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In system’s the [10]. distribu- of ronment on usual form depending very than equilibrium, the universal thermal less characterizing be tions should they that h infiac fteeFoutsae 2 et nthe in rests (2) states Floquet these of significance The nasotpormai oeette Proi Ther- “Periodic entitled note programmatic short a In a led acltdteedsrbtosfrtime- for distributions these calculated already had oaiiisfrabtaiysrn driving. strong arbitrarily for robabilities 2 harmonic n atnHolthaus Martin and , prtr hc sdffrn rmthe from different is which mperature T eulbimsed tt fadriven a of state steady nequilibrium daayial eemn h quasi- the determine analytically nd aaim o h mrigfil of field emerging the for paradigms eim oehls,teresponse the Nonetheless, netism. | proi anr vr solution every manner, -periodic ubr edsoe remarkable a discover We number. ψ 11Odnug Germany Oldenburg, 6111 { gdiig hs eagethat argue we Thus, driving. ng | vrluepce etrs even features, unexpected everal ( c p lfl,Grayand Germany elefeld, t n ) n | i } 2 siltrteeatoshv hw that shown have authors these oscillator = abr¨uck, Germany ept h rsneo time-periodic a of presence the despite , fFoutsaeocpto probabil- occupation Floquet-state of ν X samte fconvention. of matter a is 0 = n c n c n rzto o arbitrary for arization c ontdpn ntm.Hence, time. on depend not do n | u n ol edtrie solely determined be would aig circularly lating, ( t 3 ) i exp( − { p i ε n n } t emphasizing , ) | , ψ ( t ) i othe to (6) et 2 anharmonic oscillators. These investigations have been ideal paramagnet to a circularly polarized driving field. extended later by Ketzmerick and Wustmann, who have In Sec. VI we consider the rate of energy dissipated by demonstrated that structures found in the phase space of the driven spins into the bath, thus generalizing results 1 classical forced anharmonic oscillators leave their distinct derived previously for s = 2 in Ref. [29]. In Sec. VII we traces in the quasistationary Floquet-state distributions summarize and discuss our main findings, emphasizing of their quantum counterparts [12]. To date, a great va- the possible knowledge gain to be derived from future riety of different individual aspects of the “periodic ther- measurements of paramagnetic response to strong time- modynamics” envisioned by Kohn has been discussed in periodic forcing, carried out along the lines drawn in the the literature [13–23], but a coherent overall picture is present work. still lacking. In this situation it seems advisable to resort to mod- els which are sufficiently simple to admit analytical so- II. TECHNICAL TOOLS lutions and thus to unravel salient features on the one hand, and which actually open up meaningful perspec- A. Golden-rule approach to open driven systems tives for new laboratory experiments on the other. To this end, in the present work we consider a spin s ex- Let us consider a quantum system evolving according posed to both a static magnetic field and an oscillating, to a T -periodic Hamiltonian H(t) on a Hilbert space S circularly polarized magnetic field applied perpendicu- which is perturbed by a time-independent operatorHV . lar to the static one, as in the classic Rabi set-up [24], Then the transition matrix element connecting an initial and coupled to a thermal bath of harmonic oscillators. Floquet function ui(t) to a final Floquet function uf (t) The experimental measurement of the thermal paramag- can be expanded| into ai Fourier series, | i netism resulting from magnetic moments subjected to a static field alone has a long and successful history [25, 26], (ℓ) uf (t) V ui(t) = Vfi exp(iℓωt) , (7) having become a standard topic in textbooks on Statis- h | | i ℓ∈Z tical Physics [27, 28]. We argue that a future generation X of such experiments, including both a static and a strong and consequently the “golden rule” for the rate of tran- oscillating field, may set further cornerstones towards the sitions Γfi from a Floquet state labeled i to a Floquet development of full-fledged periodic thermodynamics. state f is written as [29] We proceed as follows: In Sec. II we collect the nec- Γ =2π V (ℓ) 2 δ(ω(ℓ)) , (8) essary technical tools, starting with a brief summary of fi | fi | fi
