Universality classes of thermalization for mesoscopic Floquet systems Alan Morningstar1 2David A. Huse1and Vedika Khemani2 1Department of Physics Princeton University Princeton NJ 08544 USA

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Universality classes of thermalization for mesoscopic Floquet systems
Alan Morningstar,1, 2 David A. Huse,1and Vedika Khemani2
1Department of Physics, Princeton University, Princeton, NJ 08544, USA
2Department of Physics, Stanford University, Stanford, CA 94305, USA
(Dated: May 11, 2023)
We identify several distinct phases of thermalization that describe regimes of behavior in isolated,
periodically driven (Floquet), mesoscopic quantum chaotic systems. In doing so, we also identify
a new Floquet thermal ensemble—the “ladder ensemble”—that is qualitatively distinct from the
“featureless infinite-temperature” state that has long been assumed to be the appropriate maximum-
entropy equilibrium ensemble for driven systems. The phases we find can be coarsely classified by
(i) whether or not the system irreversibly exchanges energy of order ωwith the drive, i.e., Floquet
thermalizes, and (ii) the Floquet thermal ensemble describing the final equilibrium in systems that do
Floquet thermalize. These phases are representative of regimes of behavior in mesoscopic systems,
but they are sharply defined in a particular large-system limit where the drive frequency ωscales
up with system size Nas the N→ ∞ limit is taken: we examine frequency scalings ranging from a
weakly N-dependent ω(N)log N, to stronger scalings ranging from ω(N)Nto ω(N)N.
We show that the transition where Floquet thermalization breaks down happens at an extensive
drive frequency and, beyond that, systems that do not Floquet thermalize are distinguished based
on the presence or absence of rare resonances across Floquet zones. We produce a thermalization
phase diagram that is relevant for numerical studies of Floquet systems and experimental studies
on small-scale quantum simulators, both of which lack a clean separation of scales between Nand
ω. A striking prediction of our work is that, under the assumption of perfect isolation, certain
realistic quench protocols from simple pure initial states can show Floquet thermalization to a novel
type of Schrodinger-cat state that is a global superposition of states at distinct temperatures. Our
work extends and organizes the theory of Floquet thermalization, heating, and equilibrium into the
setting of mesoscopic quantum systems.
I. INTRODUCTION
Breakthrough experimental developments in building
isolated quantum systems have led to significant recent
progress in quantum statistical mechanics. This has fu-
eled advances in our understanding of fundamental ques-
tions surrounding the process of thermalization and its
various exceptions in isolated many-body systems [17].
In the common case of a system governed by a time-
independent Hamiltonian, the system thermalizes if, at
late times, probability distributions of local observables
are indistinguishable from those in a relevant thermal
ensemble. The appropriate thermal ensemble is deter-
mined by the principle of entropy maximization, con-
strained by the conservation laws of the system. The
Eigenstate Thermalization Hypothesis (ETH) [1,813]
posits conditions for thermalization on individual eigen-
states of the dynamics, and empirically these conditions
hold in examples of thermalizing systems [1419].
Upon the addition of a periodic drive of frequency ω,
i.e., making the system “Floquet”, the Hamiltonian and
eigenstates of the stroboscopic dynamics gain a periodic
time dependence. The drive breaks the conservation of
energy and the appropriate long-time maximum-entropy
equilibrium is assumed to be a featureless “infinite tem-
perature” state [20,21]. Exceptions to this “heat death”
are possible [22,23], notably in many-body localized
(MBL) or integrable Floquet systems [2427], in which
case the system may thermalize to a generalized peri-
odic Gibbs ensemble [28,29] and/or realize novel ordered
phases such as the discrete time-crystal [3034] or the
anomalous Floquet insulator [35,36]. Heating can also be
suppressed for a time exponential in the drive frequency,
a transient phenomenon called Floquet prethermaliza-
tion [3750]. All of these results on Floquet thermal-
ization and its exceptions were obtained in works aimed
at the limit where the drive frequency ωis finite and the
number of degrees of freedom in the system Nis infinite.
