Radiation from perfect mirrors starting from rest and the black body spectrum

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dc.creatorCalogeracos, A.
dc.date2001-10-01
dc.date2002-03-21
dc.date.accessioned2026-07-07T10:51:48Z
dc.date.available2026-07-07T10:51:48Z
dc.descriptionWe address the question of radiation emission from a perfect mirror that starts from rest and follows the trajectory z=-ln(cosht) till t->Infinity. We show that a correct derivation of the black body spectrum via the calculation of the Bogolubov amplitudes requires consideration of the whole trajectory and not just of its asymptotic part.
dc.descriptionTypos corrected
dc.identifierhttps://arxiv.org/abs/gr-qc/0110010
dc.identifierhttp://arxiv.org/abs/gr-qc/0110010
dc.identifierJ.Phys.A35:3435-3446,2002
dc.identifierdoi:10.1088/0305-4470/35/15/306
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/184947
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectQuantum Physics
dc.titleRadiation from perfect mirrors starting from rest and the black body spectrum
dc.typetext

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