∈Z the golden-rule approach to time-periodically driven open Xℓ quantum systems in the form developed by Breuer et al. [11], thereby establishing our notation. We also sketch where a technique which enables one to “lift” a solution to the (ℓ) 1 ωfi = εf εi + ℓω . (9) Schr¨odinger equation for a spin s = 2 in a time-varying − magnetic field to general s. In Sec. III we discuss the Thus, a transition among Floquet states is not associated Floquet states for spins in a circularly polarized driving with only one single frequency, but rather with a set of field, obtaining the states for general s from those for frequencies spaced by integer multiples of the driving fre- s = 1 with the help of the lifting procedure. In Sec. IV 2 quency ω, reflecting the ladder-like nature of the system’s we compute the quasistationary Floquet-state distribu- quasienergies (5); this is one of the sources of the pecu- tion for driven spins under the assumption that the spec- liarities which distinguish periodic thermodynamics from tral density of the heat bath be constant, and show that usual equilibrium thermodynamics [10, 11]. this distribution is Boltzmannian with a quasitempera- Let us now assume that, instead of merely being per- ture which is different from the actual bath temperature; turbed by V , the periodically driven system is coupled the dependence of this quasitemperature on the system to a heat bath, described by a Hamiltonian H acting parameters is discussed in some detail. In Sec. V we bath on a Hilbert space B, so that the total Hamiltonian on determine the magnetization of a spin system which is the composite HilbertH space takes the form subjected to both a static and an orthogonally applied, HS ⊗ HB
circularly polarized magnetic field while being coupled ½ Htotal(t)= H(t) ½ + Hbath + Hint . (10) to a heat bath. To this end, we first establish a general ⊗ ⊗ formula for the ensuing magnetization by means of an- Stipulating further that the interaction Hamiltonian Hint other systematic use of the lifting technique, and then factorizes according to show that the resulting expression can be interpreted as a derivative of a partition function based on both the Hint = V W, (11) quasitemperature and the system’s quasienergies, in per- ⊗ fect formal analogy to the textbook treatment of para- the golden rule can be applied to joint transitions from magnetism in the absence of time-periodic driving; these Floquet states i to Floquet states f of the system ac- insights are exploited for elucidating the response of an companied by transitions from bath eigenstates n with 3
1 energy En to other bath eigenstates m with energy Em, B. The lift from s = 2 to general s acquiring the form We will make heavy use of a procedure which allows Γmn =2π V (ℓ) 2 W 2 δ(E E + ω(ℓ)) . (12) fi | fi | | mn| m − n fi one to transfer a solution to the Schr¨odinger equation
ℓ∈Z 1 X for a spin with spin quantum number s = 2 in a time- Moreover, following Breuer et al. [11], let us consider a dependent external field to a solution of the correspond- bath consisting of thermally occupied harmonic oscilla- ing Schr¨odinger equation for general s, see also Ref. [30]. tors, and an interaction of the prototypical form This procedure does not appear to be widely known, but has been applied already in 1987 to the coherent evolu- † tion of a laser-driven N-level system possessing an SU(2) W = bωe + bωe , (13) e dynamic symmetry [31], and more recently to the spin-s ω X Landau-Zener problem [32]. Here we briefly sketch this † where bωe (bωe) is the annihilation (creation) operator per- method. taining to a