Journal of Statistical Physics

, Volume 152, Issue 1, pp 93–111 | Cite as

Microscopic Structure of Shocks and Antishocks in the ASEP Conditioned on Low Current



We study the time evolution of the ASEP on a one-dimensional torus with L sites, conditioned on an atypically low current up to a finite time t. For a certain one-parameter family of initial measures with a shock we prove that the shock position performs a biased random walk on the torus and that the measure seen from the shock position remains invariant. We compute explicitly the transition rates of the random walk. For the large scale behavior this result suggests that there is an atypically low current such that the optimal density profile that realizes this current is a hyperbolic tangent with a traveling shock discontinuity. For an atypically low local current across a single bond of the torus we prove that a product measure with a shock at an arbitrary position and an antishock at the conditioned bond remains a convex combination of such measures at all times which implies that the antishock remains microscopically stable under the locally conditioned dynamics. We compute the coefficients of the convex combinations.


Asymmetric symmetric exclusion process Large deviations Shocks Antishocks 

1 Introduction

The Asymmetric Simple Exclusion Process (ASEP) on \(\mathbb{Z}\) [1, 2] describes the Markovian time evolution of identical particles according to the following rules: (1) Each particle performs a continuous time simple random walk on \(\mathbb{Z}\) with hopping rate cr to the right and c to the left; (2) The hopping attempt is rejected when the site where the particles tries to move is occupied. Without loss of generality cr>c is assumed. An important family of invariant measures for this process are the Bernoulli product measures parametrized by the particle density ρ. The stationary current j is then j=(crc)ρ(1−ρ). For cr=c (symmetric simple exclusion process) the dynamics is reversible and one has j=0. The process may also be defined on a finite integer lattice with various types of boundary conditions which may lead to non-vanishing stationary currents even in the symmetric case. The presence of a stationary current indicates the lack of reversibility of the dynamics and therefore one is interested not only with its stationary expectation j, but also its fluctuations.

Starting with the seminal papers [3, 4] the large deviation theory for the ASEP has been developed in considerable detail. Of particular interest in this context is the time-integrated current \(J_{k}(t)=J^{+}_{k}(t) - J^{-}_{k}(t)\) across a bond (k,k+1), where \(J^{+}_{k}(t)\) is the number of jumps of particles from k to k+1 up to time t and analogously \(J^{-}_{k}(t)\) is the number of jumps from k+1 to k up to time t, starting from some initial distribution of the particles. In a periodic system with L sites, i.e., on the torus \(\mathbb{T}_{L}:=\mathbb{Z}/L\mathbb {Z}\), a related quantity of interest is the time-integrated total current \(J(t) = \sum_{k\in\mathbb{T}_{L}} J_{k}(t)\) which is intimately related to the rate of entropy production [5, 6]. We denote its distribution by \(Z_{J}(t) := \operatorname{Prob}[J(t) = J]\) with \(J\in \mathbb{Z}\). One also considers the (local) mean current jk(t)=Jk(t)/t and the (global) mean current density j(t)=J(t)/(Lt). For the Bernoulli product measure one has limt→∞jk(t)=limt→∞j(t)=j. The probability to observe for a long time interval t an untypical mean jj is exponentially small in t. This is expressed in the large deviation property [7] ZJ(t)∝exp(−f(j)Lt) where f(j) is the rate function which plays a role analogous to the free energy in equilibrium statistical mechanics. Indeed, in complete analogy to equilibrium one introduces a generalized fugacity es with generalized chemical potential s and also studies the generating function Ys(t)=〈esJ(t)〉=∑JesJZJ(t). The cumulant function g(s)=limt→∞lnYs(t)/(Lt) is the Legendre transform of the rate function for the mean current, g(s)=maxj[jsf(j)]. The intensive variable s is thus conjugate to the mean current density j.

Recently a focus of attention has been on the spatio-temporal structure of the process conditioned on realizing a prolonged untypical behavior of the current. A convenient approach to study this rare and extreme behavior is to consider the process in terms of the conjugate variable s. Fixing some s≠0 corresponds to studying realizations of the process where the current fluctuates around some non-typical mean. We shall refer to this approach as grandcanonical conditioning, as opposed to a canonical condition where the current J(t) would be conditioned to have some fixed value J. For the weakly asymmetric exclusion process (WASEP) on \(\mathbb{T}_{L}\) where crc=ν/L is small, it turns out in the hydrodynamic limit that for any strictly positive s (i.e., for any current j>j) the optimal macroscopic density profile ρ(x,t) that realizes such a deviation is time-independent and flat [8]. Thus on macroscopic scale the conditioned density profile is equal to the typical (unconditioned) density profile. However, a recent microscopic approach using a form of Doob’s h-transform has revealed [10, 11] that for large s the ASEP with arbitrary strength of the asymmetry crc exhibits interesting stationary correlations. Even more remarkably, the process undergoes a phase transition from the typical dynamics in the KPZ universality class with dynamical exponent z=3/2 to ballistic dynamics with z=1.

For currents below the typical value (s<0) the large deviation approach for the WASEP yields a different phenomenon [8, 9]: For currents close to the typical current (but j<j) the optimal macroscopic density profile ρ(x,t) is time-independent and flat as is the case for any s>0. However, below some critical value sc (i.e. below some critical jc<j) the flat profile becomes unstable and a traveling wave of the form ρ(xvt) develops. In the limit ν→∞ (expected to correspond to finite asymmetry in the ASEP) the optimal profile in this regime is predicted to have the form of a step function with two constant values ρ1 and ρ2. This is a profile consisting of a shock discontinuity where the density jumps from ρ1 to ρ2>ρ1 at a position x1(t) and an antishock where the density jumps from ρ2 to ρ1 at position x2(t). Hence, conditioning on a sufficiently large negative deviation of the current j<jc induces a phase separation in the WASEP into a low density segment of length r=x1x2 with density ρ1 and a high density segment of length Lr=x2x1 with density ρ2 (positions and distances taken modulo L). A similar phase separated optimal profile, but without drift, has recently been obtained for atypically low activities K(t)=J+(t)+J(t) in the SSEP [12].

