English
Related papers

Related papers: Violent Preheating in Inflation with Nonminimal Co…

200 papers

We study preheating in a general class of supersymmetric hybrid inflation model. Supersymmetry leads to only one coupling constant in the potential and thus only one natural frequency of oscillation for the homogeneous fields, whose…

High Energy Physics - Phenomenology · Physics 2009-10-31 M. Bastero-Gil , S. F. King , J. Sanderson

We construct a two-stage inflationary model which can accommodate early inflation at a scale $\Lambda_1$ as well as a second stage of inflation at $\Lambda_2$ with a single scalar field $\phi$. We use a symmetric potential, valid in a…

Astrophysics · Physics 2008-11-26 G. German , A. de la Macorra

We propose a new mechanism of non-thermal particle production during inflation based on a narrow parametric resonance, akin to the dynamics of post-inflationary preheating. The mechanism is based on the production of scalar particles with a…

High Energy Physics - Phenomenology · Physics 2025-07-18 Diogo S. Gorgulho , João G. Rosa

A pseudoscalar inflaton $\varphi$, coupled to the topological charge density $F\tilde{F}$ of a non-Abelian sector, can decay to gauge bosons ($\varphi\to g g $), which may thermalize rapidly. The friction felt by $\varphi$ is then increased…

High Energy Physics - Phenomenology · Physics 2022-05-16 P. Klose , M. Laine , S. Procacci

According to the standard lore, a prolonged inflation leaves a quantum field theory in a cold, low entropy state. Thus, some mechanism is needed to reheat this post-inflationary state, leaving a hot, thermal, radiation-dominated Universe.…

High Energy Physics - Theory · Physics 2023-04-26 Alex Buchel

We study a recently proposed running kinetic inflation model in which the inflaton potential becomes flat due to rapid growth of the kinetic term at large inflaton field values. As concrete examples, we build a variety of chaotic inflation…

High Energy Physics - Phenomenology · Physics 2010-12-09 Kazunori Nakayama , Fuminobu Takahashi

If, after primordial inflation, the universe undergoes a relatively long reheating period, it could present a phase of matter domination supported by the oscillating inflaton field. During this epoch, small perturbations from the inflaton…

Cosmology and Nongalactic Astrophysics · Physics 2023-03-30 Luis E. Padilla , Juan Carlos Hidalgo , Gabriel German

Heavy particles with masses much bigger than the inflationary Hubble scale $H_*$, can get non-adiabatically pair produced during inflation through their couplings to the inflaton. If such couplings give rise to time-dependent masses for the…

High Energy Physics - Phenomenology · Physics 2021-12-08 Jeong Han Kim , Soubhik Kumar , Adam Martin , Yuhsin Tsai

This is the first of a three-part series of papers, in which we study the preheating phase for multifield models of inflation involving nonminimal couplings. In this paper, we study the single-field attractor behavior that these models…

Cosmology and Nongalactic Astrophysics · Physics 2018-01-30 Matthew P. DeCross , David I. Kaiser , Anirudh Prabhu , Chanda Prescod-Weinstein , Evangelos I. Sfakianakis

We study the inflationary model with a spectator scalar field $\chi$ coupled to both the inflaton and Ricci scalar. The interaction between the $\chi$ field and the gravity, denoted by $\xi R\chi^2$, can trigger the tachyonic instability of…

General Relativity and Quantum Cosmology · Physics 2024-01-03 Zhe Yu , Chengjie Fu , Zong-Kuan Guo

We study the details of preheating in Palatini Higgs inflation. We show, that contrary to what happens in the metric formulation of the model, the Universe does not reheat through the creation of gauge bosons only, but also through the…

High Energy Physics - Phenomenology · Physics 2019-04-17 Javier Rubio , Eemeli S. Tomberg

We investigate preheating in a higher-dimensional generalized Kaluza-Klein theory with a quadratic inflaton potential $V(\phi)=\frac12 m^2\phi^2$ including metric perturbations explicitly. The system we consider is the multi-field model…

High Energy Physics - Phenomenology · Physics 2009-10-31 S. Tsujikawa

In 'hilltop inflation', inflation takes place when the inflaton field slowly rolls from close to a maximum of its potential (i.e. the 'hilltop') towards its minimum. When the inflaton potential is associated with a phase transition,…

High Energy Physics - Phenomenology · Physics 2015-06-24 Stefan Antusch , David Nolde , Stefano Orani

We consider models for inflation with a stable inflaton. Reheating is achieved through scattering processes such as $\phi \phi \to h h$, where $h$ is the Standard Model Higgs boson. We consider the reheating process in detail and show that…

High Energy Physics - Phenomenology · Physics 2022-02-02 Marcos A. G. Garcia , Yann Mambrini , Keith A. Olive , Sarunas Verner

Coherent oscillations of the inflaton field at the end of inflation can parametrically excite fermions in much the same way that bosons are created in preheating. Although Pauli-blocking prohibits the occupation number of created fermions…

High Energy Physics - Phenomenology · Physics 2009-10-31 Patrick B. Greene

The existence of pseudo-Nambu-Goldstone boson (pNGB) fields is a common feature in many models beyond the Standard Model, characterized by their exclusive derivative couplings. This paper investigates a scenario where a pNGB is coupled to…

High Energy Physics - Phenomenology · Physics 2024-06-14 Kunio Kaneta , Sung Mook Lee , Kin-ya Oda , Tomo Takahashi

We present an explicit cosmological model where inflation and dark energy both could arise from the dynamics of the same scalar field. We present our discussion in the framework where the inflaton field $\phi$ attains a nearly constant…

High Energy Physics - Theory · Physics 2008-11-26 Ishwaree P. Neupane

It has been pointed out that a large non-minimal coupling $\xi$ between the Higgs and the Ricci scalar can source higher derivative operators, which may change the predictions of Higgs inflation. A variant, called critical Higgs inflation,…

High Energy Physics - Phenomenology · Physics 2018-04-03 Alberto Salvio

The coupling between a pseudo-scalar inflaton and a gauge field leads to an amount of additional density perturbations and gravitational waves (GWs) that is strongly sensitive to the inflaton speed. This naturally results in enhanced GWs at…

Cosmology and Nongalactic Astrophysics · Physics 2023-03-24 Juan Garcia-Bellido , Alexandros Papageorgiou , Marco Peloso , Lorenzo Sorbo

We study (p)reheating in modular (closed string) inflationary scenarios, with a special emphasis on Kahler moduli/Roulette models. It is usually assumed that reheating in such models occurs through perturbative decays. However, we find that…

High Energy Physics - Theory · Physics 2010-01-15 Neil Barnaby , J. Richard Bond , Zhiqi Huang , Lev Kofman