Using a derivation of black hole radiance in terms of two-point functions one can provide a quantitative estimation of the contribution of short distances to the spectrum. Thermality is preserved for black holes with $\kappa l_P <<1$. However, deviations from the Planckian spectrum can be found for mini black holes in TeV gravity scenarios, even before reaching the Planck phase
Photons emitted by light sources in the neighbourhood of a black hole can wind several times around ...
Area spectrum of black holes has been obtained via various methods such as quasinormal modes, adiaba...
We study the Hawking radiation in an analogue black hole, in which sound plays the role of light.&nb...
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 ...
As they are evaporating, black holes are emitting radiations called Hawking radiations. Our goal is ...
The quantum genesis of Hawking radiation is a long-standing puzzle in black hole physics. Semi-class...
Lorentz invariance plays a pivotal role in the derivation of the Hawking effect, which crucially req...
The many low energy modes near a black hole horizon give the thermal atmosphere a divergent entropy ...
The presence of gravity implies corrections to the Einstein-Planck formula E = hν. This gives hope t...
We describe a method for the determination of black hole masses based on information inferred from h...
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...
Photons emitted by light sources in the neighbourhood of a black hole can wind several times around ...
Area spectrum of black holes has been obtained via various methods such as quasinormal modes, adiaba...
We study the Hawking radiation in an analogue black hole, in which sound plays the role of light.&nb...
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 ...
As they are evaporating, black holes are emitting radiations called Hawking radiations. Our goal is ...
The quantum genesis of Hawking radiation is a long-standing puzzle in black hole physics. Semi-class...
Lorentz invariance plays a pivotal role in the derivation of the Hawking effect, which crucially req...
The many low energy modes near a black hole horizon give the thermal atmosphere a divergent entropy ...
The presence of gravity implies corrections to the Einstein-Planck formula E = hν. This gives hope t...
We describe a method for the determination of black hole masses based on information inferred from h...
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...
Photons emitted by light sources in the neighbourhood of a black hole can wind several times around ...
Area spectrum of black holes has been obtained via various methods such as quasinormal modes, adiaba...
We study the Hawking radiation in an analogue black hole, in which sound plays the role of light.&nb...
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