ANTIGRAVITATING BUBBLES

dc.creatorBarnaveli, Andro
dc.creatorGogberashvili, Merab
dc.date1995-05-30
dc.date.accessioned2026-07-07T03:57:40Z
dc.date.available2026-07-07T03:57:40Z
dc.descriptionWe investigate the gravitational behavior of spherical domain walls (bubbles) arising during the phase transitions in the early Universe. In the thin-wall approximation we show the existence of the new solution of Einstein equations with negative gravitational mass of bubbles and the reversed direction of time flow on the shell. This walls exhibit gravitational repulsion just as the planar walls are assumed to do. The equilibrium radius and critical mass of such objects are found for realistic models.
dc.descriptionLATEX, 26 pages, no macros, no figures, short version was published in: GRG 26 (1994) 1117
dc.identifierhttps://arxiv.org/abs/hep-ph/9505412
dc.identifierhttp://arxiv.org/abs/hep-ph/9505412
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/45525
dc.subjectHigh Energy Physics - Phenomenology
dc.titleANTIGRAVITATING BUBBLES
dc.typetext

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