Nonrelativistic Dark-Energy Fluid in a Baby Universe

Simple item page
dc.creatorStichel, P. C.
dc.creatorZakrzewski, W. J.
dc.date2008-07-23
dc.date.accessioned2026-07-07T09:52:21Z
dc.date.available2026-07-07T09:52:21Z
dc.descriptionWe show that the dynamical realization of the acceleration-enlarged Galilean symmetry leads to nonrelativistic massless particles whose energy may be negative. We present a fluid mechanical generalisation of this observation and use it to contruct a nonrelativistic two-dimensional fluid model which possesses solutions with a negative energy density. Considering this model as describing dark energy in a baby universe (two space dimensions) we show that its negative energy density leads to a repulsive gravitational interaction of the fluid with any test body.
dc.identifierhttps://arxiv.org/abs/0807.3660
dc.identifierhttp://arxiv.org/abs/0807.3660
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/165569
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Theory
dc.titleNonrelativistic Dark-Energy Fluid in a Baby Universe
dc.typetext

Files

Collections

arXiv