In order to understand this phenomenon better we develop in this paper a microscopic approach for the ASEP for atypically low currents, but without restriction to the case of weak asymmetry. For a periodic system, as discussed above, one may expect in the long-time regime a traveling wave. In order to get insight into the microscopic structure of the traveling wave we focus on short times and address the question how for global conditioning a certain initial distribution which already has a shock evolves at some later finite time t. We also consider local conditioning of the current on a single bond. For this case we study the evolution for finite times t of a shock/antishock pair with densities ρ1,2. Our rigorous analysis is an adaptation of the algebraic techniques developed in [13] and extended recently by Imamura and Sasamoto to study current moments of the ASEP [14]. This approach—which has its probabilistic origin in the self-duality of the ASEP [15, 16, 17]—constrains our approach to a specific family of initial shock measures which are certain functions of the hopping asymmetry. However, going from the weakly asymmetric case all the way to the totally asymmetric limit allows us to cover a wide range of scenarios.

The paper is organized as follows. In Sect. 2 we describe informally the well-established, but not so widely known tools required for studying grandcanonically conditioned dynamics. In Sect. 3 we introduce a new family of shock measures which are relevant for the grandcanonically conditioned time evolution of the ASEP. In Sect. 4 we state and prove the main result and in Sect. 5 we conclude with some further comments on a generalization of the present approach to more general shock measures and on the macroscopic large deviation results of [8].

2 ASEP Conditioned on a Low Current

We consider the ASEP on the one-dimensional torus \(\mathbb{T}_{L}\) with L sites. For convenience we take L even and denote sites (defined modulo L) by an integer in the interval −M+1,M where M:=L/2. We shall identify jumps to the “right” with clockwise jumps. We introduce the hopping asymmetry
$$ q = \sqrt{\frac{c_r}{c_\ell}} $$
and parametrize the densities ρ by the fugacity
$$ z := \frac{\rho}{1-\rho}. $$
The shock/antishock initial distributions considered below are characterized by two fugacities z1,2 satisfying

Condition S

$$ \frac{z_2}{z_1}=q^2 $$

This condition is motivated by properties of the representation of the quantum algebra Uq[SU(2)] which is a symmetry of the generator of the process with reflecting boundaries [13]. By convention we shall assume 1<q<∞, i.e. we consider preferred hopping to the “right” (clockwise) and we exclude the symmetric case q=1.

Grandcanonically conditioned Markov processes may be studied in the spirit of Doob’s h-transform [18], as was done for the ASEP conditioned on very large currents in [10, 11, 19], see below for the precise definition. To this end, we follow our earlier work [13] and we employ a matrix formulation to define the process. This formulation of Markovian dynamics, formalized in probabilistic terms for exclusion processes in [20] and described informally in detail in [2], allows for an alternative convenient formulation particularly of conditioned interacting particle systems, as discussed in [6]. For self-containedness we briefly explain the approach and introduce the necessary notation.

