Physics – General Physics
Scientific paper
2009-11-05
Physics
General Physics
11 pages, no figures
Scientific paper
In this work we present a simplified description and calculation of the Kerr-Newman black hole basic dynamical (horizons) and thermo-dynamical (Bekenstein-Hawking entropy, Bekenstein entropy/surface quantization, Hawking temperature and radiation) characteristics. Also, a possibility of the fission of nearly extremal black hole is considered in full analogy with remarkable, simple Bohr-Wheeler theory of the nuclear fission. Given black is physically based on the well-known principles of the classical physics (mechanics, thermodynamics and electro-dynamics). It includes the non-relativistic quantum mechanics and statistical mechanics too. Finally, it includes the elementary form of the general relativistic equivalence principle only. Also, suggested simplified description includes mathematically, practically, only simple algebraic equations. Here many steps are extremely simplified and formal, representing, in fact, a linear approximation of the quantum gravity theories (black hole entropy and temperature can be obtained by ground standing wave at horizon, while Hawking radiation can be obtained by gravitational decay of this standing wave in its traveling components). But, the final results, i.e. formulas on the black hole basic characteristics, are mostly effectively identical to corresponding results obtained by accurate quantum gravity theories. In this way suggested description can be very useful for the quantum gravity non-specialists.
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