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We examine the particle production via preheating at the end of inflation in supersymmetric theories. The inflaton and matter scalars are now necessarily complex fields, and their relevant interactions are restricted by holomorphy. In…

High Energy Physics - Phenomenology · Physics 2009-09-29 Z. Chacko , H. Murayama , M. Perelstein

We investigate the entanglement due to geometric corrections in particle creation during inflation. To do so, we propose a single-field inflationary scenario, nonminimally coupled to the scalar curvature of spacetime. We require particle…

General Relativity and Quantum Cosmology · Physics 2023-06-05 Alessio Belfiglio , Orlando Luongo , Stefano Mancini

We show that the present-day dark matter abundance can be produced through a novel mechanism that involves a very rapid thermal freeze-out caused by inhomogeneous heating and successive fast cooling of small fireballs in the early Universe.…

High Energy Physics - Phenomenology · Physics 2023-12-05 Marcos M. Flores , Chris Kouvaris , Alexander Kusenko

We investigate the circumstances under which cosmic inflation can arise from very inhomogeneous initial conditions using numerical relativity simulations. Previous studies have not considered cases with non-zero momentum density due to…

General Relativity and Quantum Cosmology · Physics 2023-12-15 Maxence Corman , William E. East

A small tensor-to-scalar ratio $r$ may lead to distinctive phenomenology of high-scale supersymmetry. Assuming the same origin of SUSY breaking between the inflation and visible sector, we show model independent features. The simplest…

High Energy Physics - Phenomenology · Physics 2015-08-26 Sibo Zheng

In this paper we follow a new approach for particle creation by a localized strong gravitational field. The approach is based on a definition of the physical vacuum drawn from Heisenberg uncertainty principle. Using the fact that the…

General Relativity and Quantum Cosmology · Physics 2007-05-23 M. B. Altaie

We show that a quadratic $U(1)$-breaking term, together with an effective chemical potential induced by a dimension five derivative coupling between the inflaton and the $U(1)$ current, can drive efficient particle production during…

Cosmology and Nongalactic Astrophysics · Physics 2026-02-03 Qi Chen , Yuan Yin

Topical phenomena in high-energy physics related to collision experiments of heavy nuclei ("Little Bang") and early universe cosmology ("Big Bang") involve far-from-equilibrium dynamics described by quantum field theory. One example…

High Energy Physics - Phenomenology · Physics 2009-06-15 J. Berges

We discuss the gravitational creation of superheavy particles $\chi$ in an inflationary scenario with a quartic potential and a non-minimal coupling between the inflaton $\varphi$ and the Ricci curvature: $\xi \varphi^2 R/2$. We show that…

High Energy Physics - Phenomenology · Physics 2020-10-14 E. Babichev , D. Gorbunov , S. Ramazanov , L. Reverberi

We investigate the particle production of a scalar field $\chi$ coupled to an inflaton field $\phi$ ($g^2\phi^2\chi^2/2$) in the {\it oscillating inflation} model, which was recently proposed by Damour and Mukhanov. Although the fluctuation…

High Energy Physics - Phenomenology · Physics 2008-11-26 S. Tsujikawa

Parametric resonance has received a considerable amount of interest as a good mathematical model to describe the initial stages of the reheating phase (matter creation) in inflationary cosmology. It is also known that exponential particle…

High Energy Physics - Phenomenology · Physics 2007-05-23 Fernando da Rocha Vaz Bandeira de Melo , Robert H. Brandenberger , Adolfo Maia Junior

An oscillating inflaton field induces small amplitude oscillations of the Hubble parameter at the end of inflation. These Hubble parameter induced oscillations, in turn, trigger parametric particle production of all light fields, even if…

High Energy Physics - Phenomenology · Physics 2023-05-22 Robert Brandenberger , Vahid Kamali , Rudnei O. Ramos

We study whether a first-order phase transition at the end of inflation can generate the observed dark matter abundance through bubble collisions. The transition occurs in a spectator scalar sector with an inflaton-dependent effective…

High Energy Physics - Phenomenology · Physics 2026-05-06 Zihong Cheng , Fa Peng Huang

The fundamental paradox of the incompatibility of the observed large-scale uniformity of the Universe with the fact that the age of the Universe is finite is overcome by the introduction of an initial a period of superluminal expansion of…

High Energy Physics - Phenomenology · Physics 2010-11-02 Konstantinos Dimopoulos

We analyze the limits on resonant particle production during inflation based upon the power spectrum of fluctuations in matter and the cosmic microwave background. We show that such a model is consistent with features observed in the matter…

Astrophysics · Physics 2009-11-10 G. J. Mathews , D. J. H. Chung , K. Ichiki , T. Kajino , M. Orito

I present the production of matter and radiation during reheating after inflation, considering only gravitational interactions between the inflaton background and the other sectors. Processes considered are the following: i) the exchange of…

High Energy Physics - Phenomenology · Physics 2023-09-26 Simon Cléry

The study of particle creation phenomena at the expense of the gravitational field is of great research interest. It might solve the cosmological puzzle single-handedly, without the need for either dark energy or the modified theory of…

General Relativity and Quantum Cosmology · Physics 2018-06-26 Abhik Kumar Sanyal , Subhra Debnath

The present work deals with a cosmological model having particle creation mechanism in the framework of irreversible thermodynamics. In the second order non-equilibrium thermodynamical prescription, the particle creation rate is treated as…

General Relativity and Quantum Cosmology · Physics 2015-05-01 Subenoy Chakraborty , Supriya Pan , Subhajit Saha

A new mechanism for generating the curvature perturbation at the end of inflaton has been investigated. The dominant contribution to the primordial curvature perturbation may be generated during the period of instant preheating. The…

High Energy Physics - Theory · Physics 2010-10-27 Tomohiro Matsuda

Particle production in the background of an external classical oscillating field is a key process describing the stage of preheating after inflation. For sufficiently strong couplings between the inflaton and matter fields, this process is…

Cosmology and Nongalactic Astrophysics · Physics 2018-10-26 Igor Rudenok , Yuri Shtanov , Stanislav Vilchinskii
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