2.1 Matrix Formulation of the ASEP

In the context of interacting particle systems with state space \(\mathbb{V}\) the Markov generator L acting on cylinder functions f(η) of the configuration \(\eta\in\mathbb{V}\) is usually defined through the relation
$$ L f(\eta) = \sum_{\eta'} w_{\eta', \eta} \bigl[f\bigl(\eta'\bigr) - f(\eta)\bigr]. $$
where wη′,η is the transition rate from a configuration η to η′. In particular for a probability measure μ(t) we have
$$ \frac{\mathrm{d}}{\mathrm{d}t} \langle f \rangle_\mu=\langle Lf \rangle_\mu $$
where 〈⋅〉μ denotes expectation w.r.t. μ. In particular, taking f to be the indicator function \({\bf1}_{\eta}\) on a fixed configuration η yields the master equation
$$ \frac{\mathrm{d}}{\mathrm{d}t} \mu(\eta;t) = \sum_{\stackrel{\eta'\in\mathbb{V}}{\eta'\neq\eta}} \bigl[w_{\eta, \eta'} \mu\bigl(\eta';t\bigr) - w_{\eta', \eta} \mu(\eta;t) \bigr] $$
for the time evolution of the probability μ(η;t) of finding the configuration η at time t. A stationary distribution, i.e., an invariant measure satisfying dμ/dt=0 is denoted by μ and a stationary probability of a configuration η is denoted μ(η).
A convenient way to write the master equation (6) in a matrix form is provided by the so-called quantum Hamiltonian formalism [2, 20]. The idea is to assign to each of the possible configurations η a column vector |η〉 which together with the transposed vectors 〈η| form an orthogonal basis of a complex vector space with inner product 〈η|η′〉=δη,η. Here δη,η is the Kronecker symbol which is equal to 1 if the two arguments are equal and zero otherwise. Therefore a measure can be written as a probability vector
$$ \big| \mu(t)\big \rangle= \sum_{\eta\in\mathbb{V}} \mu( \eta;t) |\eta \rangle $$
whose components are the probabilities μ(η;t)=〈η|μ(t)〉. The bra-ket notation for vectors is an elegant tool borrowed from quantum mechanics.
Using a standard argument (see for example Chap. XVII of Feller [21]), for all t≥0, the master equation (6) then takes the form
$$ \frac{d}{dt}\big |\mu(t) \big\rangle = -H \big|\mu(t) \big\rangle $$
with the solution
$$ \big|\mu(t) \big\rangle = \mathrm{e}^{-Ht }\big|\mu(0) \big\rangle $$
reflecting the semi-group property. The off-diagonal matrix elements Hη,η of the matrix H are the (negative) transition rates wη,η and the diagonal entries Hη,η are the sum of all outgoing transition rates wη′,η from configuration η.
For the study of expectations we also define the row vector 〈s|
$$ \langle s| :=(1,1,\ldots, 1) =\sum _{\eta\in\{0,1\}^{L}}\langle\eta| $$
which we call the summation vector. By conservation of probability we have for any probability vector \(\langle s | \mu(t) \rangle= \sum_{\eta\in\mathbb{V}} \mu (\eta ;t) = 1\). This implies 〈s|H=0, i.e., the row vector 〈s| is a left eigenvector of H with eigenvalue 0. A right eigenvector with eigenvalue 0 is an invariant measure |μ〉.
Expectation values 〈f〉=∑ηf(η)μ(η) of a function f(η) are obtained by taking the scalar product \(\langle s| \hat{f} |\mu \rangle\) of the diagonal matrix
$$ \hat{f} := \sum_{\eta\in\mathbb{V}} f(\eta) |\eta \rangle \langle \eta| $$
where |η〉〈η| is used as a shorthand for |η〉⊗〈η| as is standard in the quantum mechanics literature. Moreover, we introduce for t≥0 the non-diagonal matrices
$$ \hat{f}(t) = \mathrm{e}^{Ht} \hat{f} \mathrm{e}^{-Ht} $$
and find for any initial measure μ(0) the useful identity
$$ \bigl\langle f(t) \bigr\rangle = \langle s | \hat{f} \bigl|\mu(t) \bigr\rangle = \langle s| \hat{f}(t) \bigl|\mu(0) \bigr\rangle. $$
Correspondingly for joint expectations at different times ti+1ti≥0 one has
$$ \bigl\langle f_n (t_n) \dots f_2 (t_2) f_1 (t_1) \bigr\rangle = \langle s| \hat{f}_n (t_n) \dots\hat{f}_2 (t_2) \hat{f}_1 (t_1) \bigl|\mu(0) \bigr \rangle. $$
Notice that (5) translates into \(\mathrm{d}/(\mathrm{d}t) \langle f(t) \rangle = - \langle\hat{f}H \rangle\). As there will be no danger of confusing L and H we shall somewhat loosely refer also to H as generator of the process, since we can identify −H with usual generator acting on cylinder functions f by its action to the left on \(\langle s| \hat {f} H\).
For the ASEP the vector representation of the state space \(\mathbb{V}=\{0,1\}^{L}\) is conveniently done using a tensor basis. The tensor product is denoted by ⊗, and Ak denotes the k-fold tensor product of A. The superscript T indicates transposition. A configuration η∈{0,1}L will be represented by the vector \(|\eta \rangle\in\mathbb{C}^{2^{L}}\) which is defined in the following manner
$$ |\eta \rangle=\bigl|\eta(-M+1) \bigr\rangle \otimes \bigl|\eta(-M+2) \bigr\rangle \otimes\cdots\otimes \bigl|\eta(M) \bigr\rangle $$
where for each i=−M+1,…,M, |η(i)〉=(0,1)T, if the i-th site in the configuration η contains a particle, and |η(i)〉=(1,0)T, otherwise. Observe that for any configuration η, the corresponding vector |η〉 has 1 at one of its components and 0 at all others.
In order to construct the matrix representation of the generator H for the ASEP we introduce the three 2-by-2 matrices
$$ \sigma^+:=\left ( \begin{array}{c@{\quad }c} 0 & 1\\ 0 & 0 \end{array} \right ), \qquad \sigma^-:=\left ( \begin{array}{c@{\quad }c} 0 & 0\\ 1 & 0 \end{array} \right ), \qquad \hat{n}:=\left ( \begin{array}{c@{\quad }c} 0 & 0\\ 0 & 1 \end{array} \right ). $$
Then, denoting by Open image in new window the two-dimensional unit matrix, we introduce for each \(k \in\mathbb{T}\) where a non-identity matrix appears at the (M+k)-th position, counting from the left to the right. We also introduce Open image in new window and Open image in new window.
For readers unfamiliar with this construction we point out some simple properties of these matrices and their action on vectors. Notice that \((1,0)\sigma ^{+}=(0,1)\hat{n}=(0,1)\), (0,1)σ=(1,0), \((1,0)\hat{n}=(1,0)\sigma^{-}=(0,1)\sigma ^{+}=(0,0)\); and analogously, σ+(0,1)T=(1,0)T, \(\sigma^{-}(1,0)^{T}=\hat{n}(0,1)^{T}=(0,1)^{T}\), \(\hat{n}(1,0)^{T}=\sigma^{+}(1,0)^{T}=\sigma^{-}(0,1)^{T}=(0,0)\). These identities and the representation (15) yield the following properties of \(\sigma^{\pm}_{k}\) and \(\hat{n}_{k}\): If a configuration η does not have a particle at the site k then \(|\eta^{\prime}\rangle:=\sigma^{-}_{k}|\eta \rangle\) corresponds to the configuration that coincides with η on \(\mathbb{T}_{L}\setminus\{k\}\) and has a particle at k; if to the contrary η has a particle at k then \(\sigma^{-}_{k}|\eta \rangle=0\), i.e., the vector with all components equal to 0. If a configuration η has a particle at the site k then \(|\eta^{\ast}\rangle:=\sigma^{+}_{k} |\eta \rangle\) corresponds to the configuration that coincides with η on \(\mathbb{T}_{L}\setminus\{k\}\) and does not have a particle at k; if to the contrary η does not have a particle at k then \(\sigma^{+}_{k}|\eta \rangle=0\). Using the equality \((\sigma^{+}_{k})^{T}=\sigma^{-}_{k}\) and the above notations, we have that if η does not have a particle at k then \(\langle\eta|\sigma ^{+}_{k}=\langle\eta^{\prime}|\) and \(\langle\eta|\sigma^{-}_{k}=0\), while if η has a particle at k then \(\langle\eta|\sigma^{+}_{k}=0\) and \(\langle\eta |\sigma^{-}_{k}=\langle\eta^{\ast}|\). Accordingly, \(\sigma^{-}_{k}\) and \(\sigma^{+}_{k}\) are called the particle creation/annihilation operators. The operator \(\hat{n}_{k}\) is called the number operator; when applied to |η〉, it returns |η〉, if there was a particle at the site k, and results in 0 otherwise, i.e. we have Similarly, \(\hat{v}_{k}\) is the vacancy operator.
With these definitions the generator of the ASEP becomes
$$ H:=-\sum_{i=-M+1}^{M} \bigl[ c_r \bigl(\sigma^+_i \sigma^-_{i+1} - \hat{n}_i \hat{v}_{i+1}\bigr)+ c_\ell\bigl( \sigma^-_i \sigma^+_{i+1} - \hat{v}_{i} \hat{n}_{i+1} \bigr) \bigr]. $$
For an arbitrary distribution μ(0) on {0,1}L and its vector representation |μ(0)〉 as defined above we denote by |μ(t)〉 the vector representation of the distribution of ASEP at time t, starting from μ(0). We point out that in the tensor basis a product measure is represented by a tensor product of the single-site marginals. For the summation vector we have the tensor representation 〈s|=(1,1)L.