However, as we show in this paper, this limit provides
an incomplete description of thermalization in chaotic
Floquet systems. In particular, in mesoscopic systems
where Nis finite, there are other regimes of thermaliza-
tion captured by thermal ensembles that are qualitatively
distinct from a featureless infinite-temperature state.
These regimes, and the crossovers between them, occur
at drive frequencies that depend on the system size N, so
to study them we allow for a drive frequency ωΩ(N)
that is scaled up with N. We examine frequency scalings
ranging from a weakly N-dependent Ω(N) = log N, to
stronger scalings ranging from Ω(N) = Nto Ω(N) =
N. The distinctions between the different regimes we ob-
tain can be made sharp in a particular large-Nlimit [51
55], discussed later, where N→ ∞ is taken with ω/Ω(N)
held constant, i.e., a large-ωlimit is taken at the same
time.1This limit may appear non-standard when com-
pared to conventional thermodynamic limits studied in
1The width of the crossovers [in the control parameter ω/Ω(N)]
scales as Ω(N)1and sharpens up as the limit is taken.
arXiv:2210.13444v3 [cond-mat.stat-mech] 9 May 2023
2
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log(N)
FIG. 1. Distinct regimes of thermalization in mesoscopic Flo-
quet systems. (a) A sketch of the different regimes of ther-
malization, listed in Sec. I A. The various frequencies marked
along the axis depend on the system size Nas shown, and
also on (quasi)energy, so the line shown is a cut through the
full 2D phase diagram of Fig. 2. (b) and (c): A depiction
of the (b) “featureless infinite-temperature” and (c) “ladder”
ensembles. These are characterized by the probability dis-
tribution of energy defined by an effective Hamiltonian. In
the ladder ensemble, the system has a drive frequency ωthat
is large enough so that, while the system does Floquet ther-
malize, it maintains an approximate conservation of energy
modulo ω. The weights of the peaks follow the density of
states (DOS) at those energies, PEDOS(E).
many-body physics, but is standard in studies of meso-
scopic systems where interaction strengths and/or other
parameters are often taken to scale with N[51].
One motivation for studying the different possible
regimes of thermalization in mesoscopic Floquet sys-
tems is that many settings—for instance, experiments
on near-term quantum simulators—allow controlled ac-
cess to “intermediate-scale” [56] many-body quantum
systems where there is not a clean separation of scales
between Nand ω(measured in units of a microscopic
energy scale). This is also true for numerical studies of
Floquet phenomena, which are limited to small system
sizes [57]. There is currently a major gap in the literature
in theoretically and systematically addressing thermal-
ization, Floquet heating, and equilibrium in this setting,
which we hope to bridge with this present work.
A. Summary of results
We identify a number of distinct regimes of thermal-
ization, and crossovers between them, that can occur in
mesoscopic Floquet systems. In this work, we are only
considering isolated chaotic many-body systems subject
to periodic driving, focusing on the delocalization of en-
ergy across Floquet zones; in particular, all the crossovers
we consider are between chaotic regimes with different
degrees of energy conservation, so the physics of many-
body localization or integrability will play no role in our
discussion. Ref. [58] instead considers the fate of finite-
size driven integrable systems, with an N-dependent
driving amplitude. The different regimes of thermaliza-
tion we find are summarized below and in Fig. 1(a), and
explained in detail later:
At the smallest frequencies, the system irreversibly
exchanges energy with the drive and Floquet ther-
malizes to a conventional featureless infinite-
temperature state, i.e., the relevant Floquet ther-
mal ensemble is a uniform distribution over all
states [Fig. 1(b)].
At larger frequencies, beyond ω=ωladder(N)
log N(or, in some physically relevant cases dis-
cussed later, ωladder(N)N), the system instead
Floquet thermalizes to a ladder ensemble: In this
regime, energy conservation is not completely de-
stroyed, but downgraded to an approximate conser-
vation of energy modulo ω. Thus, energy becomes
delocalized across a “ladder” of narrow energy win-
dows that are spaced by ω. This is the relevant
maximum-entropy Floquet thermal ensemble un-
der the constraint of conservation of energy modulo
ω[Fig. 1(c)]. While in some cases this ensemble
can have the same average energy as the infinite
temperature ensemble, the distribution of energy is
distinct.
