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相关论文: Neutralino Relic Density in a Supersymmetric U(1)'…

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We evaluate the relic density of the lightest neutralino, the lightest supersymmetric particle, in the Minimal Supersymmetric extension of the Standard Model (MSSM). For the first time, we include all coannihilation processes between…

高能物理 - 唯象学 · 物理学 2008-11-26 J. Edsjo , P. Gondolo

The $U(1)_X$ extension of the minimal supersymmetric standard model(MSSM) is called as $U(1)_X$SSM with the local gauge group $SU(3)_C\times SU(2)_L \times U(1)_Y \times U(1)_X$. $U(1)_X$SSM has three singlet Higgs superfields beyond MSSM.…

高能物理 - 唯象学 · 物理学 2021-07-14 Shu-Min Zhao , Guo-Zhu Ning , Jing-Jing Feng , Hai-Bin Zhang , Tai-Fu Feng

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

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

We analyze the prospects for light neutralino dark matter in the minimal supersymmetric model extended by a $U(1)$ gauge group. We allow the neutralino to be an arbitrary admixture of singlet and doublet higgsinos, as well as of the three…

高能物理 - 唯象学 · 物理学 2014-10-22 Mariana Frank , Subhadeep Mondal

We compute the dark matter relic densities of neutralinos and axions in a supersymmetric model with a gauged anomalous U(1) symmetry, kinetically mixed with $U(1)_Y$ of hypercharge. The model is a variant of the USSM (the U(1) extended…

高能物理 - 唯象学 · 物理学 2015-05-20 Claudio Coriano , Marco Guzzi , Antonio Mariano

We compute the cosmic relic (dark matter) density of the lightest supersymmetric particle (LSP) in the framework of minimal $N=1$ Supergravity models with radiative breaking of the electroweak gauge symmetry. To this end, we re--calculate…

高能物理 - 唯象学 · 物理学 2008-11-26 M. Drees , M. M. Nojiri

We investigate SU(5) and SO(10) GUTs with vanishing scalar masses and trilinear scalar couplings at a scale higher than the unification scale. The parameter space of the models, further constrained by b-\tau Yukawa coupling unification,…

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

We enlarge our set of supersymmetric models and update accelerator constraints in our precise calculation of the relic density of the lightest neutralino, which includes relativistic Boltzmann averaging, subthreshold and resonant…

高能物理 - 唯象学 · 物理学 2007-05-23 Paolo Gondolo , Joakim Edsjo

Neutralino as the lightest supersymmetric particle (LSP) is a candidate for supersymmetric dark matter. It is known that coannihilation effects could be important in neutralino relic density calculation. Here we present some results on…

高能物理 - 唯象学 · 物理学 2009-11-07 Yudi Santoso

We analyse the relic neutralino density in supersymmetric models with an intermediate unification scale. In particular, we present concrete cosmological scenarios where the reheating temperature is as small as $\cal{O}$ $1 - 1000$ MeV).…

高能物理 - 唯象学 · 物理学 2008-11-26 S. Khalil , C. Munoz , E. Torrente-Lujan

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

We discuss the relic density of the lightest of the supersymmetric particles in view of new cosmological data, which favour the concept of an accelerating Universe with a non-vanishing cosmological constant. Recent astrophysical…

高能物理 - 唯象学 · 物理学 2008-11-26 A. B. Lahanas , D. V. Nanopoulos , V. C. Spanos

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

We consider the effects of neutralino-stau coannihilations on the cosmological relic density of the lightest supersymmetric particle (LSP) $\chi$ in the minimal supersymmetric extension of the Standard Model (MSSM), particularly in the…

高能物理 - 唯象学 · 物理学 2008-11-26 John Ellis , Toby Falk , Keith A. Olive

The neutralino relic abundance is evaluated for a wide range of the neutralino mass, ${\rm 20\ GeV} \leq m_\chi \leq {\rm 1\ TeV}$, by taking into account the full set of final states in the neutralino-neutralino annihilation. The analysis…

高能物理 - 唯象学 · 物理学 2011-05-23 A. Bottino , V. de Alfaro , N. Fornengo , G. Mignola , M. Pignone

We examine the main properties of relic neutralinos in the context of the Minimal Supersymmetric extension of the Standard Model. We present a whole set of results obtained for the relic abundance and for detection rates with a model…

天体物理学 · 物理学 2007-05-23 A. Bottino

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

高能物理 - 唯象学 · 物理学 2009-11-07 Howard Baer , Csaba Balazs , Alexander Belyaev

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 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
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