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Related papers: Gravitino Dark Matter and Light Element Adundances

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For gravitino dark matter with conserved R-parity and mass in the GeV range, very strong constraints from Big Bang Nucleosynthesis exclude the popular NLSP candidates like neutralino and charged sleptons. In this letter we therefore draw…

High Energy Physics - Phenomenology · Physics 2008-11-26 Laura Covi , Sabine Kraml

The gravitino of mass 10-100 GeV is a well motivated scenario in supergravity. If the stau is the next lightest supersymmetry particle, its life-time becomes order of $10^{6-8}$ sec. If it is the case the stau makes a big impact on the…

High Energy Physics - Phenomenology · Physics 2012-02-14 Koichi Hamaguchi , Tetsuo Hatsuda , Masayasu Kamimura , Tsutomu T. Yanagida

Standard Big Bang nucleosynthesis at baryonic density as inferred by WMAP implies a primordial Li7 abundance factor of two to three larger than that inferred by observations of low--metallicity halo stars. Recent observations of Li6 in halo…

High Energy Physics - Phenomenology · Physics 2009-11-11 Karsten Jedamzik , Ki-Young Choi , Leszek Roszkowski , Roberto Ruiz de Austri

We demonstrate that megaton-mass neutrino telescopes are able to observe the signal from long-lived particles beyond the Standard Model, in particular the stau, the supersymmetric partner of the tau lepton. Its signature is an excess of…

A search for slepton production via the decay of pair-produced neutralinos has been performed under the assumption that the sleptons have observable lifetime in the detector before each decays to a lepton and a gravitino. Sleptons,…

High Energy Physics - Experiment · Physics 2007-05-23 Luke Jones

The tau lepton's supersymmetric partner, the stau, appears in some models as the next-to-lightest supersymmetric particle. Their decay process into the lightest superpartner is usually suppressed by supersymmetry breaking, which makes it a…

High Energy Astrophysical Phenomena · Physics 2021-07-22 Jan-Henrik Schmidt-Dencker , Stephan Meighen-Berger , Christian Haack

The axino, the supersymmetric partner of axion, is a well-motivated warm/hot dark matter candidate, and provides a natural solution to the relic density problem for the bino-like neutralino if it is the lightest supersymmetric particle…

High Energy Physics - Phenomenology · Physics 2023-04-04 Wenxing Zhang , Waqas Ahmed , Imtiaz Khan , Tianjun Li , Shabbar Raza

We consider supersymmetric theories where the gravitino is the lightest superparticle (LSP). Assuming that the long-lived next-to-lightest superparticle (NSP) is a charged slepton, we investigate two complementary ways to prove the…

High Energy Physics - Phenomenology · Physics 2009-07-09 Wilfried Buchmuller , Koichi Hamaguchi , Michael Ratz , Tsutomu Yanagida

It has recently been pointed out that a component of the observed gamma ray emission in the low-latitudes of Fermi Bubble has a spectral shape that can be explained by a 10 GeV dark matter (DM) annihilating to tau leptons with a…

High Energy Physics - Phenomenology · Physics 2014-01-31 Kaoru Hagiwara , Satyanarayan Mukhopadhyay , Junya Nakamura

Various supersymmetric (SUSY) scenarios predict a sub-GeV neutralino decaying into a single photon and an invisible state. This signature has recently been studied in a number of intensity frontier experiments, finding constraints…

High Energy Physics - Phenomenology · Physics 2023-06-02 Krzysztof Jodłowski

The modest addition of the dimension-5 term lambda(H_u.H_d)^2/M to the superpotential of the minimal supersymmetric standard model (MSSM) originated from physics beyond the MSSM (BMSSM) has a significant impact on the scenario of the…

High Energy Physics - Phenomenology · Physics 2015-05-13 Kingman Cheung , Seong Youl Choi , Jeonghyeon Song

In this talk, we present the package GravitinoPack that calculates decays of unstable supersymmetric particles, involving gravitinos in the final or initial state. If the gravitino is the dark matter particle and therefore stable, the…

High Energy Physics - Phenomenology · Physics 2015-10-13 Helmut Eberl , Vassilis C. Spanos

We investigate the phenomenology of the gravitino dark matter scenario with a stau as the next-to-lightest supersymmetric particle at the LHC. For a wide range of gravitino masses the lighter stau is stable on the scale of a detector and…

High Energy Physics - Phenomenology · Physics 2011-12-16 Jan Heisig , Joern Kersten

Sleptons, neutralinos and charginos were searched for in the context of scenarios where the lightest supersymmetric particle is the gravitino. It was assumed that the stau is the next-to-lightest supersymmetric particle. Data collected with…

High Energy Physics - Experiment · Physics 2010-04-08 The DELPHI Collaboration , P. Abreu

We study the phenomenology of a supersymmetric scenario where the next-to-lightest superparticle is the lighter stau and long-lived due to a very weakly coupled lightest superparticle, such as the gravitino. We investigate the LHC…

High Energy Physics - Phenomenology · Physics 2012-12-27 Jan Heisig , Jörn Kersten

We consider the effects of neutralino-stau coannihilations on the cosmological relic density of the lightest supersymmetric particle (LSP) $\chi$ in the minimal supersymmetric extension of the Standard Model (MSSM), particularly in the…

High Energy Physics - Phenomenology · Physics 2008-11-26 John Ellis , Toby Falk , Keith A. Olive

We study effects of long-lived massive particles, which decay during the big-bang nucleosynthesis (BBN) epoch, on the primordial abundances of light elements. Compared to the previous studies, (i) the reaction rates of the standard BBN…

High Energy Physics - Phenomenology · Physics 2018-12-04 Masahiro Kawasaki , Kazunori Kohri , Takeo Moroi , Yoshitaro Takaesu

Effects of the unstable gravitino on the big-bang nucleosynthesis (BBN) and its implications to particle cosmology are discussed. If the gravitino mass is smaller than \sim 20 TeV, lifetime of the gravitino becomes longer than \sim 1sec and…

High Energy Physics - Phenomenology · Physics 2009-11-11 Takeo Moroi

We study dark matter for gaugino-mediated supersymmetry breaking and compact dimensions of order the grand unification scale. Higgs fields are bulk fields, and in general their masses differ from those of squarks and sleptons at the…

High Energy Physics - Phenomenology · Physics 2009-11-11 Wilfried Buchmuller , Laura Covi , Joern Kersten , Kai Schmidt-Hoberg

In mSUGRA model we assume that gravitino, the LSP, plays the role of cold dark matter in the universe, while the lightest stau, the NLSP, catalyzes primordial BBN reconciling the discrepancy between theory and observations. We have taken…

High Energy Physics - Phenomenology · Physics 2010-04-15 Grigoris Panotopoulos