Quasi-local energy for cosmological models

dc.creatorChen, Chiang-Mei
dc.creatorLiu, Jian-Liang
dc.creatorNester, James M.
dc.date2007-05-08
dc.date2007-05-15
dc.date.accessioned2026-07-07T11:20:34Z
dc.date.available2026-07-07T11:20:34Z
dc.descriptionFirst we briefly review our covariant Hamiltonian approach to quasi-local energy, noting that the Hamiltonian-boundary-term quasi-local energy expressions depend on the chosen boundary conditions and reference configuration. Then we present the quasi-local energy values resulting from the formalism applied to homogeneous Bianchi cosmologies. Finally we consider the quasi-local energies of the FRW cosmologies. Our results do not agree with certain widely accepted quasi-local criteria.
dc.descriptionContributed to International Symposium on Cosmology and Particle Astrophysics (CosPA 2006), Taipei, Taiwan, 15-17 Nov 2006
dc.identifierhttps://arxiv.org/abs/0705.1080
dc.identifierhttp://arxiv.org/abs/0705.1080
dc.identifierMod.Phys.Lett.A22:2039-2046,2007
dc.identifierdoi:10.1142/S0217732307025285
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/193997
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleQuasi-local energy for cosmological models
dc.typetext

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