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相关论文: Neutralino Dark Matter in mSUGRA: reopening the li…

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The constraints imposed on the Minimal Supersymmetric Standard Model (MSSM) parameter space by the Large Hadron Collider (LHC) Higgs mass limit and gluino mass lower bound are revisited. We also analyze the thermal relic abundance of…

高能物理 - 唯象学 · 物理学 2016-01-12 W. Abdallah , S. Khalil

Recent cosmological data allow to determine the universal Dark Matter (DM) density to a precision of about 10%, if a simple, well-motivated ansatz for the spectrum of primordial density perturbations is correct. Not surprisingly, a thermal…

高能物理 - 唯象学 · 物理学 2007-05-23 Manuel Drees

We study the neutralino relic density in the minimal supersymmetric standard model with natural light Higgs sector in which all Higgs masses, the supersymmetry (SUSY) breaking parameters, and the higgsino mass parameter mu are of order the…

高能物理 - 唯象学 · 物理学 2009-02-19 S. -G. Kim , N. Maekawa , K. I. Nagao , K. Sakurai , T. Yoshikawa

Within the minimal supergravity model (mSUGRA) framework, the expectation for the relic density of neutralinos exceeds the WMAP determination unless neutralinos a) have a significant higgsino component, b) have a mass close to half that of…

高能物理 - 唯象学 · 物理学 2009-11-10 Howard Baer , Azar Mustafayev , Stefano Profumo , Alexander Belyaev , Xerxes Tata

We re-investigate the question whether a light higgsino-like neutralino is a viable Dark Matter candidate. To this end we compute the dominant one-loop corrections to the masses of the higgsino-like states in the minimal Supersymmetric…

高能物理 - 唯象学 · 物理学 2014-11-17 M. Drees , M M. Nojiri , D. P. Roy , Y. Yamada

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

In the minimal supersymmetric standard models, neutralino dark matter with mass of $m_{\chi}\sim m_Z/2\sim 45$ GeV and $m_{\chi}\sim m_h/2\sim 62$ GeV can have the thermal relic abundance $\Omega_{\chi_1}h^2\simeq 0.120$ via the $Z$- and…

高能物理 - 唯象学 · 物理学 2016-03-23 Koichi Hamaguchi , Kazuya Ishikawa

We briefly review the supersymetric explanation for the cosmic dark matter. Although the neutralino in the minimal supersymmetric model (MSSM), the next-to-minimal supersymmetric model (NMSSM) and the nearly minimal supersymmetric model…

高能物理 - 唯象学 · 物理学 2010-06-03 Jin Min Yang

We investigate the prospects for neutralino dark matter within the Supersymmetric Standard Model (SSM) including the constraints from universal soft supersymmetry breaking and radiative breaking of the electroweak symmetry. The latter is…

高能物理 - 唯象学 · 物理学 2008-11-26 S. Kelley , J. Lopez , D. Nanopoulos , H. Pois , K. Yuan

We investigate both the $Z$ and $H$ poles solutions for the Higgsino mass parameter $\mu>0$ and $\mu<0$ for the neutralino dark matter in light of the LHC supersymmetry searches and the direct detection dark matter experiments, LUX-ZEPLIN…

高能物理 - 唯象学 · 物理学 2025-01-22 Imtiaz Khan , Waqas Ahmed , Tianjun Li , Shabbar Raza , Ali Muhammad

We study a specific SUGRA model with nonuniversal gaugino masses as an alternative to the minimal SUGRA model in the context of supersymmetric dark matter. The lightest supersymmetric particle in this model comes out to be a Higgsino…

高能物理 - 唯象学 · 物理学 2009-11-10 Utpal Chattopadhyay , D. P. Roy

I summarize some recent work on supersymmetric neutralinos as candidates for cold Dark Matter in the Universe. This includes a new scan of mSUGRA parameter space, with special emphasis on neutralinos annihilating predominantly through…

高能物理 - 唯象学 · 物理学 2009-11-11 Manuel Drees

The minimal supergravity (mSUGRA or CMSSM) model is an oft-used framework for exhibiting the properties of neutralino (WIMP) cold dark matter (CDM). However, the recent evidence from Atlas and CMS on a light Higgs scalar with mass m_h\simeq…

高能物理 - 唯象学 · 物理学 2015-06-04 Howard Baer , Vernon Barger , Azar Mustafayev

We calculate the relic density ($\Omega_{\chi^0_1} h^2$) of neutralino dark matter in supergravity models with radiative electroweak symmetry breaking, for values of the Higgs sector parameter $\tan\beta \equiv v_2/v_1$ between the two…

高能物理 - 唯象学 · 物理学 2016-09-06 V. Barger , Chung Kao

We study thermal neutralino dark matter in an effective field theory extension of the MSSM, called "Beyond the MSSM" (BMSSM) in Dine, Seiberg and Thomas (2007). In this class of effective field theories, the field content of the MSSM is…

高能物理 - 唯象学 · 物理学 2009-09-28 Marcus Berg , Joakim Edsjo , Paolo Gondolo , Erik Lundstrom , Stefan Sjors

We study the neutralino sector of the left-right supersymmetric model. In addition to the possibilities available in the minimal supersymmetric model, the neutralino states can be superpartners of the U(1)_{B-L} gauge boson, the neutral…

高能物理 - 唯象学 · 物理学 2009-11-11 Durmus A. Demir , Mariana Frank , Ismail Turan

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

A significant lower limit on the mass of the lightest neutralino \chi can be obtained by combining the results from sparticle searches at LEP at centre-of-mass energies up to 172 GeV with cosmological considerations, if it is assumed that…

高能物理 - 唯象学 · 物理学 2009-09-11 John Ellis , Toby Falk , Keith A. Olive , Michael Schmitt

We update and extend to larger masses our previous analysis of the MSSM with minimal $SO_{10}$ [MSO$_{10}$SM] soft SUSY breaking boundary conditions. We find a well--defined, narrow region of parameter space which provides the observed…

高能物理 - 唯象学 · 物理学 2011-08-23 R. Dermisek , S. Raby , L. Roszkowski , R. Ruiz de Austri

The measurements of WMAP on the relic density of dark matter strongly constrain supersymmetric models. In mSUGRA where the neutralino LSP is mostly a bino only rather fine-tuned models survive. On the other hand the relic density upper…

高能物理 - 唯象学 · 物理学 2007-05-23 G. Belanger , F. Boudjema , A. Cottrant , A. Pukhov , A. Semenov
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