Unification of Dark Matter and Dark Energy: the Inhomogeneous Chaplygin Gas

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dc.creatorBilic, Neven
dc.creatorTupper, Gary B.
dc.creatorViollier, Raoul D.
dc.date2001-11-16
dc.date2002-01-25
dc.date.accessioned2026-07-07T11:08:02Z
dc.date.available2026-07-07T11:08:02Z
dc.descriptionWe extend the world model of Kamenshchik et al. to large perturbations by formulating a Zeldovich-like approximation. We sketch how this model unifies dark matter with dark energy in a geometric setting reminiscent of M-theory.
dc.description10 pages, 1 figure, one sentence changed in text, acknwledgement expanded
dc.identifierhttps://arxiv.org/abs/astro-ph/0111325
dc.identifierhttp://arxiv.org/abs/astro-ph/0111325
dc.identifierPhys.Lett.B535:17-21,2002
dc.identifierdoi:10.1016/S0370-2693(02)01716-1
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/190004
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Phenomenology
dc.titleUnification of Dark Matter and Dark Energy: the Inhomogeneous Chaplygin Gas
dc.typetext

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