Black holes in Tolman-Bondi spacetimes

Journal Article · Fri Apr 20 00:00:00 EDT 1990 · Modern Physics Letters A; (USA)

DOI:https://doi.org/10.1142/S0217732390000810· OSTI ID:6592667

Gorini, V ^[1]; Grillo, G ^[2]; Pelizza, M ^[3]

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1. Dipartimento di Fisica, Gruppo Teorico, Via Amendoal 173, 70126 Bari, Italy and INFN, Sezione di Bari (IT)
2. International School for Advanced Studies, Strada Costiera 11, 34100 Miramare-Grignano, Trieste (IT)
3. Dipartimento di Fisica, Sezione di Fisica Teorica, Via Celoria 16, 20133 Milano (IT)

The authors show that the significant Tolman-Bondi metrics originated by a synchronous big bang can be divided, according to the initial conditions, into three classes. The elements of one of these classes give the dynamical description of the formation of a black hole in the background of an expanding universe.

• OSTI ID: 6592667
• Journal Information: Modern Physics Letters A; (USA), Vol. 5:10; ISSN 0217-7323
• Country of Publication: United States
• Language: English

Related Subjects

71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
BLACK HOLES
ORIGIN
UNIVERSE
GRAVITATIONAL COLLAPSE
SPACE-TIME
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Radio & X-Ray Sources
640106 - Astrophysics & Cosmology- Cosmology