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
β¦ LIBER β¦
Vacuum polarization near the horizon of a black hole in the presence of boundaries
β Scribed by T. Elster
- Publisher
- Elsevier Science
- Year
- 1982
- Tongue
- English
- Weight
- 166 KB
- Volume
- 93
- Category
- Article
- ISSN
- 0375-9601
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