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We reconsidered leptogenesis scenario from right-handed (s)neutrino produced by the decay of inflaton. Besides the well-investigated case that the neutrino decays instantaneously after the production, leptogenesis is possible if neutrino…

高能物理 - 唯象学 · 物理学 2010-04-30 Masato Senami , Tsutomu Takayama

The baryon asymmetry of the Universe should have been produced after the inflation era. We consider the possibility that the asymmetry is generated by the flavor oscillations in the reheating process after inflation, so that the baryon…

高能物理 - 唯象学 · 物理学 2016-11-10 Yuta Hamada , Ryuichiro Kitano

We present a non-thermal leptogenesis scenario following standard supersymmetric hybrid inflation, in the case where light neutrinos acquire mass via the usual seesaw mechanism and inflaton decay to heavy right-handed neutrino superfields…

高能物理 - 唯象学 · 物理学 2009-11-11 Thomas Dent , George Lazarides , Roberto Ruiz de Austri

We propose that the observed baryon asymmetry of the Universe can naturally arise from a net asymmetry generated in the sleptonic sector at fairly low reheat temperatures. The best candidate is indeed the right-handed sneutrino. The initial…

高能物理 - 唯象学 · 物理学 2009-11-10 Rouzbeh Allahverdi , Bhaskar Dutta , Anupam mazumdar

We show that the process of non-instantaneous reheating during the post-inflationary period can have a sizable impact on the charged lepton Yukawa equilibration temperature in the early Universe. This suggests relooking the effects of…

高能物理 - 唯象学 · 物理学 2024-01-19 Arghyajit Datta , Rishav Roshan , Arunansu Sil

We present a model with minimal assumptions for non-thermal leptogenesis with almost degenerate superheavy right-handed neutrinos in a supersymmetric set up. In this scenario a gauge singlet inflaton is directly coupled to the right-handed…

高能物理 - 唯象学 · 物理学 2009-11-07 Rouzbeh Allahverdi , Anupam Mazumdar

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…

高能物理 - 唯象学 · 物理学 2008-11-26 V. N. Senoguz , Q. Shafi

We discuss the reheating temperature in the instant preheating scenario. In this scenario, at the last stage of inflation, the inflaton field first decays into another scalar field with an enormous number density via the instant preheating…

高能物理 - 唯象学 · 物理学 2007-05-23 Takeshi Fukuyama , Tatsuru Kikuchi , Wade Naylor

The onset of inflation in hybrid models require fine tuning in the initial conditions. The inflaton field should have an initial value close to the Planck scale $M_{P}$, whereas the auxiliary "orthogonal" field must be close to zero with an…

高能物理 - 唯象学 · 物理学 2009-11-07 Zurab Berezhiani , Anupam Mazumdar , Abdel Pérez-Lorenzana

We analyze lepton asymmetry induced in the decay of right--handed neutrinos in a class of minimal left--right symmetric models. In these models, which assume low energy supersymmetry, the Dirac neutrino mass matrix is proportional to the…

高能物理 - 唯象学 · 物理学 2015-06-25 K. S. Babu , A. Bachri , H. Aissaoui

We study if leptogenesis works successfully together with the neutrino mass anarchy hypothesis. We find that the predicted neutrino mass spectrum is sensitive to the reheating temperature or the inflaton mass, while the distributions of the…

高能物理 - 唯象学 · 物理学 2012-08-03 Kwang Sik Jeong , Fuminobu Takahashi

We show that the leptogenesis is automatic within the supersymmetric standard model if there exist right-handed neutrinos with mass less than $H_{\it inf}$, the expansion rate during the inflation. Its scalar component grows during the…

高能物理 - 唯象学 · 物理学 2009-09-29 Hitoshi Murayama , T. Yanagida

Symmetry restoration processes during the non-equilibrium stage of ``preheating'' after inflation is studied. It is shown that symmetry restoration is very efficient when the majority of created particles are concentrated at energies much…

高能物理 - 理论 · 物理学 2009-10-28 I. I. Tkachev

We present a unified model where the same scalar field can drive inflation and account for the present dark matter abundance. This scenario is based on the incomplete decay of the inflaton field into right-handed neutrino pairs, which is…

高能物理 - 唯象学 · 物理学 2025-02-14 Antonio Torres Manso , Joao G. Rosa

Leptogenesis is studied within the seesaw neutrino mass model in a regime where all sterile neutrinos have prompt rather than delayed decays. It is shown that during neutrino thermal production lepton asymmetries are generated in both…

高能物理 - 唯象学 · 物理学 2007-05-23 Luis Bento

We use modular symmetry as an organizing principle that attempts to simultaneously address the lepton flavor puzzle, inflation, and post-inflationary reheating. We demonstrate this approach using the finite modular group $A_4$ in the lepton…

高能物理 - 唯象学 · 物理学 2025-11-05 Gui-Jun Ding , Si-Yi Jiang , Yong Xu , Wenbin Zhao

We examine the impact of charged lepton Yukawa equilibration on leptogenesis during gravitational reheating. During the post-inflationary era, the inflaton field is assumed to oscillate around the minimum of a monomial potential, leading to…

高能物理 - 唯象学 · 物理学 2025-05-30 Basabendu Barman , Arghyajit Datta , Md Riajul Haque

We perform a thorough study of thermal leptogenesis adding finite temperature effects, RGE corrections, scatterings involving gauge bosons and by properly avoiding overcounting on-shell processes. Assuming hierarchical right-handed…

高能物理 - 唯象学 · 物理学 2026-04-17 G. F. Giudice , A. Notari , M. Raidal , A. Riotto , A. Strumia

We study preheating after hilltop inflation where the inflaton couples to another scalar field, e.g. a right-handed sneutrino, which provides a mechanism for generating the correct initial conditions for inflation and also a decay channel…

高能物理 - 唯象学 · 物理学 2016-02-26 Stefan Antusch , Francesco Cefala , David Nolde , Stefano Orani

Reheating after inflation occurs due to particle production by the oscillating inflaton field. In this paper we describe the perturbative approach to reheating, and then concentrate on effects beyond the perturbation theory. They are…

高能物理 - 唯象学 · 物理学 2009-09-29 Lev Kofman , Andrei Linde , Alexei Starobinsky