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Preview Thermodynamic formalism and linear response theory for non-equilibrium steady states

Thermodynamic formalism and linear response theory for non-equilibrium steady states Thomas Speck Institut fu¨r Physik, Johannes Gutenberg-Universita¨t Mainz, Staudingerweg 7-9, 55128 Mainz, Germany We study the linear response in systems driven away from thermal equilibrium into a non- equilibrium steady state with non-vanishing entropy production rate. A simple derivation of a general response formula is presented under the condition that the generating function describes a transformationthat(tolowestorder)preservesnormalizationandthusdescribesaphysicalstochas- ticprocess. ForMarkovprocessesweexplicitlyconstructtheconjugatequantitiesanddiscusstheir relationwithknownresponseformulas. Emphasisisputontheformalanalogywiththermodynamic potentials and some consequences are discussed. 6 I. INTRODUCTION ganizedasfollows: First,webrieflyoutlinethecanonical 1 structure of intensive affinities and extensive generalized 0 distances for NESS. We then derive a general response One of the objectives of computational sciences is the 2 formula and show that it contains previously derived re- accurate prediction of material properties. The determi- g sults, in particular the response formula by Warren and nation of transport coefficients (e.g., conductivities and u Allen [11] and the path weight representation [6, 14, 18]. mobilities) remains a challenge since, in general, it im- A Before concluding we discuss our results in the light of a plies currents and thus non-equilibrium conditions. Il- possible thermodynamic formalism for NESS. 4 lustrative as well as technologically important examples includetheefficienttransportofchargesinorganicsemi- ] conductors [1, 2] and across thin membranes in reverse h c osmosis [3]. While many sophisticated numerical meth- II. THERMODYNAMIC FORMALISM e ods have been developed based on thermal equilibrium, m for driven systems one typically has to resort to brute- A. Conjugate variables force computer experiments. - at Sufficiently close to equilibrium transport coefficients The mathematical structure of equilibrium statistical t can be determined from equilibrium fluctuations via the s mechanics is based on pairs of an extensive quantity . fluctuation-dissipationtheorem[4]. Therehavebeencon- t (volume, particle number) and the conjugate intensive a siderableeffortstofindgeneralprinciplesalsoforthelin- quantity(pressure,chemicalpotential),whicharerelated m ear response of non-equilibrium states [5–11] (for more throughthermodynamicpotentials(freeenergies). What - complete reviews we refer to Refs. 12–14 and references makes the formalism so powerful is that these potentials d therein), which find application in “field-free” numeri- n are also generating functions encoding the full statistics cal algorithms [15–17]. There is now a “zoo” of dif- o of the non-conserved extensive quantities. As a corol- ferent approaches and derivations yielding (sometimes c lary, fluctuations encode the response of thermodynamic [ unrecognized) equivalent results. One reason might be that actually several conjugate observables (and their observables to a small external perturbation. 2 linear combinations) are equivalent in determining the v response [18]. 0 4 Extendingthenotionofstatisticalensemblestotrajec- (a) (b) 5 tories(time-orderedsequencesofdynamicevents)iscur- 3 rentlyreceivingconsiderableattention[19–21]. Acanoni- 0 calstructureforthejointprobabilityofmicroscopicprob- . 