P}}_{G}\rangle }_{0}}{{\langle {\hat{P}}_{G}\rangle }_{0}}.$$

To evaluate the Gutzwiller projection approximately, we replace the expectation value with the site-diagonal ones, where we decompose the projection operator as

$${\hat{P}}_{G}=\mathop{\sum}\limits_{{c}_{1},\ldots ,{c}_{N}=h,\uparrow ,\downarrow }\left(\mathop{\prod }\limits_{i = 1}^{N}{\hat{P}}_{i{c}_{i}}\right)$$

with \({\hat{P}}_{ih}\equiv (1-{\hat{n}}_{i\uparrow })(1-{\hat{n}}_{i\downarrow }),{\hat{P}}_{i\sigma }\equiv {n}_{i\sigma }(1-{n}_{i\bar{\sigma }})\). Then we can evaluate the denominator as

$${\langle {\hat{P}}_{G}\rangle }_{0}\simeq \mathop{\sum}\limits_{{c}_{1},\ldots ,{c}_{N}=h,\uparrow ,\downarrow }\mathop{\prod }\limits_{i = 1}^{N}{\langle {\hat{P}}_{i{c}_{i}}\rangle }_{0}\hskip 6pc$$
$$=\frac{N!}{(N\delta )!(Nf)!(Nf)!}{(\bar{f}\bar{f})}^{N\delta }{(f\bar{f})}^{Nf}{(f\bar{f})}^{Nf}$$
$$\sim \frac{{(\bar{f}\bar{f})}^{N\delta }{(f\bar{f})}^{Nf}{(f\bar{f})}^{Nf}}{{\delta }^{N\delta }{f}^{Nf}{f}^{Nf}}={({\bar{f}}^{2}{\delta }^{-1})}^{N\delta }{\bar{f}}^{2Nf},$$

where \(f=(1-\delta )/2,\bar{f}=(1+\delta )/2\), and we have used n! ~ (n/e)n on the last line. We can evaluate the numerators in the same manner. For the hopping, exchange, and spin-dependent three-site terms, we obtain, respectively,

$${\langle {\hat{P}}_{G}{\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{j\sigma }{\hat{P}}_{G}\rangle }_{0}\simeq {({\bar{f}}^{2}{\delta }^{-1})}^{N\delta -1}{\bar{f}}^{2Nf-1}{\langle \bar{f}{\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{j\sigma }\bar{f}\rangle }_{0}$$
$$=\frac{2\delta }{1+\delta }{\langle {\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{j\sigma }\rangle }_{0}{\langle {\hat{P}}_{G}\rangle }_{0},$$
$${\langle {\hat{P}}_{G}{\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{i}\cdot {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{j}{\hat{P}}_{G}\rangle }_{0}\simeq {({\bar{f}}^{2}{\delta }^{-1})}^{N\delta }{\bar{f}}^{2Nf-2}{\langle {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{i}\cdot {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{j}\rangle }_{0}$$
$$=\frac{4}{{(1+\delta )}^{2}}{\langle {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{i}\cdot {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{j}\rangle }_{0}{\langle {\hat{P}}_{G}\rangle }_{0},$$
$${\langle {\hat{P}}_{G}{\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{j{\sigma }^{\prime}}{\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{k}{\hat{P}}_{G}\rangle }_{0}\simeq {({\bar{f}}^{2}{\delta }^{-1})}^{N\delta -1}{\bar{f}}^{2Nf-2}{\langle \bar{f}{\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{j{\sigma }^{\prime}}\bar{f}{\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{k}\rangle }_{0}$$
$$=\frac{4\delta }{{(1+\delta )}^{2}}{\langle {\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{j{\sigma }^{\prime}}{\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{k}\rangle }_{0}{\langle {\hat{P}}_{G}\rangle }_{0}.$$

We also obtain \({\langle {\hat{P}}_{G}{\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{i}\cdot ({\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{j}\times {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{k}){\hat{P}}_{G}\rangle }_{0}\simeq [8/{(1+\delta )}^{3}]{\langle {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{i}\cdot ({\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{j}\times {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{k})\rangle }_{0}{\langle {\hat{P}}_{G}\rangle }_{0}\) in the same manner.

