The charged black hole in a cosmological context

Miscellaneous · Tue Jan 01 00:00:00 EST 1991

OSTI ID:5184070

Bruno, R V

The structure of the space time obtained from the embedding of the region between the event horizon and the Cauchy horizon of the Reissner-Nordstrom solution in a closed cosmology is investigated. It is shown that this model incorporates the spherically symmetric solution of the coupled Einstein and Maxwell's equations in a cosmological model in the same way a similar construction by Qadir and Wheeler incorporates the Schwarzschild solution in a cosmological model with S{sup 3} topology. The fate of the suture universe obtained is discussed.

• Research Organization: Texas Univ., Austin, TX (United States)
• OSTI ID: 5184070
• Resource Relation: Other Information: Thesis (Ph.D)
• Country of Publication: United States
• Language: English

Related Subjects

71 CLASSICAL AND QUANTUM MECHANICS
GENERAL PHYSICS
BLACK HOLES
COSMOLOGY
SPACE-TIME
EINSTEIN-MAXWELL EQUATIONS
SCHWARZSCHILD METRIC
CAUCHY PROBLEM
EQUATIONS
FIELD EQUATIONS
METRICS
640102* - Astrophysics & Cosmology- Stars & Quasi-Stellar
Radio & X-Ray Sources
640106 - Astrophysics & Cosmology- Cosmology