At yet larger frequencies beyond ω=ωpartial(N)
N, the system only partially thermalizes across the
rungs of the ladder. We call this the regime of par-
tial Floquet thermalization. In this regime, a
version of Floquet heating may still occur for many
initial states.
Finally, at the largest frequencies, beyond ω=
ωloc(N)N, the system does not exchange energy
of order ωor more with the drive, i.e., it does not
Floquet thermalize and instead becomes energy
localized. In this regime, there exists an extensive
energy, defined by a quasilocal effective Hamilto-
nian, that is approximately conserved for all times.
While the extensive many-body bandwidth fur-
nishes an upper bound for ωloc(N), we find that
energy localization sets in at a smaller scale, and
distinct non-trivial energy-localized regimes exist
3
that can be distinguished by the presence or ab-
sence of isolated Floquet many-body resonances in
rare states.
A few points are of note. First, complete Floquet ther-
malization occurs for frequencies less than ωpartial(N)
N, in the sense that the system effectively exchanges en-
ergy with the drive. In most of this regime, i.e., between
the two scales ωladder(N)log(N) and ωpartial(N)N,
the ladder ensemble is the relevant description of the
final thermal equilibrium. In contrast, the regime in
which the system thermalizes to a featureless infinite-
temperature state is parametrically smaller, extending
only up to ωladder(N)log(N). Second, while we have
only focused on the frequency dependence of the differ-
ent regimes in the discussion above [and in Fig. 1(a)],
there is also a strong dependence on (quasi)energy which
we explore below. In Fig. 2, we map out the full two-
parameter phase diagram of the different types of ther-
malization mentioned above, and one important message
of our work is that sometimes the thermalization of Flo-
quet systems needs to be state or energy-resolved instead
of uniformly averaging over all Floquet eigenstates or ini-
tial states.
Finally, a notable consequence of our results is that un-
der a suitable quench protocol, isolated systems in pure
states can thermalize to novel Schrodinger cat states of
temperature, i.e., superpositions of states at globally dif-
ferent energy densities [Fig. 1(c)]. Although the coher-
ences of such states are notoriously fragile, the ladder-like
distribution of energy is a stable signature of this novel
form of Floquet thermalization.
The rest of this paper is organized as follows: In Sec. II
we set up our theoretical understanding of the different
regimes of thermalization that occur in mesoscopic Flo-
quet many-body quantum systems. We support our the-
oretical reasoning with numerical evidence using a con-
crete model in Sec. III. In Sec. IV we explore some of the
prospects for studying the physics discussed in this work
experimentally, and show that indeed experimental stud-
ies seem to be accessible on some near-term platforms for
quantum simulation. Finally, we summarize and discuss
our findings in Sec. V.
II. THEORY
A. Setup and review of Floquet heating
For the purpose of discussion, we consider Nqubits
evolving under a time-periodic Hamiltonian H(t) = H0+
gω(t)V0, where gωis an O(1)-valued periodic function of
time that time-averages to zero, with period T=2π
ω.
H0is a quantum chaotic Hamiltonian that is a sum of
one- and two-body terms, and V0couples the system to
the drive, also consisting of a sum of one- and two-body
terms. A characteristic microscopic energy scale of His
set to one here. We are generally interested in behavior
at ω1, although in practice ω'ω0can be a more
accurate condition, where ω0is O(1) and depends on
the specific system. Both H0and V0are traceless, so
the energy corresponding to infinite temperature is zero.
1
N2Ntr(H2
0), 1
N2Ntr(V2
0), and 1
N2Ntr([H0, V0]2) are all of
order one, so the only small parameters present are 1
and 1/N . The stroboscopic dynamics are governed by the
Floquet unitary UF=Texp iRT
0H(t)dtthat time-
evolves the system by one period. The Floquet unitary
defines the Floquet Hamiltonian HFvia UFeiHFT.
The quasienergies θare defined such that the eigenvalues
of UFare eiθT , so θis only defined modulo ωand is
strictly conserved by the dynamics, and this may be the
only such strict conservation law. The specific model we
use for later numerical demonstrations is given in Sec. III,
but our results are more general.
