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相关论文: Uncertainties in Relic Density Calculations in mSU…

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We consider the Minimal Supersymmetric Standard Model (MSSM) with varying amounts of non-universality in the soft supersymmetry-breaking contributions to the Higgs scalar masses. In addition to the constrained MSSM (CMSSM) in which these…

高能物理 - 唯象学 · 物理学 2014-11-20 Pearl Sandick

We analyze the rate of detection of minimal supersymmetric neutralino dark matter in germanium, sapphire and sodium iodide detectors, imposing cosmological and recent accelerator bounds including those from \bsg\ decay. We find, in contrast…

高能物理 - 唯象学 · 物理学 2008-11-26 L. Bergstrom , P. Gondolo

The thermal relic density of the wino-like neutralino dark matter in the brane world cosmology is studied. The expansion law at a high energy regime in the brane world cosmology is modified from the one in the standard cosmology, and the…

高能物理 - 唯象学 · 物理学 2009-11-11 Takeshi Nihei , Nobuchika Okada , Osamu Seto

We study the implications of minimal non-Universal Boundary Conditions in the sfermion Soft SUSY Breaking (SSB) masses of mSUGRA. We impose asymptotic b-tau Yukawa coupling Unification and we resort to a parameterization of the deviation…

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

In supersymmetric models with an unbroken R-symmetry (rather than only R-parity), the neutralinos are Dirac fermions rather than Majorana. In this article, we discuss the phenomenology of neutralino dark matter in such models, including the…

高能物理 - 唯象学 · 物理学 2013-11-05 Matthew R. Buckley , Dan Hooper , Jason Kumar

In the frame of an effective MSSM model without gaugino-mass unification at a grand unification (GUT) scale, we set a lower bound on the neutralino mass based on the new WMAP data on $\Omega_{CDM}$. Our lower bound, $m_{\chi} \gsim 6$ GeV,…

高能物理 - 唯象学 · 物理学 2008-11-26 A. Bottino , F. Donato , N. Fornengo , S. Scopel

We review some properties of the neutralino as a candidate for dark matter in the Universe. After presentation of evaluations for the neutralino relic abundance, possibilities for its direct and indirect detections are discussed, with…

高能物理 - 唯象学 · 物理学 2007-05-23 A. Bottino , N. Fornengo , G. Mignola , S. Scopel

We investigate the utility of cosmological and astrophysical observations for distinguishing between supersymmetric theories. In particular we consider 276 pairs of models that give rise to nearly identical patterns of observables at hadron…

高能物理 - 唯象学 · 物理学 2008-11-26 Baris Altunkaynak , Michael Holmes , Brent D. Nelson

Considering heavy stable neutrinos of 4th generation we calculate the relic density of such neutrinos in the Universe. Taking into account the condensation of heavy neutrinos in the Galaxy and applying the results of calculations to…

天体物理学 · 物理学 2026-02-24 D. Fargion , M. Yu. Khlopov , R. V. Konoplich , R. Mignani

{\tenrm The possibility of detecting supersymmetric dark matter is examined within the framework of the minimal supergravity model (MSGM), where the $\tilde{Z}_{1}$ is the LSP for almost the entire parameter space. A brief discussion is…

高能物理 - 唯象学 · 物理学 2009-09-25 R. Arnowitt , Pran Nath

The expected event rates for ${\tilde Z_{1}}$ dark matter for a variety of dark matter detectors are studied over the full parameter space with tan $\beta\leq$ 20 for supergravity grand unified models. Radiative breaking constraints are…

高能物理 - 唯象学 · 物理学 2009-09-25 R. Arnowitt , Pran Nath

Dark matter is examined within the ``golden region'' of the Minimal Supersymmetric Standard Model. This region satisfies experimental constraints, including a lower bound on the Higgs mass of 114 GeV, and minimizes fine-tuning of the Z…

高能物理 - 唯象学 · 物理学 2009-03-12 Junya Kasahara , Katherine Freese , Paolo Gondolo

When the GUT relation on gaugino masses is relaxed, the mass and composition of the lightest neutralino are different from those in the GUT case. We discuss its phenomenological implications on the relic abundance of the neutralinos and on…

高能物理 - 唯象学 · 物理学 2009-10-22 Satoshi Mizuta , Daniel Ng , Masahiro Yamaguchi

We analyze how the measurements of the low-energy spectrum of cosmic antiprotons can provide information on relic neutralinos. The analysis is focused on the light neutralinos which emerge in supersymmetric schemes where gaugino-mass…

高能物理 - 唯象学 · 物理学 2009-11-11 A. Bottino , F. Donato , N. Fornengo , P. Salati

The $b\tau j \etslash$ signal at the ongoing LHC experiments is simulated with Pythia in the mSUGRA and other models of SUSY breaking. Special attention is given on the compatibility of this signature with the low mass neutralino dark…

高能物理 - 唯象学 · 物理学 2011-11-10 Nabanita Bhattacharyya , Arghya Choudhury , Amitava Datta

In the event that R-Parity conserving supersymmetry (SUSY) is discovered at the LHC, a key issue which will need to be addressed will be the consistency of that signal with astrophysical and non-accelerator constraints on SUSY Dark Matter.…

高能物理 - 唯象学 · 物理学 2010-02-03 G. Polesello , D. R. Tovey

Some variants of the MSSM feature a strip in parameter space where the lightest neutralino is identified as the lightest supersymmetric particle (LSP), the gluino is the next-to-lightest supersymmetric particle (NLSP) and is nearly…

高能物理 - 唯象学 · 物理学 2015-10-28 John Ellis , Feng Luo , Keith A. Olive

Event rates for dark matter detectors in neutralino--nucleus scattering are studied for supergravity unified models, including the constraint arising from the $b\rightarrow s\gamma$ experiment. The recent experimental measurement of this…

高能物理 - 唯象学 · 物理学 2009-09-25 Pran Nath , R. Arnowitt

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

After a short introduction on some general implications of recent cosmological observations, we discuss the properties of relic neutralinos in connection with present experimental strategies for detecting WIMPs.

高能物理 - 唯象学 · 物理学 2009-11-07 A. Bottino , F. Donato , N. Fornengo , S. Scopel
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