2.2 Grandcanonical Conditioning on an Atypical Current

The generator H defined above is for the hopping dynamics only, it does not include the evolution of the integrated current J(t). Since J(t) can take any integer value J, the state space for the full process is \(\{0,1\}^{L}\times\mathbb{Z}\). In order to construct the matrix representation we choose as basis for this space the set of product vectors |η〉⊗|J〉 with \(J\in\mathbb{Z}\). (Notice that the symbols 〈⋅| and |⋅〉 can be vectors in different vector spaces, as will be clear from the form of the argument.) Defining (infinite-dimensional) operators A± through the relation A±|J〉=|J±1〉 we obtain following Ref. [6] the generator
$$ G:=-\sum_{i=-M+1}^{M} \bigl[ c_r\bigl(\sigma^+_i\sigma^-_{i+1} \otimes A^+-n_i v_{i+1}\bigr)+ c_\ell\bigl( \sigma^-_i\sigma^+_{i+1}\otimes A^- -v_{i} n_{i+1}\bigr) \bigr] $$
for the full process. One sees that the elementary hopping matrices not only change the configuration η according to which jump has occurred, but also change the value of total integrated current J accordingly. An initial configuration is represented by a tensor vector |η,J〉:=|η〉⊗|J〉. We shall take J(0)=0 as initial value of J(t). Hence an initial measure for the full process has the form |μ(0)〉⊗|0〉. In order to compute expectation values we define the extended summation vector \(\langle\hat{s}| := \langle s|\otimes\langle s'|\) where 〈s′| is the infinite-dimensional summation vector for the counting variable J.
Consider now the process conditioned on J(t) having reached some fixed value J at time t≥0. The conditional distribution μ(η,J;t) of the ASEP under this conditioning has the form
$$ \mu(\eta,J;t) = \frac{\langle\eta,J| \mathrm{e}^{-Gt} |\mu(0),0 \rangle}{ Z_J(t)} $$
$$ Z_J(t) := \operatorname{Prob}\bigl[J(t)=J\bigr] = \langle s,J| \mathrm{e}^{-Gt} \bigl|\mu(0),0 \bigr\rangle $$
is the marginal distribution of the integrated current and 〈s,J|:=〈s|⊗〈J| with \(J\in\mathbb{Z}\). We write the conditional expectation of some function f of the occupation numbers of the ASEP as
$$ \bigl\langle f(t) \bigr\rangle_J = \frac{ \langle f;J(t)=J \rangle}{Z_J(t)} = \frac{\langle s,J| \hat{f} \mathrm{e}^{-Gt} |\mu(0),0 \rangle}{Z_J(t)}. $$
In actual fact, however, we are not interested in conditioning on a fixed value J of the current, but rather in expectations for an ensemble where the current is allowed to fluctuate around some generally atypical value. To this end we follow standard procedure and define a “grand canonical” current ensemble
$$ Y_s(t) = \bigl\langle\mathrm{e}^{s J(t)} \bigr\rangle= \sum _{J \in\mathbb {Z}} \mathrm{e}^{sJ} Z_J(t). $$
Analogously we define the fluctuating conditional probability of a configuration η as
$$ \mu_s(\eta;t) = \frac{\sum_{J \in\mathbb{Z}} \mathrm{e}^{sJ} \langle\eta,J| \mathrm{e}^{-Gt} |\mu(0),0 \rangle}{ Y_s(t)} $$
and the corresponding expectations
$$ \bigl\langle f(t) \bigr\rangle_s := \frac{\langle f(t) \mathrm{e}^{sJ(t)} \rangle}{ \langle\mathrm{e}^{sJ(t)} \rangle} = \frac{\sum_{J \in\mathbb{Z}} \mathrm{e}^{sJ} \langle f;J(t)=J \rangle}{Y_s(t)}. $$
Notice that Y0(t)=1 and that therefore |μ0〉=|μ〉 is the usual (unconditioned) measure and 〈f(t)〉0 is the usual (unconditioned) expectation of f. We shall refer to the latter quantity as the “typical” expectation. For s≠0 we call corresponding quantities atypical.
Consider now the unnormalized fluctuating conditional probability
$$ \tilde{\mu}_s(\eta;t) = \sum_{J \in\mathbb{Z}} \mathrm{e}^{sJ} \langle\eta,J| \mathrm{e}^{-Gt} \bigl|\mu(0),0 \bigr\rangle. $$
The following simple result is often used in the literature without proof, see e.g. [7] and, for a formal derivation using counting operators A±, see [6]. One has for the associated unnormalized probability vector
$$ \bigl|\tilde{\mu}_s(t) \bigr\rangle= \mathrm{e}^{-\tilde{H}(s)t} \bigl|\mu(0) \bigr\rangle $$
$$ Y_s(t) = \langle s| \mathrm{e}^{-\tilde{H}(s)t} \bigl|\mu(0) \bigr \rangle $$
for the normalization. Here \(\tilde{H}(s)\) is the matrix of dimension 2L obtained from G by substituting the counting operators A± by the c-numbers e±s. Notice that \(\tilde{H}(0)=H\) is the generator of the ASEP constructed above. For s≠0 the matrix \(\tilde{H}(s)\) does not conserve probability, but nevertheless has an intuitive probabilistic interpretation. It gives a weight e±s to each transition in a particular realization of the process. Hence we shall refer to \(\tilde{H}(s)\) as the weighted generator. The generalized chemical potential s parametrizes the mean current of this weighted process. Thus we arrive at the central object of our interest, which is the conditional distribution
$$ \bigl|\mu_s(t) \bigr\rangle := \frac{ \mathrm{e}^{-\tilde{H}(s) t} |\mu(0) \rangle}{ \langle s| \mathrm{e}^{-\tilde{H}(s) t} |\mu(0) \rangle}. $$
This quantity describes the approach to the long-time large deviation regime from a given initial distribution and hence provides information about the space-time structure of the long-time large deviation regime. Notice that below we shall drop the subscript s which indicates the s-dependence. (Grandcanonical) conditioned expectations at time t are then computed as follows:
$$ \bigl\langle f(t) \bigr\rangle_s = \frac{\langle s| \hat{f} \mathrm{e}^{-\tilde{H}(s) t} |\mu(0) \rangle}{ \langle s| \mathrm{e}^{-\tilde{H}(s) t} |\mu(0) \rangle} . $$

In the same spirit one can investigate the space time structure of the process under the condition that the integrated current across some fixed bond (k,k+1) has attained a certain value. Going to the grandcanonical conditioning leads to a matrix \(\tilde{H}^{(k)}(s)\) where only the hopping terms for the bond (k,k+1) have the weights e±s. As discussed in the introduction we refer to this setting as local conditioning, as opposed to the global conditioning involving the global current. Notice that the global time-integrated current J(t) is (trivially) extensive in system size L and hence its generating function does not have a good limit for L→∞. Below we shall choose under global conditioning the coefficient s to be order 1/L as this yields the generating function for the current density j. This quantity has finite expectation 〈j〉 even for L→∞.

3 Shock Measures

We shall consider the evolution of two distinct types of shock measures. First we recall the definition of a shock measure with shock at site m in the infinite integer lattice \(\mathbb{Z}\) as a Bernoulli product measure with marginal fugacity z1 up to site m−1 and fugacity z2>z1 from site m onwards [13]. We denote these measures by \(\mu^{+}_{m}\). Likewise one can define an antishock measure \(\mu^{-}_{n}\) for the infinite lattice with antishock at site n, i.e., fugacities z(k)=z2 for kn and z(k)=z1 for k>n.

