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There is mounting evidence for dark matter in the Universe and one of the favourite dark matter candidates is the neutralino, which naturally appears as the lightest supersymmetric particle (LSP) in many supersymmetric extensions of the…

天体物理学 · 物理学 2017-08-23 Joakim Edsjo

Here we examine the detectability of collisionless dark matter candidates that may constitute not all but only a subdominant component of galactic cold dark matter. We show that current axion searches are not suited for a subdominant…

高能物理 - 唯象学 · 物理学 2009-11-07 Gintaras Duda , Graciela Gelmini , Paolo Gondolo

We study the viability of the lightest neutralino as a dark matter candidate in the Next-to-Minimal Supersymmetric Standard Model. Taking into account accelerator constraints as well as bounds on low-energy observables, and imposing…

高能物理 - 唯象学 · 物理学 2008-11-26 Ana M. Teixeira

There is almost universal agreement among astronomers that most of the mass in the Universe and most of the mass in the Galactic halo is dark. Many lines of reasoning suggest that the dark matter consists of some new, as yet undiscovered,…

高能物理 - 唯象学 · 物理学 2009-10-28 G. Jungman , M. Kamionkowski , K. Griest

We investigate dark matter in a constrained $E_6$ inspired supersymmetric model with an exact custodial symmetry and compare with the CMSSM. The breakdown of $E_6$ leads to an additional $U(1)_N$ symmetry and a discrete matter parity. The…

高能物理 - 唯象学 · 物理学 2016-12-28 P. Athron , D. Harries , R. Nevzorov , A. G. Williams

We investigate the level of fine-tuning of neutralino Dark Matter below 200 GeV in the low-energy phenomenological minimal supersymmetric Standard Model taking into account the newest results from XENON100 and the Large Hadron Collider as…

高能物理 - 唯象学 · 物理学 2015-06-05 Philipp Grothaus , Manfred Lindner , Yasutaka Takanishi

In this article, we explore the ability of direct and indirect dark matter experiments to not only detect neutralino dark matter, but to constrain and measure the parameters of supersymmetry. In particular, we explore the relationship…

高能物理 - 唯象学 · 物理学 2014-11-18 Dan Hooper , Andrew M. Taylor

We investigate the possibility to detect neutralino dark matter in a scenario in which the galactic dark halo is clumpy. We find that under customary assumptions on various astrophysical parameters, the antiproton and continuum gamma-ray…

天体物理学 · 物理学 2009-10-30 L. Bergstrom , J. Edsjo , P. Gondolo , P. Ullio

Dark matter candidates arising in models of particle physics incorporating weak scale supersymmetry may produce detectable signals through their annihilation into neutrinos, photons, or positrons. A large number of relevant experiments are…

天体物理学 · 物理学 2009-10-09 Jonathan L. Feng , Konstantin T. Matchev , Frank Wilczek

We show how the material used in direct detection experiments of Dark Matter (DM), in the presence of a signal of it, can afford one with the possibility of extracting the nature of the underlying candidate. We do so for the case of a…

高能物理 - 唯象学 · 物理学 2021-05-19 Yaşar Hiçyılmaz , Stefano Moretti

In the post-LEP2 era, and in light of recent measurements of the cosmic abundance of cold dark matter (CDM) in the universe from WMAP, many supersymmetric models tend to predict 1. an overabundance of CDM and 2. pessimistically low rates…

高能物理 - 唯象学 · 物理学 2010-10-27 Howard Baer , Azar Mustafayev , Eun-Kyung Park , Xerxes Tata

We examine the present and future XENON limits on the neutralino dark matter in split supersymmetry (split-SUSY). Through a scan over the parameter space under the current constraints from collider experiments and the WMAP measurement of…

高能物理 - 唯象学 · 物理学 2011-11-16 Junjie Cao , Wenyu Wang , Jin Min Yang

The identity of dark matter is one of the greatest puzzles of our Universe. Its solution may be associated with supersymmetry which is a fundamental space-time symmetry that has not been verified experimentally so far. In many…

高能物理 - 唯象学 · 物理学 2007-08-28 Frank Daniel Steffen

Exotic dark matter together with the vacuum energy (associated with the cosmological constant) seem to dominate in the Universe. Thus its direct detection is central to particle physics and cosmology. Supersymmetry provides a natural dark…

天体物理学 · 物理学 2009-11-07 J. D. Vergados

In the Supersymmetric extension of the Standard Model with minimal particle content the three neutrinos can have non trivial masses and mixings, generated at 1 loop due to renormalizable lepton number violating interactions. We show that…

高能物理 - 唯象学 · 物理学 2009-09-25 D. Tommasini

We study natural supersymmetric scenarios with light right-handed neutrino superfields, and consider the possibility of having either a neutrino or a sneutrino as a dark matter candidate. For the former, we evaluate the possibility of…

高能物理 - 唯象学 · 物理学 2020-04-01 T. Faber , J. Jones-Pérez , Y. Liu , W. Porod

Since the expected rates for neutralino-nucleus scattering are expected to be small, one should exploit all the characteristic signatures of this reaction. Such are: (i) In the standard recoil measurements the modulation of the event rate…

高能物理 - 唯象学 · 物理学 2007-05-23 J. D. Vergados

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

One of the most well-founded candidates for dark matter remains a split-SUSY model with a Higgsino-like or Wino-like lightest superpartner and the grander SUSY model providing answers for the hierarchy problem and GUT scale unification.The…

高能物理 - 唯象学 · 物理学 2023-11-28 Carsten Rott , Pearl Sandick , Ben Sheff

Particle physics models with Natural Supersymmetry are characterized by a superpotential parameter \mu \sim m_h \sim125$ GeV, while third generation squarks have mass <0.5-1.5 TeV. Gluinos should be lighter than several TeV so as not to…

高能物理 - 唯象学 · 物理学 2015-06-04 Howard Baer , Vernon Barger , Peisi Huang , Xerxes Tata