Emergence of classicality in non relativistic quantum mechanics through gravitational self-interaction

Simple item page
dc.creatorDe Filippo, Sergio
dc.date2001-04-10
dc.date.accessioned2026-07-07T06:01:54Z
dc.date.available2026-07-07T06:01:54Z
dc.descriptionAn explicit dynamical model for non relativistic quantum mechanics with an effective gravitational interaction is proposed, which, as being well defined, allows in principle for the evaluation of every physical quantity. Its non unitary dynamics results from a unitary one in a space with twice as many degrees of freedom as the ordinary ones. It exhibits a threshold for the emergence of classical behavior for bodies of ordinary density on rather long times or instantaneously, respectively at around 10^11 or 10^20 proton masses.
dc.identifierhttps://arxiv.org/abs/quant-ph/0104052
dc.identifierhttp://arxiv.org/abs/quant-ph/0104052
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/89426
dc.subjectQuantum Physics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleEmergence of classicality in non relativistic quantum mechanics through gravitational self-interaction
dc.typetext

Files

Collections

arXiv