Electronic Resource
Springer
General relativity and gravitation
8 (1977), S. 7-13
ISSN:
1572-9532
Source:
Springer Online Journal Archives 1860-2000
Topics:
Physics
Notes:
Abstract It has been thought that mini-black-holes could only be formed in the very early stages of a big-bang universe. We show how they can be formingtoday in the cores of condensed, stellar-mass objects. The unique interactions of such “contemporary mini-black-holes” with their environment, their courses of evolution, and their astrophysical implications are then described briefly. These latter effects are critically dependent upon the existence of Hawking's “quantum evaporation” process for black holes. A rich and challenging new fieldmini—black-hole physics-is thereby introduced.
Type of Medium:
Electronic Resource
URL:
http://dx.doi.org/10.1007/BF00763468
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