AbstractSome authors have recently found that the tunneling approach gives a different Hawking temperature for a Schwarzschild black hole in a different coordinate system. In this Letter, we find that to work out the Hawking temperature in a different coordinate system by the tunneling approach, we must use the correct definition of the energy of the radiating particles. By using a new definition of the particle energy, we obtain the correct Hawking temperature for a Schwarzschild black hole in two dynamic coordinate systems, the Kruskal–Szekers and dynamic Lemaitre coordinate systems
We present a short and direct derivation of Hawking radiation as a tunneling process, based on parti...
For a single horizon spacetime, the Hawking temperature is proportional to the surface gravity at th...
In this article, we explore an alternative derivation of Hawking radiation. Instead of the field-the...
AbstractSome authors have recently found that the tunneling approach gives a different Hawking tempe...
AbstractIt has recently been suggested that the attempt to understand Hawking radiation as tunnellin...
It has recently been suggested that the attempt to understand Hawking radiation as tunnelling across...
The purpose of this thesis is to calculate the Hawking temperature for a Schwarzschild black hole, u...
AbstractWe investigate the Hawking radiation of Schwarzschild–de Sitter (SdS) black hole by massive ...
AbstractThe isotropic coordinate system of Schwarzschild spacetime has several attractive properties...
We examine Hawking radiation from a Schwarzschild black hole in several reference frames using the q...
The Hawking temperature for a Schwarzschild black hole is T=1/8πM, where M is the black hole mass. T...
AbstractUsing the null-geodesic tunneling method of Parikh and Wilczek, we derive the Hawking temper...
Recently, Angheben et.al. [hep-th/0503081] have presented a refined method for calculating the (tree...
This work show what would be the pressure of black hole. This will help to understand the black hole...
New solutions of four-dimensional asymptotically AdS black holes with scalar hair considered and Haw...
We present a short and direct derivation of Hawking radiation as a tunneling process, based on parti...
For a single horizon spacetime, the Hawking temperature is proportional to the surface gravity at th...
In this article, we explore an alternative derivation of Hawking radiation. Instead of the field-the...
AbstractSome authors have recently found that the tunneling approach gives a different Hawking tempe...
AbstractIt has recently been suggested that the attempt to understand Hawking radiation as tunnellin...
It has recently been suggested that the attempt to understand Hawking radiation as tunnelling across...
The purpose of this thesis is to calculate the Hawking temperature for a Schwarzschild black hole, u...
AbstractWe investigate the Hawking radiation of Schwarzschild–de Sitter (SdS) black hole by massive ...
AbstractThe isotropic coordinate system of Schwarzschild spacetime has several attractive properties...
We examine Hawking radiation from a Schwarzschild black hole in several reference frames using the q...
The Hawking temperature for a Schwarzschild black hole is T=1/8πM, where M is the black hole mass. T...
AbstractUsing the null-geodesic tunneling method of Parikh and Wilczek, we derive the Hawking temper...
Recently, Angheben et.al. [hep-th/0503081] have presented a refined method for calculating the (tree...
This work show what would be the pressure of black hole. This will help to understand the black hole...
New solutions of four-dimensional asymptotically AdS black holes with scalar hair considered and Haw...
We present a short and direct derivation of Hawking radiation as a tunneling process, based on parti...
For a single horizon spacetime, the Hawking temperature is proportional to the surface gravity at th...
In this article, we explore an alternative derivation of Hawking radiation. Instead of the field-the...