Topological Defect Inflation

dc.creatorSakai, Nobuyuki
dc.date1999-12-31
dc.date2000-01-01
dc.date.accessioned2026-07-07T03:33:50Z
dc.date.available2026-07-07T03:33:50Z
dc.descriptionWe address some issues of topological defect inflation. (1) We clarify the causal structure of an inflating magnetic monopole. The spacetime diagram shows explicitly that this model is free from the ``graceful exit'' problem, while the monopole itself undergoes ``eternal inflation''. (2) We extend the study of inflating topological defects to Brans-Dicke gravity. Contrary to the case of Einstein gravity, any inflating monopole eventually shrinks and takes a stable configuration. (3) We reanalyze chaotic inflation with a non-minimally coupled massive scalar field. We find a new solution of domain wall inflation, which relaxes constraints on the coupling constant for successful inflation.
dc.description8 pages, latex, 6 ps figures included, talk given at 9th Workshop on General Relativity and Gravitation, Hiroshima, Nov 1999
dc.identifierhttps://arxiv.org/abs/gr-qc/9912121
dc.identifierhttp://arxiv.org/abs/gr-qc/9912121
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/36732
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleTopological Defect Inflation
dc.typetext

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