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Recent anomalies in cosmic rays could be due to dark matter annihilation in our galaxy. In order to get the required large cross-section to explain the data while still obtaining the right relic density, we rely on a non standard thermal…

High Energy Physics - Phenomenology · Physics 2009-09-02 Bhaskar Dutta , Louis Leblond , Kuver Sinha

We motivate Higgsino dark matter from a solution to the cosmological moduli/gravitino problem. Cosmological moduli/gravitino should be heavy enough to decay before the onset of Big Bang Nucleosynthesis, and this requirement typically forces…

High Energy Physics - Phenomenology · Physics 2015-06-12 Kuver Sinha

Scenarios where gravitinos with GeV masses make up dark matter are known to be in tension with high reheating temperatures, as required by e.g. thermal leptogenesis. This tension comes from the longevity of the NLSPs, which can destroy the…

High Energy Physics - Phenomenology · Physics 2010-12-13 Jonas Schmidt , Christoph Weniger , Tsutomu T. Yanagida

The absence of supersymmetric particles at the weak scale is a puzzle if supersymmetry solves the gauge hierarchy problem. We show that, if the right-handed neutrino masses arise from hidden gaugino condensation via GUT-suppressed…

High Energy Physics - Phenomenology · Physics 2018-08-21 Ryo Nagai , Fuminobu Takahashi , Norimi Yokozaki

We study the phenomenology of generic supergravity models in which gravity mediation naturally competes with gauge mediation as the origin of supergravity-breaking. This class of hybrid models has been recently motivated in string inspired…

High Energy Physics - Phenomenology · Physics 2009-12-04 D. G. Cerdeno , Y. Mambrini , A. Romagnoni

In models with gauge mediated supersymmetry breaking the gravitino is the lightest supersymmetric particle. If R-parity is violated the gravitino decays, but with a half-live far exceeding the age of the universe and thus is, in principle,…

High Energy Physics - Phenomenology · Physics 2008-11-26 M. Hirsch , W. Porod , D. Restrepo

Properties of neutrinos may be the origin of the matter-antimatter asymmetry of the universe. In the seesaw model for neutrino masses this leads to important constraints on the properties of light and heavy neutrinos. In particular, an…

High Energy Physics - Phenomenology · Physics 2011-08-17 W. Buchmuller , P. Di Bari , M. Plumacher

As is well known, the gravitational degrees of freedom contained in $R+\zeta R^{2}$ (super)gravity lead to Starobinsky's potential, in a one-field setting for inflationary Cosmology that appears favored by Planck data. In this letter we…

General Relativity and Quantum Cosmology · Physics 2017-02-01 Andrea Addazi , Maxim Yu. Khlopov

We study the implications of a large baryogenesis temperature, $T_B = O(10^{10}$ GeV), on the mass spectrum of superparticles in supersymmetric extensions of the standard model. Models with a neutralino as lightest superparticle (LSP) are…

High Energy Physics - Phenomenology · Physics 2009-10-31 M. Bolz , W. Buchmüller , M. Plümacher

We study the light gluino scenario giving special attention to constraints from the masses of the light CP-even neutral Higgs $m_h$, the lightest chargino $m_{\chi^{\pm}_1}$, and the second lightest neutralino $m_{\chi^0_2}$, and from the…

High Energy Physics - Phenomenology · Physics 2014-11-17 Marco Aurelio Diaz

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 quite possible that the reheat temperature of the universe is extremely low close to the scale of Big Bang nucleosynthesis, i.e. $T_{R}\sim 1-10$ MeV. At such low reheat temperatures generating matter anti-matter asymmetry and…

High Energy Physics - Phenomenology · Physics 2009-11-10 Kazunori Kohri , Anupam Mazumdar , Narendra Sahu

We consider the effects of R-parity violation due to the inclusion of a bilinear $\mu^\prime L H_u$ superpotential term in high scale supersymmetric models with an EeV scale gravitino as dark matter. Although the typical phenomenological…

High Energy Physics - Phenomenology · Physics 2018-08-01 Emilian Dudas , Tony Gherghetta , Kunio Kaneta , Yann Mambrini , Keith A. Olive

We study the consequences of the gravitino decay into dark matter. We suppose that the lightest neutralino is the main component of dark matter. In our framework gravitino is heavy enough to decay before Big Bang Nucleosynthesis starts. We…

High Energy Physics - Phenomenology · Physics 2007-06-29 David Gherson

We develop a string-inspired model for particle cosmology, based on a flipped SU(5)$\times$U(1) gauge group formulated in a no-scale supergravity framework. The model realizes Starobinsky-like inflation, which we assume to be followed by…

High Energy Physics - Phenomenology · Physics 2020-02-05 John Ellis , Marcos A. G. Garcia , Natsumi Nagata , Dimitri V. Nanopoulos , Keith A. Olive

We discuss two cosmological issues in a generic gauge-mediated supersymmetry (SUSY)-breaking model, namely the Universe's baryon asymmetry and the gravitino dark-matter density. We show that both problems can be simultaneously solved if…

High Energy Physics - Phenomenology · Physics 2009-11-07 Masaaki Fujii , T. Yanagida

We propose a consistent scenario of the evolution of the universe based on the large cutoff supergravity (LCSUGRA) hypothesis of supersymmetry breaking, where the gravitino and sfermion become as heavy a $\sim O(1-10 {\rm TeV})$. With such…

High Energy Physics - Phenomenology · Physics 2009-11-11 M. Ibe , Takeo Moroi , T. Yanagida

Thermal leptogenesis and supergravity are attractive scenarios for physics beyond the standard model. However, it is well known that the super-weak interaction of the gravitino often leads to problems with primordial nucleosynthesis in the…

High Energy Physics - Phenomenology · Physics 2011-01-04 Christoph Weniger

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

Models of leptogenesis are constrained by the low reheat temperature at the end of reheating associated with the gravitino bound. However a detailed view of reheating, in which the maximum temperature during reheating, $\Tmax$, can be…

High Energy Physics - Phenomenology · Physics 2008-11-26 Raghavan Rangarajan , Narendra Sahu