On a Quasi-Local Energy Outside the Cosmological Horizon

dc.creatorNakao, Ken-ichi
dc.date1995-07-11
dc.date.accessioned2026-07-07T03:30:44Z
dc.date.available2026-07-07T03:30:44Z
dc.descriptionWe investigate a quasi-local energy naturally introduced by Kodama's prescription for a spherically symmetric space-time with a positive cosmological constant $Λ$. We find that this quasi-local energy is well behaved inside a cosmological horizon. However, when there is a scalar field with a long enough Compton wavelength, the quasi-local energy diverges in the course of its time evolution outside the cosmological horizon. This means that the quasi-local energy has a meaning only inside the cosmological horizon.
dc.description5 pages, uuencode compressed latex
dc.identifierhttps://arxiv.org/abs/gr-qc/9507022
dc.identifierhttp://arxiv.org/abs/gr-qc/9507022
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/35623
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleOn a Quasi-Local Energy Outside the Cosmological Horizon
dc.typetext

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