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相关论文: Gravitino dark matter production at finite tempera…

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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

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

Considering gravitino dark matter scenarios, we obtain the full gauge-invariant result for the relic density of thermally produced gravitinos to leading order in the Standard Model gauge couplings. For the temperatures required by thermal…

高能物理 - 唯象学 · 物理学 2010-04-06 Josef Pradler , Frank Daniel Steffen

At the end of inflation, the inflaton field decays into an initially nonthermal population of relativistic particles which eventually thermalize. We consider the production of dark matter from this relativistic plasma, focusing on the…

高能物理 - 唯象学 · 物理学 2018-12-18 Marcos A. G. Garcia , Mustafa A. Amin

We discuss thermal production of (pseudo) goldstinos, the Goldstone fermions emerging from (multiple) SUSY breaking sectors, when the reheating temperature is well below the superpartner masses. In such a case, the production during…

高能物理 - 唯象学 · 物理学 2015-08-12 Angelo Monteux , Chang Sub Shin

Affleck-Dine baryogenesis, accompanied by the formation and subsequent decay of Q-balls, can generate both the baryon asymmetry of the universe and dark matter in the form of gravitinos. The gravitinos from Q-ball decay dominate over the…

高能物理 - 唯象学 · 物理学 2010-10-27 Ian M. Shoemaker , Alexander Kusenko

Affleck-Dine baryogenesis in models where the gravitino is both the lightest supersymmetric particle and the dark matter candidate is investigated. For a high enough reheating temperature to produce sufficient gravitinos by thermal…

高能物理 - 唯象学 · 物理学 2009-11-11 Osamu Seto

The gravitino may well play an important role in cosmology, not only because its interactions are Planck-suppressed and therefore long-lived, but also because it is copiously produced via various processes such as particle scatterings in…

高能物理 - 唯象学 · 物理学 2015-06-11 Kwang Sik Jeong , Fuminobu Takahashi

The success of primordial nucleosynthesis imposes stringent bounds on the abundance of gravitational relics. This is particularly true for gravitinos, which - for models with gravitationally mediated supersymmetry breaking - are expected to…

高能物理 - 唯象学 · 物理学 2007-05-23 Hans Peter Nilles , Marco Peloso

We make use of the phase space density approach to discuss gravitino as a warm dark matter candidate. Barring fine tuning between the reheat temperature in the Universe and superparticle masses, we find that \emph{warm} gravitinos have both…

高能物理 - 唯象学 · 物理学 2009-02-09 D. Gorbunov , A. Khmelnitsky , V. Rubakov

We consider the direct $s$-channel gravitational production of dark matter during the reheating process. Independent of the identity of the dark matter candidate or its non-gravitational interactions, the gravitational process is always…

高能物理 - 唯象学 · 物理学 2021-06-16 Yann Mambrini , Keith A. Olive

We consider the simplest class of the R-invariant gauge mediation model with the gravitino mass in the one to ten keV range. We show that the entropy production from the supersymmetry breaking sector makes the gravitino into a warm dark…

高能物理 - 唯象学 · 物理学 2015-03-17 Masahiro Ibe , Ryosuke Sato , Tsutomu T. Yanagida , Kazuya Yonekura

We explore an alternative mechanism for the production of gravitino dark matter whereby relic gravitinos originate from the decays of superpartners which are still in thermal equilibrium, i.e. via freeze-in. Contributions to the gravitino…

高能物理 - 唯象学 · 物理学 2015-05-27 Clifford Cheung , Gilly Elor , Lawrence Hall

Supersymmetric thermal leptogenesis with a hierarchical right-handed neutrino mass spectrum requires the mass of the lightest right-handed neutrino to be heavier than about 10^9 GeV. This is in conflict with the upper bound on the reheating…

高能物理 - 唯象学 · 物理学 2008-11-26 G. F. Giudice , L. Mether , A. Riotto , F. Riva

In this work, we explore the "degenerate gravitino" scenario where the mass difference between the gravitino and the lightest MSSM particle is much smaller than the gravitino mass itself. In this case, the energy released in the decay of…

高能物理 - 唯象学 · 物理学 2010-05-27 Lotfi Boubekeur , Ki Young Choi , Roberto Ruiz de Austri , Oscar Vives

Many models of supersymmetry breaking, in the context of either supergravity or superstring theories, predict the presence of particles with weak scale masses and Planck-suppressed couplings. Typical examples are the scalar moduli and the…

高能物理 - 唯象学 · 物理学 2009-10-31 G. F. Giudice , A. Riotto , I. Tkachev

The origin of the hot phase of the early universe remains so far an unsolved puzzle. A viable option is entropy production through the decays of heavy Majorana neutrinos whose lifetimes determine the initial temperature. We show that…

高能物理 - 唯象学 · 物理学 2015-05-27 W. Buchmuller , K. Schmitz , G. Vertongen

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

We consider the possibility that supersymmetry is broken above the inflationary mass scale and that the only "low" energy remnant of supersymmetry is the gravitino with mass of order the EeV scale. The gravitino in this class of models…

高能物理 - 唯象学 · 物理学 2017-08-09 Emilian Dudas , Yann Mambrini , Keith Olive

We reconsider thermal production of gravitinos in the early universe, adding to previously considered 2 -> 2 gauge scatterings: a) production via 1 -> 2 decays, allowed by thermal masses; b) the effect of the top Yukawa coupling; c) a…

高能物理 - 唯象学 · 物理学 2008-11-26 Vyacheslav S. Rychkov , Alessandro Strumia