The remaining terms have an ambiguity in the Gutzwiller factor, because they are accompanied by the density operator \({\hat{P}}_{G}{\hat{n}}_{i}{\hat{P}}_{G}={\hat{P}}_{G}[\mathop{\sum}\nolimits_{\sigma }{\hat{n}}_{i\sigma }(1-{\hat{n}}_{i\bar{\sigma }})]{\hat{P}}_{G}\), which can be regarded either as an operator or a constant \({\langle {\hat{n}}_{i\sigma }(1-{\hat{n}}_{i\bar{\sigma }})\rangle }_{0}\simeq f\bar{f}\), in the above scheme. Here, we discard the second-order fluctuation around the expectation value, \(({\hat{n}}_{i\sigma }-f)(1-{\hat{n}}_{i\bar{\sigma }}-\bar{f})\), to approximate the projected density operator as \(\mathop{\sum}\nolimits_{\sigma }{\hat{n}}_{i\sigma }(1-{\hat{n}}_{i\bar{\sigma }})\simeq {\hat{n}}_{i}\delta +2{f}^{2}\). Then the Gutzwiller factors for the remaining terms are evaluated as

$${\langle {\hat{P}}_{G}{\hat{n}}_{i}{\hat{n}}_{j}{\hat{P}}_{G}\rangle }_{0} \simeq \frac{4}{{(1+\delta )}^{2}}{\langle ({\hat{n}}_{i}\delta +2{f}^{2})({\hat{n}}_{j}\delta +2{f}^{2})\rangle }_{0}{\langle {\hat{P}}_{G}\rangle }_{0}\\ =\frac{4{\delta }^{2}}{{(1+\delta )}^{2}}{\langle {\hat{n}}_{i}{\hat{n}}_{j}\rangle }_{0}{\langle {\hat{P}}_{G}\rangle }_{0}+\frac{2\delta {(1-\delta )}^{2}}{{(1+\delta )}^{2}}{\langle {\hat{n}}_{i}+{\hat{n}}_{j}\rangle }_{0}{\langle {\hat{P}}_{G}\rangle }_{0}+{{{{{{{\rm{const.}}}}}}}},$$
$${\langle {\hat{P}}_{G}{\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{j\sigma }{\hat{n}}_{k}{\hat{P}}_{G}\rangle }_{0} \simeq \frac{4\delta }{{(1+\delta )}^{2}}{\langle {\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{j\sigma }({\hat{n}}_{k}\delta +2{f}^{2})\rangle }_{0}{\langle {\hat{P}}_{G}\rangle }_{0}\\ =\frac{4{\delta }^{2}}{{(1+\delta )}^{2}}{\langle {\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{j\sigma }{\hat{n}}_{k}\rangle }_{0}{\langle {\hat{P}}_{G}\rangle }_{0}+\frac{2\delta {(1-\delta )}^{2}}{{(1+\delta )}^{2}}{\langle {\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{j\sigma }\rangle }_{0}{\langle {\hat{P}}_{G}\rangle }_{0}.$$

Note that the density-density term is known to have small effects in the variational Monte Carlo calculation in the low-doping regime, with which the present treatment is consistent.

With these expressions, the minimisation of E0 turns out to be reduced to that of \({\langle {\hat{H}}_{{{{{{{{\rm{F}}}}}}}}0}\rangle }_{0}\), where \({\hat{H}}_{{{{{{{{\rm{F}}}}}}}}0}\) is the Hamiltonian with the modified coupling constant but without the Gutzwiller projection, as given by

$${\hat{H}}_{{{{{{{{\rm{F}}}}}}}}0}= -g\delta \mathop{\sum}\limits_{ij\sigma }\left[{\tilde{t}}_{ij}+\frac{{(1-\delta )}^{2}}{2(1+\delta )}\mathop{\sum}\limits_{k}{{{\Gamma }}}_{ijk}\right]{\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{j\sigma }\hfill\\ +\frac{{g}^{2}}{2}\mathop{\sum}\limits_{ij}{J}_{ij}\left({\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{i}\cdot {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{j}-\frac{{\delta }^{2}}{4}{\hat{n}}_{i}{\hat{n}}_{j}\right)+\frac{{g}^{3}}{6}\mathop{\sum}\limits_{ijk}{J}_{ijk}^{\chi }({\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{i}\times {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{j})\cdot {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{k}\\ +{g}^{2}\delta \mathop{\sum}\limits_{ijk\sigma {\sigma }^{\prime}}{{{\Gamma }}}_{ijk}\left[({\hat{c}}_{i\sigma }^{{{{\dagger}}} }{{{{{{{{\boldsymbol{\sigma }}}}}}}}}_{\sigma {\sigma }^{\prime}}{\hat{c}}_{j{\sigma }^{\prime}})\cdot {\hat{{{{{{{{\boldsymbol{S}}}}}}}}}}_{k}-\frac{\delta }{2}{\delta }_{\sigma {\sigma }^{\prime}}{\hat{c}}_{i\sigma }^{{{{\dagger}}} }{\hat{c}}_{j\sigma }{\hat{n}}_{k}\right]$$


