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相关论文: GUT Baryogenesis after Preheating

200 篇论文

At the end of inflation the Universe is frozen in a near zero-entropy state with energy density in a coherent scalar field and must be "defrosted" to produce the observed entropy and baryon number. Baryon asymmetry may be generated by the…

高能物理 - 唯象学 · 物理学 2007-05-23 A. Riotto

We perform a fully non-linear calculation of the production of supermassive Grand Unified Theory (GUT) $X$ bosons during preheating, taking into account the fact that they are unstable with a decay width $\Gamma_X$. We show that parametric…

高能物理 - 唯象学 · 物理学 2009-10-31 E. W. Kolb , A. Riotto , I. I. Tkachev

We show that a baryon asymmetry can be generated by dissipative effects during warm inflation via a supersymmetric two-stage mechanism, where the inflaton is coupled to heavy mediator fields that then decay into light species through B- and…

高能物理 - 唯象学 · 物理学 2015-05-30 Mar Bastero-Gil , Arjun Berera , Rudnei O. Ramos , Joao G. Rosa

In models of baryogenesis based on Grand Unified Theories (GUTs), the baryon asymmetry of the universe is generated through the CP and baryon number violating, out-of-equilibrium decays of very massive gauge or Higgs bosons in the very…

高能物理 - 唯象学 · 物理学 2021-02-05 Dan Hooper , Gordan Krnjaic

We propose a new alternative for baryogenesis which resolves a number of the problems associated with GUT and electroweak scenarios, and which may allow baryogenesis even in modest extensions of the standard model. If the universe never…

高能物理 - 唯象学 · 物理学 2009-10-31 Lawrence M. Krauss , Mark Trodden

We investigate the generation of the baryon asymmetry within the framework of cosmological gra\-vi\-ta\-tional particle production, employing the Bogoliubov approach. We examine two well-known baryogenesis scenarios, namely baryogenesis in…

高能物理 - 唯象学 · 物理学 2024-04-11 Marcos M. Flores , Yuber F. Perez-Gonzalez

During inflation primordial quantum fluctuations of the spacetime metric become classical and there is a spontaneous CPT violation by the spin connection coupling terms of the metric with fermions. The energy levels of the left and the…

高能物理 - 唯象学 · 物理学 2007-05-23 Subhendra Mohanty , B. Mukhopadhyay , A. R. Prasanna

A new theory of thermal history after inflation is outlined by taking into account the effect of parametric resonance caused by inflaton oscillation. A typical outcome is existence of a high temperature phase, that makes possible GUT…

高能物理 - 唯象学 · 物理学 2007-05-23 M. Yoshimura

We reconsider the GUT-baryogenesis mechanism for generating the baryon asymmetry of the Universe. The baryon asymmetry is produced by the out of equilibrium decay of coloured Higgs bosons at the GUT scale, conserving B-L. If neutrinos are…

高能物理 - 唯象学 · 物理学 2007-05-23 J. A. Lopez-Perez , N. Rius

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…

高能物理 - 唯象学 · 物理学 2016-11-03 Mark Trodden

We show that in the vacuum inflation model, the gravitational baryogenesis mechanism will produce the baryon asymmetry. We analyze the evolution of entropy and baryon number in the vacuum inflation model. The comparison between dilution…

广义相对论与量子宇宙学 · 物理学 2017-08-31 Zhiqiang Huang , Qing-yu Cai

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…

高能物理 - 唯象学 · 物理学 2016-08-25 Juan Garcia-Bellido , Dmitri Grigoriev , Alexander Kusenko , Mikhail Shaposhnikov

The gravitational baryogensis may not generate a sufficient baryon asymmetry in the standard thermal history of the Universe when we take into account the gravitino problem. Hence it has been suggested that anisotropy of the Universe can…

高能物理 - 唯象学 · 物理学 2016-06-01 Mitsuhiro Fukushima , Shuntaro Mizuno , Kei-ichi Maeda

We propose a mechanism by which the inflaton can generate baryogenesis, by taking the inflaton to be a complex scalar field with a weakly broken global symmetry and present a new version of the Affleck-Dine mechanism. The smallness of the…

高能物理 - 唯象学 · 物理学 2014-04-02 Mark P. Hertzberg , Johanna Karouby

Fluctuations of scalar fields produced at the stage of preheating after inflation are so large that they can break supersymmetry much stronger than inflation itself. These fluctuations may lead to symmetry restoration along flat directions…

高能物理 - 唯象学 · 物理学 2009-09-29 Greg. W. Anderson , Andrei Linde , Antonio Riotto

We show that the baryon asymmetry of the universe can be explained in models where the Higgs couples to the Chern-Simons term of the hypercharge group and is away from the late-time minimum of its potential during inflation. The Higgs then…

高能物理 - 唯象学 · 物理学 2021-09-07 Yann Cado , Benedict von Harling , Eduard Masso , Mariano Quiros

Baryogenesis, through the decays of heavy bosons, was considered to be one of the major successes of the grand unified theories (GUTs). It was then realized that the sphaleron processes erased any baryon asymmetry from the GUT-baryogenesis…

高能物理 - 唯象学 · 物理学 2008-11-26 Pei-Hong Gu , Utpal Sarkar

We consider the generation of the baryon asymmetry in models with right-handed neutrinos produced through gravitational scattering of the inflaton during reheating. The right-handed neutrinos later decay and generate a lepton asymmetry,…

高能物理 - 唯象学 · 物理学 2022-05-05 Raymond T. Co , Yann Mambrini , Keith A. Olive

We discuss two cosmological issues in a generic gauge-mediated supersymmetry (SUSY)-breaking model, namely the Universe's baryon asymmetry and the gravitino dark-matter density. We show that both problems can be simultaneously solved if…

高能物理 - 唯象学 · 物理学 2009-11-07 Masaaki Fujii , T. Yanagida

In models of inflation driven by an axion-like pseudoscalar field, the inflaton, a, may couple to the standard model hypercharge via a Chern-Simons-type interaction, $L \subset a/(4\Lambda) F\tilde{F}$. This coupling results in explosive…

高能物理 - 唯象学 · 物理学 2017-12-20 Daniel Jimenez , Kohei Kamada , Kai Schmitz , Xun-Jie Xu
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