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Related papers: Warm baryogenesis

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The dynamics at the end of inflation can generate an asymmetry between particles and anti-particles of the inflaton field. This asymmetry can be transferred to baryons via decays, generating a baryon asymmetry in our Universe. We explore…

High Energy Physics - Phenomenology · Physics 2014-12-05 Kaloian D. Lozanov , Mustafa A. Amin

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

We study the evolution of a cosmological baryon asymmetry in leptogenesis when the right-handed neutrinos are produced in inflaton decays. By performing a detailed numerical study over a broad range of inflaton-neutrino couplings we show…

High Energy Physics - Phenomenology · Physics 2008-11-26 F. Hahn-Woernle , M. Plumacher

We propose that the baryon asymmetry of the Universe may originate from the amplification of quantum fluctuations of a light complex scalar field during inflation. CP-violation is sourced by complex mass terms, which are smaller than the…

Astrophysics · Physics 2008-12-18 Bjorn Garbrecht , Tomislav Prokopec

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

We study the generation of baryon asymmetry as well as dark matter (DM) in an extended reheating period after the end of slow-roll inflation. Within the regime of perturbative reheating, we consider different monomial potential of the…

High Energy Physics - Phenomenology · Physics 2025-02-27 Basabendu Barman , Arindam Basu , Debasish Borah , Amit Chakraborty , Rishav Roshan

We argue that inflationary dynamics may support a scenario where significant matter-antimatter asymmetry is generated from initially small-scale quantum fluctuations that are subsequently stretched out over large scales. This scenario can…

High Energy Physics - Phenomenology · Physics 2015-06-18 Neil D. Barrie , Archil Kobakhidze

We present a new mechanism for baryogenesis: at preheating after inflation fermions acquire a varying mass by their coupling to a time dependent field. Their CP-violating mass matrix can generate a charge asymmetry to be transformed into a…

High Energy Physics - Phenomenology · Physics 2017-08-23 Bjorn Garbrecht , Tomislav Prokopec , Michael G. Schmidt

Baryogenesis driven by curvature effects is investigated by taking into account gravitationally induced particle production in the very early Universe. In our scenario, the baryon asymmetry is generated dynamically during an inflationary…

General Relativity and Quantum Cosmology · Physics 2016-11-23 J. A. S. Lima , Douglas Singleton

A variation of Affleck-Dine mechanism was proposed to generate the observed baryon asymmetry in [1], in which the inflaton was assumed to be a complex scalar field with a weakly broken $U(1)$ symmetry, and the baryon asymmetry generation…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-22 Nan Li , Ding-fang Zeng

Electroweak baryogenesis could be very efficient at the end of an electroweak-scale inflation. Reheating that followed inflation could create a highly non-equilibrium plasma, in which the baryon number violating transitions were rapid. In…

High Energy Physics - Phenomenology · Physics 2007-05-23 Alexander Kusenko

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 supergravity models (such as standard superstring constructions) that possess a Heisenberg symmetry, supersymmetry breaking by the inflationary vacuum energy does not lift flat directions at tree level. One-loop corrections give small…

High Energy Physics - Phenomenology · Physics 2009-09-15 Bruce A. Campbell , Mary K. Gaillard , Hitoshi Murayama , Keith A. Olive

We propose a new scenario of Affleck-Dine baryogenesis where a flat direction in the MSSM generates B-L asymmetry just after the end of inflation. The resulting amount of baryon asymmetry is independent of low-energy supersymmetric models…

High Energy Physics - Phenomenology · Physics 2016-04-27 Masaki Yamada

Thermal inflation is an attractive idea to dilute cosmic density of unwanted particles such as moduli fields which cause cosmological difficulties. However, it also dilutes preexisting baryon asymmetry and some viable baryogenesis is…

High Energy Physics - Phenomenology · Physics 2016-04-06 Taku Hayakawa , Masahiro Kawasaki , Masaki Yamada

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

We study an inflection point inflation scenario where a flat direction of the minimal supersymmetric standard model (MSSM) is identified with the inflaton. We focus on the case where the flat direction (inflaton) has non-zero baryon number,…

High Energy Physics - Phenomenology · Physics 2024-10-17 Naoyuki Haba , Yasuhiro Shimizu , Yoshihiro Tanabe , Toshifumi Yamada

The coupling of an axion-like particle driving inflation to the Standard Model particle content through a Chern-Simons term generically sources a dual production of massless helical gauge fields and chiral fermions. We demonstrate that the…

High Energy Physics - Phenomenology · Physics 2019-10-16 Valerie Domcke , Benedict von Harling , Enrico Morgante , Kyohei Mukaida

I describe a new way for baryogenesis to proceed, which evades many of the problems of GUT and electroweak scenarios. If the reheat temperature after inflation is below the electroweak scale, neither GUT baryon production nor traditional…

High Energy Physics - Phenomenology · Physics 2016-11-03 Mark Trodden

We propose a scenario for the generation of baryon number asymmetry based on the inflaton decay in a radiative neutrino mass model extended with singlet scalars. In this scenario, lepton number asymmetry is produced through the decay of…

High Energy Physics - Phenomenology · Physics 2016-08-24 Daijiro Suematsu