Spherical Domain Wall formed by Field Dynamics of Hawking Radiation and Structure Near Horizon

Simple item page
dc.creatorNagatani, Yukinori
dc.date2003-07-30
dc.date.accessioned2026-07-07T04:15:34Z
dc.date.available2026-07-07T04:15:34Z
dc.descriptionThe Hawking radiation in the vacuum of the spontaneous symmetry breaking in the gauge-Higgs-Yukawa theory is investigated by a general relativistic formulation of the the ballistic model. The restoration of the symmetry on the horizon and the formation of the spherical domain wall around the black hole are shown even if the Hawking temperature is lower than the critical temperature of the phase transition in the gauge-Higgs-Yukawa theory. When the Hawking temperature is much lower than the critical temperature, the domain wall closely near the horizon is formed. The wall is formed by the field dynamics rather than the thermal phase transition.
dc.description42 pages, 15 figures, LaTeX2e with graphicx and latexsym macros
dc.identifierhttps://arxiv.org/abs/hep-th/0307295
dc.identifierhttp://arxiv.org/abs/hep-th/0307295
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/52051
dc.subjectHigh Energy Physics - Theory
dc.titleSpherical Domain Wall formed by Field Dynamics of Hawking Radiation and Structure Near Horizon
dc.typetext

Files

Collections

arXiv