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Vacuum polarization near a distorted black hole

✍ Scribed by V.P. Frolov; Alberto García D.

Publisher
Elsevier Science
Year
1983
Tongue
English
Weight
175 KB
Volume
99
Category
Article
ISSN
0375-9601

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Let a scalar charged field with the Lagrangian interact with the gravitational field described by the liobertson-Walker mctric. Here, F(p \* p) is an arbitrary self-coupling function. Proposition 2. The U(r)-gaugc symmetry 01 the ficld (2) is spoiitancously hrokcn if I ) the evolution of the univer