English
Related papers

Related papers: Formation of small-scale structure in SUSY CDM

200 papers

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…

High Energy Physics - Phenomenology · Physics 2007-05-23 Antonio Masiero , Stefano Profumo , Piero Ullio

If the spontaneous breaking of Peccei-Quinn symmetry comes from soft supersymmetry breaking, the fermionic partners of the symmetry-breaking fields have mass of order the gravitino mass, and are called flatinos. The lightest flatino, called…

High Energy Physics - Phenomenology · Physics 2008-11-26 Eung Jin Chun , Hang Bae Kim , Kazunori Kohri , David H. Lyth

The viability of the lightest neutralino as a dark matter candidate in the Next-to-Minimal Supersymmetric Standard Model is analysed. We carry out a thorough analysis of the parameter space, taking into account accelerator constraints as…

High Energy Physics - Phenomenology · Physics 2010-10-27 D. G. Cerdeno , E. Gabrielli , D. E. Lopez-Fogliani , C. Munoz , A. M. Teixeira

One of the best motivated hypotheses in cosmology states that most of the matter in the universe is in the form of weakly-interacting massive particles that decoupled early in the history of the universe and cooled adiabatically to an…

Astrophysics · Physics 2009-11-10 Abraham Loeb , Matias Zaldarriaga

A detailed analysis of dark matter event rates in minimal supergravity models (MSGM) is given. It is shown analytically that the lightest neutralino the ${{\tilde {Z}_{1}}}$ is the LSP over almost all of the parameter space, and hence the…

High Energy Physics - Phenomenology · Physics 2008-11-26 R. Arnowitt , Pran Nath

I argue that the cold dark matter (CDM) model requires that even within a few kpc of the center of a galactic halo a significant fraction (greater than a few percent) of the surface density is contained in substructures with masses > 10^3…

Astrophysics · Physics 2007-05-23 R. Benton Metcalf

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…

High Energy Physics - Phenomenology · Physics 2008-11-26 J. Edsjo , P. Gondolo

We consider the neutralino as a dominant Dark Matter particle in the galactic halo and investigate some general issues of direct Dark Matter searches via elastic neutralino-nucleus scattering. On the basis of conventional assumptions about…

High Energy Physics - Phenomenology · Physics 2007-05-23 V. A. Bednyakov , H. V. Klapdor-Kleingrothaus , S. G. Kovalenko

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…

High Energy Physics - Phenomenology · Physics 2014-11-20 Pearl Sandick

We report the most recent results from high-resolution numerical simulations of structure formation in two flat cold+hot dark matter models with neutrino mass densities $\onu=0.2$ and 0.3. We find that structure forms too late in all…

Astrophysics · Physics 2009-10-22 Chung-Pei Ma

Some doubts have been expressed about low energy supersymmetry (SUSY) following the first run of the LHC. In this talk I will try to present a more upbeat view based on data, rather than theoretical expectations. In particular, I will make…

High Energy Physics - Phenomenology · Physics 2015-07-28 K. Kowalska , L. Roszkowski , E. M. Sessolo , S. Trojanowski , A. J. Williams

The extra particles provided by Supersymmetry (SUSY) appear as natural candidates for exotica such as the missing Dark Matter of the Universe. The particle candidates for Dark Matter, and the basic elements of the minimal supersymmetric…

High Energy Physics - Phenomenology · Physics 2007-05-23 Pavel Fileviez Perez

Massive neutrinos make up a fraction of the dark matter, but due to their large thermal velocities, cluster significantly less than cold dark matter (CDM) on small scales. An accurate theoretical modelling of their effect during the…

Cosmology and Nongalactic Astrophysics · Physics 2015-08-21 Yacine Ali-Haïmoud , Simeon Bird

Dark matter neutralinos in the constrained minimal supersymmetric model (CMSSM) may account for the recent cosmic ray electron and positron observations reported by the PAMELA and ATIC experiments either through self annihilation or via…

High Energy Physics - Phenomenology · Physics 2010-04-14 Ilia Gogoladze , Rizwan Khalid , Qaisar Shafi , Hasan Yuksel

Supersymmetric models based on anomaly-mediated SUSY breaking (AMSB) generally give rise to a neutral wino as a WIMP cold dark matter (CDM) candidate, whose thermal abundance is well below measured values. Here, we investigate four…

High Energy Physics - Phenomenology · Physics 2014-11-20 Howard Baer , Radovan Dermisek , Shibi Rajagopalan , Heaya Summy

The lightest neutralino in the minimal supersymmetric extension of the Standard Model can be, in principle, massless. If super-light neutralinos are the dark matter, structure formation constrains their mass to be above a few keV. We show…

High Energy Physics - Phenomenology · Physics 2008-11-26 Stefano Profumo

In the minimal supersymmetric standard model (MSSM) the lightest superparticle (LSP) can be a TeV neutralino (mainly dominated by higgsino or wino) which serves as a dark matter candidate with correct thermal relic density. In this work we…

High Energy Physics - Phenomenology · Physics 2019-03-27 Murat Abdughani , Jie Ren , Jun Zhao

Within the framework of the Minimal Supersymmetric Standard Model (MSSM), we explore a decoupling of the parameters into separate sectors that determine consistency with collider data, the abundance of dark matter, and potential signatures…

High Energy Physics - Phenomenology · Physics 2016-07-27 Pearl Sandick

If the axino is the lightest superpartner and satisfies cosmological bounds, including a preferred range of the relic abundance of cold dark matter, then the usual stringent constraints on the parameter space of the CMSSM become greatly…

High Energy Physics - Phenomenology · Physics 2009-11-10 Laura Covi , Leszek Roszkowski , Roberto Ruiz de Austri , Michael Small

It is pointed out that there is a strong correlation between the neutralino dark matter scattering cross section $\sigma_{\tilde{\chi} p}$ and the branching ratio for $B_s \to \mu^+ \mu^-$ within minimal supergravity (mSUGRA) and its…

High Energy Physics - Phenomenology · Physics 2008-11-26 Seungwon Baek , Yeong Gyun Kim , P. Ko