Add to ORKGLorentz invariance plays a pivotal role in the derivation of the Hawking effect, which crucially requires an integration in arbitrarily small distances or, equivalently, in unbounded energies. New physics at the Planck scale could, therefore, potentially modify the emission spectrum. We argue, however, that the kinematic invariance can be deformed in such a way that the thermal spectrum remains insensitive to trans-Planckian physics
In this thesis, we study several features of Hawking radiation in the presence of ultraviolet Lorent...
A modified formulation of energy-momentum relation is proposed in the context of doubly special rela...
We explore the possibility that, in a quantum field theory with Planck scale cutoff Λ ' mp, obs...
A disturbing aspect of Hawking's derivation of black hole radiance is the need to invoke extreme con...
A uniformly accelerating observer perceives the Minkowski vacuum state as a thermal bath of radiatio...
Nonlinear deformations of relativistic symmetries at the Planck scale are usually addressed in terms...
The presence of gravity implies corrections to the Einstein-Planck formula E = hν. This gives hope t...
The Hawking effect can be rederived in terms of two-point functions and in such a way that it makes ...
Using a derivation of black hole radiance in terms of two-point functions one can provide a quantita...
Planck-scale corrections to the black-hole radiation spectrum in the Parikh-Wilczek tunneling framew...
AbstractHawking radiation has thermal spectrum corresponding to the temperature TH=(8πM)−1, where M ...
An important question in the derivation of the acceleration radiation, which also arises in Hawking'...
Using a derivation of black hole radiance in terms of two-point functions one can provide a quantita...
The presence of gravity implies corrections to the Einstein-Planck formula E = hν. This gives hope t...
It is well known that radiative corrections evaluated in nontrivial backgrounds lead to effective di...
In this thesis, we study several features of Hawking radiation in the presence of ultraviolet Lorent...
A modified formulation of energy-momentum relation is proposed in the context of doubly special rela...
We explore the possibility that, in a quantum field theory with Planck scale cutoff Λ ' mp, obs...
A disturbing aspect of Hawking's derivation of black hole radiance is the need to invoke extreme con...
A uniformly accelerating observer perceives the Minkowski vacuum state as a thermal bath of radiatio...
Nonlinear deformations of relativistic symmetries at the Planck scale are usually addressed in terms...
The presence of gravity implies corrections to the Einstein-Planck formula E = hν. This gives hope t...
The Hawking effect can be rederived in terms of two-point functions and in such a way that it makes ...
Using a derivation of black hole radiance in terms of two-point functions one can provide a quantita...
Planck-scale corrections to the black-hole radiation spectrum in the Parikh-Wilczek tunneling framew...
AbstractHawking radiation has thermal spectrum corresponding to the temperature TH=(8πM)−1, where M ...
An important question in the derivation of the acceleration radiation, which also arises in Hawking'...
Using a derivation of black hole radiance in terms of two-point functions one can provide a quantita...
The presence of gravity implies corrections to the Einstein-Planck formula E = hν. This gives hope t...
It is well known that radiative corrections evaluated in nontrivial backgrounds lead to effective di...
In this thesis, we study several features of Hawking radiation in the presence of ultraviolet Lorent...
A modified formulation of energy-momentum relation is proposed in the context of doubly special rela...
We explore the possibility that, in a quantum field theory with Planck scale cutoff Λ ' mp, obs...