We study the emission of large-scales wavelength space–time waves during the inflationary expansion of the universe, produced by back-reaction effects. As an example, we study an inflationary model with variable time scale, where the scale factor of the universe grows as a power of time. The coarse-grained field to describe space–time waves is defined by using the Levy distribution, on the wavenumber space. The evolution for the norm of these waves on cosmological scales is calculated, and it is shown that decreases with time.Fil: Musmarra, Juan Ignacio. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - Mar del Plata. Instituto de Investigaciones Físicas de Mar del Plata. Universidad Naciona...
Using Relativistic Quantum Geometry (RQG), we study the emergence of back-reaction modes with solito...
Using the techniques of out-of-equilibrium field theory, we study the influence on properties of cos...
We investigate, in the transverse traceless (TT) gauge, the generation of the relic background of gr...
This thesis is concerned with the evolution of long wavelength cosmological perturbations in the ve...
International audienceOscillations in the frequency profile of the scalar-induced contribution to th...
International audiencePreheating after inflation involves large, time-dependent field inhomogeneitie...
Preheating after inflation involves large, time-dependent field inhomogeneities, which act as a clas...
We study cosmological gravitational waves generated during inflation under the influence of a decayi...
Because of the non-linearity of the Einstein equations, the cosmological fluctuations which are gene...
We discuss the cosmological evolution of the inflationary gravitational wave background (IGWB) in th...
We study a collapsing system attracted by a spherically symmetric gravitational source, with an incr...
Extending previous results [Phys. Rev.D {\bf 56}, 6351 (1997)], we estimate the back reaction of cos...
In cosmological scenarios with thermal inflation, extra eras of moduli matter domination, thermal in...
The gravitational-wave-noise power spectrum P(ω) is found for a simple cosmological model with an ‘‘...
We discuss a scenario in which extra dimensional effects allow a scalar field with a steep potential...
Using Relativistic Quantum Geometry (RQG), we study the emergence of back-reaction modes with solito...
Using the techniques of out-of-equilibrium field theory, we study the influence on properties of cos...
We investigate, in the transverse traceless (TT) gauge, the generation of the relic background of gr...
This thesis is concerned with the evolution of long wavelength cosmological perturbations in the ve...
International audienceOscillations in the frequency profile of the scalar-induced contribution to th...
International audiencePreheating after inflation involves large, time-dependent field inhomogeneitie...
Preheating after inflation involves large, time-dependent field inhomogeneities, which act as a clas...
We study cosmological gravitational waves generated during inflation under the influence of a decayi...
Because of the non-linearity of the Einstein equations, the cosmological fluctuations which are gene...
We discuss the cosmological evolution of the inflationary gravitational wave background (IGWB) in th...
We study a collapsing system attracted by a spherically symmetric gravitational source, with an incr...
Extending previous results [Phys. Rev.D {\bf 56}, 6351 (1997)], we estimate the back reaction of cos...
In cosmological scenarios with thermal inflation, extra eras of moduli matter domination, thermal in...
The gravitational-wave-noise power spectrum P(ω) is found for a simple cosmological model with an ‘‘...
We discuss a scenario in which extra dimensional effects allow a scalar field with a steep potential...
Using Relativistic Quantum Geometry (RQG), we study the emergence of back-reaction modes with solito...
Using the techniques of out-of-equilibrium field theory, we study the influence on properties of cos...
We investigate, in the transverse traceless (TT) gauge, the generation of the relic background of gr...