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相关论文: Is gravitino still a warm dark matter candidate?

200 篇论文

In the cosmological paradigm, cold dark matter (DM) dominates the mass content of the Universe and is present at every scale. Candidates for DM include many extensions of the Standard Model with weakly interacting massive particles (WIMPs)…

高能天体物理现象 · 物理学 2017-08-25 Benjamin Zitzer , VERITAS Collaboration

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

Light gravitinos, with mass in the eV to MeV range, are well-motivated in particle physics, but their status as dark-matter candidates is muddled by early-Universe uncertainties. We investigate how upcoming data from colliders may clarify…

高能物理 - 唯象学 · 物理学 2011-10-12 Jonathan L. Feng , Marc Kamionkowski , Samuel K. Lee

Supersymmetric extensions of the Standard Model when combined with the Peccei-Quinn solution to the strong CP problem necessarily contain also the axino, the fermionic partner of the axion. In contrast to the neutralino and the gravitino,…

高能物理 - 唯象学 · 物理学 2007-05-23 Leszek Roszkowski

We show that hidden hot dark matter, hidden-sector dark matter with interactions that decouple when it is relativistic, is a viable dark matter candidate provided it has never been in thermal equilibrium with the particles of the standard…

宇宙学与河外天体物理 · 物理学 2009-12-15 Kris Sigurdson

We explore the production of thermal dark matter (DM) candidates (WIMPs, SIMPs, ELDERs and Cannibals) during cosmic reheating. Assuming a general parametrization for the scaling of the inflaton energy density and the standard model (SM)…

高能物理 - 唯象学 · 物理学 2024-08-28 Nicolás Bernal , Kuldeep Deka , Marta Losada

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

In the cosmological paradigm, cold dark matter (DM) dominates the mass content of the Universe and is present at every scale. Candidates for DM include many extensions of the standard model, with a weakly interacting massive particle (WIMP)…

高能天体物理现象 · 物理学 2019-08-14 B. Zitzer

High-scale supersymmetry (SUSY) with a split spectrum has become increasingly interesting given the current experimental results. A SUSY scale above the weak scale could be naturally associated with a heavy unstable gravitino, whose decays…

高能物理 - 唯象学 · 物理学 2015-06-19 JiJi Fan , Bithika Jain , Ogan Ozsoy

We address the question how light the lightest MSSM neutralino can be as dark matter candidate in a scenario where all supersymmetric scalar particles are heavy. The hypothesis that the neutralino accounts for the observed dark matter…

高能物理 - 唯象学 · 物理学 2015-06-23 Lorenzo Calibbi , Jonas M. Lindert , Toshihiko Ota , Yasutaka Takanishi

The possibility of the CDM axino is presented. From the early days of supersymmetry, axino has been considered as hot dark matter and warm dark matter. But the CDM axino has been considered quite recently. It is because the low reheating…

天体物理学 · 物理学 2007-05-23 Jihn E. Kim

We investigate density fluctuations in a scenario with gravitino dark matter in the framework of modulated reheating, which is known to generate large non-Gaussianity. We show that gravitino dark matter is disfavored if primordial…

宇宙学与河外天体物理 · 物理学 2010-04-28 Tomo Takahashi , Masahide Yamaguchi , Jun'ichi Yokoyama , Shuichiro Yokoyama

The Large Volume Scenario for getting a non-supersymmetric vacuum in type IIB string theory leads, through the Weyl anomaly and renormalization group running, to an interesting phenomenology. However, for gravitino masses below 500 TeV…

高能物理 - 唯象学 · 物理学 2015-06-04 Senarath de Alwis , Kevin Givens

We study the consequences of the gravitino decay into dark matter. We suppose that the lightest neutralino is the main component of dark matter. In our framework gravitino is heavy enough to decay before Big Bang Nucleosynthesis starts. We…

高能物理 - 唯象学 · 物理学 2007-06-29 David Gherson

In the light of recent experimental data on gaugino searches, we revisit the direct-transmission model of dynamical supersymmery breaking with the gravitino mass m_{\tilde{G}}\leq 16 eV, which does not have any cosmological or astrophysical…

高能物理 - 唯象学 · 物理学 2010-04-05 Masahiro Ibe , Kazuhiro Tobe , Tsutomu Yanagida

We point out that there is no cosmological gravitino problem in a certain class of gauge-mediated supersymmetry-breaking (GMSB) models. The constant term in the superpotential naturally causes small mixings between the standard-model and…

高能物理 - 唯象学 · 物理学 2009-11-07 Masaaki Fujii , T. Yanagida

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…

高能物理 - 唯象学 · 物理学 2014-10-22 Mariana Frank , Subhadeep Mondal

Gravitino Dark Matter represents a compelling scenario in Supersymmetry, which brings together a variety of data from cosmology and collider physics. We discuss the constraints obtained from the LHC on supersymmetric models with gravitino…

高能物理 - 唯象学 · 物理学 2015-12-23 Alexandre Arbey , Marco Battaglia , Laura Covi , Jasper Hasenkamp , Farvah Mahmoudi

In the cosmological paradigm, cold dark matter (DM) dominates the mass content of the Universe and is present at every scale. Candidates for DM include many extensions of the standard model, such as weakly interacting massive particles…

高能天体物理现象 · 物理学 2019-08-13 Benjamin Zitzer

In supergravity models with low supersymmetry breaking scale the gravitinos can be superlight with mass in the micro-eV to keV range. In such a case, gravitino emission provides a new cooling mechanism for protoneutron stars and therefore…

高能物理 - 唯象学 · 物理学 2014-11-17 Duane A. Dicus , Rabindra N. Mohapatra , Vigdor L. Teplitz