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Related papers: Inflaton freeze-out

200 papers

We present a detailed examination of thermalization after inflation for perturbative inflaton decay. Different interactions among particles in the plasma of inflaton decay products are considered and it will be shown that 2 -> 2 scatterings…

High Energy Physics - Phenomenology · Physics 2009-10-31 Rouzbeh Allahverdi

In the Starobinsky model of inflation, the observed dark matter abundance can be produced from the direct decay of the inflaton field only in a very narrow spectrum of close-to-conformal scalar fields and spinors of mass $\sim 10^7$ GeV.…

High Energy Physics - Phenomenology · Physics 2020-11-05 Nicolás Bernal , Javier Rubio , Hardi Veermäe

Assuming gauge/gravity correspondence we study reheating of the Universe using its holographic dual. Inflaton decay and thermalisation of the decay products correspond to collapse of a spherical shell and formation of a blackhole in the…

High Energy Physics - Theory · Physics 2016-06-29 Shinsuke Kawai , Yu Nakayama

We revisit Higgs inflation in the framework of a minimal extension of the Standard Model gauge symmetry by a $U(1)_{B-L}$ factor. Various aspects are taken into account with particular focus on the role of the supersymmetry breaking (SUSY)…

High Energy Physics - Phenomenology · Physics 2021-09-29 Waqas Ahmed , Athanasios Karozas , George K. Leontaris

Spontaneous breaking of conformal symmetry has been widely exploited in successful model building of both inflationary cosmology and particle physics phenomenology. Conformal Grand Unified Theory (CGUT) inflation provides the same scalar…

High Energy Physics - Phenomenology · Physics 2020-07-28 Simone Biondini , K. Sravan Kumar

In this paper we investigate the vacuum stability of the non-minimally coupled Standard-Model Higgs during a phase of kinetic domination following the end of inflation. The non-minimal coupling to curvature stabilises the Higgs fluctuations…

High Energy Physics - Phenomenology · Physics 2024-05-01 Giorgio Laverda , Javier Rubio

We demonstrate how a dark sector can provide a crucial link between a vacuum-dominated early universe and the later radiation-dominated epoch. As an example, we consider a feeble axion-like coupling of dark non-Abelian gauge fields with a…

High Energy Physics - Phenomenology · Physics 2024-09-19 Simone Biondini , Helena Kolesova , Simona Procacci

The existence of Dark Matter (DM) has been well established from various cosmological and astrophysical evidences. However, the particle properties of DM are largely undetermined and attempts to probe its interactions with the Standard…

High Energy Physics - Phenomenology · Physics 2018-12-26 Nicolás Bernal , Arindam Chatterjee , Arnab Paul

In this letter I discuss a class of extensions of the standard model that have a minimal number of possible parameters, but can in principle explain dark matter and inflation. It is pointed out that the so-called new minimal standard model…

High Energy Physics - Phenomenology · Physics 2009-11-11 J. J. van der Bij

In supersymmetric models of warm inflation, the large temperature of the radiation bath produced by the dissipative motion of the inflaton field may induce a significant thermal abundance of potentially dangerous gravitinos. While previous…

High Energy Physics - Phenomenology · Physics 2013-01-16 Sam Bartrum , Arjun Berera , Joao G. Rosa

In the present work we study non-thermal leptogenesis and baryon asymmetry in the universe in different neutrino mass models discussed recently. For each model we obtain a formula relating the reheating temperature after inflation to the…

High Energy Physics - Phenomenology · Physics 2008-11-26 G. Panotopoulos

In this work, we study the non-minimally-coupled Higgs model in the context of warm inflation scenario on both metric and Palatini approaches. We particularly consider a dissipation parameter of the form $\Gamma=C_{T}T$ with $C_{T}$ being a…

General Relativity and Quantum Cosmology · Physics 2023-07-20 Thammarong Eadkhong , Punsiri Dam-O , Phongpichit Channuie , Davood Momeni

We study in detail a scenario in which the inflaton scalar field couples to both a visible sector (VS) and a hidden sector (HS). The VS is assumed to contain the Standard Model (SM), while the HS contains a dark matter (DM) candidate. We…

High Energy Physics - Phenomenology · Physics 2026-05-12 Simon Cléry , Jean Kimus , Michel H. G. Tytgat

The axion is a well-motivated candidate for the inflaton, as the radiative corrections that spoil many single-field models are avoided by virtue of its shift symmetry. However, axions generically couple to gauge sectors. As the axion…

High Energy Physics - Phenomenology · Physics 2021-11-09 William DeRocco , Peter W. Graham , Saarik Kalia

Since an acceptable dark matter candidate may interact only weakly with ordinary matter and radiation, it is of interest to consider the limiting case where the dark matter interacts only with gravity and itself, the matter originating by…

Astrophysics · Physics 2016-08-25 P. J. E. Peebles , A. Vilenkin

The Starobinsky inflation model is one of the simplest inflation models that is consistent with the cosmic microwave background observations. In order to explain dark matter of the universe, we consider a minimal extension of the…

High Energy Physics - Phenomenology · Physics 2022-07-27 Qiang Li , Takeo Moroi , Kazunori Nakayama , Wen Yin

During inflation in the early universe, the Higgs field continuously acquires long-wave quantum fluctuations. They accumulate to yield a non-vanishing value with an exponentially large correlation length. We study consequences of such Higgs…

High Energy Physics - Phenomenology · Physics 2012-10-30 Taro Kunimitsu , Jun'ichi Yokoyama

Dynamics of the inflaton is studied when it interacts with boson and fermion fields and in minimal supersymmetric models. This encompasses multifield inflation models, such as hybrid inflation, and typical reheating models. For much of the…

High Energy Physics - Phenomenology · Physics 2009-11-10 Arjun Berera , Rudnei O. Ramos

One of the simplest possible candidates for dark matter is a stable scalar singlet beyond the Standard Model. If its mass is below the Hubble scale during inflation, long-wavelength modes of this scalar will be excited during inflation, and…

High Energy Physics - Phenomenology · Physics 2025-03-03 Marcos A. G. Garcia , Wenqi Ke , Yann Mambrini , Keith A. Olive , Sarunas Verner

The end of a thermal inflation era, driven by the rolling of a flaton field coupled to the curvaton, cause a huge increment in the curvaton mass and decay rate while the curvaton is still frozen. It is shown that, if this increment is…

High Energy Physics - Phenomenology · Physics 2009-04-08 Yeinzon Rodriguez