1 abilitiesandtheircurrentsasbeenformulatedinRef.22. φ 0 Incontrast,hereweareconcernedwithmacroscopiccur- f 6 rents without information about microscopic probabili- enzyme 1 ties (or densities). Another concept is that of “canoni- : v cal” path ensembles (also appearing under the names s- FIG. 1: Examples for affinities and distances. (a) Colloidal i ensemble [23, 24], tilted ensemble, or Esscher transform) X particleinaringtrapwithradiusR. Theparticleisdrivenby in which trajectories are biased by a time-integrated ob- a constant force f (the affinity) while X = Rφ is the total r τ a servable. Under certain conditions typical trajectories distance travelled during time τ. (b) Sketch of an enzyme in the canonical path ensemble are equivalent to trajec- drivingthereaction◦→(cid:46). Thegeneralized“distance”X = τ tories in the original processes with fixed value of the N(cid:46) = −N◦ now corresponds to the number of (cid:46) molecules τ τ observable [25–28]. The purpose of this paper is to fol- producedduringtimeτ. Theaffinityf =−(µ(cid:46)−µ◦)isgiven low these ideas and apply them to the linear response by the difference of chemical potential, which we assume to around a non-equilibrium steady state (NESS). It is or- be fixed by chemiostats. 2 Pairs of apparently conjugate quantities (fi,Xi) also with symmetric Onsager coefficients Lij = Lji following arise for non-equilibrium steady states (NESS), where from the Green-Kubo relations non-zero intensive affinities fi (the generalized forces) ∂ 1 give rise to transport and thus extensive (generalized) (cid:104)XiXj(cid:105)(cid:16)Lij. (5) distances Xi ∼ τ (measured over time τ), see Fig. 1 ∂τ 2 τ τ τ for two examples. Their product determines the entropy production Σ = (cid:80) fiXi. Truly conjugate quantities, τ i τ C. Canonical path ensembles however,wouldrequiretheexistenceofanon-equilibrium “potential” Φ(f;τ) so that (cid:104)Xi(cid:105)= ∂Φ, which more gen- τ ∂fi Away from the linear response regime for NESS char- erally would determine state functions and justify vari- acterized by the affinities f we can still define the gener- ation principles [29, 30]. Since this also implies strict ating function convexity, it would preclude established phenomena like a negative differential mobility [31]. (cid:90) Zf(s;τ)≡ dX esXPf(X;τ)(cid:16)eτφ∗f(s), (6) B. Linear response regime wheresatthispointisjusttheargumentofthisfunction. Moments and cumulants are obtained through differen- A thermodynamic description does, however, apply to tiation with respect to s around s = 0. The function the linear response regime. To this end, consider a gen- φ∗f(s) is the large deviation function, which by construc- eralized distance X ∼ τ measured in thermal equilib- tionisaconvexfunction. Itisrelatedtotheratefunction τ rium(i.e., f =0)withprobabilitydistributionP0(X;τ). Pf(X;τ) (cid:16) e−τφf(x) for the current x ≡ Xτ/τ through Clearly, the average (cid:104)X (cid:105)=0 vanishes. The time τ now the Legendre-Fenchel transform [33] τ plays a role similar to system size N in conventional sta- φ∗(s)=sup[xs−φ (x)]. (7) tistical mechanics. We define the generating function f f x (cid:90) Z0(f;τ)≡ dX e21fXP0(X;τ)(cid:16)eτ12σ(f) (1) Oconnedcitainonnothweapsaktthheenfsoellmowbliengtoqucoensttiaoinn:oAnslysutmraejethctaotrwiees with large deviation function σ(f), where (cid:16) denotes the asymptotic limit of τ becoming larger than the longest �� dctioeorsnrcaerlliabttehioetnrhmetoimsdayemn.eamFpoihclysloswwiceianlagsskyt:hsteDemoaensbaluZotg0(ynfo;wwτi)thwfoitcrhofnnv(cid:54)=oenn0-- ����������� �� ��� ���������� ���� ��� zeroaffinity(i.e.,drivenintoaNESS)?Apositiveanswer ��� �� ��� �� would imply that � ��� ���� ��� ���� �� �� �� �� �� �� ∂σ � ��������� (cid:104)X (cid:105)=τ (2) τ ∂f �� holds, which, however, is not the case for arbitrary f. ����� �� � ������������������ Onlyforsmall|f|(cid:28)1inthelinearresponseregimedoes ��� � suchaninterpretationyieldthecorrectresultwithmean �� ��� 1 (cid:90) �� �� �� (cid:104)Xτ(cid:105)= Z dX Xe12fXP0(X;τ) ������� 0 (3) = 1(cid:104)(X )2(cid:105)f +O(f2). FIG.2: Illustrationofthedualityofsandcurrentx=Xτ/τ 2 τ fortheasymmetricrandomwalk(fordetailsseeAppendixA, with f = 1 and k+ =1): (a) Large deviation function φ∗(s) 2 f This result is the well-known fluctuation-dissipation the- (thickline). Theslopeats=0(steadystateI)correspondsto orem [4] through which fluctuations in thermal equilib- the mean current x0. (b) Rate function φf(x) of the current (thick line) with minimum at x . Conditioning currents to riumdeterminehowthesystemreactstoasmallapplied 0 a value x > x leads to the steady state (II) with s > 0 force f. Indeed, Onsager’s seminal insight has been that s 0 determined by the slope. (c) The unbiased average current in the linear response regime (half) “the rate of increase as a function of driving force f (thick line) and the current of the entropy plays the role of a potential” [32], namely x = ∂ φ∗ (thin line) from the generating function, where s s f the large deviation function s=(f −f)/2 quantifies a perturbation of the steady state eff with effective force f . Both currents agree for s = 0 but eff σ(f)= 1(cid:88)Lijfifj (4) deviate for increasing values of the perturbation s. For fixed 2 k+ the unbiased current is bounded (dashed black line). ij 3 with a fixed value x for the current. As discussed in nowexploretheconsequencesofdemanding thatφˆ (ω,t) s s detail by Chetrite and Touchette [25, 26], in the limit of remains a normalized function for s (cid:54)= 0. Since for non- large τ this “microcanonical” ensemble becomes equiva- negative φ(ω,R,t) Eq. (9) implies that also φˆ (ω,t) is s lent (under mild assumptions) to a “canonical” ensem- non-negative,itcanbeinterpretedastheprobabilitydis- ble in which the current fluctuates but its mean equals tribution of state ω for a system parametrized by s. At xs. This canonical path ensemble is described through this point the physical meaning of s is not obvious but the generating function Eq. (6) for a value of s deter- in the next section we will construct explicitly conjugate minedthroughtheconditions=∂xφf|xs. Whilesandx pairs (s,R). are thus conjugate quantities (see Fig. 2 for an illustra- Now consider a system described by the probability tion for a specific system), changing s does not trace a distribution φˆ (ω,t). The expectation value for an arbi- s changeoftheaffinitiesbutinvolvesarathercomplicated, trary observable A(ω) becomes non-local transformation (Doob’s transform) also of the interactions [25, 26, 34–36]. It is exactly this behavior (cid:104)A(t)(cid:105) =(cid:88)A(ω)φˆ (ω,t), (10) s s that complicates a general thermodynamic description ω of NESS. However, in the following we demonstrate that whichreducesto(cid:104)A(cid:105)forφˆ (ω,t)=ψ(ω)ats=0. Hence, smallscanbeinterpretedasaperturbationofthesteady 0 inthefollowingweinterprettheconjugatevariablesap- state,leadingtriviallytolinearresponserelations. More- pearinginthegeneratingfunctiontodescribeanexternal over,basedonthisresultwecanconstructadifferentset perturbation applied