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Related papers: Affleck-Dine baryogensis in large extra dimensions

200 papers

We study the conditions for successful Affleck-Dine baryogenesis in generic inflation and supergravity scenarios, finding powerful restrictions on them. String-based SUGRA models are especially interesting since they are surprisingly…

High Energy Physics - Phenomenology · Physics 2007-05-23 J. A. Casas

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…

High Energy Physics - Phenomenology · Physics 2009-11-07 Edmund J. Copeland , David Lyth , Arttu Rajantie , Mark Trodden

We discuss the curvaton scenario with the Affleck-Dine baryogenesis. In this scenario, non-vanishing baryonic entropy fluctuation may be generated even without primordial fluctuation of the Affleck-Dine field. Too large entropy fluctuation…

High Energy Physics - Phenomenology · Physics 2009-11-10 Maki Ikegami , Takeo Moroi

The Affleck-Dine leptogenesis scenario along the LHu flat direction is reconsidered. It is known that successful Affleck-Dine leptogenesis requires that the lightest neutrino mass is extremely small. This situation can be significantly…

High Energy Physics - Phenomenology · Physics 2017-03-08 Kyu Jung Bae , Howard Baer , Koichi Hamaguchi , Kazunori Nakayama

The origin of the matter-antimatter asymmetry remains one of the most fundamental problems of cosmology. In this talk I present a novel scenario for baryogenesis at the electroweak scale, without the need for a first order phase transition.…

High Energy Physics - Phenomenology · Physics 2016-11-03 Juan Garcia-Bellido

In models with the fundamental gravity scale in the TeV range, early cosmology is quite different from the standard picture, because the universe must have arisen at a much lower temperature and the electroweak symmetry was probably never…

High Energy Physics - Phenomenology · Physics 2010-10-27 C. Bambi , A. D. Dolgov , K. Freese

We discuss the mechanism of reheating in pre-big bang string cosmology and we calculate the amount of moduli and gravitinos produced gravitationally and in scattering processes of the thermal bath. We find that this abundance always exceeds…

High Energy Physics - Theory · Physics 2009-09-15 Alessandra Buonanno , Martin Lemoine , Keith A. Olive

We consider a model of baryogenesis based on adding lepton number-violating quadratic mass terms to the inflaton potential of a non-minimally coupled inflation model. The $L$-violating mass terms generate a lepton asymmetry in a complex…

High Energy Physics - Phenomenology · Physics 2023-07-12 Kit Lloyd-Stubbs , John McDonald

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…

High Energy Physics - Phenomenology · Physics 2007-05-23 Alexander Kusenko

A variation of Affleck-Dine mechanism was proposed to generate the observed baryon asymmetry in [1], in which the inflaton was assumed to be a complex scalar field with a weakly broken $U(1)$ symmetry, and the baryon asymmetry generation…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-22 Nan Li , Ding-fang Zeng

In general the gravitino mass and/or the soft supersymmetry breaking masses in the observable sector can be much larger than the TeV scale. Depending on the relation between the masses, new important channels for gravitino production in the…

High Energy Physics - Phenomenology · Physics 2007-05-23 Rouzbeh Allahverdi , Steen Hannestad , Asko Jokinen , Anupam Mazumdar , Silvia Pascoli

Possible effects due to nonequilibrium dynamics in the Affleck-Dine mechanism of baryogenesis are examined. Using the closed-time-path formalism, the quantum fluctuation and the back reaction of the Affleck-Dine scalar field are…

High Energy Physics - Phenomenology · Physics 2009-11-11 Yeo-Yie Charng , Da-Shin Lee , Chung Ngoc Leung , Kin-Wang Ng

A typical problem of the leptogenesis scenario is the mismatch between the maximum reheat temperature implied by gravitino overproduction bound and the minimum temperature required to create thermally the lightest right-handed neutrino. We…

High Energy Physics - Phenomenology · Physics 2007-05-23 Lotfi Boubekeur

In this letter we show that the inflaton can generate the cosmological baryon asymmetry. We take the inflaton to be a complex scalar field with a weakly broken global symmetry and develop a new variant on the Affleck-Dine mechanism. The…

High Energy Physics - Phenomenology · Physics 2014-08-26 Mark P. Hertzberg , Johanna Karouby

A baryogenesis scenario in supersymmetric standard models with Dirac neutrinos proposed by Abel and Page is reconsidered with introducing intermediate scale physics to stabilize the runaway potential along a right-handed sneutrino…

High Energy Physics - Phenomenology · Physics 2008-11-26 Masato Senami , Tsutomu Takayama

The freeze-in mechanism has been shown to allow the simultaneous generation of cosmic dark matter and a viable matter-antimatter asymmetry in the universe. When the underlying interactions are described by higher-dimensional,…

High Energy Physics - Phenomenology · Physics 2023-04-18 Ioannis Dalianis , Andreas Goudelis , Dimitrios Karamitros , Pantelis Papachristou , Vassilis C. Spanos

We study the scenario of baryogenesis through leptogenesis in higher-dimensional theories, in which the scale of quantum gravity is many orders of magnitude smaller than the usual Planck mass. The minimal realization of these theories…

High Energy Physics - Phenomenology · Physics 2009-10-31 Apostolos Pilaftsis

In models for thermal baryogenesis from particle decays, the mass of the decaying particle is typically many orders of magnitude above the TeV scale. We will discuss different ways to lower the energy scale of baryogenesis and present the…

High Energy Physics - Phenomenology · Physics 2015-06-16 J. Racker

We present here a realistic model to produce a very large lepton asymmetry L of 0.1 to 1, without producing a large baryon asymmetry. The model is based on the Affleck and Dine scenario, in which the field acquiring a large vacuum…

High Energy Physics - Phenomenology · Physics 2009-10-30 J. A. Casas , Wai Yan Cheng , G. B. Gelmini

We consider the presence of cosmic string induced density fluctuations in the universe at temperatures below the electroweak phase transition temperature. Resulting temperature fluctuations can restore the electroweak symmetry locally,…

High Energy Physics - Phenomenology · Physics 2009-11-07 Biswanath Layek , Soma Sanyal , Ajit M. Srivastava