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Related papers: Warm baryogenesis

200 papers

We show that both the baryon asymmetry of the Universe and the dark matter abundance can be explained within a single framework that makes use of maximally helical hypermagnetic fields produced during pseudoscalar inflation and the chiral…

High Energy Physics - Phenomenology · Physics 2019-10-10 Yann Cado , Eray Sabancilar

Recent studies suggest that the process of symmetry breaking after inflation typically occurs very fast, within a single oscillation of the symmetry-breaking field, due to the spinodal growth of its long-wave modes, otherwise known as…

High Energy Physics - Phenomenology · Physics 2009-11-07 Juan Garcia-Bellido , Ester Ruiz Morales

The concept of early Universe inflation resolves several problems of hot Big Bang theory and quantitatively explains the origin of the inhomogeneities in the present Universe. However, it is not possible to arrange inflation in a scalar…

High Energy Physics - Phenomenology · Physics 2024-02-06 Anna Tokareva

Simply on CP arguments, we argue against a Standard Model explanation of baryogenesis via the charge transport mechanism. A CP-asymmetry is found in the reflection coefficients of quarks hitting the electroweak phase boundary created during…

High Energy Physics - Phenomenology · Physics 2008-02-03 M. B. Gavela , P. Hernández , J. Orloff , O. Pène

We propose a universal mechanism of producing dark matter and baryon (lepton) charge at the stage of the quasi-de Sitter expansion of the Universe---inflation. The key ingredient of the mechanism is a linear coupling of the field,…

Cosmology and Nongalactic Astrophysics · Physics 2018-07-04 Eugeny Babichev , Dmitry Gorbunov , Sabir Ramazanov

Multi-natural inflation is studied in the context of warm inflation. We study the warm multi-natural inflation scenario with both linear and cubic temperature-dependent dissipation coefficients. The model is motivated by axion-like…

High Energy Physics - Phenomenology · Physics 2025-09-01 Asuka Ito , Rudnei O. Ramos

We discuss leptogenesis in a realistic supersymmetric model of inflation with a low reheat temperature 1-10 GeV. The lepton asymmetry is generated by a decaying right handed sneutrino, which is produced after inflation during preheating.…

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

We calculate the baryon asymmetry created by the decay of a pseudo Nambu-Goldstone boson whose interactions violate baryon number conservation. Our results are in disagreement with previous results in the original spontaneous baryogenesis…

High Energy Physics - Phenomenology · Physics 2009-10-30 Alexandre Dolgov , Katherine Freese , Raghavan Rangarajan , Mark Srednicki

A two-components mixture fluid which complies with the gamma law is considered in the framework of inflation with finite temperature. The model is developed for a quartic scalar potential without symmetry breaking. The radiation energy…

General Relativity and Quantum Cosmology · Physics 2009-11-07 Mauricio Bellini

In a previous paper, we proposed a simple extension of the Minimal Supersymmetric Standard Model which gives rise to thermal inflation and baryogenesis in a natural and remarkably consistent way. In this paper, we consider the $\lambda_\phi…

High Energy Physics - Phenomenology · Physics 2009-02-12 Seongcheol Kim , Wan-Il Park , Ewan D. Stewart

A model for GUT baryogenesis, coherent baryogenesis within the framework of supersymmetric SO(10), is considered. In particular, we discuss the Barr-Raby model, where at the end of hybrid infl ation charge asymmetries can be created through…

High Energy Physics - Phenomenology · Physics 2009-11-11 Bjorn Garbrecht , Tomislav Prokopec , Michael G. Schmidt

We use the general formalism of squeezed rotated states to calculate baryon asymmetry in the wake of inflation through parametric amplification. We base our analysis on a B and CP violating Lagrangian in an isotropically expanding universe.…

General Relativity and Quantum Cosmology · Physics 2008-11-26 Bindu A. Bambah , K. V. S. Shiv Chaitanya , C. Mukku

Several models of baryo(lepto)-genesis that give rise to large inhomogeneities in the composition of the universe are presented. In particular, a variation of primordial abundances of light elements by the factor 2-5 at large distances is…

High Energy Physics - Phenomenology · Physics 2007-05-23 A. D. Dolgov

Inflationary reheating via resonant production of non-minimally coupled scalar particles with only gravitational coupling is shown to be extremely strong, exhibiting a negative coupling instability for $\xi < 0$ and a wide resonance decay…

High Energy Physics - Phenomenology · Physics 2014-11-17 Bruce A. Bassett , Stefano Liberati

The "gravitational baryogenesis" scenario is extended to generate both baryon and dark matter asymmetries, in the matter dominated era corresponding to post-inflationary reheating. A minimal extension requires a singlet fermion X for dark…

High Energy Physics - Phenomenology · Physics 2013-11-13 Hooman Davoudiasl

We consider a baryogenesis scenario, where the difference of baryon (B) and lepton (L) number is conserved in such a way that the B-L asymmetry in the standard model sector is compensated by an asymmetry of opposite sign stored in the dark…

High Energy Physics - Phenomenology · Physics 2010-11-26 Florian Bauer , Marc-Thomas Eisele , Mathias Garny

We present an inflationary scenario based on a phenomenologically viable model with direct gauge mediation of low-scale supersymmetry breaking. Inflation can occur in the supersymmetry-breaking hidden sector. Although the reheating…

High Energy Physics - Phenomenology · Physics 2011-06-06 Kohei Kamada , Yuichiro Nakai , Manabu Sakai

The nonsupersymmetric as well as the supersymmetric hybrid inflationary model is reviewed. The scenario of baryogenesis via a primordial leptogenesis is discussed and the role of the nonperturbative electroweak sphaleron effects is…

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

We study the imprints of high scale non-thermal leptogenesis on cosmic microwave background (CMB) from the measurements of inflationary spectral index ($n_s$) and tensor-to-scalar ratio ($r$), which otherwise is inaccessible to the…

High Energy Physics - Phenomenology · Physics 2024-04-25 Anish Ghoshal , Dibyendu Nanda , Abhijit Kumar Saha

Once a light axionlike scalar field couples to the electroweak gauge bosons, its classical motion during reheating induces an effective chemical potential for the fermion number. In the presence of rapid lepton number (L)-violating…

High Energy Physics - Phenomenology · Physics 2015-07-08 Alexander Kusenko , Kai Schmitz , Tsutomu T. Yanagida