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We present a novel scenario for baryogenesis in a hybrid inflation model at the electroweak scale, in which the Standard Model Higgs field triggers the end of inflation. One of the conditions for successful baryogenesis, the departure from…

High Energy Physics - Phenomenology · Physics 2016-08-25 Juan Garcia-Bellido , Dmitri Grigoriev , Alexander Kusenko , Mikhail Shaposhnikov

Certain inflation models undergo pre-heating, in which inflaton oscillations can drive parametric resonance instabilities. We discuss several phenomena stemming from such instabilities, especially in weak-scale models; generically, these…

High Energy Physics - Phenomenology · Physics 2009-10-31 John M. Cornwall , Alexander Kusenko

At the end of inflation, the coherent oscillations of the inflaton field may resonantly amplify the long wavelength modes of both bosons and fermions coupled to it. We study the resonant production of both kinds of particles during…

High Energy Physics - Phenomenology · Physics 2009-10-31 Juan Garcia-Bellido , Silvia Mollerach , Esteban Roulet

We review recent progress in the understanding of the preheating stage of Higgs inflation formulated within the Einstein-Cartan framework of gravity. This setup smoothly interpolates between the metric and Palatini formulations of the…

High Energy Physics - Phenomenology · Physics 2026-03-20 Javier Rubio

If the inflaton field is coupled to the hypercharge Chern-Simons density $F\tilde F$, an explosive production of helical gauge fields when inflation ends can trigger baryogenesis at the electroweak phase transition. Besides, Higgs inflation…

High Energy Physics - Phenomenology · Physics 2023-07-26 Yann Cado , Mariano Quirós

It has recently been suggested that the baryon washout problem of the standard electroweak baryogenesis scenario could be avoided if inflation ends with a period of parametric resonance at a low enough energy density. I present results of…

High Energy Physics - Phenomenology · Physics 2017-08-23 A. Rajantie

In this letter we show that the inflaton can generate the cosmological baryon asymmetry. We take the inflaton to be a complex scalar field with a weakly broken global symmetry and develop a new variant on the Affleck-Dine mechanism. The…

High Energy Physics - Phenomenology · Physics 2014-08-26 Mark P. Hertzberg , Johanna Karouby

In many inflationary models, a large amount of energy is transferred rapidly to the long-wavelength matter fields during a period of preheating after inflation. We study how this changes the dynamics of the electroweak phase transition if…

High Energy Physics - Phenomenology · Physics 2009-10-31 A. Rajantie , P. M. Saffin , E. J. Copeland

We propose a mechanism by which the inflaton can generate baryogenesis, by taking the inflaton to be a complex scalar field with a weakly broken global symmetry and present a new version of the Affleck-Dine mechanism. The smallness of the…

High Energy Physics - Phenomenology · Physics 2014-04-02 Mark P. Hertzberg , Johanna Karouby

In models of inflation driven by an axion-like pseudoscalar field, the inflaton, a, may couple to the standard model hypercharge via a Chern-Simons-type interaction, $L \subset a/(4\Lambda) F\tilde{F}$. This coupling results in explosive…

High Energy Physics - Phenomenology · Physics 2017-12-20 Daniel Jimenez , Kohei Kamada , Kai Schmitz , Xun-Jie Xu

The baryon asymmetry of the universe may originate in the phase transition at the end of hybrid inflation, provided that the reheat temperature is low enough. I show that if the field that triggers the end of inflation is the electroweak…

High Energy Physics - Phenomenology · Physics 2007-05-23 Arttu Rajantie

$R^2$-Higgs inflation stands out as one of the best-fit models of Planck data. Using a covariant formalism for the inflationary dynamics and the production of helical gauge fields, we show that the observed baryon asymmetry of the Universe…

Cosmology and Nongalactic Astrophysics · Physics 2024-02-20 Yann Cado , Christoph Englert , Tanmoy Modak , Mariano Quirós

In this study, we introduce a novel approach aimed at addressing the longstanding baryon-anti-baryon asymmetry conundrum. Our proposed mechanism suggests that baryon numbers were generated during the inflationary epoch through the dynamics…

Cosmology and Nongalactic Astrophysics · Physics 2024-09-10 Haipeng An , Qi Chen , Yuan Yin

The electroweak symmetry breaking transition may supply the appropriate out-of-equilibrium conditions for baryogenesis if it is triggered sufficiently fast. This can happen at the end of low-scale inflation, prompting baryogenesis to occur…

High Energy Physics - Phenomenology · Physics 2010-10-27 Anders Tranberg , Jan Smit , Mark Hindmarsh

The dynamics of both the preinflationary and the preheating epochs for a model consisting of a Higgs inflaton plus an additional auxiliary field are studied in full General Relativity. The minimally coupled auxiliary field allows for…

Cosmology and Nongalactic Astrophysics · Physics 2022-07-20 Cristian Joana

A scalar Higgs field can be repeatedly switched on and off when it couples to a classically oscillating scalar modulus field. The modulus flips the Higgs mass term between stable and tachyonic values. We study a cosmological scenario in…

High Energy Physics - Theory · Physics 2020-05-20 JiJi Fan , Matthew Reece , Yi Wang

We consider the generation of the baryon asymmetry in models with right-handed neutrinos produced through gravitational scattering of the inflaton during reheating. The right-handed neutrinos later decay and generate a lepton asymmetry,…

High Energy Physics - Phenomenology · Physics 2022-05-05 Raymond T. Co , Yann Mambrini , Keith A. Olive

We examined the possibility of spontaneous baryogenesis driven by the inflaton in the scenario of \textit{spiral inflation}, and found the parametric dependence of the late-time baryon number asymmetry. As a result, it is shown that,…

High Energy Physics - Phenomenology · Physics 2019-06-26 Gabriela Barenboim , Wan-Il Park

We present an effective model where the inflaton is a relaxion that scans the Higgs mass and sets it at the weak scale. The dynamics consist of a long epoch in which inflation is due to the shallow slope of the potential, followed by a few…

High Energy Physics - Phenomenology · Physics 2017-06-05 Walter Tangarife , Kohsaku Tobioka , Lorenzo Ubaldi , Tomer Volansky

We consider the complex inflaton field with a CP asymmetric term for its potential. This CP asymmetric term produces the global charge of the inflaton after inflation. With the assignment of the baryon number to the inflaton, the baryon…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-28 Naoyuki Takeda
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