bath oscillator of frequency ω. We now have Let t Ψ(t) SU(2) be a smooth curve such that 7→ ∈ to distinguish two cases: If En Em = ω > 0, so that Ψ(0) = ½, as given by a 2 2-matrix of the form − × the bath is de-excited and transfers energye to the system, the required annihilation-operator matrix element reads z1(t) z2(t) e Ψ(t)= ∗ ∗ (21) z2 (t) z1 (t) Wmn = n(ω) , (14) − 2 p with complex functions z1(t), z2(t) obeying z1(t) + where n(ω) is the occupation number of a bath oscilla- 2 | | tor with frequency ω, and the squaree W 2 entering z2(t) = 1 for all times t. One then has | mn| | | the goldene rule (12) has to be replaced by the thermal d avarage Ψ(t) Ψ(t)−1 iH(t) su(2) , (22) e dt ≡− ∈ 1 N(ω) n(ω) = , (15) ≡ h i exp(βω) 1 where su(2) denotes the Lie algebra of SU(2), i.e., the − space of anti-Hermitean, traceless 2 2-matrices which with β denotinge the inversee bath temperature. Con- is closed under commutation [33]. Hence× the columns versely, if E E = ω < 0 so thate the system loses n − m ψ1(t) , ψ2(t) of Ψ(t) are linearly independent solutions energy to the bath and a bath phonon is created, one of| thei Schr¨odinger| i equation has e d W = n( ω)+1 , (16) i ψj (t) = H(t) ψj (t) , j =1, 2 . (23) mn − dt| i | i giving p e Next we consider the well-known irreducible Lie algebra 1 representation of su(2), N(ω) n( ω) +1= . (17) ≡ h − i 1 exp(βω) − r(s) : su(2) su(2s + 1) , (24) −→ Finally, let Je(ω) be thee spectral density of the bath. Then e the total rate Γfi of bath-induced transitions among the which is parametrized by a spin quantum number s such
Floquet states i and f of the driven system is expressed that 2s Æ, together with the corresponding irreducible e ∈ as a sum of partial rates, group representation (“irrep” for brevity)
Γ = Γ(ℓ) , (18) R(s) : SU(2) SU(2s + 1) . (25) fi fi −→
ℓ∈Z X It follows that where r(s)(is ) = iS , j = x, y, z , (26) Γ(ℓ) =2π V (ℓ) 2 N(ω(ℓ)) J( ω(ℓ) ) . (19) j j fi | fi | fi | fi | where s = 1 σ denote the three s = 1 spin operators These total rates (18) now determine the desired quasi- j 2 j 2 given by the Pauli matrices σ , and the S denote the stationary distribution p as a solution to the equa- j j n corresponding spin operators for general s. Recall the tion [11] { } standard matrices
Γnmpm Γmnpn =0 . (20) − (Sz) = nδmn , (27) m m,n X 1 s(s + 1) n(n 1) : m = n 1 , It deserves to be emphasized again that the very details (S ) = 2 x m,n − ± 0 : else , ± of the system-bath coupling enter here, so that the pre- p cise form of the respective distribution p may depend 1 s(s + 1) n(n 1) : m = n 1 , n (S ) = 2i strongly on such details [10]. { } y m,n ± − ± 0 : else , ± p 4 where m,n = s,s 1,..., s, and The Floquet states (2) brought about by this Hamilto- − − nian (34) are given by [34] S± Sx iSy . (28) ≡ ± e∓iΩt/2 √Ω δ e−iωt/2 It follows from the general theory of representations [33] ψ±(t) = ± ± +iωt/2 , (36) | i √2Ω √Ω δ e that r(s) and R(s) may be applied to Eq. (22) and yield ∓ where d −1 R(s) Ψ(t) R(s) Ψ(t) = r(s) iH(t) . (29) dt − δ = ω0 ω (37) − Since H(t) can always be written in the form of a Zeeman denotes the detuning of the transition frequency ω0 from term with a time-dependent magnetic field b(t), namely, the driving frequency ω, and Ω is the Rabi frequency, 2 2 3 Ω= δ + F . (38) H(t)= b(t) s = b (t) s , (30) · j j The 2 2-matrix Ψ(t) constructedp from these states does j=1 × X not satisfy Ψ(0) = ½. This is of no concern, since Ψ(t) −1 Eq. (26) implies that could be replaced by Ψ(t) Ψ(0) . The distinct advan- tage of these Floquet solutions (36) lies in the fact that 3 they yield a particularly convenient starting point for the r(s) iH(t) = i b(t) S = i b (t) S . (31) · j j lifting procedure outlined in Sec. II B: One has j=1 X 1 √Ω+ δ √Ω δ In (30) we have chosen the + sign convention adapted to Ψ(t) = iωt iωt− − √2Ω e √Ω δ e √Ω+ δ electrons for which the magnetic moment is opposite to − −i(ω+Ω)t/2 their spin s. Hence, the “lifted” matrix e 0 × 0 e−i(ω−Ω)t/2 Ψ(s)(t) R(s) Ψ(t) (32) ≡ −iωt/2 P (t)e exp( iΩtsz) . (39) will be a matrix solution of the lifted Schr¨odinger equa- ≡ − tion This decomposition possesses the general Floquet form d i Ψ(s)(t)= b(t) S Ψ(s)(t) . (33) Ψ(t)= P (t) exp( iGt) , (40) dt · − where the unitary matrix P (t) = P (t + T ) again is Note that the matrix Ψ(s)(t) is unitary, and hence its T -periodic, and the eigenvalues of the “Floquet ma- columns span the general (2s + 1)-dimensional solution trix” G, to be obtained from the matrix logarithm space of the lifted Schr¨odinger equation (33). −1 of Ψ(T ) Ψ(0) = exp( iGT ), provide the system’s quasienergies [35–38]. Since−G already is diagonal in this 1 III. FLOQUET FORMULATION OF THE RABI representation (39), the quasienergies of a spin 2 driven PROBLEM by a circularly polarized field according to the Hamilto- nian (34) can be read off immediately: A. Floquet decomposition for s = 1/2 ω Ω ε± = ± mod ω , (41) 1 2 A spin 2 subjected to both a constant magnetic field applied in the z-direction and an orthogonal, circularly satisfying ε+ + ε− = 0 mod ω. For later application we polarized time-periodic field, as constituting the classic express the periodic part P (t) of the decomposition (39) Rabi problem [24], is described by the Hamiltonian in the following way: −iωt/2 ω F iωt/2 e 0 0 P (t) = e +i 2 H(t)= σz + (σx cos ωt + σy sin ωt) . (34) 0 e ωt/ 2 2 1 √Ω+ δ √Ω δ Here ω0 denotes the transition frequency pertaining to − − ×√2Ω √Ω δ √Ω+ δ the spin states in the static field alone, while F denotes − the frequency associated with the amplitude of the peri- eiωt/2 exp( iωts ) Ξ . (42) odic drive. This is a special form of the Zeeman Hamil- ≡ − z tonian (30) with the particular choices The time-independent matrix Ξ = Ψ(0) introduced here bx(t) = F cos ωt can be written as by(t) = F sin ωt cos(λ/2) sin(λ/2) Ξ = exp( iλsy)= − (43) bz(t) = ω0 . (35) − sin(λ/2) cos(λ/2) 5
(s) 2s+1 C with where ½ denotes the unit matrix in . Therefore, the quasienergies now read δ +Ω λ/2 = arccos . (44) ω 2Ω εm = + m Ω mod ω (52) r ! 2 Hence, one has the identities for half-integer m = s,...,s. − Denoting the eigenstates of Sz by m , in both cases (i) 2 2 | i † δ √Ω δ and (ii) the Floquet states can now be written as Ξ sxΞ = sx + − sz Ω Ω (s) (s) Ψ (t) m = P (t) m exp( iεmt) † | i | i − Ξ syΞ = sy , u (t) exp( iε t) , (53) ≡ | m i − m 2 2 † δ √Ω δ thereby introducing the T -periodic Floquet functions Ξ szΞ = sz − sx , (45) Ω − Ω (s) um(t) = P (t) m . (54) which may be easily verified. | i | i Since Ω ω0 ω when F 0, the quasienergies (50) and (52)→ properly | − connect| to the→ respective eigenvalues of B. Floquet decomposition for general s ω0Sz for vanishing driving amplitude. There is, however, an important further distinction to be observed at this 1 σj point: In either case (i) and (ii) one finds Replacing the spin- 2 operators sj = 2 in the Hamil- tonian (34) by their conterparts Sj for general spin quan- εm mω0 mod ω if ω<ω0 , (55) tum number s, one obtains → whereas H(s)(t) = b(t) S · εm mω0 mod ω if ω>ω0 . (56) = ω0 Sz + F (Sx cos ωt + Sy sin ωt) . (46) →− That is, if the driving frequency ω is detuned to the blue According to Sec. II B the general matrix solution to the side of the transition frequency ω0, the labeling of the corresponding Schr¨odinger equation (33) now is obtained quasienergy representatives (50) and (52) differs from as the lift (32) of the 2 2-matrix (39). Invoking Eqs. (42) that of the eigenvalues of S by a minus sign, effectively × z and (43), and applying the irrep R(s) to this decomposi- reversing their order. This feature needs to be kept in tion yields mind for correctly assessing the following results. We also note that in the adiabatic limit, when the spin Ψ(s)(t) = R(s) exp( iωts )exp( iλs ) exp( iΩts ) − z − y − z is exposed to an arbitrarily slowly varying magnetic field enabling adiabatic following to the instantaneous