Type I shock measures for the torus \(\mathbb{T}_{L}\) are defined in analogy to these shock measures as follows:

Definition 3.1

For the torus \(\mathbb{T}_{L}\) a shock measure \(\mu^{\mathrm {I}}_{m,n}\) of type I with nm is a Bernoulli product measure with fugacities
$$\left. \begin{array}{l@{\quad }l} z_2 & \mbox{at the set of sites } P^{m<n}_{\mathit{high}} := \{ k \in \mathbb{T}_L : m < k \leq n \}\\ \noalign{\vspace{3pt}} z_1 & \mbox{at the set of sites } P^{m<n}_{\mathit{low}} := \mathbb{T}_L \setminus P^{n<m}_{\mathit{high}} \end{array} \right\}\quad \mbox{if } {-}M+1 \leq m < n \leq M $$
$$\left.\begin{array}{l@{\quad }l} z_1 & \mbox{at the set of sites } P^{n<m}_{\mathit{low}} := \{ k \in\mathbb {T}_L : n< k \leq m \} \\ \noalign{\vspace{3pt}} z_2 & \mbox{at the set of sites } P^{n<m}_{\mathit{high}} := \mathbb{T}_L \setminus P^{n<m}_{\mathit{low}} \end{array} \right\} \quad \mbox{if } {-}M+1 \leq n < m \leq M. $$
Due to Condition S and the convention cr>c we have z2>z1 and therefore ρ2>ρ1. Hence in the definition (3.1) the first index marks the site after which the high density region Phigh begins, which extends up to site n, counted modulo L in the principal domain {−M+1,…,M}. We call site m the microscopic position of the shock and site n the microscopic position of the antishock in the shock measure of type I. In vector representation we have with \(A^{+}_{m,n} = (1+z_{1})^{2M+m-n}(1+z_{2})^{n-m}\) and \(A^{-}_{m,n} = (1+z_{2})^{2M-m+n}(1+z_{1})^{m-n}\). Tensor products with exponent 0 are defined to be absent. We remark that in terms of densities ρi=zi/(1+zi) these vectors read The unnormalized (!) restriction of \(\mu^{\mathrm{I}}_{m,n}\) to the sector with N particles is denoted by \(\mu^{\mathrm{I},N}_{m,n}\), i.e.,
$$ \big|\mu^{\mathrm{I},N}_{m,n} \big\rangle = P_N \big|\mu^{\mathrm{I}}_{m,n} \big\rangle $$
where the projector on configurations with N particles is defined by Shock measures of type I are a particular microscopic realization of a shock/antishock pair in a macroscopic step function density profile with density ρ2 in the interval [x,y) of rescaled coordinates mx, ny (modulo 1) under suitable rescaling of space. For M→∞, n→∞ and m fixed we recover the Bernoulli shock measures \(\mu^{+}_{m}\) of [13] for the ASEP defined on \(\mathbb{Z}\) fugacities z(k)=z1 for km and z(k)=z2 for k>m. In a similar fashion one can recover an antishock measure \(\mu^{-}_{n}\) by taking the thermodynamical limit such that n remains fixed and both M and m are taken to infinity.
For n=M we shall drop the second subscript and write \(\mu^{\mathrm {I}}_{m} := \mu^{\mathrm{I}}_{m,M}\) and similarly for the vectors and the projections on N particles. For n=M and mM the shock measures reduce to the usual Bernoulli product measures which we denote by
$$ |\mu_{y} \rangle = \frac{1}{(1+y)^L} \binom{1}{y} ^{\otimes L} = \binom{1-\rho}{\rho} ^{\otimes L} $$
where y=ρ/(1−ρ)∈[0,∞) is the fugacity. In particular,
$$ \big|\mu^{\mathrm{I}}_{M,M} \big\rangle \equiv\big| \mu^{\mathrm{I}}_{M} \big\rangle = |\mu_{z_1} \rangle , \quad \big| \mu^{\mathrm{I}}_{-M,M} \big\rangle \equiv\big|\mu^{\mathrm {I}}_{-M} \big\rangle = |\mu_{z_2} \rangle . $$
We stress that \(\mu^{\mathrm{I}}_{M} \neq\mu^{\mathrm{I}}_{-M}\).

We shall make use of the following transformation property.

Lemma 3.2

Let |μybe the vector representation of the Bernoulli product measure with fugacityyforLsites and\(\hat{N}_{m} = \sum_{k=m+1}^{M} \hat{n}_{k}\)be the partial number operator. Thenz1, z2∈(0,∞) andMmM
$$ \bigl|\mu^{\mathrm{I}}_{m} \bigr\rangle = \biggl( \frac{1+z_1}{1+z_2} \biggr)^{M-m} \biggl( \frac{z_2}{z_1} \biggr)^{\hat{N}_m} \bigl|\mu ^{\mathrm {I}}_{M,M} \bigr\rangle, $$
and for fixed particle numberN
$$ \bigl|\mu^{\mathrm{I},N}_{-M} \bigr\rangle = \biggl( \frac{1+z_1}{1+z_2} \biggr)^L \biggl( \frac{z_2}{z_1} \biggr)^{N} \bigl|\mu^{\mathrm{I},N}_{M,M} \bigr\rangle. $$


With the matrix representation of the number operator \(\hat{n}\) for a single site the tensor property Open image in new window and the vector representation (33) the proof of the first equality becomes elementary multilinear algebra. The second equality follows from \(\hat{N}_{-M} = \hat{N}\) and the fact that the projection on N sites can be interchanged with the number operator and that the projected vector is an eigenstate with eigenvalue N of the number operator \(\hat{N}\). □
Notice that when we work with Condition S, the family of shock measures of type I is a one-parameter family of measures indexed by z1. In particular, (39) may be written
$$ \bigl|\mu^{\mathrm{I}}_{m} \bigr\rangle = \biggl( \frac{1+z_1}{1+q^2 z_1} \biggr)^{M-m} q^{2\hat{N}_m} | \mu_{z_1} \rangle $$
and for m=−M we have the analogue of (40) for the sector of fixed N:
$$ \bigl|\mu^{\mathrm{I},N}_{-M} \bigr\rangle = \biggl( \frac{1+z_1}{1+q^2 z_1} \biggr)^{L} q^{2N} \bigl|\mu^N_{z_1} \bigr\rangle. $$

Next we introduce a new one-parameter family of shock measures which—to our knowledge—has not yet been considered in the literature.

