中文
相关论文

相关论文: Unstable Gravitino Dark Matter and Neutrino Flux

200 篇论文

Cosmological issues of the gravitino production by the decay of a heavy scalar field $X$ are examined, assuming that the damped coherent oscillation of the scalar once dominates the energy of the universe. The coupling of the scalar field…

高能物理 - 唯象学 · 物理学 2009-11-11 Takehiko Asaka , Shuntaro Nakamura , Masahiro Yamaguchi

A brief review of supersymmetric models and their candidates for dark matter is carried out. The neutralino is a WIMP candidate in the MSSM where $R$-parity is conserved, but this model has the $\mu$ problem. There are natural solutions to…

高能物理 - 唯象学 · 物理学 2017-04-05 Carlos Munoz

If the gravitino is sufficiently light and stable it will behave as an effective massless neutrino species at the time of nucleosynthesis. Depending on the temperature at which it decouples from the thermal bath in the early universe, the…

高能物理 - 唯象学 · 物理学 2009-10-28 Tony Gherghetta

In supersymmetric extensions of the Standard Model, the lightest neutralino, the gravitino, and the axino can appear as the lightest supersymmetric particle and as such provide a compelling explanation of the non-baryonic dark matter in our…

高能物理 - 唯象学 · 物理学 2007-11-28 Frank Daniel Steffen

We propose a new class of R-parity violating extension of MSSM with type II seesaw mechanism for neutrino masses where an unstable gravitino is the dark matter of the Universe. It decays predominantly into three leptons final states,…

高能物理 - 唯象学 · 物理学 2014-11-18 Shao-Long Chen , Rabindra N. Mohapatra , Shmuel Nussinov , Yue Zhang

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

The existence of dark matter provides strong evidence for physics beyond the Standard Model. Extending the Standard Model with the Peccei-Quinn symmetry and/or supersymmetry, compelling dark matter candidates appear. For the axion, the…

高能物理 - 唯象学 · 物理学 2009-02-18 Frank Daniel Steffen

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

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

We study the phenomenology of neutralino dark matter within generic supersymmetric scenarios where the Gaugino and Higgsino masses are much lighter than the scalar soft breaking masses (Split Supersymmetry). We consider a low-energy…

高能物理 - 唯象学 · 物理学 2007-05-23 Antonio Masiero , Stefano Profumo , Piero Ullio

Supersymmetry breaking sectors generically have an approximate global U(1) $R$-symmetry. Thermal effects tend to restore the $R$-symmetry in the reheated early universe. We revisit the gravitino generation from the thermal plasma and we…

高能物理 - 唯象学 · 物理学 2013-05-30 Ioannis Dalianis

Axino and gravitino are promising candidates to solve the dark matter (DM) problem in the framework of supersymmetry. In this work, we assume that the axino is the lightest supersymmetric particle (LSP), and therefore contributes to DM. In…

高能物理 - 唯象学 · 物理学 2020-02-05 German A. Gomez-Vargas , Daniel E. Lopez-Fogliani , Carlos Munoz , Andres D. Perez

Scenarios where gravitinos with GeV masses make up dark matter are known to be in tension with high reheating temperatures, as required by e.g. thermal leptogenesis. This tension comes from the longevity of the NLSPs, which can destroy the…

高能物理 - 唯象学 · 物理学 2010-12-13 Jonas Schmidt , Christoph Weniger , Tsutomu T. Yanagida

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

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

Supersymmetry offers a cold dark matter candidate, provided that lepton number is {\em not violated by an odd number of units}. On the other hand, lepton number violation by even (two) units gives us an attractive mechanism of neutrino mass…

高能物理 - 唯象学 · 物理学 2008-11-26 Biswarup Mukhopadhyaya , Soumitra SenGupta , Raghavendra Srikanth

After reviewing the theoretical, phenomenological and experimental motivations for supersymmetric extensions of the Standard Model, we recall that supersymmetric relics from the Big Bang are expected in models that conserve R parity. We…

宇宙学与河外天体物理 · 物理学 2010-01-21 John Ellis , Keith A. Olive

It is possible that the strongest interactions between dark matter and the Standard Model occur via the neutrino sector. Unlike gamma rays and charged particles, neutrinos provide a unique avenue to probe for astrophysical sources of dark…

We investigated the viability of neutralino dark matter in the gauge mediation from emergent supersymmetry proposal. In this proposal, supersymmetry is broken at Planck scale and consequently, the gravitino is superheavy and completely…

高能物理 - 唯象学 · 物理学 2009-01-06 Siew-Phang Ng , Nobuchika Okada

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