energy = exp( iωtSz)exp( iλSy) exp( iΩtSz) . (47) eigenstates, the quasienergies should be given by the one- − − − cyle averages of the instantaneous energy eigenvalues. In- In order to bring this factorization into the standard Flo- deed, in this limit the Rabi frequency (38) reduces to 2 2 quet form analogous to Eq. (40), Ω = ω0 + F , while the time-independent instanta- neous energy levels are Em = m Ω, yielding the expected (s) (s) (s) Ψ (t)= P (t)exp iG t (48) identity.p − with a T -periodic matrix P (s)(t)= P (s)(t + T ), we have to distinguish two cases: IV. THE QUASISTATIONARY DISTRIBUTION (i) For integer s we may set
(s) Now we stipulate that the periodically driven spin be P (t) = exp( iωtSz) exp( iλSy) , − − coupled to a thermal bath of harmonic oscillators, as (s) G = Ω Sz , (49) sketched in Sec. II A, taking the coupling operator to be obtaining the quasienergies of the natural form [39] V = γSx . (57) εm = m Ω mod ω (50) In order to calculate the Fourier decompositions (7) of with integer m = s,...,s. − (s) the Floquet matrix elements of V , and referring to the (ii) For half-integer s the requirement that P (t) above representation (54) of the Floquet functions, we be T -periodic demands insertion of additional factors thus need to consider the operator e±iωt/2, in analogy to the representation (42) for s = 1 . 2 (s)† (s) This gives P (t) Sx P (t)
(s) iωt/2 = exp (iλSy) exp (iωtSz) Sx exp( iωtSz)exp( iλSy) P (t) = e exp( iωtSz) exp( iλSy) , − − − − (ℓ) (s) ω (s) V exp(iℓωt) ; (58) G = ½ +Ω Sz , (51) ≡
∈Z 2 Xℓ 6 note that the additional phase factor eiωt/2 contained in for all n = s + 1, ... , s 1, since the term with m = n the expression (51) for P (s)(t) with half-integer s cancels in Eq. (20)− cancels. In the− border cases n = s or n = s here. Using the su(2) commutation relations and their this identity still holds, but only one bracket− survives. counterparts for general s, we deduce Upon setting the first bracket in this Eq. (64) to zero, one obtains exp (iωtSz) Sx exp( iωtSz) − pn Γn,n−1 1 iωt −iωt = (65) = e S +e S− . (59) 2 + pn−1 Γn−1,n Hence, as in the case s = 1 studied in Ref. [29], the only for n = s+1, ... , s 1. Together with the normalization 2 − − non-vanishing Fourier components V (ℓ) occur for ℓ = 1: requirement, this relation already determines the entire ± distribution pm . In particular, it entails (±1) γ { } V = exp (iλSy) S± exp( iλSy) . (60) 2 − pn+1 Γn+1,n = , (66) Applying R(s) to Eqs. (45), this yields pn Γn,n+1
2 2 thus ensuring that also the second bracket in Eq. (64) (±1) γ δ √Ω δ V = Sx + − Sz i Sy . (61) vanishes, confirming detailed balance. 2 Ω Ω ± ! A further factor of substantial importance is the spec-
(±1) tral density J(ω), which may allow one to manipulate the Thus, V is a tridiagonal matrix. For computing the quasistationary distribution to a considerable extent. For partial transition rates (19) we therefore have to con- the sake of simplicity and transparent discussion, here we (±1) e sider only frequencies ωmn of pseudotransitions [29], for assume that J(ω) J0 is constant. The distinction be- which m = n, and of transitions between neighboring tween the physically≡ different positive and negative tran- Floquet states, m = n 1. In view of the definition (9), sition frequencies, which lead to the two different expres- ± e and taking the quasienergies given by Eqs. (50) and (52) sions (15) and (17) entering the transition rates (19), now without “mod ω” as the canonical representatives of their prompts us to treat the cases 0 <ω< Ω and 0 < Ω <ω respective quasienergy classes (5), one has separately, while the resonant case ω = Ω can be dealt with by means of limit procedures. ω : m = n , (±1) ± ωmn = Ω ω : m = n +1 , (62) Ω ± ω : m = n 1 . − ± − A. Low-frequency case 0 <ω< Ω According to the Pauli master equation (20), the quasi- stationary distribution pm m=s,...,−s which establishes In order to utilize the above Eq. (66) for