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相关论文: Neutralino Dark Matter beyond CMSSM Universality

200 篇论文

Supersymmetric radiative neutrino mass models have often two dark matter candidates. One is the usual lightest neutralino with odd R parity and the other is a new neutral particle whose stability is guaranteed by a discrete symmetry that…

高能物理 - 唯象学 · 物理学 2011-07-07 Hiroki Fukuoka , Daijiro Suematsu , Takashi Toma

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

We investigate the viability of light neutralino scenarios as promoted by dark matter direct detection experiments. Using high statistics scans in the pMSSM we have identified several scenarios which give rise to very light neutralinos with…

高能物理 - 唯象学 · 物理学 2012-10-08 A. Arbey , M. Battaglia , F. Mahmoudi

Dark matter detection rates for supergravity models with R parity where supersymmetry is broken at a scale >~M_G are discussed. Non-universal soft breaking masses in both the Higgs and squark sectors are considered, and it is seen that…

高能物理 - 唯象学 · 物理学 2008-11-26 R. Arnowitt , Pran Nath

We evaluate the relic density of neutralinos in the minimal supergravity (mSUGRA) model. All 2->2 neutralino annihilation diagrams, as well as all initial states involving sleptons, charginos, neutralinos and third generation squarks are…

高能物理 - 唯象学 · 物理学 2007-05-23 Howard Baer , Csaba Balazs , Alexander Belyaev

Several new effects have been investigated in recent analyses of supersymmetric dark matter. These include the effects of the uncertainties of wimp velocity distributions, of the uncertainties of quark densities, of large CP violating…

高能物理 - 唯象学 · 物理学 2007-05-23 Achille Corsetti , Pran Nath

We review here the status of different dark matter candidates in the context of supersymmetric models, in particular the neutralino as a realization of the WIMP-mechanism and the gravitino. We give a summary of the recent bounds in direct…

高能物理 - 唯象学 · 物理学 2015-06-17 Riccardo Catena , Laura Covi

Principle of neutralino dark matter detection with neutrino telescopes and predictions are reviewed. The future Antares detector is described. Prospection in the CMSSM is exposed including comparison with experiment sensitivities of both…

高能物理 - 唯象学 · 物理学 2007-05-23 E. Nezri

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 examine the detectability through indirect means of weakly interacting dark matter candidates that may constitute not all but only a subdominant component of galactic cold dark matter. We show that the possibility of indirect detection…

高能物理 - 唯象学 · 物理学 2009-11-07 Gintaras Duda , Graciela Gelmini , Paolo Gondolo , Joakim Edsjo , Joseph Silk

Supersymmetric grand unified theories based on the gauge group SO(10) are highly motivated. In the simplest models, one expects t-b-\tau Yukawa coupling unification, in addition to gauge, matter and Higgs unification. Yukawa unification…

高能物理 - 唯象学 · 物理学 2015-05-18 Howard Baer

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

One of the most well-founded candidates for dark matter remains a split-SUSY model with a Higgsino-like or Wino-like lightest superpartner and the grander SUSY model providing answers for the hierarchy problem and GUT scale unification.The…

高能物理 - 唯象学 · 物理学 2023-11-28 Carsten Rott , Pearl Sandick , Ben Sheff

With the latest Planck results the dark matter relic density is determined to an unprecedented precision. In order to reduce current theoretical uncertainties in the dark matter relic density prediction, we have calculated next-to-leading…

高能物理 - 唯象学 · 物理学 2015-10-22 Julia Harz , Björn Herrmann , Michael Klasen , Karol Kovarik , Patrick Steppeler

The possible solution of dark matter problem with neutralinos of supersymmetric models within the supergravity framework is reviewed. A novel correlation between the neutralino relic abundance $\Omega_\chi$ and the soft supersymmetry…

高能物理 - 唯象学 · 物理学 2007-05-23 Kajia Yuan

SUSY/SUGRA models with naturalness defined via small $\mu$ are constrained due to experiment on the relic density and the experimental limits on the WIMP-proton cross-section and WIMP annihilation cross-section from indirect detection…

高能物理 - 唯象学 · 物理学 2020-05-20 Amin Aboubrahim , Wan-Zhe Feng , Pran Nath

The direct detection of neutralino dark matter is analysed in general supergravity scenarios, where non-universal soft scalar and gaugino masses can be present. In particular, the theoretical predictions for the neutralino-nucleon cross…

高能物理 - 唯象学 · 物理学 2009-11-11 S. Baek , D. G. Cerdeno , Y. G. Kim , P. Ko , C. Munoz

We calculate expected event rates for direct detection of relic neutralinos as a function of parameter space of the minimal supergravity model. Numerical results are presented for the specific case of a $^{73}$Ge detector. We find…

高能物理 - 唯象学 · 物理学 2008-11-26 Howard Baer , Michal Brhlik

We discuss the possibilities for the direct detection of neutralino dark matter via elastic scattering in variants of the minimal supersymmetric extension of the Standard Model (MSSM) with non-universal supersymmetry-breaking contributions…

高能物理 - 唯象学 · 物理学 2010-04-28 John Ellis , Keith A. Olive , Pearl Sandick

We analyse the direct detection of neutralino dark matter in supergravity scenarios with non-universal soft scalar and gaugino masses. In particular, the neutralino-nucleon cross section is computed and compared with the sensitivity of…

高能物理 - 唯象学 · 物理学 2008-11-26 D. G. Cerdeno , C. Munoz