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Bilinear R-parity violation provides an attractive origin for neutrino masses and mixings. In such schemes the gravitino is a viable decaying dark matter particle whose R-parity violating decays lead to monochromatic photons with rates…

高能物理 - 唯象学 · 物理学 2013-05-30 Diego Restrepo , Marco Taoso , J. W. F. Valle , Oscar Zapata

If R-parity is only mildly violated then the lightest supersymmetric particle (LSP) can be stable over cosmologically time-scales and still account for the dark matter relic density. We examine the possibility of generating detectable X-ray…

高能物理 - 唯象学 · 物理学 2014-07-30 Christopher Kolda , James Unwin

We show that in the case of small R-parity and lepton number breaking couplings, primordial nucleosynthesis, thermal leptogenesis and gravitino dark matter are naturally consistent for gravitino masses m_{3/2} \gsim 5 GeV. We present a…

高能物理 - 唯象学 · 物理学 2010-04-06 Wilfried Buchmuller , Laura Covi , Koichi Hamaguchi , Alejandro Ibarra , Tsutomu Yanagida

In this paper, we revisit the gravitino dark matter scenario in the presence of the bilinear $R$-parity violating interaction. In particular, we discuss a consistency with the thermal leptogenesis. For a high reheating temperature required…

高能物理 - 唯象学 · 物理学 2017-06-01 Masahiro Ibe , Motoo Suzuki , Tsutomu T. Yanagida

In theories with a gauge-mediated mechanism of supersymmetry breaking the gravitino is likely to be the lightest superparticle and, hence, a candidate for dark matter. We show that the decay of the next-to-lightest superparticle into a…

高能物理 - 唯象学 · 物理学 2009-10-28 Stefano Borgani , Antonio Masiero , Masahiro Yamaguchi

A new scheme for lightest supersymmetric particle (LSP) dark matter is introduced and studied in theories of TeV supersymmetry with a QCD axion, $a$, and a high reheat temperature after inflation, $T_R$. A large overproduction of axinos…

高能物理 - 唯象学 · 物理学 2017-03-20 Raymond T. Co , Francesco D'Eramo , Lawrence J. Hall

The gravitino is a promising supersymmetric dark matter candidate, even without strict R-parity conservation. In fact, with some small R-parity violation, gravitinos are sufficiently long-lived to constitute the dark matter of the universe,…

高能物理 - 唯象学 · 物理学 2014-08-01 Michael Grefe

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.…

高能物理 - 唯象学 · 物理学 2025-01-23 Helmut Eberl , Ioannis D. Gialamas , Vassilis C. Spanos

Current observations of the cosmic microwave background could confirm an increase in the radiation energy density after primordial nucleosynthesis but before photon decoupling. We show that, if the gravitino problem is solved by a light…

高能物理 - 唯象学 · 物理学 2015-05-28 Jasper Hasenkamp

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 2015-05-14 Wilfried Buchmuller

Stable particle dark matter may well originate during the decay of long-lived relic particles, as recently extensively examined in the cases of the axino, gravitino, and higher-dimensional Kaluza-Klein (KK) graviton. It is shown that in…

天体物理学 · 物理学 2009-11-13 Karsten Jedamzik , Martin Lemoine , Gilbert Moultaka

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

Axino as the superpartner of axion that solves the strong CP problem can be a good candidate of dark matter. Inspired by the 3.5 keV X-ray line signal found to be originated from galaxy clusters and Andromeda galaxy, we study axino models…

高能物理 - 唯象学 · 物理学 2014-06-02 Seng Pei Liew

Thermal leptogenesis requires the reheating temperature $T_R \gsim 3\times 10^{9}$ GeV, which contradicts a recently obtained constraint on the reheating temperature, $T_R \lsim 10^6$ GeV, for the gravitino mass of 100 GeV-10 TeV. This…

高能物理 - 唯象学 · 物理学 2015-06-25 M. Fujii , M. Ibe , T. Yanagida

We investigate the LHC sensitivity to supersymmetric models with light higgsinos, small R-parity breaking and gravitino dark matter. The limits on decaying gravitino dark matter from gamma-ray searches with the Fermi-LAT put a lower bound…

高能物理 - 唯象学 · 物理学 2013-03-06 S. Bobrovskyi , J. Hajer , S. Rydbeck

Gravitinos with a mass in the keV range are an interesting candidate for warm dark matter. Recent measurements of the matter density of the universe and of cosmic structures at the dwarf galaxy scale rule out the simplest gravitino models…

天体物理学 · 物理学 2009-11-07 Edward A. Baltz , Hitoshi Murayama

We investigate gravitino dark matter produced thermally at high temperatures and in decays of a long-lived sneutrino. We consider the Non-Universal Higgs Model and a generalized gauge mediation model, and in each case identify sneutrino…

高能物理 - 唯象学 · 物理学 2015-06-12 Leszek Roszkowski , Sebastian Trojanowski , Krzysztof Turzynski , Karsten Jedamzik

Observations of nearby galaxies and galaxy clusters have reported an unexpected X-ray emission line around 3.5 kilo-electron volts (keV). Proposals to explain this line include decaying dark matter$-$in particular, that the decay of sterile…

宇宙学与河外天体物理 · 物理学 2021-03-03 Christopher Dessert , Nicholas L. Rodd , Benjamin R. Safdi

Cosmological issues are examined when gravitino is the lightest superparticle (LSP) and R-parity is broken. Decays of the next lightest superparticles occur rapidly via R-parity violating interaction, and thus they do not upset the big-bang…

高能物理 - 唯象学 · 物理学 2011-05-05 Fumihiro Takayama , Masahiro Yamaguchi

Successful implementation of thermal leptogenesis requires re-heat temperatures T_R\agt 2\times 10^9 GeV, in apparent conflict with SUSY models with TeV-scale gravitinos, which require much lower T_R in order to avoid Big Bang…

高能物理 - 唯象学 · 物理学 2010-12-08 Howard Baer , Sabine Kraml , Andre Lessa , Sezen Sekmen
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