2001/02/28 by G. L. Alberghi, R. Casadio, Roberto Casadio +3 · 2 citations
Physics and Astronomy · #Black Holes and Theoretical Physics #Classical mechanics #Cosmology and Gravitation Theories #Excited state #Geometry #Gravitation #Gravitational collapse #Gravitational field #Massless particle #Physics #Quantum #Quantum Electrodynamics and Casimir Effect #Quantum electrodynamics #Quantum mechanics #Scalar (mathematics) #Scalar field #Semiclassical physics #Shell (structure) #astro-ph #gr-qc #hep-ph #hep-th
paper · pdf · doi:10.1103/physrevd.64.104012
published as Phys.Rev.D64:104012,2001 · LaTeX, 34 pages, 21 EPS figures included
arxiv created 2001/08/31 · openalex publication_date 2001/10/19 · arxiv updated 2009/11/30 · openalex created_date 2025/10/10 · openalex updated_date 2026/08/05
We study the collapse of a self-gravitating and radiating shell of bosonic matter. The matter constituting the shell is quantized and the construction is viewed as a semiclassical model of possible black hole formation. It is shown that the shell internal degrees of freedom are excited by the quantum nonadiabaticity of the collapse and, consequently, on coupling them to a massless scalar field, the collapsing matter emits a burst of coherent (thermal) radiation. The back reaction on the trajectory is also estimated.