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We review the current status of the Brookhaven muon g - 2 experiment, and it's effects on the SUSY parameter space when combined with dark matter relic density bounds, b->s\gamma and Higgs mass constraints. If the 3\sigma deviation of g - 2…

高能物理 - 唯象学 · 物理学 2017-08-23 R. Arnowitt , B. Dutta

We update a previously-proposed set of supersymmetric benchmark scenarios, taking into account the precise constraints on the cold dark matter density obtained by combining WMAP and other cosmological data, as well as the LEP and b -> s…

高能物理 - 唯象学 · 物理学 2009-09-11 M. Battaglia , A. De Roeck , J. Ellis , F. Gianotti , K. A. Olive , L. Pape

We study direct detection of dark matter in supersymmetric (SUSY) model where most of SUSY particles have very high-scale masses beyond the weak scale. In the scenario, Wino-like or Higgsino-like neutralino is a good candidate for the dark…

高能物理 - 唯象学 · 物理学 2013-03-04 Junji Hisano , Koji Ishiwata , Natsumi Nagata

We investigate the thermal relic density of the cold dark matter in the context of the brane world cosmology. Since the expansion law in a high energy regime is modified from the one in the standard cosmology, if the dark matter decouples…

高能物理 - 唯象学 · 物理学 2016-09-06 Nobuchika Okada , Osamu Seto

We show some phenomenological implications for the dark matter problem of a class of models with deflected anomaly mediated supersymmetry breaking in the context of the MSSM. This scenario can be naturally embedded in a brane world model…

高能物理 - 唯象学 · 物理学 2017-08-23 Andrea M. Lionetto

We investigate the relic abundance of asymmetric Dark Matter particles that were in thermal equilibrium in the early universe. The standard analytic calculation of the symmetric Dark Matter is generalized to the asymmetric case. We…

高能物理 - 唯象学 · 物理学 2015-05-28 Hoernisa Iminniyaz , Manuel Drees , Xuelei Chen

Considering dark matter capture in astrophysical objects such as neutron stars and brown dwarfs, followed by their annihilation into two neutrino and four neutrino final states, we derive new constraints on the mass and coupling of a novel…

高能物理 - 唯象学 · 物理学 2025-09-16 Basabendu Barman , Pooja Bhattacharjee , Arindam Das

Recent measurements of cosmological parameters from the microwave background radiation, type Ia supernovae, and the age of globular clusters help determine the relic matter density in the universe. It is first shown with mild cosmological…

高能物理 - 唯象学 · 物理学 2009-10-31 James D. Wells

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

We discuss the SUSY dark matter phenomenology in some simple and predictive models of nonuniversal gaugino masses at the GUT scale. Assuming the gaugino masses to transform as a sum of singlet and a nonsinglet representation of the GUT…

高能物理 - 唯象学 · 物理学 2012-11-16 D. P. Roy

The cosmological relic density of a Bino-like Lightest Supersymmetric Particle is calculated in the framework of the Minimal Supersymmetric Standard Model. We include annihilation and coannihilation effects of the Bino with the lightest…

高能物理 - 唯象学 · 物理学 2007-05-23 Constantinos Pallis

We study natural supersymmetric scenarios with light right-handed neutrino superfields, and consider the possibility of having either a neutrino or a sneutrino as a dark matter candidate. For the former, we evaluate the possibility of…

高能物理 - 唯象学 · 物理学 2020-04-01 T. Faber , J. Jones-Pérez , Y. Liu , W. Porod

We demonstrate that the recent measurement of the anomalous magnetic moment of the muon and dark matter can be simultaneously explained within the Minimal Supersymmetric Standard Model. Dark matter is a mostly-bino state, with the relic…

高能物理 - 唯象学 · 物理学 2021-10-29 Peter Cox , Chengcheng Han , Tsutomu T. Yanagida

In this paper we study sneutrino dark matter in a recently proposed supersymmetric electroweak-scale inverse seesaw model, in which the majority of the sneutrino dark matter particle is a mixture of the right-handed sneutrino $\tilde{N}^c$…

高能物理 - 唯象学 · 物理学 2018-09-18 Jung Chang , Kingman Cheung , Hiroyuki Ishida , Chih-Ting Lu , Martin Spinrath , Yue-Lin Sming Tsai

Semi-annihilation is a generic feature of particle dark matter that is most easily probed by cosmic ray experiments. We explore models where the semi-annihilation cross section is enhanced at late times and low temperatures by the presence…

高能物理 - 唯象学 · 物理学 2018-11-14 Yi Cai , Andrew Spray

In the Minimal Supersymmetric Standard Model light neutralinos can satisfy the dark matter (DM) abundance constraint by resonant annihilation via a $Z$ or a light Higgs ($h$) boson. In this work we study the current and future status of…

高能物理 - 唯象学 · 物理学 2019-01-09 Giancarlo Pozzo , Yang Zhang

Higher-dimensional braneworld models which contain both bulk and brane curvature terms in the action admit cosmological singularities of rather unusual form and nature. These `quiescent' singularities, which can occur both during the…

广义相对论与量子宇宙学 · 物理学 2009-11-07 Yuri Shtanov , Varun Sahni

Non-universal boundary conditions in grand unified theories can lead to non-universal gaugino masses at the unification scale. In R-parity preserving theories the lightest supersymmetric particle is a natural candidate for the dark matter.…

高能物理 - 唯象学 · 物理学 2009-09-29 Katri Huitu , Jari Laamanen , Sourov Roy

We consider possibly observable effects of asymmetric dark matter (ADM) in neutron stars. Since dark matter does not self-annihilate in the ADM scenario, dark matter accumulates in neutron stars, eventually reaching the Chandrasekhar limit…

高能物理 - 唯象学 · 物理学 2012-01-27 Samuel D. McDermott , Hai-Bo Yu , Kathryn M. Zurek

We investigate the production and freeze-out of dark matter with a constant thermally averaged cross-section in a generic bouncing universe framework. Our result shows that, there is a novel avenue that dark matter is produced thermally and…

宇宙学与河外天体物理 · 物理学 2015-09-16 Changhong Li