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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…

高能物理 - 唯象学 · 物理学 2010-01-15 Koichi Hamaguchi , Fuminobu Takahashi , T. T. Yanagida

We show that a mini-thermal inflation occurs naturally in a class of gauge mediation models of supersymmetry (SUSY) breaking, provided that the reheating temperature T_R of the primary inflation is much higher than the SUSY-breaking scale,…

高能物理 - 唯象学 · 物理学 2009-11-10 M. Fujii , M. Ibe , T. Yanagida

We discuss the upper bound on the gluino mass in supersymmetric models with vector-like extra matters. In order to realize the observed Higgs mass of 125 GeV, the gluino mass is bounded from above in supersymmetric models. With the…

高能物理 - 唯象学 · 物理学 2016-08-24 Takeo Moroi , Tsutomu T. Yanagida , Norimi Yokozaki

We study the production of spin 1/2 gravitinos in a thermal Universe. Taking into account supersymmetry breaking due to the finite thermal energy density of the Universe, there is a large enhancement in the cross section of production of…

宇宙学与河外天体物理 · 物理学 2017-08-04 Richa Arya , Namit Mahajan , Raghavan Rangarajan

The production and the final abundance of gravitino dark matter appear to depend crucially on the restoration of the global U(1) $R$-symmetry of GMSB sectors in a threefold way. An $R$-symmetric phase effectively suppresses the production…

高能物理 - 唯象学 · 物理学 2015-06-15 Iannis Dalianis

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 gravitino problem gives a severe constraint on the thermal leptogenesis scenario. This problem leads us to consider some alternatives to it if we try to keep the gravitino mass around the weak scale $m_{3/2} \sim 100$ GeV. We consider,…

高能物理 - 唯象学 · 物理学 2009-11-11 Takeshi Fukuyama , Tatsuru Kikuchi , Toshiyuki Osaka

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…

高能物理 - 唯象学 · 物理学 2009-11-11 Takeo Moroi

We investigate the possibility of probing high reheating temperature scenarios at the LHC, in supersymmetric models where the gravitino is the lightest supersymmetric particle, and the stau is the next-to-lightest supersymmetric particle.…

高能物理 - 唯象学 · 物理学 2010-11-09 Motoi Endo , Koichi Hamaguchi , Kouhei Nakaji

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

Motivated by the absence of signals of new physics in both searches for new particles at LHC and for a Weakly Interacting Massive Particle (WIMP) dark matter candidate, we consider a scenario where supersymmetry is broken at a scale above…

高能物理 - 唯象学 · 物理学 2017-05-10 Karim Benakli , Yifan Chen , Emilian Dudas , Yann Mambrini

The low reheat temperature at the end of inflation from the gravitino bound constrains the creation of heavy Majorana neutrinos associated with models of leptogenesis. However, a detailed view of the reheating of the Universe at the end of…

高能物理 - 唯象学 · 物理学 2014-11-18 Raghavan Rangarajan , Narendra Sahu

Gravitino dark matter, together with thermal leptogenesis, implies an upper bound on the masses of superparticles. In the case of broken R-parity the constraints from primordial nucleosynthesis are naturally satisfied and decaying…

高能物理 - 唯象学 · 物理学 2010-04-21 Wilfried Buchmuller , Motoi Endo , Tetsuo Shindou

We re-consider the gravitino as dark matter in the framework of the Constrained MSSM. We include several recently suggested improvements on: (i) the thermal production of gravitinos, (ii) the calculation of the hadronic spectrum from NLSP…

高能物理 - 唯象学 · 物理学 2010-04-23 Sean Bailly , Ki-Young Choi , Karsten Jedamzik , Leszek Roszkowski

A successful implementation of thermal leptogenesis requires the re-heat temperature after inflation T_R to exceed ~2\times 10^9 GeV. Such a high T_R value typically leads to an overproduction of gravitinos in the early universe, which will…

高能物理 - 唯象学 · 物理学 2015-05-20 Howard Baer , Sabine Kraml , Andre Lessa , Sezen Sekmen

In this talk, we studied the implication of the constraint on the reheating temperature coming from the gravitino problem on models of leptogenesis. We point out that in supersymmetric extensions of the standard model, all existing models…

高能物理 - 唯象学 · 物理学 2007-05-23 D. Delepine

If the lightest supersymmetric particle (LSP) is Higgsino-like, the thermal relic density is lower than the observed dark matter content for a LSP mass in the sub-TeV region. We outline constraints arising from the Fermi Gamma-Ray Telescope…

高能物理 - 唯象学 · 物理学 2013-05-30 Rouzbeh Allahverdi , Bhaskar Dutta , Kuver Sinha

Gravitino problem is discussed in detail. We derive an upperbound on the reheating temperature from the constraints of the big-bang nucleosynthesis and the present mass density of the universe. Compared to previous works, we have improve…

高能物理 - 唯象学 · 物理学 2016-09-01 Takeo Moroi

For supersymmetric theories with gravitino dark matter, the maximal reheating temperature consistent with big bang nucleosynthesis bounds arises when the physical gaugino masses are degenerate. We consider the cases of a stau or sneutrino…

高能物理 - 唯象学 · 物理学 2009-12-15 Marek Olechowski , Stefan Pokorski , Krzysztof Turzynski , James D. Wells

The gravitino dark matter with neutralino NLSP hypothesis is investigated in the framework of NMSSM. We have considered both the thermal and non-thermal gravitino production mechanisms, and we have taken into account all the collider and…

高能物理 - 唯象学 · 物理学 2011-01-27 Grigoris Panotopoulos