The process of Floquet heating entails a system reso-
nantly exchanging energy with the drive in quanta of size
ω. In this work, we will ideally consider frequencies ω
that are large compared to the microscopic energy scale
of H, which is set to 1 here (the regime when ωis com-
parable to the local energy scales leads to rapid heating,
but the ωO(1) boundary between these two regimes
is system dependent). In this high-frequency regime, ab-
sorbing a quanta ωof energy requires a high-order
process involving O(ω) local energy moves, which occurs
at a rate that is exponentially suppressed in ω. Because
these processes can happen anywhere in the system, the
system as a whole exchanges “photons” with the drive at
a rate [3741]
ΓNeω0,(1)
with some microscopic (order one) ω0that may, in gen-
eral, depend on the energy density.2This is the behavior
in the drive frequency range ω0/ωNω0, and, in this
regime, there is an effective (“prethermal”) quasi-local
Hamiltonian Heff that captures the dynamics of the sys-
tem on timescales shorter than tΓ1.Heff can be
obtained perturbatively, and represents the most opti-
mal quasi-local truncation of a high-frequency Magnus
expansion for HF[39]. The leading term in the expan-
sion is the time-averaged Hamiltonian, H0(see App. A).
The time-scale Γ1sets the crossover time between
the prethermal regime with dynamics governed by Heff
(which has an extensive conserved energy), and the
regime of Floquet thermalization, where the system ther-
malizes across different Floquet zones due to a reso-
nant drive-mediated coupling between states separated
in energy by ωand therefore becomes delocalized in en-
ergy [23]. The slow thermalization across Floquet zones
2In one dimension there is a logarithmic correction such that the
heating rate is bounded by Γ Ne(ωlog ω)0[5961]. We
focus on the general case in higher dimensions for our discussion
and numerical studies below, but the results are qualitatively the
same in one dimension.
4
is reflected in the non-perturbative, non-local character of
HF. The difference between UF=eiHFTand eiHeff T
is the thermalization process across Floquet zones visible
on times t > Γ1.
B. Floquet thermal ensembles and nonstandard
large-Nlimits
We now discuss the featureless infinite temperature
and ladder ensembles for Floquet thermalization, the
crossover between these, and how this crossover sharp-
ens in a particular large-Nlimit.
For a system that absorbs/emits energy slowly enough,
an eigenstate of UFwith eigenvalue eiθT will be sup-
ported on eigenstates of Heff near a “ladder” of energies
that differ in steps of ω, i.e., with energies
Eeff =θ±(2)
with nZ. However, due to the nonzero heating rate,
each of the “rungs” of the energy ladder will have an
energy uncertainty ΓNeω/ω0(see Fig. 1(c) for a
depiction). In the commonly prioritized limit of finite ω
and N→ ∞, the rate Γ grows with Nand eventually
becomes larger than ω(when Nωeω/ω0). For Nwell
in excess of this, the ladder is not resolvable as the width
of the rungs exceeds the spacings between rungs, and the
energy conservation (even modulo ω) is fully lost. The
resulting equilibrium is then “infinite temperature” in a
strict sense, because the relevant Floquet thermal ensem-
ble is a uniform distribution over all energy eigenstates,
as shown in Fig. 1(b).
The strict infinite-temperature property of Floquet
thermalized states (and eigenstates of UF) can break
down to various degrees when Γ ω. This can occur in
systems with finite Nand ω, or in large Nsystems where
we allow ωto scale up with Nin such a way that some
behavior characteristic of finite-size systems is retained in
the limit. For example, consider ωladder(N) = ω0log N:
If ωis scaled up with Nfaster, so that ωωladder(N),
then Γ ωat large enough N. In this regime, the distri-
butions of energy in the eigenstates of UFhave significant
weight only near a well-resolved ladder of energies with
spacing ω, as shown in Fig. 1(c). In other words, the en-
ergy defined by Heff is conserved modulo ωto a precision
of Γ.