determining itself under the combined{ influence} of time-periodic driv- the distribution pm recursively we only need to eval- { } (±1) (±1) ing and the thermal oscillator bath is the eigenvector of uate the partial rates Γm,m+1 and Γm+1,m according to a tridiagonal matrix Γ corresponding to the eigenvalue 0, the general prescription (19). In the low-frequency case where Γ is obtained from Γ Γ(1) +Γ(−1) by subtracting 0 <ω< Ω this leads to the expressions ≡ from the diagonal elementse the respective column sums, 2 ± s(s + 1) m(m + 1) Ω δ i.e., e Γ( 1) = − ∓ m,m+1 16 1 e−β(Ω∓ω) Ω s − 2 Γmn =Γmn δmn Γkn . (63) s(s + 1) m(m + 1) Ω δ − (±1) − Γm+1,m = − ± (67) kX= s 16 eβ(Ω±ω) 1 Ω e − Since Γ is tridiagonal with non-vanishing secondary di- which have been scaled by Γ = 2πγ 2J , and have thus agonal elements, this eigenvector is unique up to nor- 0 0 been made dimensionless. Evidently, these representa- malization.e Moreover, it is evident that we only need tions imply that the desired ratio the matrix elements of Γ in the secondary diagonals for calculating the quasistationary distribution, whereas the Γm+1,m qL (68) diagonal elements will be required for computing the dis- Γm,m+1 ≡ sipation rate [29]. The very fact that V (±1), and hence Γ, merely is a is independent of both s and m; a tedious but straight- tridiagonal matrix has a conceptually important conse- forward calculation readily yields quence: It enforces detailed balance, meaning that each 2δΩ sinh(βω)+ δ2 +Ω2 e−βΩ cosh(βω) term of the sum (20) vanishes individually. With Γ being − qL = 2 2 βΩ . tridiagonal, this sum reduces to 2δΩ sinh(βω) (δ +Ω) (e cosh(βω)) − − (69) (Γ − p − Γ − p ) n,n 1 n 1 − n 1,n n Therefore, not only does one find detailed balance here, + (Γ p Γ p )=0 (64) but the occupation probabilities even generate a finite n,n+1 n+1 − n+1,n n 7 geometric sequence: By construction, the geometric se- Boltzmann distribution with the inverse bath temper- quence ature β, thereby indicating thermal equilibrium of the spin system; the unfamiliar “plus”-sign appearing in this 2s 2s−1 qL (q , q ,...,qL, 1) (70) limit (76) in the case of blue detuning merely reflects the ≡ L L reversed labeling (56). is an eigenvector of the matrix Γ introduced in Eq. (63) More importantly, in both cases 0 < ω < Ω and with eigenvalue 0, and hence yields the desired quasista- 0 < Ω <ω the occupation probabilities p of the Flo- { m} tionary Floquet-state occupatione probabilites pm after quet states constitute a geometric sequence even under normalization. { } arbitrarily strong driving, when the system is far remote from usual thermal equilibrium. Since the quasiener- gies (50) and (52) are equidistant, the quasistationary B. High-frequency case 0 < Ω <ω distribution can therefore still be regarded as a Boltz- mann distribution, but now being parametrized by an Analogously, in the high-frequency case 0 < Ω <ω we effective quasitemperature: require the dimensionless partial rates 1 1 1 p = qs+m = e−ϑεm = e−ϑΩm (77) 2 m ± s(s + 1) m(m + 1) Ω δ Z1 Z2 Zq Γ( 1) = − ∓ m,m+1 ± 16 eβ(±ω−Ω) 1 Ω − with m = s, . . . , s for both integer and half-integer s, 2 − s(s + 1) m(m + 1) Ω δ where the factors Z1, Z2, and Zq are adjusted to ensure (±1) s Γm+1,m = − ± (71) the normalization p = 1, and ± 16 eβ(Ω±ω) 1 Ω m=−s m − P ln q for constructing the matrix Γ = Γ(1) +Γ (−1). Once more, ϑ (78) the ratio ≡− Ω is the inverse quasitemperature of the periodically driven Γm+1,m qH (72) spin system coupled to an oscillator bath with inverse Γm,m+1 ≡ regular temperature β. When defining the quasitemper- does depend neither on s nor on m, so that the occupa- ature in this analytically convenient manner (78) we do tion probabilities again form a geometric sequence; after not distinguish between the cases (76) of red and blue some juggling, one finds detuning, so that our quasitemperature will be negative under weak driving with blue detuning. In accordance δ2 +Ω2 