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相关论文: Baryon Asymmetry and Dark Matter

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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

We consider a minimal grand unified model where the dark matter arises from non-thermal decays of a messenger particle in the TeV range. The messenger particle compensates for the baryon asymmetry in the standard model and gives similar…

高能物理 - 唯象学 · 物理学 2007-05-23 Ryuichiro Kitano , Ian Low

The gravitino dark matter with neutralino NLSP hypothesis is investigated in the framework of NMSSM. We have considered both the thermal and non-thermal gravitino production mechanisms, and we have taken into account all the collider and…

高能物理 - 唯象学 · 物理学 2011-01-27 Grigoris Panotopoulos

We explore a scenario of high scale supersymmetry where all supersymmetric particles except gauginos stay at a high energy scale $M_{\rm SUSY}$ which is much larger than the reheating temperature $T_\text{RH}$. The dark matter is dominated…

高能物理 - 唯象学 · 物理学 2023-12-11 Chengcheng Han , Peiwen Wu , Jin Min Yang , Mengchao Zhang

A brief review is given of some recent works where baryogenesis and dark matter have a common origin within the $U(1)$ extensions of the standard model and of the minimal supersymmetric standard model. The models considered generate the…

高能物理 - 唯象学 · 物理学 2017-05-31 Wan-Zhe Feng , Pran Nath

In the framework of the CMSSM we study the gravitino as the lightest supersymmetric particle and the dominant component of cold dark matter in the Universe. We include both a thermal contribution to its relic abundance from scatterings in…

高能物理 - 唯象学 · 物理学 2010-04-06 Leszek Roszkowski , Roberto Ruiz de Austri , Ki-Young Choi

We implement the asymmetric dark matter framework, linking the ordinary and dark matter abundances, within a supersymmetric context. We consider a supersymmetric model that respects an approximate $U(1)_R$ symmetry, which is broken in such…

高能物理 - 唯象学 · 物理学 2025-02-13 Marco Ardu , Daniel Queiroz Correa , Oscar Vives

In this talk we discuss the origin and nature of the dark matter in the Affleck-Dine (AD) baryogenesis. The AD baryogenesis via most of the flat directions predict formations of large Q-balls, and a great number of the lightest…

高能物理 - 唯象学 · 物理学 2007-05-23 Masaaki Fujii , K. Hamaguchi

We consider the production of asymmetric dark matter during hidden sector baryogenesis. We consider a particular supersymmetric model where the dark matter candidate has a number density approximately equal to the baryon number density,…

高能物理 - 唯象学 · 物理学 2011-10-03 Bhaskar Dutta , Jason Kumar

We present a new scenario of gravitino dark matter which is compatible with the thermal leptogenesis. We confirm by an explicit calculation in supergravity that the relic abundance of thermally produced gravitino becomes insensitive to the…

高能物理 - 唯象学 · 物理学 2015-06-18 Hiraku Fukushima , Ryuichiro Kitano

We study supersymmetric scenarios where the dark matter is the gaugino of an unbroken hidden U(1) which interacts with the visible world only via a small kinetic mixing with the hypercharge. Strong constraints on the parameter space can be…

高能物理 - 唯象学 · 物理学 2009-02-12 A. Ibarra , A. Ringwald , C. Weniger

We investigate the dark matter and the cosmological baryon asymmetry in a simple theory where baryon (B) and lepton (L) number are local gauge symmetries that are spontaneously broken. In this model, the cold dark matter candidate is the…

高能物理 - 唯象学 · 物理学 2015-03-17 Timothy R. Dulaney , Pavel Fileviez Perez , Mark B. Wise

Neutralino dark matter is generally assumed to be relatively heavy, with a mass near the electroweak scale. This does not necessarily need to be the case, however. In the Next-to-Minimal Supersymmetric Standard Model (NMSSM) and other…

高能物理 - 唯象学 · 物理学 2008-11-26 John F. Gunion , Dan Hooper , Bob McElrath

Light neutralino dark matter can be achieved in the Minimal Supersymmetric Standard Model if staus are rather light, with mass around 100 GeV. We perform a detailed analysis of the relevant supersymmetric parameter space, including also the…

The cosmological baryon asymmetry is closely related to neutrino properties due to the non-perturbative sphaleron processes in the high-temperature symmetric phase of the standard model. We review some aspects of this connection with…

高能物理 - 唯象学 · 物理学 2007-05-23 W. Buchmüller

Within a supersymmetric (SUSY) type-I seesaw framework with flavor-blind universal boundary conditions, we study the consequences of requiring that the observed baryon asymmetry of the Universe be explained by either thermal or non-thermal…

高能物理 - 唯象学 · 物理学 2010-11-15 Steve Blanchet , Danny Marfatia , Azar Mustafayev

The lightest supersymmetric particle (LSP) is stable in an R-parity conserving theory. In this article the steps needed to calculate the present day mass density of such a particle are detailed. It is shown that there can be a…

高能物理 - 唯象学 · 物理学 2007-05-23 James D. Wells

In the supersymmetric framework, a higgsino asymmetry exists in the universe before the electroweak phase transition. We investigate whether the higgsino is a viable asymmetric dark matter candidate. We find that this is indeed possible.…

高能物理 - 唯象学 · 物理学 2013-05-30 Kfir Blum , Aielet Efrati , Yuval Grossman , Yosef Nir , Antonio Riotto

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 a simple extension of the Standard Model to consistently explain the observation of a peak in the galactic X-ray spectrum at 3.55 keV and the light neutrino masses along with the baryon asymmetry of the universe. The baryon…

高能物理 - 唯象学 · 物理学 2018-01-17 Sin Kyu Kang , Ayon Patra