$$g=\frac{2}{1+\delta }.$$

Differenciating \({\langle {\hat{H}}_{{{{{{{{\rm{F}}}}}}}}0}\rangle }_{0}\) by uk, vk in Eq. (46), we arrive at the Bogoliubov-de Gennes Hamiltonian Eq. (8) in the main text. In particular, the detailed form for the present system is given as

$$\varepsilon ({{{{{{{\boldsymbol{k}}}}}}}})= -\mu +\frac{1}{2}{\varepsilon }_{x}(\cos {k}_{x}+\cos {k}_{y})+{\varepsilon }_{x+y}\cos {k}_{x}\cos {k}_{y}\hfill\\ -4g\delta (1-\delta ){{{{{{{\rm{Re}}}}}}}}{{{\Gamma }}}_{i-x-y,i+x;i}(\cos 2{k}_{x}\cos {k}_{y}+\cos {k}_{x}\cos 2{k}_{y})\\ -g\delta (1-\delta ){{{{{{{\rm{Re}}}}}}}}(2{{{\Gamma }}}_{i-x,i+x;i+y}+{{{\Gamma }}}_{i-x,i+x;i})(\cos 2{k}_{x}+\cos 2{k}_{y})\\ -2g\delta (1-\delta ){{{{{{{\rm{Re}}}}}}}}{{{\Gamma }}}_{i-x-y,i+x+y;i}\cos 2{k}_{x}\cos 2{k}_{y}\hfill\\ +\frac{3}{2}{g}^{3}{J}_{\chi }^{\prime}{{{{{{{\rm{Re}}}}}}}}({{{\Delta }}}^{* }{{{\Delta }}}^{\prime})(\cos 2{k}_{x}\cos {k}_{y}+\cos {k}_{x}\cos 2{k}_{y}),$$
$${\varepsilon }_{x}= -4g\delta \tilde{t}-\frac{3-{\delta }^{2}}{2}{g}^{2}J{\chi }_{x}-8g\delta (1-\delta ){{{{{{{\rm{Re}}}}}}}}{{{\Gamma }}}_{i-x,i;i+y}\hfill\\ -2{g}^{2}\delta (3-\delta ){{{{{{{\rm{Re}}}}}}}}(2{{{\Gamma }}}_{i-x,i+y;i}+{{{\Gamma }}}_{i-x,i+x;i}){\chi }_{x}\\ -4{g}^{2}\delta (3-\delta ){{{{{{{\rm{Re}}}}}}}}({{{\Gamma }}}_{i-x,i;i+y}+{{{\Gamma }}}_{i-x-y,i+x;i}){\chi }_{x+y}\\ +\frac{3}{2}{g}^{3}{{{{{{{\rm{Re}}}}}}}}\left[2{J}_{\chi }{{{\Delta }}}^{\prime}{{{\Delta }}}^{* }+{J}_{\chi }^{\prime}{{{\Delta }}}^{\prime}({{{\Delta }}}_{x+2y}^{* }-{{{\Delta }}}_{2x+y}^{* })\right],$$
$${\varepsilon }_{x+y}= -4g\delta {\tilde{t}}^{\prime}-\frac{3-{\delta }^{2}}{2}{g}^{2}{J}^{\prime}{\chi }_{x+y}-4g\delta (1-\delta ){{{{{{{\rm{Re}}}}}}}}{{{\Gamma }}}_{i-x,i+y;i}\hfill\\ -2{g}^{2}\delta (3-\delta ){{{{{{{\rm{Re}}}}}}}}(2{{{\Gamma }}}_{i-x,i+x;i+y}+{{{\Gamma }}}_{i-x-y,i+x+y;i}){\chi }_{x+y}\\ -4{g}^{2}\delta (3-\delta ){{{{{{{\rm{Re}}}}}}}}({{{\Gamma }}}_{i-x,i;i+y}+{{{\Gamma }}}_{i-x-y,i+x;i}){\chi }_{x}\hfill\\ -\frac{3}{2}{g}^{3}{{{{{{{\rm{Re}}}}}}}}\left[2{J}_{\chi }^{^{\prime\prime} }{{{\Delta }}}_{2x}^{* }{{{\Delta }}}^{\prime}-i{J}_{\chi }^{\prime}{{{\Delta }}}^{* }({{{\Delta }}}_{2x+y}+{{{\Delta }}}_{x+2y})\right],$$
