An outline of approach linking black-hole-evaporation with quantum-field effects in flat spacetime

Details An outline of approach linking black-hole-evaporation with quantum-field effects in flat spacetime An outline of approach linking black-hole-evaporation with quantum-field effects in flat spacetime

Mar 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983ap%26ss..91...53n&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 91, no. 1, March 1983, p. 53-62.

Astronomy and Astrophysics

Astronomy

3

Black Holes (Astronomy), Evaporation, Field Theory (Physics), Gravitational Collapse, Quantum Theory, Black Body Radiation, Electromagnetic Fields, Scalars, Space-Time Functions

Scientific paper

The results of various calculations of the Casimir effect and of the effect of particle creation by accelerated mirrors are applied to the case of a collapse-formed black hole, which in consequence produces black-body radiation. Its temperature coincides exactly with Hawking's result. The difference between the vacuum expectation values of the energy-momentum tensors of scalar and electromagnetic fields near the horizon is found. Further investigation of expanding spheres in flat-space-time should disclose where the radiation is being created and what happens near the horizon.

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