to the system at t = 0 and driving of conjugate quantities which extend Onsager’s result to it towards a neighboring steady state. The response to NESS driven beyond the linear response regime. this perturbation is III. A GENERAL RESPONSE FORMULA ∂(cid:104)A∂(sτ)(cid:105)s(cid:12)(cid:12)(cid:12)(cid:12)s=0 =(cid:88)ω A(ω) ∂φˆs∂(ωs,τ)(cid:12)(cid:12)(cid:12)(cid:12)(cid:12)s=0 We consider a steady state maintained by at least one (cid:88)(cid:90) (11) = dRA(ω)Rφ(ω,R,τ) non-vanishing affinity and thus having a non-vanishing entropy production rate (cid:104)Σ (cid:105) > 0. For clarity, in this ω τ section we consider a single perturbation but the gener- =(cid:104)A(τ)Rτ(cid:105), alizationtomorethanoneisstraightforward. Tobesuffi- whichfollowsinsertingEq.(9). Thisisourcentralresult. cientlygeneral,wedefineourquantityofinterestthrough It relates the response (sometimes called sensitivity) of the stochastic (Riemann-Stieltjes) integral of the form an observable to the correlations of this observable with (cid:90) τ (cid:90) τ theamountofRaccumulatedsincetheperturbationwas R [ω ]≡ dr(ω ) = dtr˙(ω ,ω˙ ) (8) τ t t t t applied. The correlations are to be determined in the 0 0 unperturbed steady state corresponding to s = 0. The over a process ω representing the state ω of the system t result Eq. (11) is quite general and does not require any at time t. The integral maps a single trajectory {ω }τ t 0 assumptions on the dynamics. of length τ (cid:62) 0 onto a real number. Clearly, R ∼ τ is τ a time-extensive quantity. It will be convenient later to also introduce the generalized velocity r˙(ω,ω˙), which for IV. CONSTRUCTING CONJUGATE PAIRS stochasticprocessesistobeunderstoodsymbolicallyand followsthenotationalconventionthattypicallyisusedin The response Eq. (11) follows for functions φˆ (ω,t) s physics. that, at least for small s, are normalized. This places Thejointprobabilityφ(ω,R,t)describestheprobabil- some restrictions onto what integrals R [ω ] are actually τ t ity to observe the system in state ω at time t having admissible. One property follows immediately by choos- accumulated an amount R = R up to time t (cid:54) τ start- t ing A(ω) = 1, which implies that the average (cid:104)R (cid:105) = 0 t ing with R = 0. Hence, the initial condition factorizes 0 vanishes for any t>0. toφ(ω,R,0)=ψ(ω)δ(R), whereψ(ω)isthesteadystate probability of state ω and δ(R) is the Dirac δ-function. It is often more convenient to work with the (Laplace) A. Stochastic dynamics transform (cid:90) φˆ (ω,t)≡ dResRφ(ω,R,t) (9) To be more specific, we consider a continuous Markov s process with initial condition φˆ (ω,0)=ψ(ω) following from the dω =F(ω )dt+dξ(ω ) (12) s t t t factorization of the joint probability, where the integral with effective drift vector F(ω) and random increments runs over all possible values of R. Moreover, for s = 0 we have that φˆ (ω,t) = ψ(ω) is the steady state prob- (cid:88) 0 dξ(ω)= σ (ω)◦dW (t), (13) ability. While in general φˆ (ω,t) is not normalized, we α α s α 4 where W (t) are independent Wiener processes and the C. Coupling to state changes α symbol ◦ denotes the Stratonovich rule for stochastic in- tegrals. With the symmetric diffusion matrix A more general form of time-extensive observables is 1(cid:88) given by Dij(ω)≡ σi(ω)σj(ω) (14) 2 α α α dr(ω)=h(ω)dt+g(ω)◦dω, (22) the Markov generator reads wherethevectorg(ω)nowcouplestotheevolutionofthe L =F ·D·∇+∇·D·∇=(F +∇)·D·∇. (15) state ω. The generator follows as 0 Its adjoint L† generates the time evolution of the proba- L =F·D·(∇+sg)+(∇+sg)·D·(∇+sg)+sh. (23) 0 s bilitydistribution,∂ ψ =L†ψ. Here,F(ω)isthephysical t 0 Expanding to lowest order we again find Eq. (21) for the force such that the effective drift becomes coefficient g(ω) and the condition to preserve normaliza- 1(cid:88) F =D·F + (∇·σ )σ . (16) tion now becomes 2 α α α F ·D·g+∇·(D·g)+h=0. (24) Throughout we set Boltzmann’s constant and temper- ature to unity so that entropies are dimensionless and It is straightforward to check that the time-integrated the mobility matrix coincides with the diffusion matrix observable R following from Eq. (22) can be written as τ Eq. (14). the derivative (cid:12) B. The response formula of Warren and Allen Rτ =− ∂∂Asτ(cid:12)(cid:12)(cid:12) (25) s=0 with stochastic action We first consider (cid:90) τ dr(ω)=h(ω)dt+g(ω)◦dξ(ω), (17) A [ω ]≡ dtL (ω ,ω˙ ), (26) τ t s t t 0 where the vector g(ω) couples to the same noise as in Eq. (12). Following Chetrite and Touchette [25, 26], the where (still employing the Stratonovich rule) tilted (or deformed) generator for the evolution ∂ φˆ = t s 1 L†φˆ becomes L (ω,ω˙)= (ω˙ −D·F )·D−1·(ω˙ −D·F ) s s s 4 s s L =F ·D·∇+(∇+sg)·D·(∇+sg)+sh, (18) 1 s + ∇·(D·F ). (27) 2 s which for s=0 reduces to the generator L in Eq. (15). 0 Expanding the second term to linear order of s, we can Hence, employing Eq. (22), the conjugate observable R τ recast this generator into the form nowcorrespondstothe“pathweightrepresentation”dis- L =(F+2sg+∇)·D·∇+s[∇·(D·g)+h]+O(s2), (19) cussed in Refs. 6, 14, 18. s which manifestly preserves normalization if ∇·(D·g)+ h = 0, which thus determines h(ω). Note that changing V. DISCUSSION from Stratonovich to Itˆo calculus, this condition implies that dr = g · dξ. Clearly, since then state and noise A. Thermodynamic formalism are independent, the expectation value of R vanishes as required. It is straightforward to extend Eq. (11) to multiple We now assume that the perturbed steady state is de- affinities s = {si}. We restrict our considerations to the scribed by the forces F (ω) depending on s. Expanding s set of observables {Ri} with vanishing mean, for which the forces to linear order, τ we can derive a local potential. To this end, from the (cid:12) Fs(ω)=F(ω)+s ∂F∂ss(ω)(cid:12)(cid:12)(cid:12) +O(s2), (20) terraantisnfogrfmunedctjioonint probability Eq. (9) we define the gen- s=0 we read off the coefficient Zf(s;τ)=(cid:88)φˆs(ω,τ)(cid:16)eτϕ∗f(s), (28) (cid:12) g(ω)= 1 ∂Fs(ω)(cid:12)(cid:12) (21) ω 2 ∂s (cid:12) s=0 where we make explicit the dependency on the affinities by comparing with Eq. (19). This is the result found f driving the system. In the limit τ → ∞ the large de- in Ref. 11 following quite a different approach. Pro- viationfunctionagainfollowsfromtheLegendre-Fenchel vided we know how the forces depend on s, we have transform thus constructed one possible observable R to be used τ ϕ∗(s)=sup[r·s−ϕ (r)], (29) in Eq. (11). f f r 5 where we have assumed that a large deviation principle afterinsertingthespeedv(f+s)=(cid:104)x˙(cid:105) =D [−(cid:104)∂ U(cid:105) + s 0 x s Pf(R;τ) (cid:16) e−τϕf(r) holds with ri ≡ Ri/τ. As a conse- f+s]. Duetotheadditivityoftheperturbation,thecon- quence,ϕ∗(s)isalways aconvexfunctionandconstitutes jugate variable (cid:104)r˙(cid:105) is a simple linear function of s inde- f our local potential around a steady state determined by pendentoff implyingthepotentialsϕ∗(s)= 1D s2 and 4 0 theaffinitiesf. Forapotentialϕ∗(s)thatisdifferentiable ϕ(r) = 1 r2. Hence, while v(f) is a non-linear function at s = 0, the correlations are mfanifestly symmetric