Definition 3.3

For −M+1≤mM−1 a shock measure \(\mu^{\mathrm{II}}_{m}\) of type II on \(\mathbb{T}_{L}\) with shock at position m is a Bernoulli product measure with space-dependent fugacities
$$ z(k) = \left \{ \begin{array}{l@{\quad }l} z_1 q^{2\frac{m-M-k}{L}} & \mbox{for } {-}M < k \leq m \\[6pt] z_1 q^{2\frac{m+M-k}{L}} & \mbox{for } m < k \leq M \end{array} \right \} . $$
Furthermore, \(\mu^{\mathrm{II}}_{-M}\equiv\mu^{\mathrm{II}}_{M}\) is a Bernoulli product measure with space-dependent fugacities
$$ z(k) = z_1 q^{\frac{-2k}{L}} \quad \mbox{for } {-}M < k \leq M. $$
We write down the vector presentation of these measures
$$ \bigl|\mu^{\mathrm{II}}_{m} \bigr\rangle = \frac{1}{Z_{m}} \binom{1}{z({-M+1})} \otimes \binom{1}{z({-M+2})} \otimes\cdots \otimes \binom{1}{z(M)} $$
$$ Z_{m} = \prod_{k=-M+1}^m \bigl(1+z_1q^{2\frac{m-M-k}{L}} \bigr) \prod _{k=m+1}^M \bigl(1+z_1q^{2\frac{m+M-k}{L}} \bigr) \quad(m<n). $$
The unnormalized restrictions of these measures on the sectors with N particles are denoted \(\mu^{\mathrm{II},N}_{m}\).

Shock measures of type I and type II are related by a similarity transformation. This is the content of the following lemma.

Lemma 3.4

Assume Condition S and let
$$ U := q^{-\frac{2}{L} \sum_{k\in\mathbb{T}_L} k \hat{n}_k}. $$
Then forMmMwe have
$$ \bigl|\mu^{\mathrm{II}}_{m} \bigr\rangle = \frac{1}{Y_{m}} q^{\frac {2(m-M)}{L}\hat{N}} U \bigl|\mu^{\mathrm{I}}_{m} \bigr\rangle $$
$$ Y_{m} = \prod_{k=-M+1}^m \biggl(\frac{1+z_1q^{2\frac {m-M-k}{L}}}{1+z_1} \biggr) \prod_{k=m+1}^M \biggl(\frac{1+z_1q^{2\frac {m+M-k}{L}}}{1+q^2z_1} \biggr). $$
Moreover, for fixed particle numberN
$$ \bigl|\mu^{\mathrm{II},N}_{m} \bigr\rangle = \frac{1}{Y_{m}} q^{\frac {2(m-M)}{L}N} U \bigl|\mu^{\mathrm{I},N}_{m} \bigr\rangle. $$


Observing that \(z_{1} q^{2\frac{2M}{L}} = z_{1} q^{2} = z_{2}\) the proof works like for Lemma 3.2, but using also that not only the projector PN on N particles and the number operator \(\hat{N}\) are diagonal in the basis used throughout this work, but also the transformation U. Hence all three operations can be arbitrarily interchanged. □

To elucidate the nature of these type II shock measures we define parameters c, E through e2E:=q2, e−2Ec:=z1. Using Condition S gives z2=e−2E(c−1) and we can then express \(\mu^{\mathrm{II}}_{m}\) as a Bernoulli product measure with densities
$$ \rho(k) = \left\{ \begin{array}{l@{\quad }l} \frac{1}{2} [1 - \tanh{ (\frac{E(k+cL)}{L} )}], & {-}M < k \leq m \\ \noalign{\vspace{3pt}} \frac{1}{2} [1 - \tanh{ (\frac{E(k+(c-1)L)}{L} )} ], & m < k \leq M. \end{array} \right. $$
For hopping asymmetry q of order 1 the variation of density between neighboring sites is of order 1/L, except between site m and m+1 where there is a jump of order 1. On the other hand, for strong asymmetry with E of order L the density jumps from nearly 0 to nearly 1 at the shock position m and there is a sharp transition from nearly 1 to nearly 0, extending over a few lattice sites in the vicinity of k=−cL (modulo L). Here “nearly” means up to corrections that are exponentially small in L. This sharp transition is the microscopic analogue of an antishock in the type II shock measure which exists only for strong asymmetry. For small asymmetry the density profile is almost linear, see Fig. 1.
Fig. 1

Interpolated density profiles for type II shock measures for lattice size L=200, shock position m=10 and different asymmetries and total densities: (a) E=0.2, c=0.5, (b) E=2, c=1, (c) E=2, c=0.5, (d) E=40, c=0.3

4 Microscopic Conditioned Evolution of Shocks

4.1 Main Results

We are now in a position to state and prove our main results on the time evolution of the ASEP under conditioned dynamics, viz. for type II shocks under global conditioning, and for type I shocks under local conditioning. Throughout this section we assume Condition S to be satisfied.

Theorem 4.1

(Shock evolution under global conditioning)

Consider the ASEP on\(\mathbb{T}_{L}\)withNparticles and hopping ratescandcrto the left and to the right respectively. Let the initial distribution at timet=0 be given by the type II shock measure\(\mu^{\mathrm{II},N}_{m}\)and let\(\mu ^{\mathrm{II},N}_{m}(t)\)denote the grandcanonically conditioned distribution of the ASEP at timetunder global conditioning with weight esL=c/cr. Then for\(m \in\mathbb{T}_{L} \)and anyt≥0
$$ \mu^{\mathrm{II},N}_{m}(t) = \sum _{l=-M+1}^{M}p_t(l |m) \mu ^{\mathrm{II},N}_{l} $$
$$p_t(l|m)= e^{-(\tilde{c}_r + \tilde{c}_\ell)t} \sum_{p=-\infty}^\infty \biggl( \frac{\tilde{c}_r}{\tilde{c}_\ell} \biggr)^{(l-m+pL)/2} I_{m-l+pL}\bigl(2\sqrt{ \tilde{c}_r \tilde{c}_\ell}\, t\bigr) $$
with the modified Bessel functionIn(⋅) and\(\tilde{c}_{r} = c_{r} q^{-\frac{2N}{L}}\)and\(\tilde{c}_{\ell}= c_{\ell}q^{\frac{2N}{L}}\).

