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We consider the framework of quintessential inflation in the warm background which is caused by the dissipation of the scalar field energy density into relativistic degrees of freedom. The dissipation process has important consequences for…

Cosmology and Nongalactic Astrophysics · Physics 2021-03-03 Mayukh R. Gangopadhyay , Shynaray Myrzakul , Mohammad Sami , Mohit K. Sharma

In this paper, we investigate a scenario of variable gravity and apply it to the unified description of inflation and late time cosmic acceleration dubbed quintessential inflation. The scalar field called "cosmon" which in this model…

General Relativity and Quantum Cosmology · Physics 2014-07-14 Md. Wali Hossain , R. Myrzakulov , M. Sami , Emmanuel N. Saridakis

A large class of quintessential inflationary models, recently proposed by Peebles and Vilenkin, leads to post-inflationary phases whose effective equation of state is stiffer than radiation. The expected gravitational waves logarithmic…

Astrophysics · Physics 2009-10-31 Massimo Giovannini

We investigate the dependence of the gravitational wave spectrum from quintessential inflation on the reheating process. We consider two extreme reheating processes. One is the gravitational reheating by particle creation in the expanding…

General Relativity and Quantum Cosmology · Physics 2009-10-09 Hiroyuki Tashiro , Takeshi Chiba , Misao Sasaki

One of the most important issues in an inflationary theory as standard or quintessential inflation is the mechanism to reheat the universe after the end of the inflationary period in order to match with the Hot Big Bang universe. In…

General Relativity and Quantum Cosmology · Physics 2023-01-03 Jaume Haro , Llibert Aresté Saló

Quintessential inflation describes a scenario in which both inflation and dark energy (quintessence) are described by the same scalar field. In conventional braneworld models of quintessential inflation gravitational particle production is…

High Energy Physics - Theory · Physics 2009-11-10 M. Sami , V. Sahni

We provide a detailed study of gravitational reheating in quintessential inflation generalizing previous analyses only available for the standard case when inflation is followed by an era dominated by the energy density of radiation.…

High Energy Physics - Phenomenology · Physics 2009-07-22 E. J. Chun , S. Scopel , I. Zaballa

We discuss a scenario in which extra dimensional effects allow a scalar field with a steep potential to play the dual role of the inflaton as well as dark energy (quintessence). The post-inflationary evolution of the universe in this…

General Relativity and Quantum Cosmology · Physics 2009-11-07 Varun Sahni , M. Sami , Tarun Souradeep

The reheating of the universe after hybrid inflation proceeds through the nucleation and subsequent collision of large concentrations of energy density in the form of bubble-like structures moving at relativistic speeds. This generates a…

High Energy Physics - Phenomenology · Physics 2008-11-26 Juan Garcia-Bellido , Daniel G. Figueroa , Alfonso Sastre

Parametric resonance or preheating is a plausible mechanism for bringing about the transition between the inflationary phase and a hot, radiation dominated universe. This epoch results in the rapid production of heavy particles far from…

Astrophysics · Physics 2008-11-26 Richard Easther , John T. Giblin , Eugene A. Lim

We compute numerically the reheating temperature due to the gravitational production of conformally coupled superheavy particles during the phase transition from the end of inflation to the beginning of kination in two different…

General Relativity and Quantum Cosmology · Physics 2023-01-03 Jaume de Haro , Llibert Aresté Saló

The energy spectra of gravitational waves (GW) produced in quintessential inflationary models increase in frequency and exhibit a sharp spike around 170 GHz where the associated fraction of critical energy density today stored in relic…

High Energy Physics - Phenomenology · Physics 2009-10-31 Massimo Giovannini

In many models of inflation, the period of accelerated expansion ends with preheating, a highly non-thermal phase of evolution during which the inflaton pumps energy into a specific set of momentum modes of field(s) to which it is coupled.…

Astrophysics · Physics 2009-11-11 Richard Easther , Eugene A. Lim

We investigate the generation of gravitational waves in the hybrid quintessential inflationary model. The full gravitational-wave energy spectrum is calculated using the method of continuous Bogoliubov coefficients. The post-inflationary…

General Relativity and Quantum Cosmology · Physics 2015-03-13 Paulo M. Sá , Alfredo B. Henriques

The generated relic gravitational waves were underwent several stages of evolution of the universe such as inflation and reheating. These stages were affected on the shape of spectrum of the waves. As well known, at the end of inflation,…

General Relativity and Quantum Cosmology · Physics 2019-08-06 Basem Ghayour

We compute numerically the reheating temperature due to the gravitational production of conformally coupled superheavy particles during the phase transition from the end of inflation to the beginning of kination in two different…

General Relativity and Quantum Cosmology · Physics 2021-11-10 Llibert Aresté Saló , Jaume de Haro

The reheating of the universe after hybrid inflation proceeds through the nucleation and subsequent collision of large concentrations of energy density in the form of bubble-like structures moving at relativistic speeds. This generates a…

General Relativity and Quantum Cosmology · Physics 2008-01-29 Juan Garcia-Bellido , Daniel G. Figueroa

We present three-dimensional direct numerical simulations of the production of magnetic fields and gravitational waves (GWs) in the early Universe during a low energy scale matter-dominated post-inflationary reheating era, and during the…

Cosmology and Nongalactic Astrophysics · Physics 2021-10-13 Axel Brandenburg , Ramkishor Sharma

The super-inflationary phase is predicted by the Loop Quantum Cosmology. In this paper we study the creation of gravitational waves during this phase. We consider the inverse volume corrections to the equation for the tensor modes and…

General Relativity and Quantum Cosmology · Physics 2007-10-16 Jakub Mielczarek , Marek Szydlowski

Quintessential inflation models provide a framework that simultaneously describes inflation and dynamical dark energy, the latter of which has recently received growing support from DESI observations. A distinctive feature of these models…

Cosmology and Nongalactic Astrophysics · Physics 2026-05-04 Changcheng Jing , George Alestas , Sachiko Kuroyanagi
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