Gravitons are described by the propagator in teleparallel gravity in nearly flat space-time. Finite temperature is introduced by using Thermofield Dynamics formalism. The gravitational Casimir effect and Stefan-Boltzmann law are calculated as a function of temperature. Then an equation of state for gravitons is determined
We investigate Casimir effect as well as thermal Casimir effect for a pair of parallel perfectly pla...
AbstractColeman–Weinberg (CW) phenomena for the case of gravitons minimally coupled to massless scal...
Coleman–Weinberg (CW) phenomena for the case of gravitons minimally coupled to massless scalar field...
Temperature effects in a scalar field non-minimally coupled to gravity are investigated. The Thermo ...
The Thermo Field Dynamics (TFD) formalism is used to investigate the regular black holes at finite t...
The standard model and general relativity are local Lorentz invariants. However, it is possible that...
We use the scalar field constructed in phase space to analyze the analogous Stefan-Boltzmann law and...
Lorentz and CPT symmetries are foundations for important processes in particle physics. Recent studi...
The Dirac field, spin 1/2 particles, is investigated in phase space. The Dirac propagator is defined...
We discuss a thermodynamic identity which helps explain why ≠ at finite temperature. In addition we ...
We discuss a thermodynamic identity which helps explain why 〈H〉≠〈T00〉 at finite temperature. In addi...
We discuss a thermodynamic identity which helps explain why (Hiss(Too) at finite temperature. In add...
Studies about a formal analogy between the gravitational and the electromagnetic fields lead to the ...
AbstractLorentz and CPT symmetries are foundations for important processes in particle physics. Rece...
Abstract Starting from an analytical expression for the Helmholtz free energy we calculate the therm...
We investigate Casimir effect as well as thermal Casimir effect for a pair of parallel perfectly pla...
AbstractColeman–Weinberg (CW) phenomena for the case of gravitons minimally coupled to massless scal...
Coleman–Weinberg (CW) phenomena for the case of gravitons minimally coupled to massless scalar field...
Temperature effects in a scalar field non-minimally coupled to gravity are investigated. The Thermo ...
The Thermo Field Dynamics (TFD) formalism is used to investigate the regular black holes at finite t...
The standard model and general relativity are local Lorentz invariants. However, it is possible that...
We use the scalar field constructed in phase space to analyze the analogous Stefan-Boltzmann law and...
Lorentz and CPT symmetries are foundations for important processes in particle physics. Recent studi...
The Dirac field, spin 1/2 particles, is investigated in phase space. The Dirac propagator is defined...
We discuss a thermodynamic identity which helps explain why ≠ at finite temperature. In addition we ...
We discuss a thermodynamic identity which helps explain why 〈H〉≠〈T00〉 at finite temperature. In addi...
We discuss a thermodynamic identity which helps explain why (Hiss(Too) at finite temperature. In add...
Studies about a formal analogy between the gravitational and the electromagnetic fields lead to the ...
AbstractLorentz and CPT symmetries are foundations for important processes in particle physics. Rece...
Abstract Starting from an analytical expression for the Helmholtz free energy we calculate the therm...
We investigate Casimir effect as well as thermal Casimir effect for a pair of parallel perfectly pla...
AbstractColeman–Weinberg (CW) phenomena for the case of gravitons minimally coupled to massless scal...
Coleman–Weinberg (CW) phenomena for the case of gravitons minimally coupled to massless scalar field...