We remark that pt(l|m) is the probability that a particle that performs a continuous-time simple random walk on \(\mathbb{T}_{L}\) with hopping rates \(\tilde{c}_{r}\) to the right and \(\tilde{c}_{\ell}\) to the left, respectively, is at site l at time t, starting from site m. Hence the interpretation of (52) is that at any time t≥0 the distribution of this process is a convex combination of shock measures of a conserved microscopic structure equal to that of the initial one. The probabilistic interpretation of the weights in this convex combinations allows us to say that the shocks (or better, the shock positions) perform continuous time random walks on \(\mathbb{T}_{L}\) with hopping rates \(\tilde{c}_{r}\) (to the right) and \(\tilde{c}_{\ell}\) (to the left). Seen from the shock position the measure is invariant. As opposed to the macroscopic results of [8] our results provide exact information for any t≥0 and for finite lattice distances. Notice however, that our results require the choice esL=c/cr with arbitrary asymmetry q, while the phenomena observed in [8] are valid for any s, but require weak asymmetry.

Proof of Theorem 4.1

In order to prove (52) we observe that with (41) (which follows from (38) and (39) in Lemma 3.2) and with Lemma 3.4 we can write the initial measure
$$ \bigl|\mu^{\mathrm{II},N}_{m} \bigr\rangle = V_m \bigl| \mu^{N}_{z_1} \bigr\rangle $$
$$ V_m = \frac{1}{W} q^{\frac{2}{L} (\sum_{k=-M+1}^m (-M+m-k) \hat{n}_k + \sum_{k=m+1}^M (M+m-k) \hat{n}_k )} $$
and a non-zero normalization factor
$$ W = (1+z_1)^L \prod_{k=-M+1}^M \bigl(1+z_1 q^{-\frac{2k}{L}} \bigr) $$
that does not depend on m. We recall (8) and get for the unnormalized measure
$$ \frac{\mathrm{d}}{\mathrm{d}t} \bigl|\tilde{\mu}^{\mathrm {II},N}_{m}(t) \bigr\rangle = - V_m \tilde{H}^{(m)} \bigl|\tilde{\mu}^{N}_{z_1}(t) \bigr\rangle $$
with \(\tilde{H}^{(m)} = V_{m}^{-1} \tilde{H} V_{m}\).
Similarity transformations of the diagonal number operators on the particle creation and annihilation operators are of the form From (57) and Condition S we thus find where the prime at the summation indicates the absence of the term with i=m. We add \(-(c_{r} - c_{\ell}) (\hat{n}_{i+1} - \hat{n}_{i})\) to each term in (58) and \(-(c_{r} - c_{\ell}) (\hat{n}_{m+1} - \hat{n}_{m})\) to (59). Since the sum of these terms is zero we arrive at which we write in the form \(\tilde{H}^{(m)} = \tilde{H}^{(m)}_{b} + B^{(m)}\) with bulk term \(\tilde{H}^{(m)}_{b} = \sum^{\prime}_{i} \tilde{h}^{b}_{i}\) given by (60) and transformation term B(m) given by (61).
Using the properties of the particle creation and annihilation operators listed above it is easy to check by straightforward computation that \(h^{b}_{i} |\mu^{N}_{z_{1}} \rangle = 0\). On the other hand, \(B^{(m)} |\mu^{N}_{z_{1}} \rangle = - (c_{r}-c_{\ell}) (\hat{n}_{m+1} - \hat{n}_{m}) |\mu^{N}_{z_{1}} \rangle\). This implies \(V_{m} B^{(m)} |\mu^{N}_{z_{1}} \rangle = - (c_{r}-c_{\ell}) (\hat{n}_{m+1} - \hat{n}_{m}) V_{m} |\mu^{N}_{z_{1}} \rangle\) since Vm and the number operators \(\hat{n}_{i}\) are both diagonal and hence commute. With the projector property \(\hat{n}_{k}^{2} = \hat{n}_{k}\) one has \(q^{-2N/L} V_{m+1} = (1 + (q^{-2}-1) \hat{n}_{m+1} ) V_{m}\) and \(q^{2N/L} V_{m-1} = (1 + (q^{2}-1) \hat{n}_{m}) V_{m}\). Therefore \(c_{r} q^{-2N/L} V_{m+1} + c_{\ell}q^{2N/L} V_{m-1} - (c_{r}+c_{\ell}) V_{m} = - (c_{r}-c_{\ell}) (\hat {n}_{m+1} - \hat{n}_{m}) V_{m}\). Putting these results together yields
$$ \frac{\mathrm{d}}{\mathrm{d}t} \tilde{\mu}^{\mathrm{II},N}_{m}(t) = c_r q^{-\frac{2N}{L}} \tilde{\mu}^{\mathrm{II},N}_{m+1}(t) + c_l q^{\frac{2N}{L}} \tilde{\mu}^{\mathrm{II},N}_{m-1}(t) - (c_r+c_\ell) \tilde{\mu }^{\mathrm{II},N}_{m}(t) $$
for any \(m\in\mathbb{T}_{L}\) and any t≥0.
Next we compute the time derivative of the normalization \(R_{m}(t) = \langle s| \mathrm{e}^{-\tilde{H} t} |\mu^{\mathrm {II},N}_{m} \rangle\). Using (62) we get where the last line follows from translation invariance. Therefore which implies the system of linear ODE’s Now it only remains to show that (52) satisfies this system of ODE’s with the initial condition \(\mu^{\mathrm{II}}_{m}(0) = \mu^{\mathrm{II}}_{m}\). It is elementary that the random walk transition probability of the theorem satisfies the forward evolution equation with initial condition p0(l|m)=δl,m. The theorem thus follows from translation invariance pt(l+r|m+r)=pt(l|m) \(\forall r \in\mathbb{Z}\) and periodicity pt(l+pL|m)=pt(l|m) \(\forall p \in\mathbb{Z}\) of the transition probability. □

Corollary 4.2

The unique stationary grandcanonically conditioned measure
$$ \mu^{\mathrm{II}^\ast,N} := \lim_{t\to\infty} \mu^{\mathrm {II},N}_m(t) = \frac{1}{L} \sum_{l=-M+1}^{M} \mu^{\mathrm{II},N}_{l} $$
is the uniform mixture of the initial shock measures\(\mu^{\mathrm {II},N}_{l}\), \(l\in\mathbb{T}_{L}\). The approach to stationary is exponential with a relaxation time that grows asymptotically with system size proportional toL2.

This corollary is a simple consequence of the fact that the shock position performs a continuous-time random walk on \(\mathbb{T}_{L}\).