$$F({{{{{{{\boldsymbol{k}}}}}}}})= \frac{1}{2}{F}_{x}(\cos {k}_{x}-\cos {k}_{y})+i{F}_{x+y}\sin {k}_{x}\sin {k}_{y}\hfill\\ +\frac{3{g}^{3}{J}_{\chi }^{^{\prime\prime} }}{2}{{{\Delta }}}^{\prime}{\chi }_{x+y}(\cos 2{k}_{x}-\cos 2{k}_{y})\hfill\\ -\frac{3i{g}^{3}{J}_{\chi }^{\prime}}{2}{{\Delta }}{\chi }_{x+y}(\sin 2{k}_{x}\sin {k}_{y}+\sin {k}_{x}\sin 2{k}_{y})\hfill\\ -\frac{3{g}^{3}{J}_{\chi }^{\prime}}{2}{\chi }_{x}{{{\Delta }}}^{\prime}(\cos {k}_{x}\cos 2{k}_{y}-\cos 2{k}_{x}\cos {k}_{y}),$$
$${F}_{x}= {g}^{2}\left[\frac{3+{\delta }^{2}}{2}J-2\delta (3+\delta ){{{{{{{\rm{Re}}}}}}}}(2{{{\Gamma }}}_{i-x,i+y;i}-{{{\Gamma }}}_{i-x,i+x;i})\right]{{\Delta }}\hfill\\ -{g}^{2}\left[4\delta (3+\delta )\gamma +3g{J}_{\chi }{\chi }_{x}+\frac{3}{2}g{J}_{\chi }^{\prime}({\chi }_{2x+y}+{\chi }_{x+2y})\right]{{{\Delta }}}^{\prime}\\ -\frac{3}{2}i{g}^{3}{J}_{\chi }^{\prime}({{{\Delta }}}_{2x+y}+{{{\Delta }}}_{x+2y}){\chi }_{x+y},$$
$${F}_{x+y}= {g}^{2}\left[4\delta (3+\delta )\gamma +3g{J}_{\chi }{\chi }_{x}+\frac{3}{2}g{J}_{\chi }^{\prime}({\chi }_{2x+y}+{\chi }_{x+2y})\right]{{\Delta }}\hfill\\ -{g}^{2}\left[\frac{3+{\delta }^{2}}{2}{J}^{\prime}-2\delta (3+\delta ){{{{{{{\rm{Re}}}}}}}}(2{{{\Gamma }}}_{i-x,i+x;i+y}-{{{\Gamma }}}_{i-x-y,i+x+y;i})\right]{{{\Delta }}}^{\prime}\\ -\frac{3}{2}{g}^{3}\left[{J}_{\chi }^{\prime}{\chi }_{x}({{{\Delta }}}_{2x+y}-{{{\Delta }}}_{x+2y})+2{J}_{\chi }^{^{\prime\prime} }{{{\Delta }}}_{2x}{\chi }_{x+y}\right].$$

When Δ is real, we can further simplify the expressions using χmx+ny = χnx+my and \({{{\Delta }}}_{mx+ny}=-{{{\Delta }}}_{nx+my}^{* }\), after which the first line of Fx+y gives Fxy(k) in the main text.

Data availability

Data are available upon reasonable request.

Code availability

Code is available upon reasonable request.


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S.K. acknowledges JSPS KAKENHI Grant 20K14407, and CREST (Core Research for Evolutional Science and Technology; Grant number JPMJCR19T3) for support. H.A. thanks CREST (Grant number JPMJCR18T4), and JSPS KAKENHI Grant JP17H06138.

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H.A. conceived the basic idea for the topological superconductivity. S.K. has performed the theoretical formulation and numerical calculations. Both authors wrote the manuscript.

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Correspondence to Hideo Aoki.

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Kitamura, S., Aoki, H. Floquet topological superconductivity induced by chiral many-body interaction. Commun Phys 5, 174 (2022).

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