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相关论文: Baryogenesis via Gravitational Spontaneous Symmetr…

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Lorentz-violating theories of gravity typically contain constrained vector fields. We show that the lowest-order coupling of such vectors to $\mathrm{U}(1)$-symmetric scalars can naturally give rise to baryogenesis in a manner akin to the…

高能物理 - 唯象学 · 物理学 2017-09-14 Jeremy Sakstein , Adam R. Solomon

We put forward a new proposal for generating the baryon asymmetry of the universe by making use of the dynamics of a $\mathrm{U}(1)$ scalar field coupled to dark matter. High dark matter densities cause the $\mathrm{U}(1)$ symmetry to break…

高能物理 - 唯象学 · 物理学 2017-11-22 Jeremy Sakstein , Mark Trodden

We present a new mechanism of spontaneous baryogenesis. Usually such mechanisms require a derivative coupling between a scalar field and baryon current. In our model, the scalar field instead derivatively couples to a current associated…

高能物理 - 唯象学 · 物理学 2011-07-19 Takeshi Chiba , Fuminobu Takahashi , Masahide Yamaguchi

We propose a variant scenario of spontaneous baryogenesis from asymmetric inflaton based on current-current interactions between the inflaton and matter fields with a non-zero B-L charge. When the inflaton starts to oscillate around the…

高能物理 - 唯象学 · 物理学 2016-03-16 Fuminobu Takahashi , Masaki Yamada

A novel mechanism of baryogenesis is proposed on the basis of the phase transition from the conformal invariant space-time to the Einstein space-time in quantum gravity. Strong-coupling gravitational excitations with dynamical mass about…

高能物理 - 唯象学 · 物理学 2008-11-26 Ken-ji Hamada , Azusa Minamizaki , Akio Sugamoto

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

We introduce a class of non-supersymmetric models explaining baryogenesis a la Affleck-Dine, which use a decay of two superheavy scalar fields with close masses. These scalars acquire non-zero expectation values during inflation through…

宇宙学与河外天体物理 · 物理学 2019-04-08 Eugeny Babichev , Dmitry Gorbunov , Sabir Ramazanov

The mechanism of gravitational baryogenesis, based on the CPT-violating gravitational interaction between the derivative of the Ricci scalar curvature and the baryon-number current, is investigated in the context of the Gauss-Bonnet…

高能物理 - 唯象学 · 物理学 2009-11-11 M. C. Bento , R. Gonzalez Felipe , N. M. C. Santos

We study the cosmology of supersymmetric models in which the supersymmetry breaking effects are mediated by gauge interactions at about the 10^5 GeV scale. We first point out that the gravitino is likely to overclose the Universe in this…

高能物理 - 唯象学 · 物理学 2009-09-29 Andre de Gouvea , Takeo Moroi , Hitoshi Murayama

We describe a simple and predictive scenario for baryogenesis in theories with large extra dimensions which resembles Affleck-Dine baryogenesis. The Affleck-Dine field is a complex scalar field carrying a $U(1)_{\chi}$ charge which is…

高能物理 - 唯象学 · 物理学 2009-11-07 Rouzbeh Allahverdi , Kari Enqvist , Anupam Mazumdar , Abdel Pérez-Lorenzana

Supersymmetry breaking close to the scale of grand unification can explain cosmic inflation. As we demonstrate in this paper, this can be achieved in strongly coupled supersymmetric gauge theories, such that the energy scales of inflation…

高能物理 - 唯象学 · 物理学 2018-06-26 Valerie Domcke , Kai Schmitz

We consider a renormalizable extension of the minimal supersymmetric standard model endowed by an R and a gauged B - L symmetry. The model incorporates chaotic inflation driven by a quartic potential, associated with the Higgs field which…

高能物理 - 唯象学 · 物理学 2018-04-20 C. Pallis

We investigate axion-inflation baryogenesis models, embedded into U(1) gauge symmetric extensions of the Standard Model (SM), in which the new gauge field couples to the pseudo-scalar inflaton via the Chern-Simons coupling. The motion of…

高能物理 - 唯象学 · 物理学 2024-09-30 Wei Chao , Yonghua Wang , Chenhui Xie

We investigate the viability of Affleck-Dine baryogenesis in D=4, N=1 supergravity descending from string theory. The process relies on an initial condition where visible sector supersymmetric flat directions obtain tachyonic masses during…

高能物理 - 理论 · 物理学 2010-11-11 Bhaskar Dutta , Kuver Sinha

We present a realistic non-supersymmetric inflation model based on a gauged U(1)$_{B-L}$ symmetry and a tree-level Higgs potential. The inflaton is identified with the scalar field which spontaneously breaks U(1)$_{B-L}$, and we include…

高能物理 - 唯象学 · 物理学 2013-11-06 Nobuchika Okada , Qaisar Shafi

We present a novel Affleck-Dine scenario for the generation of the observed baryon asymmetry of the Universe based on the non-trivial interplay between quintessential inflationary models containing a kinetic dominated post-inflationary era…

宇宙学与河外天体物理 · 物理学 2018-07-30 Dario Bettoni , Javier Rubio

We briefly review the present status of Affleck-Dine baryo/leptogenesis scenarios in the minimal supersymmetric standard model (MSSM) in the context of the gravity-mediated SUSY breaking, and show that there is a serious cosmological…

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

$f(R)$-theories of gravity are reviewed in the context of the so called gravitational baryogenesis. The latter is a mechanism for generating the baryon asymmetry in the Universe, and relies on the coupling between the Ricci scalar curvature…

天体物理学 · 物理学 2009-11-11 G. Lambiase , G. Scarpetta

We propose a new scenario of Affleck-Dine baryogenesis where a flat direction in the MSSM generates B-L asymmetry just after the end of inflation. The resulting amount of baryon asymmetry is independent of low-energy supersymmetric models…

高能物理 - 唯象学 · 物理学 2016-04-27 Masaki Yamada

We consider a renormalizable extension of the minimal supersymmetric standard model endowed by an R and a gauged B - L symmetry. The model incorporates chaotic inflation driven by a quartic potential, associated with the Higgs field which…

高能物理 - 唯象学 · 物理学 2018-03-06 C. Pallis
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