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Related papers: Baryogenesis in Brans-Dicke theory

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We present a new scenario for baryogenesis in the context of heterotic brane-world models. The baryon asymmetry of the universe is generated at a small-instanton phase transition which is initiated by a moving brane colliding with the…

High Energy Physics - Theory · Physics 2009-11-07 Mar Bastero-Gil , Edmund J. Copeland , James Gray , Andre Lukas , Michael Plumacher

Thermal inflation is an attractive idea to dilute cosmic density of unwanted particles such as moduli fields which cause cosmological difficulties. However, it also dilutes preexisting baryon asymmetry and some viable baryogenesis is…

High Energy Physics - Phenomenology · Physics 2016-04-06 Taku Hayakawa , Masahiro Kawasaki , Masaki Yamada

We study on the electroweak baryogenesis problem in the vector-like quark model. This model can add to the minimal standard model the extra CP-violation source which breaks CP spontaneously. Using charge transport mechanism suggested by…

High Energy Physics - Phenomenology · Physics 2007-05-23 Tomoko Uesugi

The electroweak symmetry breaking transition may supply the appropriate out-of-equilibrium conditions for baryogenesis if it is triggered sufficiently fast. This can happen at the end of low-scale inflation, prompting baryogenesis to occur…

High Energy Physics - Phenomenology · Physics 2010-10-27 Anders Tranberg , Jan Smit , Mark Hindmarsh

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…

High Energy Physics - Phenomenology · Physics 2007-05-23 A. Riotto

Baryon asymmetry of the universe is generated in the supersymmetric standard model (SSM) through the charge transport mechanism mediated by top squarks. Necessary CP violation originates from a complex phase contained in mass-squared…

High Energy Physics - Phenomenology · Physics 2007-05-23 Mayumi Aoki , Noriyuki Oshimo

We study the dynamics of the Affleck-Dine field after inflation in more detail. After inflation, the Affleck-Dine field inevitably oscillates around the potential minimum. This oscillation is hard to decay and can cause accidental…

High Energy Physics - Phenomenology · Physics 2017-09-27 Fuminori Hasegawa , Masahiro Kawasaki

We study the cosmological evolution of asymmetries in the two-Higgs doublet extension of the Standard Model, prior to the electroweak phase transition. If Higgs flavour-exchanging interactions are sufficiently slow, then a relative…

High Energy Physics - Phenomenology · Physics 2015-06-16 Sacha Davidson , Ricardo Gonzalez Felipe , H. Serodio , Joao P. Silva

The discovery of the primordial B-mode polarisation by the BICEP2 experiment indicates inflation with a relatively high energy scale. Taking this indication into account, we propose consistent scenarios to account for the observed baryon…

High Energy Physics - Phenomenology · Physics 2014-08-20 Keisuke Harigaya , Ayuki Kamada , Masahiro Kawasaki , Kyohei Mukaida , Masaki Yamada

We study the transference of an initial leptonic charge contained in a complex scalar field (waterfall field) at the end of the inflation to the leptons of the standard model and then convert this leptonic charge in baryonic charge by…

High Energy Physics - Phenomenology · Physics 2009-06-24 Carlos Martinez Prieto

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…

High Energy Physics - Phenomenology · Physics 2018-04-20 C. Pallis

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

We consider a phenomenological extension of the minimal supersymmetric standard model (MSSM) which incorporates non-minimal chaotic inflation, driven by a quadratic potential in conjunction with a linear term in the frame function.…

High Energy Physics - Phenomenology · Physics 2012-07-27 C. Pallis , Q. Shafi

The derivative coupling of baryonic current to the curvature scalar in gravitational baryogenesis scenarios leads to higher order equations for gravitational field. It is shown that these equations are strongly unstable and destroy standard…

General Relativity and Quantum Cosmology · Physics 2017-06-14 E. V. Arbuzova , A. D. Dolgov

In this paper, the cosmological dynamics of Brans-Dicke theory in which there are fermions with a coupling to BD scalar field as well as a self-interaction potential is investigated. The conditions that there exists a solution which is…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-21 Dao-Jun Liu

We consider a phenomenological extension of the minimal supersymmetric standard model which incorporates non-minimal chaotic inflation, driven by a quartic potential associated with the lightest right-handed sneutrino. Inflation is followed…

High Energy Physics - Phenomenology · Physics 2015-03-17 C. Pallis , N. Toumbas

We present a model with a complex and a real scalar fields and a potential whose symmetry is explicitly broken by Planck-scale physics. For exponentially small breaking, the model accounts for the period of inflation in the early universe…

Astrophysics · Physics 2009-11-11 Eduard Masso , Gabriel Zsembinszki

We argue that an extension of the Minimal Supersymmetric Standard Model that gives rise to viable thermal inflation, and so does not suffer from a Polonyi/moduli problem, should contain right-handed neutrinos which acquire their masses due…

High Energy Physics - Phenomenology · Physics 2009-10-28 E. D. Stewart , M. Kawasaki , T. Yanagida

It has recently been realized that many theories of physics beyond the Standard Model give rise to cosmological histories exhibiting extended epochs of cosmological stasis. During such epochs, the abundances of different energy components…

Cosmology and Nongalactic Astrophysics · Physics 2024-12-17 Keith R. Dienes , Lucien Heurtier , Fei Huang , Tim M. P. Tait , Brooks Thomas

In this work we focus on a novel completion of the well-known Brans-Dicke theory that introduces an interaction between the dark energy and dark matter sectors, known as complete Brans-Dicke (CBD) theory. We obtain viable cosmological…

General Relativity and Quantum Cosmology · Physics 2017-10-10 Georgios Kofinas , Nelson A. Lima
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