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Related papers: Probing Non-Thermal Gravitinos Through Large-Scale…

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We present a full one-loop calculation of the gravitino thermal production rate, beyond the so-called hard thermal loop approximation, using the corresponding thermal spectral functions in numerical form on both sides of the light cone.…

High Energy Physics - Phenomenology · Physics 2025-01-23 Helmut Eberl , Ioannis D. Gialamas , Vassilis C. Spanos

In the minimal supersymmetric standard models, neutralino dark matter with mass of $m_{\chi}\sim m_Z/2\sim 45$ GeV and $m_{\chi}\sim m_h/2\sim 62$ GeV can have the thermal relic abundance $\Omega_{\chi_1}h^2\simeq 0.120$ via the $Z$- and…

High Energy Physics - Phenomenology · Physics 2016-03-23 Koichi Hamaguchi , Kazuya Ishikawa

Dark matter may be composed of superWIMPs, superweakly-interacting massive particles produced in the late decays of other particles. We focus on the case of gravitinos produced in the late decays of sleptons or sneutrinos and assume they…

High Energy Physics - Phenomenology · Physics 2009-11-10 Jonathan L. Feng , Shufang Su , Fumihiro Takayama

We study implications of thermal leptogenesis for the superparticle mass spectrum. A consistent picture is obtained if the lightest superparticle is the gravitino, which can be the dominant component of cold dark matter. In the case of a…

High Energy Physics - Phenomenology · Physics 2008-11-26 Wilfried Buchmuller

Neutralino dark matter is well motivated, but also suffers from two shortcomings: it requires gravity-mediated supersymmetry breaking, which generically violates flavor constraints, and its thermal relic density \Omega is typically too…

High Energy Physics - Phenomenology · Physics 2008-11-26 Jonathan L. Feng , Bryan T. Smith , Fumihiro Takayama

In a recent work, a model of gauge mediation with sequestered supersymmetry (SUSY) breaking was proposed. In this model, the mass of the gravitino is O(100) GeV without causing the flavor-changing neutral-current problem. In contrast to…

High Energy Physics - Phenomenology · Physics 2010-04-30 Motoi Endo , Satoshi Shirai , Kazuya Yonekura

We study the growth of density perturbations in a universe with unstable dark matter particles. The mass (m_\nu) range 30 eV < m_\nu < 10 keV with lifetimes ($t_d$) in the range 10^7 sec < t_d < 10^16 sec are considered. We calculate the…

Astrophysics · Physics 2009-10-30 Somnath Bharadwaj , Shiv K. Sethi

The cold dark matter may be in a meta-stable state and decays to other particles with a very long lifetime. If the decaying products of the dark matter are weakly interacting, e.g. neutrinos, then it would have little impact on…

Astrophysics · Physics 2008-11-26 Yan Gong , Xuelei Chen

Gravitino is one feasible candidate for the dark matter in supergravity models. With its couplings being suppressed by the Plank mass, gravitino interacts very weakly with other particles, making its direct detection, or production at…

High Energy Physics - Phenomenology · Physics 2007-09-26 Yudi Santoso

We study supersymmetric scenarios where the dark matter is the gaugino of an unbroken hidden U(1) which interacts with the visible world only via a small kinetic mixing with the hypercharge. Strong constraints on the parameter space can be…

High Energy Physics - Phenomenology · Physics 2009-02-12 A. Ibarra , A. Ringwald , C. Weniger

We present the first attempt to analytically study the nonlinear matter power spectrum for a mixed dark matter (cold dark matter plus neutrinos of total mass ~0.1eV) model based on cosmological perturbation theory. The suppression in the…

Astrophysics · Physics 2009-06-23 Shun Saito , Masahiro Takada , Atsushi Taruya

If dark matter particles are not perfectly stable, their decay products might be seen in the cosmic-ray fluxes. A natural candidate for decaying dark matter is the gravitino in R-parity violating scenarios. In the relevant GeV-TeV energy…

High Energy Astrophysical Phenomena · Physics 2011-10-31 Xiaoyuan Huang , Gilles Vertongen , Christoph Weniger

We study the freeze-in of gravitationally interacting dark matter in extra dimensions. Focusing on a minimal dark matter candidate that only interacts with the SM via gravity in a five-dimensional model we find that a large range of dark…

High Energy Physics - Phenomenology · Physics 2023-04-26 Arturo de Giorgi , Stefan Vogl

Non-universal boundary conditions in grand unified theories can lead to non-universal gaugino masses at the unification scale. In R-parity preserving theories the lightest supersymmetric particle is a natural candidate for the dark matter.…

High Energy Physics - Phenomenology · Physics 2009-09-29 Katri Huitu , Jari Laamanen , Sourov Roy

We show that, if decaying gravitino dark matter is responsible for the PAMELA and ATIC/PPB-BETS anomalies in the cosmic-ray electron and positron fluxes, both a reheating temperature and a gluino mass are constrained from above. In…

High Energy Physics - Phenomenology · Physics 2010-01-15 Koichi Hamaguchi , Fuminobu Takahashi , T. T. Yanagida

We investigate the possibility of testing supergravity unified models with scalar masses in the range 50-100 TeV and much lighter gaugino masses at the Large Hadron Collider. The analysis is carried out under the constraints that models…

High Energy Physics - Phenomenology · Physics 2017-10-18 Amin Aboubrahim , Pran Nath

We revisit indirect detection possibilities for neutralino dark matter, emphasizing the complementary roles of different approaches. While thermally produced dark matter often requires large astrophysical "boost factors" to observe…

High Energy Physics - Phenomenology · Physics 2008-10-16 Phill Grajek , Gordon Kane , Daniel J. Phalen , Aaron Pierce , Scott Watson

In Split-SUSY with BRpV we show that the Gravitino DM solution is consistent with experimental evidence on its relic density and life time. We arrive at this conclusion by performing a complete numerical and algebraic study of the parameter…

High Energy Physics - Phenomenology · Physics 2015-01-26 Giovanna Cottin , Marco A. Díaz , María José Guzmán , Boris Panes

We analyze the prospects for light neutralino dark matter in the minimal supersymmetric model extended by a $U(1)$ gauge group. We allow the neutralino to be an arbitrary admixture of singlet and doublet higgsinos, as well as of the three…

High Energy Physics - Phenomenology · Physics 2014-10-22 Mariana Frank , Subhadeep Mondal

Within the minimal supergravity model (mSUGRA) framework, the expectation for the relic density of neutralinos exceeds the WMAP determination unless neutralinos a) have a significant higgsino component, b) have a mass close to half that of…

High Energy Physics - Phenomenology · Physics 2009-11-10 Howard Baer , Azar Mustafayev , Stefano Profumo , Alexander Belyaev , Xerxes Tata