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相关论文: Towards the Final Word on Neutralino Dark Matter

200 篇论文

In spite of rapid experimental progress, windows for light superparticles remain. One possibility is a ~100 GeV tau slepton whose t-channel exchange can give the correct thermal relic abundance for a relatively light neutralino. We…

高能物理 - 唯象学 · 物理学 2013-10-18 Aaron Pierce , Nausheen R. Shah , Katherine Freese

We present an overview of supersymmetry searches, both at collider experiments and via searches for dark matter (DM). We focus on three DM possibilities in the SUSY context: the thermally produced neutralino, a mixture of axion and axino,…

高能物理 - 唯象学 · 物理学 2014-11-18 Howard Baer , Eun-Kyung Park , Xerxes Tata

The neutralino, the lightest stable supersymmetric particle, is a strong theoretical candidate for the missing astronomical "dark matter". Depending on their annihilation cross section, relic neutralinos from early formation of the Universe…

天体物理学 · 物理学 2007-05-23 Lazar Fleysher

We examine the prospects for supersymmetry discovery in the minimal supergravity (mSUGRA) model via indirect detection of neutralino dark matter. We investigate rates for muon detection in neutrino telescopes, and detection of photons,…

高能物理 - 唯象学 · 物理学 2011-07-19 Howard Baer , Alexander Belyaev , Tadas Krupovnickas , Jorge O'Farrill

The lightest neutralino of R-parity conserving supersymmetric models serves as a compelling candidate to account for the presence of cold dark matter in the universe. In the minimal supergravity (mSUGRA) model, a relic density can be found…

高能物理 - 唯象学 · 物理学 2009-11-10 Howard Baer , Jorge O' Farrill

In supersymmetric models whose gauge group includes an additional U(1) factor at the TeV scale, broken by the VEV of an standard model singlet S, the parameter space can accommodate a very light neutralino not ruled out experimentally. This…

高能物理 - 唯象学 · 物理学 2009-10-30 B. de Carlos , J. R. Espinosa

We compute the neutralino direct detection rate in non-standard cosmological scenarios where neutralinos account for the dark matter of the Universe. Significant differences are found when such rates are compared with those predicted by the…

高能物理 - 唯象学 · 物理学 2008-11-26 G. Gelmini , P. Gondolo , A. Soldatenko , C. E. Yaguna

We revisit indirect detection possibilities for neutralino dark matter, emphasizing the complementary roles of different approaches. While thermally produced dark matter often requires large astrophysical "boost factors" to observe…

高能物理 - 唯象学 · 物理学 2008-10-16 Phill Grajek , Gordon Kane , Daniel J. Phalen , Aaron Pierce , Scott Watson

In a scenario with heavy supersymmetric sfermions and decoupled supersymmetric Higgs sector, a well tempered neutralino is the remaining candidate for thermal single-component sub-TeV dark matter. Well tempered neutralinos are studied in…

高能物理 - 唯象学 · 物理学 2014-03-26 Archana Anandakrishnan , Kuver Sinha

We studied the interplay between the mass reach for electroweakinos at future hadron colliders and direct detection experiments. The lack of new phenomena at the LCH motivates us to focus on split supersymmetry scenarios with different…

高能物理 - 唯象学 · 物理学 2015-10-27 Giovanni Grilli di Cortona

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

In this paper, we will describe the results of SUSY parameter space searches including minimal supergravity, non-universal supergravity and minimal supersymmetry and the implications on the indirect detection of neutralino dark matter. We…

高能物理 - 唯象学 · 物理学 2009-11-07 Dan Hooper

Indirect detection constraints on gamma rays (both continuum and lines) have set strong constraints on wino dark matter. By combining results from Fermi-LAT and HESS, we show that: light nonthermal wino dark matter is strongly excluded;…

高能物理 - 唯象学 · 物理学 2015-06-16 JiJi Fan , Matthew Reece

We examine a scenario in which the reheating temperature $T_R$ after inflation is so low that it is comparable to, or lower than, the freeze out temperature of ordinary WIMPs. In this case the dark matter relic abundance is reduced, thus…

高能物理 - 唯象学 · 物理学 2015-06-19 Leszek Roszkowski , Sebastian Trojanowski , Krzysztof Turzynski

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

Relic neutralinos produced after the Big Bang are favoured candidates for Dark Matter. They can accumulate at the centre of massive celestial objects like our Sun. Their annihilation can result in a high-energy neutrino flux that could be…

天体物理学 · 物理学 2019-08-13 Gordon Lim

Minimal Dark Matter models feature one neutral particle that serves as a thermal relic dark matter candidate, as well as quasi-degenerate charged states with TeV masses. When the charged states are produced at colliders, they can decay into…

高能物理 - 唯象学 · 物理学 2024-05-16 Rodolfo Capdevilla , Federico Meloni , Jose Zurita

We examine the properties of relic neutralinos in the regions of the parameter space selected by recent fits to all the electroweak observables within the Minimal Supersymmetric Standard Model. We discuss the relic neutralino cosmic…

高能物理 - 唯象学 · 物理学 2009-10-28 A. Bottino , G. Mignola , M. Olechowski , S. Scopel

We perform a detailed analysis of the detection prospects of neutralino dark matter in the mSUGRA framework. We focus on models with a thermal relic density, estimated with high accuracy using the DarkSUSY package, in the range favored by…

天体物理学 · 物理学 2009-11-10 Joakim Edsjo , Mia Schelke , Piero Ullio

The electroweak sector may play a crucial role in discovering supersymmetry. We systematically investigate the patterns of the MSSM-like electroweakinos, when the neutralino relic abundance $\Omega_\chi h^2\leq 0.12$, that is, also…

高能物理 - 唯象学 · 物理学 2016-01-20 Marcin Badziak , Antonio Delgado , Marek Olechowski , Stefan Pokorski , Kazuki Sakurai