BLACK HOLE NONEXTENSIVE ENTROPY: FORMATION PROCESSES SIGNALIZED BY GRAVITATIONAL WAVE EMISSION
2008 ◽
Vol 17
(03n04)
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pp. 541-544
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Keyword(s):
We show that gravitational wave emission, both in the linear approximation and in the full nonlinear regime of general relativity, gives a hint of black hole thermodynamic processes by which a black hole evolves emitting part of its perturbation in the form of gravitational waves and absorbing the remnant, reaching a final configuration with a larger entropy. The partition of energy in this process is constrained by the maximum entropy principle, and the final entropy obtained numerically is given as a distribution function of the efficiency of the process. The distribution function is in the realm of nonextensive thermostatistics with entropic index q ≃ 1/2, a result that is validated analytically by the linear approximation.
2010 ◽
Vol 726
(1)
◽
pp. L14
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Keyword(s):
2017 ◽
Vol 36
(5)
◽
pp. 1480-1489
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2014 ◽
Vol 23
(10)
◽
pp. 1430022
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2012 ◽
Vol 605-607
◽
pp. 806-810
2007 ◽
Vol 48
(4)
◽
pp. 1140-1149
◽
2016 ◽
Vol 12
(S324)
◽
pp. 291-294
Keyword(s):
2016 ◽
Vol 12
(S324)
◽
pp. 99-106
Keyword(s):
2013 ◽
Vol 14
(4)
◽
pp. 306-317
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Keyword(s):