This “energy ladder” is a maximum-entropy Floquet
thermal ensemble that is distinct from “infinite tempera-
ture”, and notably it sets in already at a frequency scale
ωladder =ω0log Nthat is only weakly dependent on N.
If we consider the rescaled frequency ν=ω
ωladder(N)=
ω
ω0log N, then the crossover from the featureless infinite
temperature ensemble to the ladder ensemble happens
near ν= 1. This crossover in the rescaled variable ν
becomes sharp in the large-Nlimit as can be seen from
the behavior of Γ
ω=Neω/ω0
ω=N1ν
νω0log(N)near ν= 1: it
diverges with Nif ν < 1 and approaches zero if ν > 1.
The ladder ensemble sets in at ωlog(N) and ex-
tends to parametrically larger frequency scalings, ω=
ωpartial(N)N. First consider ωNα, with 0 < α < 1.
As long as α < 1, consecutive rungs on the ladder have
different energies but the same energy density as N→ ∞,
i.e., the spacing in energy density between the rungs
tends to zero. Each Floquet quasienergy θcorresponds to
populating a ladder of energies Eeff mod ω=θthat spans
across all energy densities. In particular, the ladder con-
tains a subset of rungs that have the same energy (and
entropy) density as infinite temperature in the N→ ∞
limit, E
eff /N =1
N2NTr[Heff ] = 0. Thus the final equilib-
rium is one where the average energy density corresponds
to infinite temperature, but the distribution of energy is
markedly distinct from the uniform distribution and in-
stead concentrated near a ladder of well-spaced energies.
Finally, we have the case of ωN(α= 1). In this
case, the frequency ωis extensive and corresponds to
transitions between different energy densities e; thus we
denote ∆eω
Nin the rest of this paper. Since ωis exten-
sive in this case, it is not generally true that the system
thermalizes to the same average energy density as infi-
nite temperature in the N→ ∞ limit, even when it does
equilibrate across Floquet zones (Floquet thermalizes).
This is because the final energy distribution resides on a
ladder of different energy densities, and the infinite tem-
perature energy density (e= 0) is not generally one of
them (see Fig. 5for a demonstration).
This brings us to an important point: Floquet ther-
malization (also referred to as Floquet heating) refers to
reaching the appropriate equilibrium ensemble with en-
ergies distributed either according to the uniform infinite
temperature ensemble or the appropriate ladder ensem-
ble. The ladder ensemble is always a distinct ensem-
ble from infinite temperature, and need not even have
the same average energy density as infinite temperature.
Thus, Floquet thermalization does not imply that the sys-
tem thermalizes to infinite temperature, even on average.
Some comments are in order before concluding this
section. When defining the ladder ensemble, we consid-
ered energies defined according to Heff , the most optimal
quasi-local truncation of HF. In this case, the energy
defined by Heff is conserved modulo ωto a precision of
Γ set by the heating rate. However, if Heff is not
chosen optimally—for instance, if energy is defined with
respect to the leading term H0—then the precision is
lower and the width of the rungs is accordingly broader,
as discussed in App. A. Likewise, if we consider thermal-
ization of generic initial states (instead of eigenstates of
UF), then the energy uncertainty of the initial state also
contributes to the broadening of the rungs. A typical
product initial state has energy uncertainty N, and
hence requires ωNαwith α > 1
2to resolve the rungs of
the ladder for large enough N. In this case, the crossover
from the featureless infinite temperature ensemble to the
ladder ensemble happens at ωladder(N)Nand it does
not sharpen up in the large-Nlimit.
In sum, in this section we’ve discussed different Flo-
摘要:

UniversalityclassesofthermalizationformesoscopicFloquetsystemsAlanMorningstar,1,2DavidA.Huse,1andVedikaKhemani21DepartmentofPhysics,PrincetonUniversity,Princeton,NJ08544,USA2DepartmentofPhysics,StanfordUniversity,Stanford,CA94305,USA(Dated:May11,2023)Weidentifyseveraldistinctphasesofthermalizationth...

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Universality classes of thermalization for mesoscopic Floquet systems Alan Morningstar1 2David A. Huse1and Vedika Khemani2 1Department of Physics Princeton University Princeton NJ 08544 USA.pdf

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