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We investigate the cosmological gravitino problem in gauge-mediated supersymmetry breaking models, where the gravitino becomes in general the lightest supersymmetric particle (LSP). In order to avoid the overclosure of the stable gravitino,…

高能物理 - 唯象学 · 物理学 2009-10-31 T. Asaka , K. Hamaguchi , Koshiro Suzuki

We consider the dynamics of the supersymmetry-breaking scalar field and the production of dark matter gravitinos via its decay in a gauge-mediated supersymmetry breaking model with metastable vacuum. We find that the scalar field amplitude…

高能物理 - 唯象学 · 物理学 2013-05-30 Andrea Ferrantelli , John McDonald

In the framework of the Constrained MSSM we re--examine the gravitino as the lightest superpartner and a candidate for cold dark matter in the Universe. Unlike in other recent studies, we include both a thermal contribution to its relic…

高能物理 - 唯象学 · 物理学 2011-05-05 David G. Cerdeno , Ki-Young Choi , Karsten Jedamzik , Leszek Roszkowski , Roberto Ruiz de Austri

In all supersymmetric theories, gravitinos, with mass suppressed by the Planck scale, are an obvious candidate for dark matter; but if gravitinos ever reached thermal equilibrium, such dark matter is apparently either too abundant or too…

高能物理 - 唯象学 · 物理学 2017-08-03 Raymond T. Co , Francesco D'Eramo , Lawrence J. Hall , Keisuke Harigaya

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…

高能物理 - 唯象学 · 物理学 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…

高能物理 - 唯象学 · 物理学 2008-11-26 Raghavan Rangarajan , Narendra Sahu

Supersymmetric models provide very interesting scenarios to account for the dark matter of the Universe. In this talk we discuss scenarios with gravitino dark matter in R-parity breaking vacua, which not only reproduce very naturally the…

高能物理 - 唯象学 · 物理学 2009-02-02 Alejandro Ibarra

In supersymmetric models of warm inflation, the large temperature of the radiation bath produced by the dissipative motion of the inflaton field may induce a significant thermal abundance of potentially dangerous gravitinos. While previous…

高能物理 - 唯象学 · 物理学 2013-01-16 Sam Bartrum , Arjun Berera , Joao G. Rosa

Supersymmetric scenarios where the lightest superparticle (LSP) is the gravitino are an attractive alternative to the widely studied case of a neutralino LSP. A strong motivation for a gravitino LSP arises from the possibility of achieving…

高能物理 - 唯象学 · 物理学 2014-04-24 Jan Heisig

Scenarios with gravitino dark matter face potential cosmological problems induced by the presence of the Next-to-Lightest Supersymmetric Particle (NLSP) at the time of Big Bang Nucleosynthesis (BBN). A very simple, albeit radical, solution…

高能物理 - 唯象学 · 物理学 2007-10-16 Alejandro Ibarra

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…

高能物理 - 唯象学 · 物理学 2009-11-10 Rouzbeh Allahverdi , Manuel Drees

We analyze a simple Split Supersymmetry scenario where fermion masses come from anomaly mediation, yielding m_s ~ 1000 TeV, m_{3/2} ~ 100 TeV, and m_f ~ 1 TeV. We consider non-thermal dark matter production in the presence of moduli, and we…

高能物理 - 唯象学 · 物理学 2010-02-03 Jared Kaplan

We examine dark matter production rates in supersymmetric axion models typified by the mass hierarchy m_gravitino << m_neutralino << m_axino. In such models, one expects the dark matter to be composed of an axion/gravitino admixture. After…

高能物理 - 唯象学 · 物理学 2015-04-20 Kyu Jung Bae , Howard Baer , Eung Jin Chun , Chang Sub Shin

The presence of high reheating temperatures in the thermal history of the universe challenges supersymmetric scenarios owing to the gravitino problem. We revise a general R-parity conserving gravitino dark matter scenario with a stau as the…

高能物理 - 唯象学 · 物理学 2014-05-26 Jan Heisig

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…

高能物理 - 唯象学 · 物理学 2009-10-31 M. Bolz , W. Buchmüller , M. Plümacher

The gravitino is a promising supersymmetric dark matter candidate which does not require exact R-parity conservation. In fact, even with some small R-parity breaking, gravitinos are sufficiently long-lived to constitute the dark matter of…

高能物理 - 唯象学 · 物理学 2010-04-21 Laura Covi , Michael Grefe , Alejandro Ibarra , David Tran

We implement the asymmetric dark matter framework, linking the ordinary and dark matter abundances, within a supersymmetric context. We consider a supersymmetric model that respects an approximate $U(1)_R$ symmetry, which is broken in such…

高能物理 - 唯象学 · 物理学 2025-02-13 Marco Ardu , Daniel Queiroz Correa , Oscar Vives

We study the effects of the unstable gravitino on the big-bang nucleosynthesis. If the gravitino mass is smaller than \sim 10 TeV, primordial gravitinos produced after the inflation are likely to decay after the big-bang nucleosynthesis…

高能物理 - 唯象学 · 物理学 2008-11-26 Kazunori Kohri , Takeo Moroi , Akira Yotsuyanagi

The impact of a kination-dominated phase generated by a quintessential exponential model on the thermal abundance of gravitinos and axinos is investigated. We find that their abundances become proportional to the transition temperature from…

高能物理 - 唯象学 · 物理学 2009-07-20 M. E. Gomez , S. Lola , C. Pallis , J. Rodriguez-Quintero

In higher-dimensional supersymmetric theories gauge couplings of the effective four-dimensional theory are determined by expectation values of scalar fields. We find that at temperatures above a critical temperature $T_*$, which depends on…

高能物理 - 唯象学 · 物理学 2008-11-26 W. Buchmüller , K. Hamaguchi , M. Ratz