Gravitational Collapse of a Shell of Quantized Matter

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dc.creatorAlberghi, G. L.
dc.creatorCasadio, R.
dc.creatorVacca, G. P.
dc.creatorVenturi, G.
dc.date1998-08-10
dc.date1998-08-11
dc.date.accessioned2026-07-07T11:46:26Z
dc.date.available2026-07-07T11:46:26Z
dc.descriptionThe semi-classical collapse, including lowest order back-reaction, of a thin shell of self-gravitating quantized matter is illustrated. The conditions for which self-gravitating matter forms a thin shell are first discussed and an effective Lagrangian for such matter is obtained. The matter-gravity system is then quantized, the semi-classical limit for gravitation is taken and the method of adiabatic invariants is applied to the resulting time dependent matter Hamiltonian. The governing equations are integrated numerically, for suitable initial conditions, in order to illustrate the effect of back-reaction, due to the creation of matter, in slowing down the collapse near the horizon.
dc.description20 pages, 1 eps figure. Problem with figure fixed
dc.identifierhttps://arxiv.org/abs/gr-qc/9808026
dc.identifierhttp://arxiv.org/abs/gr-qc/9808026
dc.identifierClass.Quant.Grav.16:131-147,1999
dc.identifierdoi:10.1088/0264-9381/16/1/010
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/202228
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleGravitational Collapse of a Shell of Quantized Matter
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