Thermodynamics of Schwarzschild-like black holes in bumblebee gravity models

Over the last decades, many methods were developed to prove Hawking radiation. Recently, a semiclassical method known as tunneling method, has been proposed as a simpler way of derivating black hole thermodynamical properties. This method has been widely applied to a huge 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 changes the Schwarzschild black hole temperature, entropy and heat capacity by perturbative terms of the LSB parameter.