dc.creator | Wreszinski, Walter Felipe | |
dc.date.accessioned | 2012-10-20T04:06:58Z | |
dc.date.accessioned | 2018-07-04T15:40:09Z | |
dc.date.available | 2012-10-20T04:06:58Z | |
dc.date.available | 2018-07-04T15:40:09Z | |
dc.date.created | 2012-10-20T04:06:58Z | |
dc.date.issued | 2010 | |
dc.identifier | JOURNAL OF STATISTICAL PHYSICS, v.138, n.4/Mai, p.567-578, 2010 | |
dc.identifier | 0022-4715 | |
dc.identifier | http://producao.usp.br/handle/BDPI/29266 | |
dc.identifier | 10.1007/s10955-009-9889-8 | |
dc.identifier | http://dx.doi.org/10.1007/s10955-009-9889-8 | |
dc.identifier.uri | http://repositorioslatinoamericanos.uchile.cl/handle/2250/1625906 | |
dc.description.abstract | We consider random generalizations of a quantum model of infinite range introduced by Emch and Radin. The generalizations allow a neat extension from the class l (1) of absolutely summable lattice potentials to the optimal class l (2) of square summable potentials first considered by Khanin and Sinai and generalised by van Enter and van Hemmen. The approach to equilibrium in the case of a Gaussian distribution is proved to be faster than for a Bernoulli distribution for both short-range and long-range lattice potentials. While exponential decay to equilibrium is excluded in the nonrandom l (1) case, it is proved to occur for both short and long range potentials for Gaussian distributions, and for potentials of class l (2) in the Bernoulli case. Open problems are discussed. | |
dc.language | eng | |
dc.publisher | SPRINGER | |
dc.relation | Journal of Statistical Physics | |
dc.rights | Copyright SPRINGER | |
dc.rights | restrictedAccess | |
dc.subject | Approach to equilibrium | |
dc.subject | Non-Markovian | |
dc.subject | Random systems | |
dc.subject | Exponential versus non-exponential decay | |
dc.subject | Gaussian and Bernoulli distributions | |
dc.subject | State-dependent Heisenberg time-evolution | |
dc.title | Approach to Equilibrium for a Class of Random Quantum Models of Infinite Range | |
dc.type | Artículos de revistas | |