and ofthedrDiv0ingforcef,thelocalpotentialdescribestrivial, follow as equilibrium-like fluctuations [7]. Close to equilibrium in (cid:104)RτiRτj(cid:105)= ∂s∂i∂2sj lnZf(cid:12)(cid:12)(cid:12)(cid:12)s=0 (cid:16) τ∂∂s2iϕ∂s∗fj(cid:12)(cid:12)(cid:12)(cid:12)(cid:12)s=0 =τLifj tahseelxipneeactrerde.sponseregimeonerecovers(cid:104)x˙(cid:105)=2(cid:104)r˙(cid:105)=D0f (30) with steady state susceptibilities C. Fluctuation theorem 1∂(cid:104)Ri(cid:105) ∂(cid:104)r˙i(cid:105) Lij ≡ lim τ s = s. (31) Whatisthephysicalmeaningofs? Togetsomeinsight f τ→∞τ ∂sj ∂sj let us assume that s shifts the steady state to f+s with ThisresultextendstheOnsagerpotentialEq.(4)tonon- probability zero affinities and emphasizes the canonical structure. P (R;τ)∼esRP (R;τ), (36) An interesting consequence is that, employing Legendre f+s f transforms as in conventional thermodynamics, we can which is the expression that appears in the generating now switch between affinity si and current (cid:104)r˙i(cid:105) depend- function. For a large class of observables (including ing on what is the more convenient variable for a spe- the example from the previous subsection) we can write cific situation. Moreover, susceptibilities are related by R = 1(X −S )asacurrentX minusanothertermS , Maxwell and further relations (similar to, e.g., the rela- boτth o2f whτich hτave the same avτerage (cid:104)X (cid:105)=(cid:104)S (cid:105) in thτe τ τ tion between the heat capacities at constant volume and unperturbed NESS. While the current is antisymmetric constant pressure). with respect to time reversal, X† = −X , the second τ τ term S† =S is invariant. The fluctuation theorem [13] τ τ then becomes B. Illustration: Single particle in a ring trap P (R;τ) P (X,S;τ) f+s = f esX =e(f+s)X, (37) Tobrieflyillustrateourresultsweconsidertheparadig- Pf+s(R†;τ) Pf(−X,S;τ) matic single colloidal particle moving in a ring trap [36– where the final expression involves the entropy Σ = τ 39], see Fig. 1(a). The state of the system is given by (f +s)X produced in the perturbed NESS. This shows τ the position x with force F(x) = −∂ U(x)+f, where x that the parameter s of the generating function, for U(x) is an external, periodic potential energy and f is the pair (s,R), indeed corresponds to a change of the the constant driving force. The diffusion coefficient D 0 affinity f determining the unperturbed NESS. The im- isindependentofx. Theparticleisdrivenintotheunper- portance of the time-symmetric contribution S for the τ turbed NESS through the force f with non-zero average non-equilibriumlinearresponsehasbeendiscussedbyC. speed v(f) = (cid:104)x˙(cid:105) = D [f −(cid:104)∂ U(cid:105)]. As perturbation we 0 x Maes and coworkers [6, 40]. consider a change of the driving force, f →f +s, with F (x)=−∂ U(x)+f +s. (32) s x D. Linear response regime From Eq. (20) we immediately find g = 1∂Fs(cid:12)(cid:12)(cid:12) = 1. (33) peAarsinegluidneEdqt.o(i1n1t)hiesninottroudnuiqcutieo.nT,thhisebobecsoemrveasblaepRpaτraenpt- 2 ∂s (cid:12) 2 s=0 inthelinearresponseregimeperturbingthermalequilib- From Eq. (24) one then obtains h(x)=−1D F (x) and rium when choosing the current Rτ → Xτ, which also 2 0 f has vanishing mean. Again appealing to the fluctuation thus from Eq. (22) the generalized velocity theorem we have for small |f|(cid:28)1 1 r˙(x,x˙)= 2[x˙ −D0Ff(x)]. (34) Pf(X;τ) = e12f·XP0(X;τ) =efX. (38) Thisisindeedoneoftheadmissiblechoicesfordetermin- Pf(−X;τ) e−12f·XP0(−X;τ) ing the response with respect to a change of the driving Here we have used that the currents change sign un- force [18]. der time reversal, whereby in equilibrium P (−X;τ) = 0 The average of Eq. (34) for a perturbed NESS with P (X;τ) holds. Following Eq. (36) one sees that now we 0 f +s becomes have to use s → 1f leading to the definition of the gen- 2 1 1 erating function Eq. (6) given in Sec. IIB, which in turn (cid:104)r˙(cid:105)s = 2[v(f +s)+D0(cid:104)∂xU(cid:105)s−D0f]= 2D0s (35) leads to the famous Onsager result. 