In general, the Gibbons-Hawking temperature based on the Euclidean functional approach shows that de Sitter space in the Bunch-Davies vacuum is globally thermal. In the exactly soluble semiclassical Jackiw-Teitelboim model, we investigate thermal property of de Sitter space by taking into account the quantum back reaction of the geometry. The proper temperature of de Sitter space in the Bunch-Davies vacuum is found to vanish. In case of a certain quantum state breaking the de Sitter symmetry, de Sitter space can be made thermally exited; however, in this case the dilaton singularity cannot be avoided. Consequently, in the Jackiw-Teitelboim model the proper temperature of de Sitter space in the Bunch-Davies vacuum turns out to be zero and th...
The structure of the thermal equilibrium state of a weakly interacting Bose gas is of current intere...
Quantum particle creation from spacetime horizons, or accelerating boundaries in the dynamical Casim...
It is possible to associate temperatures with the nonextremal horizons of a large class of spherical...
The activation temperature $T$ in the de Sitter environment is twice larger than the Gibbons-Hawking...
The seminar discovery by Gibbons and Hawking that a freely falling detector observes an isotropic ba...
In three dimensions, Kerr-de Sitter spacetime as a solution of Einstein gravity with positive cosmol...
Quantized fields (e.g., the graviton itself) in de Sitter (dS) spacetime lead to particle production...
It is shown how the results of Deser and Levin on the response of accelerated detectors in anti-de S...
We calculate the energy density and pressure of a scalar field after its decoupling from a thermal b...
We analyse the response and thermal behaviour of an Unruh-DeWitt detector as it travels through cosm...
Using Relativistic Quantum Geometry we study back-reaction effects of space-time inside the causal h...
The de Sitter (dS) entropy bound gives the maximal number of e-folds that non-eternal inflation can ...
Abstract: In this paper we study some thermal properties of quantum field theories in de Sitter spac...
Schwarzschild-de Sitter (SdS) black holes do not admit a completely smooth Euclidean continuation. W...
We present a 4-dimensional back reaction analysis of de Sitter space for a conformally coupled scala...
The structure of the thermal equilibrium state of a weakly interacting Bose gas is of current intere...
Quantum particle creation from spacetime horizons, or accelerating boundaries in the dynamical Casim...
It is possible to associate temperatures with the nonextremal horizons of a large class of spherical...
The activation temperature $T$ in the de Sitter environment is twice larger than the Gibbons-Hawking...
The seminar discovery by Gibbons and Hawking that a freely falling detector observes an isotropic ba...
In three dimensions, Kerr-de Sitter spacetime as a solution of Einstein gravity with positive cosmol...
Quantized fields (e.g., the graviton itself) in de Sitter (dS) spacetime lead to particle production...
It is shown how the results of Deser and Levin on the response of accelerated detectors in anti-de S...
We calculate the energy density and pressure of a scalar field after its decoupling from a thermal b...
We analyse the response and thermal behaviour of an Unruh-DeWitt detector as it travels through cosm...
Using Relativistic Quantum Geometry we study back-reaction effects of space-time inside the causal h...
The de Sitter (dS) entropy bound gives the maximal number of e-folds that non-eternal inflation can ...
Abstract: In this paper we study some thermal properties of quantum field theories in de Sitter spac...
Schwarzschild-de Sitter (SdS) black holes do not admit a completely smooth Euclidean continuation. W...
We present a 4-dimensional back reaction analysis of de Sitter space for a conformally coupled scala...
The structure of the thermal equilibrium state of a weakly interacting Bose gas is of current intere...
Quantum particle creation from spacetime horizons, or accelerating boundaries in the dynamical Casim...
It is possible to associate temperatures with the nonextremal horizons of a large class of spherical...