Gravitational collapse of a radiating shell and radiation bursts

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dc.creatorCasadio, Roberto
dc.date2001-07-02
dc.date.accessioned2026-07-07T03:26:03Z
dc.date.available2026-07-07T03:26:03Z
dc.descriptionWe study the collapse of a self-gravitating thick shell of bosons coupled to a scalar radiation field. Due to the non-adiabaticity of the collapse, the shell (quantum) internal degrees of freedom absorb energy from the (classical) gravitational field and are excited. The excitation energy is then emitted in the form of bursts of (thermal) radiation and the corresponding backreaction on the trajectory is estimated.
dc.descriptionLaTeX2e with Rinton style, 4 pages, 2 figure EPS files, to appear in the Proceedings of PASCOS 2001
dc.identifierhttps://arxiv.org/abs/gr-qc/0107006
dc.identifierhttp://arxiv.org/abs/gr-qc/0107006
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/33945
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.subjectHigh Energy Physics - Theory
dc.titleGravitational collapse of a radiating shell and radiation bursts
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