English
Related papers

Related papers: Affleck-Dine baryogenesis just after inflation

200 papers

We present a concrete supersymmetric grand unified model based on the Pati-Salam gauge group SU(4)_c x SU(2)_L x SU(2)_R and leading naturally to smooth hybrid inflation, which avoids the cosmological disaster encountered in the standard…

High Energy Physics - Phenomenology · Physics 2008-11-26 R. Jeannerot , S. Khalil , G. Lazarides

By using a string-inspired modular invariant supergravity, which was proved well to explain WMAP observations appropriately, a mechanism of supersymmetry breaking (SSB) and Gravitino Production just after the end of inflation are…

High Energy Physics - Phenomenology · Physics 2010-03-17 Kenji Takagi , Yuta Koshimizu , Toyokazu Fukuoka , Hikoya Kasari , Mitsuo J. Hayashi

We show by studying the Abelian Higgs model with numerical lattice simulations that non-thermal phase transitions arising out of preheating after inflation are possible in gauge-Higgs models under rather general circumstances. This may lead…

High Energy Physics - Phenomenology · Physics 2009-10-31 A. Rajantie , E. J. Copeland

We investigate a novel scenario of cosmological inflation in a gauged $B-L$ extended minimal supersymmetric Standard Model with R-symmetry. We use a noncanonical K\"{a}hler potential and a superpotential, both preserving the R-symmetry to…

High Energy Physics - Phenomenology · Physics 2014-05-22 Masato Arai , Shinsuke Kawai , Nobuchika Okada

In this clarifying note we discuss the late decay of an Affleck-Dine condensate by providing a no-go theorem that attributes to conserved global charges which are identified by the net particle number in fields which are included in the…

High Energy Physics - Phenomenology · Physics 2008-11-26 Rouzbeh Allahverdi , Anupam Mazumdar

We discuss two independent issues about the baryon asymmetry of the universe. First, assuming that it is generated by an unspecified source at high temperatures, we study the effects of non-perturbative $SU(2)_W$ dynamics above the…

High Energy Physics - Phenomenology · Physics 2009-10-22 Luis E. Ibanez , Fernando Quevedo

We consider the constraints that can be imposed on a wide class of Inflation models in modified gravity scenarios in which the Friedmann equation is modified by the inclusion of $\rho^2$ terms, where $\rho$ is the total energy density. In…

High Energy Physics - Phenomenology · Physics 2009-11-11 Edmund J. Copeland , Osamu Seto

We explore the possibility of baryogenesis in the framework of quintessential inflation. We focus on the model independent features of the underlying paradigm and demonstrate that the required baryon asymmetry can successfully be generated…

General Relativity and Quantum Cosmology · Physics 2020-07-01 Safia Ahmad , Antonio De Felice , Nur Jaman , Sachiko Kuroyanagi , M. Sami

We analyse non-thermal leptogenesis after models of Majoron hilltop inflation, where the scalar field that provides masses for the right-handed neutrinos and sneutrinos via its vacuum expectation value acts as the inflaton. We discuss…

High Energy Physics - Phenomenology · Physics 2018-05-16 Stefan Antusch , Kenneth Marschall

Supersymmetric thermal leptogenesis with a hierarchical right-handed neutrino mass spectrum requires the mass of the lightest right-handed neutrino to be heavier than about 10^9 GeV. This is in conflict with the upper bound on the reheating…

High Energy Physics - Phenomenology · Physics 2008-11-26 G. F. Giudice , L. Mether , A. Riotto , F. Riva

We discuss, in the context of a concrete supersymmetric grand unified model based on the Pati-Salam gauge group SU(4)_c x SU(2)_L x SU(2)_R, two "natural" extensions of supersymmetric hybrid inflation, which avoid the cosmological disaster…

High Energy Physics - Phenomenology · Physics 2007-05-23 R. Jeannerot , S. Khalil , G. Lazarides

No-scale supergravity provides a successful framework for Starobinsky-like inflation models. Two classes of models can be distinguished depending on the identification of the inflaton with the volume modulus, $T$ (C-models), or a…

High Energy Physics - Phenomenology · Physics 2020-01-15 Kunio Kaneta , Yann Mambrini , Keith A. Olive , Sarunas Verner

In the standard model and most of its extensions the electroweak transition is too weak to affect the cosmological baryon asymmetry. Due to sphaleron processes baryogenesis in the high-temperature, symmetric phase of the standard model is…

High Energy Physics - Phenomenology · Physics 2007-05-23 W. Buchmüller

We present real-time lattice simulations of Cold Electroweak Baryogenesis, in which the baryon asymmetry of the Universe is generated during tachyonic electroweak symmetry breaking at the end of inflation. In the minimal realisation of the…

High Energy Physics - Phenomenology · Physics 2008-11-26 Anders Tranberg , Jan Smit , Mark Hindmarsh

We propose a primeval baryon isocurvature model in the context of the Affleck-Dine (AD) baryogenesis mechanism. Quantum fluctuations of the AD field during inflation produce fluctuations in the baryon number. We obtain a model which gives…

Astrophysics · Physics 2009-10-31 Kazuya Koyama , Jiro Soda

We consider hybrid inflation in the braneworld scenario. In particular, we consider inflation in global supersymmetry with the D-terms in the scalar potential for the inflaton field to be the dominant ones (D-term inflation). We find that…

High Energy Physics - Phenomenology · Physics 2009-11-11 G. Panotopoulos

We study the evolution of a cosmological baryon asymmetry in leptogenesis when the right-handed neutrinos are produced in inflaton decays. By performing a detailed numerical study over a broad range of inflaton-neutrino couplings we show…

High Energy Physics - Phenomenology · Physics 2008-11-26 F. Hahn-Woernle , M. Plumacher

We study the onset of symmetry breaking after hybrid inflation in a model having the field content of the SU(2) gauge-scalar sector of the standard model, coupled to a singlet inflaton. This process is studied in (3+1)-dimensions in a fully…

High Energy Physics - Phenomenology · Physics 2009-11-10 Juan Garcia-Bellido , Margarita Garcia Perez , Antonio Gonzalez-Arroyo

We revisit the Affleck-Dine leptogenesis via the $L H_u$ flat direction with a light slepton field. Although the light slepton field is favored in low-energy SUSY phenomenologies, such as the muon $g-2$ anomaly and bino-slepton…

High Energy Physics - Phenomenology · Physics 2023-07-12 Kazuki Enomoto , Koichi Hamaguchi , Kohei Kamada , Juntaro Wada

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