In this paper we compute the effective Lagrangian of static gravitational fields interacting with thermal fields of generalized electrodynamics at high temperature. We employ the usual Matsubara imaginary-time formalism to obtain a closed form expression to the thermal effective Lagrangian at one-loop and two-loop order, in an arbitrary omega-dimensional spacetime, in which the equivalence between the static hard thermal loops and those with zero external energy momentum is widely explored. Afterwards, the symmetries of the resulting expressions are discussed as well as the presence of the Tolman local temperature.Fundação de Amparo à Pesquisa do Estado de São Paulo (FAPESP
In the case of a gravitating mass of perfect fluid which has come to thermodynamic equilibrium, it h...
Abstract In this work we use momentum-space techniques to evaluate the propagator G(x, x ′) for a sp...
We present compact expressions for the power corrections to the hard thermal loop (HTL) Lagrangian o...
We compute the effective Lagrangian of static gravitational fields interacting with thermal fields. ...
We examine, in the imaginary-time formalism, the high temperature behavior of n-point thermal loops ...
We examine, through a Boltzmann equation approach, the generating action of hard thermal loops in th...
AbstractWe examine, through a Boltzmann equation approach, the generating action of hard thermal loo...
We prove that the hard thermal loop contribution to static thermal amplitudes can be obtained by set...
We derive a closed form expression for the long wavelength limit of the effective action for hard th...
Investigamos certas propriedades físicas da teoria de campos a temperatura finita. Mostramos que, na...
Finite-temperature corrections to the effective potential and the energy-momentum tensor of a scalar...
We study the Yang-Mills theory and quantum gravity at finite temperature, in the presence of La-gran...
AbstractWe study, in the long wave-length and static limits, the structure of the n-point graviton f...
In the absence of any appreciable gravitational field the conditions satisfied by the temperature of...
We discuss the high-temperature behavior of retarded thermal loops in static external fields. We emp...
In the case of a gravitating mass of perfect fluid which has come to thermodynamic equilibrium, it h...
Abstract In this work we use momentum-space techniques to evaluate the propagator G(x, x ′) for a sp...
We present compact expressions for the power corrections to the hard thermal loop (HTL) Lagrangian o...
We compute the effective Lagrangian of static gravitational fields interacting with thermal fields. ...
We examine, in the imaginary-time formalism, the high temperature behavior of n-point thermal loops ...
We examine, through a Boltzmann equation approach, the generating action of hard thermal loops in th...
AbstractWe examine, through a Boltzmann equation approach, the generating action of hard thermal loo...
We prove that the hard thermal loop contribution to static thermal amplitudes can be obtained by set...
We derive a closed form expression for the long wavelength limit of the effective action for hard th...
Investigamos certas propriedades físicas da teoria de campos a temperatura finita. Mostramos que, na...
Finite-temperature corrections to the effective potential and the energy-momentum tensor of a scalar...
We study the Yang-Mills theory and quantum gravity at finite temperature, in the presence of La-gran...
AbstractWe study, in the long wave-length and static limits, the structure of the n-point graviton f...
In the absence of any appreciable gravitational field the conditions satisfied by the temperature of...
We discuss the high-temperature behavior of retarded thermal loops in static external fields. We emp...
In the case of a gravitating mass of perfect fluid which has come to thermodynamic equilibrium, it h...
Abstract In this work we use momentum-space techniques to evaluate the propagator G(x, x ′) for a sp...
We present compact expressions for the power corrections to the hard thermal loop (HTL) Lagrangian o...