Add to ORKGUsing a derivation of black hole radiance in terms of two-point functions one can provide a quantitative estimate of the contribution of short distances to the spectrum. Thermality is preserved for black holes with κlP 1. However, deviations from the Planckian spectrum can be found for mini black holes in TeV gravity scenarios, even before reaching the Planck phase. © 2006 The American Physical Society
Lorentz invariance plays a pivotal role in the derivation of the Hawking effect, which crucially req...
As they are evaporating, black holes are emitting radiations called Hawking radiations. Our goal is ...
A coarse-grained version of the effective action is used to study the thermodynamics of black holes,...
Using a derivation of black hole radiance in terms of two-point functions one can provide a quantita...
Using a derivation of black hole radiance in terms of two-point functions one can provide a quantita...
The Hawking effect can be rederived in terms of two-point functions and in such a way that it makes ...
The Hawking effect can be rederived in terms of two-point functions and in such a way that it makes ...
The presence of gravity implies corrections to the Einstein-Planck formula E = hν. This gives hope t...
AbstractThe quantum genesis of Hawking radiation is a long-standing puzzle in black hole physics. Se...
The role played by ultrahigh frequencies or ultrashort distances in the usual derivation of the Hawk...
AbstractLarge extra dimensions lower the Planck scale to values soon accessible. Motivated by string...
Recently, a new framework for solving the hierarchy problem was proposed which does not rely on low ...
The many low energy modes near a black hole horizon give the thermal atmosphere a divergent entropy ...
Bekenstein and Mukhanov have put forward the idea that, in a quantum theory of gravity a black hole ...
Our understanding of black holes changed drastically, when Stephen Hawking discovered their evaporat...
Lorentz invariance plays a pivotal role in the derivation of the Hawking effect, which crucially req...
As they are evaporating, black holes are emitting radiations called Hawking radiations. Our goal is ...
A coarse-grained version of the effective action is used to study the thermodynamics of black holes,...
Using a derivation of black hole radiance in terms of two-point functions one can provide a quantita...
Using a derivation of black hole radiance in terms of two-point functions one can provide a quantita...
The Hawking effect can be rederived in terms of two-point functions and in such a way that it makes ...
The Hawking effect can be rederived in terms of two-point functions and in such a way that it makes ...
The presence of gravity implies corrections to the Einstein-Planck formula E = hν. This gives hope t...
AbstractThe quantum genesis of Hawking radiation is a long-standing puzzle in black hole physics. Se...
The role played by ultrahigh frequencies or ultrashort distances in the usual derivation of the Hawk...
AbstractLarge extra dimensions lower the Planck scale to values soon accessible. Motivated by string...
Recently, a new framework for solving the hierarchy problem was proposed which does not rely on low ...
The many low energy modes near a black hole horizon give the thermal atmosphere a divergent entropy ...
Bekenstein and Mukhanov have put forward the idea that, in a quantum theory of gravity a black hole ...
Our understanding of black holes changed drastically, when Stephen Hawking discovered their evaporat...
Lorentz invariance plays a pivotal role in the derivation of the Hawking effect, which crucially req...
As they are evaporating, black holes are emitting radiations called Hawking radiations. Our goal is ...
A coarse-grained version of the effective action is used to study the thermodynamics of black holes,...