Zusammenfassung
Over the last decades, many methods were developed to prove Hawking
radiation. Recently, a semiclassical method known as the tunneling
method has been proposed as a more straightforward way of derivating
black hole thermodynamical properties. This method has been widely
applied to a vast sort of spacetimes with satisfactory results. In this
work, we obtain the black hole thermodynamics in the presence of a
Lorentz symmetry breaking (LSB). We apply the Hamilton-Jacobi method to
Schwarzschild-like black holes, and we investigate whether the LSB
affects their thermodynamics. The results found show that the LSB not
only changes the black hole thermodynamic quantities but also makes it
necessary to modify the standard first law of thermodynamics. (C) 2020
Elsevier Inc. All rights reserved.
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