On the Energy Increase in Space-Collapse Models

dc.creatorBassi, Angelo
dc.creatorIppoliti, Emiliano
dc.creatorVacchini, Bassano
dc.date2005-06-10
dc.date.accessioned2026-07-07T06:19:58Z
dc.date.available2026-07-07T06:19:58Z
dc.descriptionA typical feature of spontaneous collapse models which aim at localizing wavefunctions in space is the violation of the principle of energy conservation. In the models proposed in the literature the stochastic field which is responsible for the localization mechanism causes the momentum to behave like a Brownian motion, whose larger and larger fluctuations show up as a steady increase of the energy of the system. In spite of the fact that, in all situations, such an increase is small and practically undetectable, it is an undesirable feature that the energy of physical systems is not conserved but increases constantly in time, diverging for $t \to \infty$. In this paper we show that this property of collapse models can be modified: we propose a model of spontaneous wavefunction collapse sharing all most important features of usual models but such that the energy of isolated systems reaches an asymptotic finite value instead of increasing with a steady rate.
dc.description14 pages, revtex, no figures
dc.identifierhttps://arxiv.org/abs/quant-ph/0506083
dc.identifierhttp://arxiv.org/abs/quant-ph/0506083
dc.identifierJ. Phys. A: Math. Gen. 38 (2005) 8017-8038
dc.identifierdoi:10.1088/0305-4470/38/37/007
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/95212
dc.subjectQuantum Physics
dc.titleOn the Energy Increase in Space-Collapse Models
dc.typetext

Files

Collections