It is not an exaggeration to say that one of the most exciting predictions of Einstein's theory of gravitation is that there may exist "black holes": putative objects whose gravitational fields are so strong that no physical bodies or ...
For this state, the average number of B-quanta out-going from the horizon is described by the thermal distribution, i.e., the particle number per mode n = [exp(w/6) – 1]", (4.84) where, 6 = k/2T, is the black hole temperature.
Frolov (physics, U. of Alberta) and Novikov (theoretical astrophysics, U. of Copenhagen) focus on questions that have been answered relatively recently.
The book covers the rest of the needed background material in the main text or the appendices. This textbook gradually introduces the reader to several topics related to black hole physics with a didactic approach.
In these last years Black hole Physics has developed rapidly both from theoretical and observational aspects: especially as regards quantum aspects many things must be clarified as for instance the...