The expansive nondecelerative universe - Gravitational effects and their manifestation in black holes evaporation and far-infrared spectra

Simple item page
dc.creatorSima, Jozef
dc.creatorSukenik, Miroslav
dc.date1999-03-24
dc.date.accessioned2026-07-07T03:33:05Z
dc.date.available2026-07-07T03:33:05Z
dc.descriptionThe paper summarizes the background of Expensive Nondecelerative Universe model and its main consequences for gravitation. Applying the Vaidya metrics, the model allows for the localization and determination of the density and quantity of gravitational energy created by a body with the mass m in the distance r. The consequences are manifested both in a macrosystem (Hawking's phenomenon of black holes evaporation) and microworld phenomenon (far-infrared spectral properties)
dc.description7 pages, AmsTex
dc.identifierhttps://arxiv.org/abs/gr-qc/9903090
dc.identifierhttp://arxiv.org/abs/gr-qc/9903090
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36479
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleThe expansive nondecelerative universe - Gravitational effects and their manifestation in black holes evaporation and far-infrared spectra
dc.typetext

Files

Collections

arXiv