By globally embedding curved spaces into higher dimensional flat ones, we show that Hawking thermal properties map into their Unruh equivalents: The relevant curved space detectors become Rindler ones, whose temperature and entropy reproduce the originals. Specific illustrations include Schwarzschild, Schwarzschild-(anti)deSitter, Reissner-Nordstrom and BTZ spaces
The paper deals with universal thermodynamics for FRW model of the universe bounded by apparent (or ...
We study the Unruh effect for an observer with a finite lifetime, using the thermal time hypothesis....
We study the matching between the Hawking temperature of a large class of static D-dimensional black...
By globally embedding curved spaces into higher dimensional flat ones, we show that Hawking thermal ...
We present a unified description of temperature and entropy in spaces with either ‘true’ or ‘acceler...
We develop an adiabatic formalism to study the Hawking phenomenon from the perspective of Unruh-DeWi...
Several approaches to Hawking radiation on Schwarzschild spacetime rely in some way or another on th...
The notions of temperature, entropy and `evaporation', usually associated with spacetimes with horiz...
A peculiar prediction of quantum field theory in curved spacetime is that the existence of particles...
We analyse the response and thermal behaviour of an Unruh-DeWitt detector as it travels through cosm...
In this thesis, we study the Hawking and Unruh effects in time-dependent situations, as registered b...
The notions of temperature, entropy and 'evaporation', usually associated with spacetimes with horiz...
The Hawking temperature for a Schwarzschild black hole is T=1/8πM, where M is the black hole mass. T...
We study the perception of the radiation phenomena of Hawking radiation and Unruh effect by using tw...
© 2018 IOP Publishing Ltd. Ultracold fermionic atoms in an optical lattice, with a sudden position-d...
The paper deals with universal thermodynamics for FRW model of the universe bounded by apparent (or ...
We study the Unruh effect for an observer with a finite lifetime, using the thermal time hypothesis....
We study the matching between the Hawking temperature of a large class of static D-dimensional black...
By globally embedding curved spaces into higher dimensional flat ones, we show that Hawking thermal ...
We present a unified description of temperature and entropy in spaces with either ‘true’ or ‘acceler...
We develop an adiabatic formalism to study the Hawking phenomenon from the perspective of Unruh-DeWi...
Several approaches to Hawking radiation on Schwarzschild spacetime rely in some way or another on th...
The notions of temperature, entropy and `evaporation', usually associated with spacetimes with horiz...
A peculiar prediction of quantum field theory in curved spacetime is that the existence of particles...
We analyse the response and thermal behaviour of an Unruh-DeWitt detector as it travels through cosm...
In this thesis, we study the Hawking and Unruh effects in time-dependent situations, as registered b...
The notions of temperature, entropy and 'evaporation', usually associated with spacetimes with horiz...
The Hawking temperature for a Schwarzschild black hole is T=1/8πM, where M is the black hole mass. T...
We study the perception of the radiation phenomena of Hawking radiation and Unruh effect by using tw...
© 2018 IOP Publishing Ltd. Ultracold fermionic atoms in an optical lattice, with a sudden position-d...
The paper deals with universal thermodynamics for FRW model of the universe bounded by apparent (or ...
We study the Unruh effect for an observer with a finite lifetime, using the thermal time hypothesis....
We study the matching between the Hawking temperature of a large class of static D-dimensional black...