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Related papers: GUT Baryogenesis after Preheating

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$R^2$-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

We investigate thermal leptogenesis within a supersymmetric grand unified theory (SUSY GUT) based on the $SO(10) \times U(1)_A$ symmetry, where both the doublet--triplet splitting problem and the unrealistic Yukawa relations are resolved…

High Energy Physics - Phenomenology · Physics 2025-11-17 Nobuhiro Maekawa , Kei Shibata , Masato Yamanaka

The possible role of supersymmetry in our understanding of big bang baryogenesis and cosmological dark matter is explored. The discussion will be limited to the out-of equilibrium decay scenario in SUSY GUTs, the decay of scalar…

High Energy Physics - Phenomenology · Physics 2016-09-01 Keith A. Olive

An overview of baryogenesis in the early Universe is presented. The standard big bang model including big bang nucleosynthesis and inflation is breifly reviewed. Three basic models for baryogenesis will be developed: The ``standard"…

High Energy Physics - Phenomenology · Physics 2015-06-25 Keith A. Olive

We propose a novel framework where baryon asymmetry of the universe can arise due to forbidden decay of dark matter (DM) enabled by finite-temperature effects in the vicinity of a first order phase transition (FOPT). In order to implement…

High Energy Physics - Phenomenology · Physics 2023-10-13 Debasish Borah , Arnab Dasgupta , Matthew Knauss , Indrajit Saha

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

Late-decaying string moduli dilute the baryon asymmetry of the universe created in any previous era. The reheat temperature for such moduli is below a GeV, thus motivating baryogenesis at very low temperatures. We present an extension of…

High Energy Physics - Phenomenology · Physics 2014-11-21 Rouzbeh Allahverdi , Bhaskar Dutta , Kuver Sinha

It was recently found that the decay of inflaton and the SUSY breaking field produces many gravitinos in the gravity mediation scenario. These discoveries led to an exclusion of many inflation models such as chaotic, (smooth) hybrid,…

High Energy Physics - Phenomenology · Physics 2008-11-26 H. Nakajima , Y. Shinbara

We investigate the impact of preheating on baryogenesis in $R^2$-Higgs inflation. In this scenario, the inclusion of a dimension-six operator ${(R/ \Lambda^2)} B_{\mu\nu} \widetilde{B}^{\mu\nu} $ abundantly generates helical hypermagnetic…

High Energy Physics - Phenomenology · Physics 2025-01-28 Yann Cado , Christoph Englert , Tanmoy Modak , Mariano Quirós

We consider the presence of cosmic string induced density fluctuations in the universe at temperatures below the electroweak phase transition temperature. Resulting temperature fluctuations can restore the electroweak symmetry locally,…

High Energy Physics - Phenomenology · Physics 2009-11-07 Biswanath Layek , Soma Sanyal , Ajit M. Srivastava

We present real-time lattice simulations of Cold Electroweak Baryogenesis, in which the baryon asymmetry of the Universe is generated during tachyonic electroweak symmetry breaking at the end of inflation. In the minimal realisation of the…

High Energy Physics - Phenomenology · Physics 2008-11-26 Anders Tranberg , Jan Smit , Mark Hindmarsh

We reconsider a class of well motivated supersymmetric models in which inflation is associated with the breaking of a gauge symmetry G to H, with the symmetry breaking scale M~10^16 GeV. Starting with a renormalizable superpotential, we…

High Energy Physics - Phenomenology · Physics 2008-11-26 V. N. Senoguz , Q. Shafi

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 present a novel baryogenesis mechanism in which the asymmetry is sourced from heavy particles which either gain their mass or are created during bubble expansion in a strong first order phase transition. These particles then decay in a…

High Energy Physics - Phenomenology · Physics 2022-01-12 Iason Baldes , Simone Blasi , Alberto Mariotti , Alexander Sevrin , Kevin Turbang

The preheating after the inflation, which can be interpreted as particle creation in the oscillating inflaton background, provides a state far from thermal equilibrium. We extend the field theoretical treatment of the preheating by Linde et…

High Energy Physics - Phenomenology · Physics 2009-10-31 K. Funakubo , A. Kakuto , S. Otsuki , F. Toyoda

Leptogenesis scenarios in supersymmetric hybrid inflation models are considered. Sufficient lepton asymmetry leading to successful baryogenesis can be obtained if the reheat temperature T_r>10^6 GeV and the superpotential coupling parameter…

High Energy Physics - Phenomenology · Physics 2008-11-26 V. N. Senoguz , Q. Shafi

The observed baryon asymmetry of the Universe is suitably created in thermal leptogenesis through the out-of-equilibrium decay of $N_1$, the lightest of the three heavy singlet neutral fermions which anchor the seesaw mechanism to obtain…

High Energy Physics - Phenomenology · Physics 2007-05-23 Ernest Ma , Narendra Sahu , Utpal Sarkar

Baryogenesis appears to require lepton number violation. This is naturally realized in extensions of the standard model containing right-handed neutrinos. We discuss the generation of a baryon asymmetry by the out-of-equilibrium decay of…

High Energy Physics - Phenomenology · Physics 2007-05-23 W. Buchmuller , M. Plumacher

We discuss the possibility of generating the baryon asymmetry of the Universe when the temperature of the Universe is much below the electroweak scale. In our model the evaporation of primordial black holes or the decay of massive particles…

High Energy Physics - Phenomenology · Physics 2011-05-23 Raghavan Rangarajan , Supratim Sengupta , Ajit M. Srivastava , ;

In this letter, we quantify the challenge of explaining the baryon asymmetry using initial conditions in a universe that undergoes inflation. Contrary to lore, we find that such an explanation is possible if net $B-L$ number is stored in a…

High Energy Physics - Phenomenology · Physics 2017-09-06 Gordan Krnjaic