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 have derived the Hawking temperature of the Reissner-Nordstrom-Vaidya black hole by the use of bo...
In this paper, the tunneling of scalar particles near the event horizons of Riemann space time, BTZ ...
We analyze Hawking radiation as perceived by a freely-falling observer and try to draw an inference ...
AbstractSome authors have recently found that the tunneling approach gives a different Hawking tempe...
It has recently been suggested that the attempt to understand Hawking radiation as tunnelling across...
AbstractIt has recently been suggested that the attempt to understand Hawking radiation as tunnellin...
We examine Hawking radiation from a Schwarzschild black hole in several reference frames using the q...
AbstractWe investigate the Hawking radiation of Schwarzschild–de Sitter (SdS) black hole by massive ...
We present a short and direct derivation of Hawking radiation as a tunneling process, based on parti...
The paper deals with Hawking radiation from both a general static black hole and a nonstatic spheric...
AbstractUsing the null-geodesic tunneling method of Parikh and Wilczek, we derive the Hawking temper...
Hawking radiation is computed in different coordinate systems using the method of complex paths. In ...
The Hawking temperature for a Schwarzschild black hole is T=1/8πM, where M is the black hole mass. T...
AbstractWe show that the recent tunneling formulas for black hole radiation in static, spherically s...
We apply the technique of complex paths to obtain Hawking radiation in different coordinate represen...
We have derived the Hawking temperature of the Reissner-Nordstrom-Vaidya black hole by the use of bo...
In this paper, the tunneling of scalar particles near the event horizons of Riemann space time, BTZ ...
We analyze Hawking radiation as perceived by a freely-falling observer and try to draw an inference ...
AbstractSome authors have recently found that the tunneling approach gives a different Hawking tempe...
It has recently been suggested that the attempt to understand Hawking radiation as tunnelling across...
AbstractIt has recently been suggested that the attempt to understand Hawking radiation as tunnellin...
We examine Hawking radiation from a Schwarzschild black hole in several reference frames using the q...
AbstractWe investigate the Hawking radiation of Schwarzschild–de Sitter (SdS) black hole by massive ...
We present a short and direct derivation of Hawking radiation as a tunneling process, based on parti...
The paper deals with Hawking radiation from both a general static black hole and a nonstatic spheric...
AbstractUsing the null-geodesic tunneling method of Parikh and Wilczek, we derive the Hawking temper...
Hawking radiation is computed in different coordinate systems using the method of complex paths. In ...
The Hawking temperature for a Schwarzschild black hole is T=1/8πM, where M is the black hole mass. T...
AbstractWe show that the recent tunneling formulas for black hole radiation in static, spherically s...
We apply the technique of complex paths to obtain Hawking radiation in different coordinate represen...
We have derived the Hawking temperature of the Reissner-Nordstrom-Vaidya black hole by the use of bo...
In this paper, the tunneling of scalar particles near the event horizons of Riemann space time, BTZ ...
We analyze Hawking radiation as perceived by a freely-falling observer and try to draw an inference ...