Bubbles with an O(3) Symmetric Scalar Field in Curved Spacetime

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dc.creatorSakai, Nobuyuki
dc.creatorKim, Yoonbai
dc.creatorMaeda, Kei-ichi
dc.date1995-12-28
dc.date.accessioned2026-07-07T04:21:47Z
dc.date.available2026-07-07T04:21:47Z
dc.descriptionWe study the first-order phase transition in a model of scalar field with $O(3)$ symmetry coupled to gravity, and, in high temperature limit, discuss the existence of new bubble solution with a global monopole at the center of the bubble.
dc.description3 pages, latex, uuencoded postscript figures; talk given at 7th Marcel Grossmann Meeting on General Relativity, Stanford University, July 24-29, 1994
dc.identifierhttps://arxiv.org/abs/hep-th/9512213
dc.identifierhttp://arxiv.org/abs/hep-th/9512213
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/54465
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleBubbles with an O(3) Symmetric Scalar Field in Curved Spacetime
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