The infinite-range (mean-field) spherical quantum pp-rotor model with p≥3p\ge 3, a longitudinal field hh, and quantum coupling gg has a spin-glass phase with one-step replica symmetry breaking, but the N→∞N\to\infty saddle-point equations leave the breakpoint xx of the Parisi order parameter undetermined. Two prescriptions complete the solution: extremizing the free energy with respect to xx — the rigorously established equilibrium rule in the classical g=0g=0 limit, which yields a local excitation spectrum with an energy gap — or imposing the marginal-stability condition of glassy dynamics, which yields a gapless spectrum whose density vanishes linearly with frequency. Which prescription the thermodynamic equilibrium state obeys at g≠0g\ne 0, h≠0h\ne 0, and which one is realized in physically or experimentally prepared states (for example in programmable Rydberg-atom simulators), is unresolved. The problem is to determine the selection principle for xx, in equilibrium and under dynamical preparation, and thereby to decide whether the realized quantum glass is gapped or marginally stable and gapless, together with observable diagnostics that distinguish the two.

Background

Mean-field spin glasses and replica symmetry breaking. In an infinite-range (fully connected) spin glass, NN degrees of freedom are coupled by independent random exchanges; the paradigmatic example is the Sherrington–Kirkpatrick (SK) model of Ising spins. After averaging the free energy over the disorder using the replica trick — computing the disorder-averaged nn-replica partition function Zn‾\overline{Z^n} and sending n→0n\to 0 — the mean-field spin-glass solution requires replica symmetry breaking (RSB): the order parameter, the matrix of overlaps QabQ_{ab} between replicas aa and bb, is no longer diagonal. In Parisi's solution the overlaps are organized by a monotone function q(u)q(u) on 0≤u≤10\le u\le 1. With full RSB, q(u)q(u) varies continuously; with one-step RSB, q(u)q(u) takes only two values, q0q_0 for u<xu<x and q1q_1 for u>xu>x, and the breakpoint xx is an additional variational parameter. The spherical pp-spin model replaces Ising spins by real variables σi\sigma_i obeying the global spherical constraint ∑iσi2=N\sum_i \sigma_i^2 = N and interacting through random pp-spin couplings; its classical statics were solved by Crisanti and Sommers, and Talagrand proved rigorously that the Parisi formula with the equilibrium breakpoint fixed by stationarity of the free energy in xx gives the exact classical free energy.

Quantum spin glasses in a field. Quantum fluctuations can be introduced either by a transverse field (Ising case, a term −g∑iXi-g\sum_i X_i flipping spins) or, for the spherical model, by letting the σi\sigma_i be quantum rotors with canonically conjugate momenta πi\pi_i, [σi,πj]=iδij[\sigma_i,\pi_j]=i\delta_{ij}, and a kinetic energy g2∑iπi2\frac{g}{2}\sum_i \pi_i^2; larger gg means stronger quantum fluctuations, and at large gg both models are gapped quantum paramagnets (non-glassy phases without spin-glass order). The equilibrium dynamics of both infinite-range quantum spin glasses at nonzero longitudinal field hh — an essential ingredient in optimization applications — were obtained at N=∞N=\infty by Tikhanovskaya, Sachdev, and Samajdar (2024). For the quantum Ising (SK) model they found full RSB and a gapless local spectrum, with a spectral density vanishing linearly with frequency, for all hh. For the spherical quantum pp-rotor model with p≥3p\ge 3, in contrast, the spin-glass phase has only one-step RSB, and the N→∞N\to\infty saddle-point equations for the order parameter Qab(τ1,τ2)Q_{ab}(\tau_1,\tau_2) (a bilocal function of two imaginary times, and a matrix in replica space) determine all quantities except the breakpoint xx. At the free-energy-stationary xx — and indeed at generic xx — the local rotor spectrum Im Qr(ω)\mathrm{Im}\,Q_r(\omega) (the spectral density of the site-diagonal rotor correlation function) is gapped; the marginal-stability condition selects precisely the special xx at which the gap closes and Im Qr(ω)∝ω\mathrm{Im}\,Q_r(\omega)\propto\omega at small ω\omega, an equation that coincides, at h=0h=0, with the one obtained from the real-time aging dynamics of the quantum spherical model by Cugliandolo and Lozano.

Marginal stability and why the choice matters physically. In classical mean-field glasses, relaxational dynamics does not reach equilibrium: it is trapped at marginally stable 'threshold' states whose energy density lies above the equilibrium value and whose escape barriers diverge with NN; the aging dynamics — so called because relaxation keeps slowing down as the system ages — is then described by an effective temperature that violates the fluctuation–dissipation relation (the linear-response relation between correlation and response that holds in equilibrium). Whether the same dichotomy — a gapped, stationarity-selected equilibrium glass versus marginally stable, gapless dynamically prepared states — persists once quantum fluctuations (g≠0g\ne 0) and a longitudinal field (h≠0h\ne 0) are present is unknown. The question bears directly on programmable quantum simulators: random arrays of trapped Rydberg atoms (atoms excited to states of large principal quantum number) realize disordered, long-range-interacting effective spins in which the laser detuning acts as a longitudinal field, and the presence or absence of a spectral gap in the glassy phase governs the feasibility of adiabatically preparing low-energy states.

