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相关论文: Gaugino non-universality and dark matter

200 篇论文

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

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 analyze the indirect detection of neutralino dark matter in supergravity scenarios with non-universal soft scalar and gaugino masses. In particular, the gamma-ray flux arising from the galactic center due to neutralino annihilation is…

高能物理 - 唯象学 · 物理学 2011-05-23 Y. Mambrini , C. Munoz

The effects of nonuniversality of gaugino masses on dark matter are examined within supersymmetric grand unification, and in string and D brane models with R parity invariance. In SU(5) unified models nonuniversality in the gaugino sector…

高能物理 - 唯象学 · 物理学 2008-11-26 Achille Corsetti , Pran Nath

Motivated by the fact that neutrinos are massive, we study the effect of neutrino Yukawa couplings on neutralino dark matter observables within the framework of a supersymmetric seesaw. We find that neutrino couplings significantly affect…

高能物理 - 唯象学 · 物理学 2008-11-26 Vernon Barger , Danny Marfatia , Azar Mustafayev

The lightest neutralino of R-parity conserving supersymmetric models serves as a compelling candidate to account for the presence of cold dark matter in the universe. In the minimal supergravity (mSUGRA) model, a relic density can be found…

高能物理 - 唯象学 · 物理学 2009-11-10 Howard Baer , Jorge O' Farrill

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

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 present brief synopses of supersymmetric models where either the neutralino composition or its mass is adjusted so that thermal relic neutralinos from the Big Bang saturate the measured abundance of cold dark matter in the universe. We…

高能物理 - 唯象学 · 物理学 2009-01-06 Howard Baer , Azar Mustafayev , Eun-Kyung Park , Xerxes Tata

We investigate the enhancement of neutralino relic density in the context of a realistic cosmological scenario with Quintessence. The accurate relic density computation we perform allows us to be sensitive to both cases with shifts in the…

高能物理 - 唯象学 · 物理学 2009-11-10 Stefano Profumo , Piero Ullio

An analysis is given of the effects of non-universal soft SUSY breaking masses in the Higgs sector and in the third generation squark sector, and it is shown that they are highly coupled. Analytic expressions are obtained for their effects…

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

Almost degenerate bino and wino masses at the weak scale is one of unique features of gauge messenger models. The lightest neutralino is a mixture of bino, wino and higgsino and can produce the correct amount of the dark matter density if…

高能物理 - 唯象学 · 物理学 2008-11-26 Kyu Jung Bae , Radovan Dermisek , Hyung Do Kim , Ian-Woo Kim

We study dark matter physics in the Minimal Supersymmetric Standard Model with non-universal gaugino masses at the unification scale. In this scenario, the specific ratio of wino and gluino masses realizes the electro-weak scale naturally…

高能物理 - 唯象学 · 物理学 2017-09-13 Junichiro Kawamura , Yuji Omura

We study the neutralino dark matter phenomenology in the context of effective field theories derived from the weakly--coupled heterotic string. We consider in particular direct detection and indirect detection with neutrino telescopes…

高能物理 - 唯象学 · 物理学 2011-05-23 Pierre Binetruy , Yann Mambrini , Emmanuel Nezri

We compute the neutralino direct detection rate in non-standard cosmological scenarios where neutralinos account for the dark matter of the Universe. Significant differences are found when such rates are compared with those predicted by the…

高能物理 - 唯象学 · 物理学 2008-11-26 G. Gelmini , P. Gondolo , A. Soldatenko , C. E. Yaguna

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

The cosmological significance of the neutralino sector is studied for a class of models in which electroweak symmetry breaking is seeded by a gauge singlet. Extensive use is made of the renormalisation group equations to significantly…

高能物理 - 唯象学 · 物理学 2011-02-16 S. A. Abel , S. Sarkar , I. B. Whittingham

The range of neutralino-proton cross sections for R-parity preserving supergravity models with GUT scale unification of the gauge coupling constants is examined. The models considered here are mSUGRA, models with non universal soft breaking…

高能物理 - 唯象学 · 物理学 2007-05-23 R. Arnowitt , B. Dutta , Y. Santoso

We study supersymmetric dark matter in the general flavor diagonal MSSM by means of an extensive random scan of its parameter space. We find that, in contrast with the standard mSUGRA lore, the large majority of viable models features…

高能物理 - 唯象学 · 物理学 2008-11-26 Stefano Profumo , Carlos E. Yaguna

We carry out a comparison between different kinds of experiments for the detection of neutralino dark matter. In particular, we compare the theoretical predictions for the direct detection of these particles, through their elastic…

高能物理 - 唯象学 · 物理学 2011-07-19 Y. Mambrini , C. Munoz