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相关论文: GUT Baryogenesis after Preheating

200 篇论文

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…

高能物理 - 唯象学 · 物理学 2014-11-17 Bruce A. Bassett , Stefano Liberati

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…

高能物理 - 唯象学 · 物理学 2008-11-26 G. Panotopoulos

The process of baryogenesis through the evaporation of black holes formed at the end of inflation phase is considered. The increase of black hole mass due to accretion from the surrounding radiation after the reheating is taken into…

天体物理学 · 物理学 2015-06-24 E. V. Bugaev , M. G. Elbakidze , K. V. Konishchev

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…

高能物理 - 唯象学 · 物理学 2007-05-23 Arttu Rajantie

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…

高能物理 - 唯象学 · 物理学 2014-12-05 Kaloian D. Lozanov , Mustafa A. Amin

No-scale supergravity and the flipped SU(5)$\times$U(1) gauge group provide an ambitious prototype string-inspired scenario for physics below the string scale, which can accommodate the Starobinsky-like inflation favoured by observation…

高能物理 - 唯象学 · 物理学 2019-04-17 John Ellis , Marcos A. G. Garcia , Natsumi Nagata , Dimitri V. Nanopoulos , Keith A. Olive

In this letter we explore the possibility of creating the baryon asymmetry of the universe during inflation and reheating due to the decay of a field associated with the inflaton. CP violation is attained by assuming that this field is…

高能物理 - 唯象学 · 物理学 2014-11-17 D. V. Nanopoulos , Raghavan Rangarajan

We discuss two important modifications of inflationary paradigm. Until very recently we believed that inflation automatically leads to flatness of the universe, Omega = 1. We also thought that post-inflationary phase transitions in GUTs may…

天体物理学 · 物理学 2007-05-23 Andrei Linde

We discuss a mechanism for producing baryon density perturbations during inflationary stage and study the evolution of the baryon charge density distribution in the framework of the low temperature baryogenesis scenario. This mechanism may…

天体物理学 · 物理学 2009-10-31 D. P. Kirilova , M. V. Chizhov

The gravitational baryogenesis plays an important role in the study of the baryon asymmetry. However, the original mechanism of gravitational baryogenesis in the radiation dominated era leads to the asymmetry factor $\eta$ is equal to zero,…

广义相对论与量子宇宙学 · 物理学 2022-07-12 Zhong-Wen Feng , Xia Zhou , Shi-Qi Zhou

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…

宇宙学与河外天体物理 · 物理学 2024-09-10 Haipeng An , Qi Chen , Yuan Yin

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…

高能物理 - 唯象学 · 物理学 2007-05-23 Alexander Kusenko

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…

高能物理 - 唯象学 · 物理学 2009-11-11 Bjorn Garbrecht , Tomislav Prokopec , Michael G. Schmidt

We study the details of preheating in Palatini Higgs inflation. We show, that contrary to what happens in the metric formulation of the model, the Universe does not reheat through the creation of gauge bosons only, but also through the…

高能物理 - 唯象学 · 物理学 2019-04-17 Javier Rubio , Eemeli S. Tomberg

We consider the construction of inverted hybrid inflation models in which the vacuum energy during inflation is at the TeV scale, and the inflaton couples to the Higgs field. Such models are of interest in the context of some recently…

高能物理 - 唯象学 · 物理学 2009-11-07 Edmund J. Copeland , David Lyth , Arttu Rajantie , Mark Trodden

We propose a framework of baryogenesis and leptogenesis that relies on a supercooled confining phase transition (PT) in the early universe. The baryon or lepton asymmetry is sourced by decays of hadrons of the strong dynamics after the PT,…

高能物理 - 唯象学 · 物理学 2024-01-25 Maximilian Dichtl , Jacopo Nava , Silvia Pascoli , Filippo Sala

These lectures provide a pedagogical review of the present status of theories explaining the observed baryon asymmetry of the Universe. Particular emphasis is given on GUT baryogenesis and electroweak baryogenesis. The key issues, the…

高能物理 - 唯象学 · 物理学 2007-05-23 Antonio Riotto

It has been considered that baryogenesis models without a generation of $B$-$L$ asymmetry such as the GUT baryogenesis do not work since the asymmetry is washed out by the electroweak sphalerons. Here, we point out that helical…

高能物理 - 唯象学 · 物理学 2018-07-05 Kohei Kamada

We consider an inflationary model in the hidden-sector broken supergravity with an effectively large cutoff. The inflaton decay into right-handed neutrinos naturally causes the observed baryon asymmetry of the universe with a reheating…

高能物理 - 唯象学 · 物理学 2009-11-11 M. Ibe , K. -I. Izawa , Y. Shinbara , T. T. Yanagida

We revisit the gravitational leptogenesis scenario in which the inflaton is coupled to gravity by the Chern-Simons term and the lepton asymmetry is generated through the gravitational anomaly in the lepton number current during inflation.…

高能物理 - 唯象学 · 物理学 2020-02-05 Kohei Kamada , Jun'ya Kume , Yusuke Yamada , Jun'ichi Yokoyama