Real-time formulation. The replica equilibrium results can be recast in the Schwinger–Keldysh real-time path-integral formalism, a closed-time-contour construction for nonequilibrium quantum dynamics. Lang, Sachdev, and Diehl (2024) showed that the replica-free Keldysh Dyson equations recover the Parisi algebra — the hierarchical (ultrametric) organization of replica overlaps — in the late-time glassy limit, with replica symmetry breaking appearing as spontaneous breaking of the thermal (Kubo–Martin–Schwinger) symmetry, the imaginary-time periodicity that characterizes equilibrium correlation functions. They derived this for the quantum Ising spin glass in transverse and longitudinal fields, with full RSB, and applied the same formalism to the spherical pp-spin model, whose glassy phase has only one-step RSB. However, in that framework the one-step breakpoint xx is still fixed only 'by an additional criterion, requiring either marginal stability or minimization of the free energy': the selection problem has been transposed into the real-time formalism, not solved.

Problem Statement

The single objective is to determine the physical selection principle for the one-step replica-symmetry-breaking breakpoint — and hence the low-frequency spectrum — of the infinite-range spherical quantum pp-rotor glass, both in thermodynamic equilibrium and in physically prepared states.

Consider the spherical quantum pp-rotor model with p≥3p\ge 3, rotor variables [σi,πj]=iδij[\sigma_i,\pi_j]=i\delta_{ij}, kinetic term g2∑iπi2\frac{g}{2}\sum_i \pi_i^2 (so that gg tunes the strength of quantum fluctuations), independent Gaussian pp-spin couplings with variance p!2J2N1−p\frac{p!}{2}J^2 N^{1-p}, the global spherical constraint ∑iσi2=N\sum_i \sigma_i^2 = N, and a longitudinal field h≠0h\ne 0:

H=∑i1<⋯<ipJi1⋯ip σi1⋯σip+g2∑iπi2−h∑iσi.H=\sum_{i_1<\cdots<i_p}J_{i_1\cdots i_p}\,\sigma_{i_1}\cdots\sigma_{i_p}+\frac{g}{2}\sum_i \pi_i^2-h\sum_i \sigma_i .

In the N→∞N\to\infty spin-glass phase, the saddle-point equations for the bilocal order parameter Qab(τ1,τ2)Q_{ab}(\tau_1,\tau_2) (the disorder-averaged correlation function of the rotors in replicas aa and bb at imaginary times τ1\tau_1 and τ2\tau_2) admit a one-step replica-symmetry-breaking solution in which every parameter is fixed except the breakpoint xx.

(a) Equilibrium selection. Determine, without assuming the answer, which prescription selects xx in the thermodynamic equilibrium state at g≠0g\ne 0, h≠0h\ne 0: free-energy stationarity ∂F/∂x=0\partial\mathcal{F}/\partial x=0, which yields a local spectrum with an energy gap, or the marginal-stability condition of glassy dynamics, which yields a gapless spectrum with Im Qr(ω)∝ω\mathrm{Im}\,Q_r(\omega)\propto\omega as ω→0\omega\to 0 (here Im Qr(ω)\mathrm{Im}\,Q_r(\omega) is the spectral density of the local rotor correlation function). A complete answer derives the selection rule within a controlled framework (replica free-energy analysis made rigorous, a Thouless–Anderson–Palmer (TAP) and complexity analysis — the mean-field treatment of the exponentially many metastable glassy states, with the complexity, i.e. the configurational entropy counting those states — or a real-time Schwinger–Keldysh formulation) and must reduce, at g=0g=0, to the established classical results: the stationary xx with a gapped equilibrium spectrum (Talagrand), and the marginal threshold states of the dynamics (Cugliandolo–Kurchan).

(b) Physical preparation. Determine which selection principle governs the states actually prepared by physical protocols at g≠0g\ne 0, h≠0h\ne 0 — quench, annealing, aging — that is, whether prepared states relax to the stationary (gapped) glass, remain at marginally stable threshold states as classical dynamics does, or reach other states accessible through quantum tunneling; and specify observable diagnostics — for example, the low-frequency behavior of the local spectral function, or fluctuation–dissipation-relation violations and aging effective temperatures — that distinguish the gapped glass from the marginally stable, gapless glass and can be measured in platforms such as Rydberg-atom arrays.

The problem is solved when both (a) and (b) are settled for the stated model — by derivation, rigorous argument, or thermodynamic-limit computation with controlled errors — with the classical g→0g\to 0 limits reproduced and with quantitative diagnostic predictions.

References

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