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After a period of inflationary expansion, the Universe reheated and reached full thermal equilibrium at the reheating temperature. In this talk, based on the paper, arXiv:0710.3349, we point out that, in the context of effective low-energy…

High Energy Physics - Phenomenology · Physics 2009-05-01 Ki-Young Choi , Leszek Roszkowski , Roberto Ruiz de Austri

A generic feature of gauge-mediated supersymmetry breaking models is that the gravitino is the lightest supersymmetric particle (LSP). In order not to overclose the universe, the gravitino LSP should be light enough (~ 1 keV), or…

High Energy Physics - Phenomenology · Physics 2009-11-10 Gi-Chol Cho , Yosuke Uehara

We investigate the leptogenesis via decays of heavy Majorana neutrinos which are produced non-thermally in inflaton decays. We make a comprehensive study on the leptogenesis assuming various supersymmetric (SUSY) models for hybrid, new and…

High Energy Physics - Phenomenology · Physics 2014-11-17 T. Asaka , K. Hamaguchi , M. Kawasaki , T. Yanagida

We investigate the possibility that the entropy producing decay of a right-handed sneutrino condensate can simultaneously be the source of the baryon asymmetry, of gravitino dark matter, and of cosmological density perturbations. For…

High Energy Physics - Phenomenology · Physics 2009-11-10 Rouzbeh Allahverdi , Manuel Drees

In the first stages of inflationary reheating, the temperature of the radiation produced by inflaton decays is typically higher than the commonly defined reheating temperature $T_{RH} \sim (\Gamma_\phi M_P)^{1/2}$ where $\Gamma_\phi$ is the…

High Energy Physics - Phenomenology · Physics 2017-11-22 Marcos A. G. Garcia , Yann Mambrini , Keith A. Olive , Marco Peloso

Gravitinos are a fundamental prediction of supergravity, their mass ($m_{G}$) is informative of the value of the SUSY breaking scale, and, if produced during reheating, their number density is a function of the reheating temperature…

High Energy Physics - Phenomenology · Physics 2018-07-11 Emanuela Dimastrogiovanni , Lawrence M. Krauss

We examine axino dark matter in the regime of a low reheating temperature T_R after inflation and taking into account that reheating is a non-instantaneous process. This can have a significant effect on the dark matter abundance, mainly due…

High Energy Physics - Phenomenology · Physics 2016-01-20 Leszek Roszkowski , Sebastian Trojanowski , Krzysztof Turzynski

Motivated by our earlier paper \cite{am}, we discuss how the infamous gravitino problem has a natural built in solution within supersymmetry. Supersymmetry allows a large number of flat directions made up of {\it gauge invariant}…

High Energy Physics - Phenomenology · Physics 2009-11-11 Rouzbeh Allahverdi , Anupam Mazumdar

It is known that the radiative neutrino mass model proposed by Ma could be a consistent framework for dark matter, leptogenesis and suppressed lepton flavor violation if a neutral component of the inert doublet is identified as dark matter…

High Energy Physics - Phenomenology · Physics 2015-05-27 Daijiro Suematsu

Recent developments in thermal leptogenesis are reviewed. Neutrino mixing data favor a simple picture where the matter-anti matter asymmetry is generated by the decays of the heavy RH neutrinos mildly close to thermal equilibrium and,…

High Energy Physics - Phenomenology · Physics 2007-05-23 P. Di Bari

Gravitinos with a mass in the keV range are an interesting candidate for warm dark matter. Recent measurements of the matter density of the universe and of cosmic structures at the dwarf galaxy scale rule out the simplest gravitino models…

Astrophysics · Physics 2009-11-07 Edward A. Baltz , Hitoshi Murayama

In some supergravity models, the superlight gravitino is accompanied by a light weakly coupled scalar (S) and pseudo-scalar (P) particle. The coupling of these particles to matter is inversely proportional to the product of the gravitino…

High Energy Physics - Phenomenology · Physics 2009-10-30 J. A. Grifols , R. N. Mohapatra , A. Riotto

We consider, in the context of the minimal supersymmetric standard model, the case where the gravitino weighs 10^6 GeV or more, which is preferred by various cosmological difficulties associated with unstable gravitinos. Despite the large…

High Energy Physics - Phenomenology · Physics 2015-06-03 Kwang Sik Jeong , Masatoshi Shimosuka , Masahiro Yamaguchi

We analyse the reheating in the modification of \nuMSM (Standard Model with three right handed neutrinos with masses below the electroweak scale) where the sterile neutrino providing the Dark Matter is generated in decays of the additional…

High Energy Physics - Phenomenology · Physics 2009-01-14 Alexey Anisimov , Yannick Bartocci , Fedor L. Bezrukov

If the gravitino is sufficiently light and stable it will behave as an effective massless neutrino species at the time of nucleosynthesis. Depending on the temperature at which it decouples from the thermal bath in the early universe, the…

High Energy Physics - Phenomenology · Physics 2009-10-28 Tony Gherghetta

We consider the case of very low reheating scenarios ($T_{\rm RH}\sim\mathcal{O}({\rm MeV})$) with a better calculation of the production of the relic neutrino background (with three-flavor oscillations). At 95% confidence level, a lower…

Cosmology and Nongalactic Astrophysics · Physics 2015-12-30 P. F. de Salas , M. Lattanzi , G. Mangano , G. Miele , S. Pastor , O. Pisanti

We derive novel limits on the masses of the light and heavy Majorana neutrinos by requiring successful leptogenesis in seesaw models of minimal flavour violation (MFV). Taking properly into account radiative flavour effects and avoiding the…

High Energy Physics - Phenomenology · Physics 2015-10-14 Apostolos Pilaftsis , Daniele Teresi

We study reheating processes and its cosmological consequences in the Starobinsky model embedded in the old-minimal supergravity. First, we consider minimal coupling between the gravity and matter sectors in the higher curvature theory, and…

High Energy Physics - Phenomenology · Physics 2015-06-23 Takahiro Terada , Yuki Watanabe , Yusuke Yamada , Jun'ichi Yokoyama

In supersymmetric models where the magnitude of the GUT scale gaugino mass parameter M_3 is suppressed relative to M_1 and M_2, the lightest neutralino can be a mixed higgsino-bino state with a thermal relic abundance in agreement with the…

High Energy Physics - Phenomenology · Physics 2008-11-26 Howard Baer , Azar Mustafayev , Stefano Profumo , Xerxes Tata

Affleck-Dine baryogenesis in models where the gravitino is both the lightest supersymmetric particle and the dark matter candidate is investigated. For a high enough reheating temperature to produce sufficient gravitinos by thermal…

High Energy Physics - Phenomenology · Physics 2009-11-11 Osamu Seto
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