Theorem 4.3

(Shock/antishock evolution under local conditioning)

Let the initial distribution of the ASEP withNparticles be given by the type I shock measure\(\mu^{\mathrm{I},N}_{m}\)satisfying Condition S with shock at bondmand antishock at bondMand let\(\tilde{\mu}^{\mathrm{I},N}_{m}(t)\)denote the unnormalized grandcanonically conditioned measure at timetunder local conditioning at bondMwith weight es=c/cr. Then we havet≥0
$$ \tilde{\mu}^{\mathrm{I},N}_m(t) = \mathrm{e}^{(\tilde{c}_r + \tilde {c}_\ell- c_r - c_\ell)t} \sum_{l=-M+1}^{M}p_t(l |m) \delta^{l-m} q^{\frac{2N(l-m)}{L}} \mu ^{\mathrm{I},N}_{l} $$
withpt(l|m) defined in (4.1) and\(\delta=\frac {1+z_{1}}{1+q^{2}z_{1}}\).


First we consider the evolution of unnormalized measures \(\tilde{\mu}^{\mathrm{I},N}_{m}(t)\). By construction (described informally in Sect. 2) the matrix \(\tilde{H}^{M}\) defined by (58) and boundary term BM given by (59) is the generator for the grandcanonically conditioned evolution under local conditioning at bond (M,−M+1) with weight es=c/cr. Therefore \(\mathrm{d}/\mathrm{d}t |\tilde{\mu}^{\mathrm{I},N}_{m} \rangle = - \tilde{H}^{M} |\tilde{\mu}^{\mathrm{I},N}_{m} \rangle\). Notice next that U=WVM where U is defined in (47) and VM is defined in (54). Therefore we may write \(\tilde{H}^{M} = U^{-1} \tilde{H} U\) and we have by Theorem 4.1 in conjunction with Lemma 3.4
From (49) we have Ym/Ym+1=(1+z1)/(1+z2) and therefore
For m=M we have Straightforward computation yields YM/YM+1=[(1+z2)/(1+z1)]L−1.
For m=−M we use Lemma 3.2. This yields

From (70)–(73) one finds that the transformed measure \(|\tilde{\nu}^{\mathrm{I},N}_{m} \rangle(t) = \delta^{m} q^{2Nm/L} |\tilde{\mu}^{\mathrm{I},N}_{m} \rangle(t)\) satisfies the system of linear ODE’s (62). Hence, by the same arguments as used in Theorem 4.1 we obtain (68). □

Corollary 4.4

The normalized grandcanonically conditioned measure at timetof Theorem 4.3 \(\mu^{\mathrm {I},N}_{m}(t)\)is of the form
$$ \mu^{\mathrm{I},N}_m(t) = \frac{1}{C(t)} \sum_{l=-M+1}^{M}p_t(l |m) \delta^{l-m} q^{\frac{2N(l-m)}{L}} \mu ^{\mathrm{I},N}_{l} $$
with a normalization constant\(C(t) = \sum_{l=-M+1}^{M}p_{t}(l |m) \delta^{l-m} q^{\frac{2N(l-m)}{L}} \langle s | \mu^{\mathrm{I},N}_{l} \rangle\)that is strictly positive and finite for allt≥0. In particular, with\(C^{\ast}:= \sum_{l=-M+1}^{M} \delta^{l-m} q^{\frac{2N(l-m)}{L}} \langle s | \mu^{\mathrm{I},N}_{l} \rangle\),
$$ \mu^{\mathrm{I}^\ast,N}_m := \lim _{t\to\infty} \mu^{\mathrm {I},N}_m(t) = \frac{1}{C^\ast} \sum_{l=-M+1}^{M} \delta^{l-m} q^{\frac{2N(l-m)}{L}} \mu^{\mathrm{I},N}_{l} $$
is the unique stationary conditioned limiting measure.

The properties of C(t) are obvious from the fact it is a transition probability for a random walk with unnormalized positive initial distribution and that the random walk propagator on \(\mathbb{T}_{L}\) satisfies limt→∞pt(l|m)=1/L\(\forall l,m \in\mathbb{T}_{L}\). The uniqueness of the measure follows from the Perron-Frobenius theorem for the weighted generator.  □

We remark that due to the boundary conditions (72), (73) there is no simple random walk interpretation of the shock position in a finite system under locally conditioned dynamics. However, the system of Eqs. (70), (72), (73) is straightforwardly diagonalized by lattice Fourier transformation and yields an exponential relaxation with asymptotically finite relaxation time approaching \(1/(\tilde{c}_{r} + \tilde{c}_{\ell}- c_{r} - c_{\ell})\) as system size L tends to infinity.

5 Final Remarks

Our results are exact results on the lattice scale and for finite times. With regard to the macroscopic large-deviation theory of [8] Theorem 4.1 suggests that there exists a value of s(ν) such that the optimal macroscopic density profile obtained from the large-deviation theory of [8] in the limit ν→∞ is of the form ρ(x,t)=1/2[1−tanh(E(x+avt))] with speed v=crexp(−2ρs)−cexp(2ρs) and a jump discontinuity at some point x(t) that also travels with speed v. The stationary solution in Theorem 4.3 for local conditioning with weight es=c/cr indicates the existence of an antishock that remains microscopically sharp and does not fluctuate. This behavior is in sharp contrast to the typical behavior of the ASEP where an antishock evolves into a rarefaction wave.

The evolution of the shock initial measures as a one-particle random walk indicates a self-duality relation of the conditioned ASEP with periodic boundary conditions, which is absent for the unconditioned dynamics. From a Bethe-ansatz perspective it is interesting to note that (52) can be understood as an exact resummation of a whole family of special Bethe eigenvectors where the Bethe roots are carried by the particles themselves [9, 19]. Furthermore, results from [13] for the microscopic dynamics of more than one shock, each satisfying Condition S, and properties of the underlying representation theory of the quantum group Uq[SU(2)] for periodic systems [22] suggests that one may study the behavior of shock/antishock measures with several shocks under global and local conditioning. One then expects the evolution of n shocks to be given by the dynamics of n interacting particles. The results of [14] might then provide information about more general solutions of the large deviation theory and about their fluctuations.



G.M.S. thanks FAPESP for financial support and IME at the University of São Paulo for kind hospitality. V.B. acknowledges financial support of FAPESP and CNPq.


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Copyright information

© Springer Science+Business Media New York 2013

Authors and Affiliations

  1. 1.Instituto de Matemática e EstatísticaUniversidade de São PauloSão PauloBrazil
  2. 2.Institute of Complex Systems IIForschungszentrum Jülich GmbHJülichGermany
  3. 3.Interdisziplinäres Zentrum für komplexe SystemeUniversität BonnBonnGermany

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