sinh(βω)+2δΩ e−βΩ cosh(βω) with the distinction (75) we will also designate the inverse qH = − . quasitemperature as ϑ and ϑ , respectively. Note that (δ2 +Ω2) sinh(βω) 2δΩ (eβΩ cosh(βω)) L H the parametrization of the geometric distribution (77) − − (73) in terms of the system’s quasienergies and a quasitem- This quantity determines the solution vector perature, in formal analogy to the canonical distribu- 2s 2s−1 tion of equilibrium thermodynamics [28], requires that qH (q , q ,...,qH , 1) (74) ≡ H H the “modulo ω-indeterminacy” of the quasienergies has been resolved in some way, so that the quasienergies en- to the equation Γ q = 0 in the high-frequency regime, H tering this distribution refer to particular, well defined providing the corresponding quasistationary Floquet dis- representatives of their classes (5); here we have selected tribution upon normalization. e the representatives given by Eqs. (50) and (52) without “mod ω”. This implies that the definition of the quasi- C. The quasitemperature temperature still contains a certain degree of arbitrari- ness. Notwithstanding this remark, the very distribution pm itself, governing the observable physics, is defined For ease of notation, let us define uniquely.{ } The dimensionless inverse quasitemperature ω0ϑ ulti- qL : 0 <ω< Ω q (75) mately depends on the scaled driving amplitude F/ω0, ≡ qH : 0 < Ω < ω . the scaled driving frequency ω/ω0, and the dimension- less inverse actual temperature ω β of the heat bath, but Recalling Ω ω ω in the limit F 0 of vanishing 0 0 not on the spin quantum number s. In contrast, the par- driving amplitude,→ | − one| then finds → tition function Zq depends on s: −βω0 e : ω<ω0 q +βω0 (76) 2s +1 → e : ω>ω0 . s sinh ϑΩ 2 Zq = exp( ϑΩm)= . (79) Hence, in the absence of the time-periodic driving field − ϑΩ m=−s sinh the above solutions (70) and (74) correctly lead to a X 2 8
where the latter equation defines the boundary ω = Ωbe- tween the low- and the high-frequency regime, see Fig. 1. At this boundary there is a continuous change from ϑL to ϑH , since
lim ϑL = lim ϑH =0 . (81) ω↑ωc ω↓ωc
However, the two functions ϑL and ϑH do not join smoothly at ω = ωc, since their derivatives with respect to ω adopt limits with opposite signs:
3 4 4 ∂ϑL 4βω0 F + ω0 lim = 2 , FIG. 1: Dimensionless inverse quasitemperature ω0ϑ of the ω↑ωc ∂ω − 4 2 2 F (F + ω0) spin system under the influence of a circularly polarized 3 4 4 monochromatic driving force with amplitude F and fre- ∂ϑH 4βω0 F + ω0 lim = 2 . (82) quency ω, being coupled to a harmonic-oscillator bath of in- ω↓ωc ∂ω 4 2 2 F (F + ω0) verse actual temperature ω0β = 1. The blue part of the graph corresponds to the high-frequency regime 0 < Ω <ω, the red part to the low-frequency regime 0 <ω< Ω. Along the line We will now investigate the behavior of the function segment ω = ω0 with F <ω0 and along the parabola ω = ωc given by Eq. (80), both marked by blue dashes, the inverse ω0ϑ(ω0β,ω/ω0,F/ω0) in the limits corresponding to the quasitemperature vanishes. A few functions ϑ(ω) for con- four sideways faces of the box bounding the plot dis- stant F are highlighted, showing a kink at ω = ωc according played in Fig. 1: to Eqs. (82). The limit ω0ϑ = ω0β for ω/ω0 → 0 is indicated (i) As already noted at the end of Sec. IIIB, in the low- by the green line. frequency limit ω/ω0 0 the canonical representatives of the quasienergies (50)→ and (52) approach the actual 2 2 energies Em = m ω0 + F (with m = s, . . . , s) of a The inverse quasitemperature ϑ vanishes — meaning that spin exposed to a slowly varying drive. Hence,− in this the periodically driven system effectively becomes in- limit the “periodicp thermodynamics” investigated here finitely hot, so that all its Floquet states are populated must reduce to the usual thermodynamics described by equally — regardless of the bath temperature, if either a canonical ensemble; in particular, the inverse quasi- ω = ω0 while 0