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相关论文: Gravitino Dark Matter and low-scale Baryogenesis

200 篇论文

In the present universe visible and dark matter contribute comparable energy density although they have different properties. This coincidence can be elegantly explained if the dark matter relic density, originating from a dark matter…

高能物理 - 唯象学 · 物理学 2011-09-05 Pei-Hong Gu , Manfred Lindner , Utpal Sarkar , Xinmin Zhang

We propose a scenario where dark matter (DM) with a wide mass range from a few keV to PeV can be produced solely from evaporating primordial black holes (PBH), while being consistent with the required free streaming length for structure…

高能物理 - 唯象学 · 物理学 2022-09-07 Basabendu Barman , Debasish Borah , Suruj Jyoti Das , Rishav Roshan

We consider a simple class of models in which the relic density of dark matter is determined by the baryon asymmetry of the universe. In these models a $B - L$ asymmetry generated at high temperatures is transfered to the dark matter, which…

高能物理 - 唯象学 · 物理学 2009-07-09 David E. Kaplan , Markus A. Luty , Kathryn M. Zurek

We study the possibility of improving the constraints on the lifetime of gravitino dark matter in scenarios with bilinear R-parity violation by estimating the amount of cosmic-ray antideuterons that can be produced in gravitino decays.…

高能物理 - 唯象学 · 物理学 2015-07-09 Timur Delahaye , Michael Grefe

Supersymmetric extensions of the Standard Model with small R-parity and lepton number violating couplings are naturally consistent with primordial nucleosynthesis, thermal leptogenesis and gravitino dark matter. We consider supergravity…

高能物理 - 唯象学 · 物理学 2010-11-01 Sergei Bobrovskyi , Wilfried Buchmuller , Jan Hajer , Jonas Schmidt

We propose late-time moduli decay as the common origin of baryons and dark matter. The baryon asymmetry is produced from the decay of new TeV scale particles, while dark matter is created from the (chain) decay of R-parity odd particles…

高能物理 - 唯象学 · 物理学 2011-04-22 Rouzbeh Allahverdi , Bhaskar Dutta , Kuver Sinha

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

In models with gauge mediated supersymmetry breaking the gravitino is the lightest supersymmetric particle. If R-parity is violated the gravitino decays, but with a half-live far exceeding the age of the universe and thus is, in principle,…

高能物理 - 唯象学 · 物理学 2008-11-26 M. Hirsch , W. Porod , D. Restrepo

We estimate the Baryon Asymmetry of the Universe (BAU) produced in an inverse seesaw model containing extra light singlets, and with lepton number conservation prior to the electroweak phase transition. An order one CP asymmetry epsilon is…

高能物理 - 唯象学 · 物理学 2015-06-11 Sacha Davidson , Martin Elmer

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

We propose a unified theory of dark matter (DM) genesis and baryogenesis. It explains the observed link between the DM density and the baryon density, and is fully testable by a combination of collider experiments and precision tests. Our…

高能物理 - 唯象学 · 物理学 2010-10-04 Lawrence J. Hall , John March-Russell , Stephen M. West

We present a new mechanism of Baryogenesis and dark matter production in which both the dark matter relic abundance and the baryon asymmetry arise from neutral $B$ meson oscillations and subsequent decays. This set-up is testable at hadron…

高能物理 - 唯象学 · 物理学 2019-02-22 Gilly Elor , Miguel Escudero , Ann E. Nelson

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

We examine a scenario in which the reheating temperature $T_R$ after inflation is so low that it is comparable to, or lower than, the freeze out temperature of ordinary WIMPs. In this case the dark matter relic abundance is reduced, thus…

高能物理 - 唯象学 · 物理学 2015-06-19 Leszek Roszkowski , Sebastian Trojanowski , Krzysztof Turzynski

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

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

We show that late Q-ball decay in the MSSM with gauge-mediated SUSY breaking can provide a natural source of non-thermal NLSPs which subsequently decay to gravitino dark matter without violating nucleosynthesis constraints. To show this, we…

高能物理 - 唯象学 · 物理学 2015-06-12 Francesca Doddato , John McDonald

The gravitino in models with a small violation of R-parity is a well-motivated decaying dark matter candidate that leads to a cosmological scenario that is consistent with big bang nucleosynthesis and thermal leptogenesis. The gravitino…

高能物理 - 唯象学 · 物理学 2012-08-07 Michael Grefe

We propose a new framework for explaining the proximity of the baryon and dark matter relic densities \Omega_{DM} \approx 5\Omega_B. The scenario assumes that the number density of the observed dark matter states is generated due to decays…

高能物理 - 唯象学 · 物理学 2015-06-12 James Unwin

The similarity of the observed mass densities of baryons and cold dark matter may be a sign they have a related origin. The baryon-to-dark matter ratio can be understood in the MSSM with right-handed (RH) neutrinos if CDM is due to a d = 4…

高能物理 - 唯象学 · 物理学 2007-10-24 John McDonald