6 VI. CONCLUSIONS ward with rates k+ and k−, respectively. The affinity is simply the force f = ln(k+/k−). For N+ steps for- τ InthispaperwehavestudiedthetiltedMarkovgener- ward and Nτ− steps backward, the distance traveled is ator under the condition that for small tilt s it preserves Xτ =Nτ+−Nτ− with average normalization and thus describes a physical stochastic process. Identifyingthisprocessasashiftedsteadystate (cid:104)Xτ(cid:105)=τ(k+−k−)=τk+(1−e−f). (A1) has allowed us to interpret the abstract tilt parameter s of the generating function as a perturbation of the Note that here the distance takes only discrete integer original steady state. For Markov processes we have ex- values. Its probability is known analytically [44] plicitly constructed two types of conjugate observables √ R that encode the system’s response and thus allow to P (X;τ)=I (2 k+k−τ)(k+/k−)X/2e−(k++k−)τ, f X determine transport coefficients from correlations in the (A2) unperturbedsteadystate. Onlyforcesarerequiredasin- where I (z) is the modified Bessel function of the first n put, no explicit knowledge of the stationary distribution kind of order n. The generating function or entropy production is necessary. Whatisperhapsmostinterestingisthenotionofdiffer- ∞ (cid:88) ent ensembles analogous to conventional thermodynam- Zf(s;τ)= esXPf(X;τ) (A3) ics. Consider for example the situation that we require X=−∞ can be calculated exactly using [45] a transversal transport coefficient for fixed longitudinal field (affinity) although the simulations (or experiments) ∞ have to be performed at fixed current. Transport coef- (cid:88) I (z)cX =exp(cid:2)(z/2)(c+c−1)(cid:3). (A4) ficients in one ensemble could then be calculated from X X=−∞ those in another ensemble much in the same way the heat capacity at constant pressure is calculated from the The result is Z (s;τ)=exp[τφ∗(s)] with heat capacity at constant volume. The approach pre- f f sented here might pave the way for a systematic theory (cid:16) (cid:17) althoughthesimpleexampleofatrappedBrownianpar- φ∗(s)=k+ es+e−(f+s)−e−f −1 . (A5) f ticle demonstrates that not all informations about the steady state are encoded in the corresponding local po- Clearly, the derivative tential. ∂φ∗ (cid:16) (cid:17) x = f =k+ es−e−(f+s) (A6) s ∂s Appendix A: Asymmetric random walk only agrees with the current Eq. (A1) for s = 0. Note Asaspecificexampleweconsidertheasymmetricran- that for this simple example the same current can be dom walk (ARW) [41–43], for which we can perform the achieved through the effective force f = f +2s while eff transformations analytically. The ARW describes the simultaneously rescaling time. The slightly more com- motion of a walker on an infinite lattice [cf. Fig. 1(a)] plex example of a bias random walker with two internal with discrete sites. The walker jumps forward and back- states has been treated in Ref. 35. [1] V.Coropceanu,J.Cornil,D.A.daSilvaFilho,Y.Olivier, [9] T. Speck, Prog. Theor. Phys. Suppl. 184, 248 (2010). R.Silbey,andJ.-L.Br´edas,Chem.Rev.107,926(2007). [10] U. Seifert, Eur. 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