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相关论文: Dark Matter in Supergravity

200 篇论文

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…

高能物理 - 唯象学 · 物理学 2008-11-26 Seungwon Baek , Yeong Gyun Kim , P. Ko

We analyse the phenomenology of orbifold scenarios from the heterotic superstring, and the resulting theoretical predictions for the direct detection of neutralino dark matter. In particular, we study the parameter space of these…

高能物理 - 唯象学 · 物理学 2008-11-26 D. G. Cerdeno , T. Kobayashi , C. Munoz

The $b\tau j \etslash$ signal at the ongoing LHC experiments is simulated with Pythia in the mSUGRA and other models of SUSY breaking. Special attention is given on the compatibility of this signature with the low mass neutralino dark…

高能物理 - 唯象学 · 物理学 2011-11-10 Nabanita Bhattacharyya , Arghya Choudhury , Amitava Datta

The higgsino-like neutralino is a compelling dark matter candidate motivated by both cosmology and naturalness considerations. While a pure higgsino typically requires a mass of around $1.1~\mathrm{TeV}$ to satisfy the observed thermal…

高能物理 - 唯象学 · 物理学 2026-03-26 Yuanfang Yue , Yuetao Wang

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 calculate the relic density of the lightest neutralino in a supersymmetric seesaw type-II (``triplet seesaw'') model with minimal supergravity boundary conditions at the GUT scale. The presence of a triplet below the GUT scale, required…

高能物理 - 唯象学 · 物理学 2009-11-10 J. N. Esteves , M. Hirsch , S. Kaneko , W. Porod , J. C. Romao

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…

高能物理 - 唯象学 · 物理学 2007-05-23 Antonio Masiero , Stefano Profumo , Piero Ullio

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…

高能物理 - 唯象学 · 物理学 2008-11-26 R. Arnowitt , Pran Nath

We extend previous analyses on the interplay between nonuniversalities in the gaugino mass sector and the thermal relic densities of LSP neutralinos, in particular to the case of moderate to large tan beta. We introduce a set of parameters…

高能物理 - 唯象学 · 物理学 2014-11-17 Andreas Birkedal-Hansen , Brent D. Nelson

The lightest supersymmetric particles could be higgsinos that have a small mixing with gauginos. If the lightest higgsino-like state makes up some or all of the dark matter with a thermal freezeout density, then its mass must be between…

高能物理 - 唯象学 · 物理学 2024-05-08 Stephen P. Martin

We map the parameter space for MSSM neutralino dark matter which freezes out to the observed relic abundance, in the limit that all superpartners except the neutralinos and charginos are decoupled. In this space of relic neutralinos, we…

高能物理 - 唯象学 · 物理学 2015-03-30 Joseph Bramante , Patrick J. Fox , Adam Martin , Bryan Ostdiek , Tilman Plehn , Torben Schell , Michihisa Takeuchi

The appearance of a natural dark matter candidate, the neutralino, is among the principal successes of minimal supergravity (mSUGRA) and its descendents. In lieu of a suitable ultraviolet completion, however, theories of gravity-mediated…

高能物理 - 唯象学 · 物理学 2009-10-29 Nathaniel J. Craig , Daniel Green

We study natural supersymmetry in the Generalized Minimal Supergravity (GmSUGRA). For the parameter space with low energy electroweak fine-tuning measures less than 50, we are left with only the $Z$-pole, Higgs-pole and Higgsino LSP…

高能物理 - 唯象学 · 物理学 2018-08-08 Waqas Ahmed , Xiao-Jun Bi , Tianjun Li , Jia Shu Niu , Shabbar Raza , Qian-Fei Xiang , Peng-Fei Yin

Where is the long--awaited one? A supersymmetric neutralino has been a favored candidate for the WIMP dark matter but, so far, it has not been found. One way to locate it is to identify where it can be hiding in the vast supersymmetric…

高能物理 - 唯象学 · 物理学 2007-05-23 Leszek Roszkowski

The neutralino sector of the semi-constrained next-to-minimal supersymmetric standard model is explored under recent experimental constraints, with special attention to dark matter (DM) limits. The effects of the upper and lower bounds of…

高能物理 - 唯象学 · 物理学 2021-02-02 Elham Aldufeery , Maien Binjonaid

Galactic halo neutralinos ($\chi$) captured by the Sun or Earth produce high-energy neutrinos as end-products of various annihilation modes. These neutrinos can travel from the Sun or Earth cores to the neighborhood of underground detectors…

天体物理学 · 物理学 2009-08-25 Raj Gandhi , Jorge L. Lopez , D. V. Nanopoulos , Kajia Yuan , A. Zichichi

We consider dark matter annihilation into Standard Model particles and show that the least detectable final states, namely neutrinos, define an upper bound on the total cross section. Calculating the cosmic diffuse neutrino signal, and…

天体物理学 · 物理学 2008-11-26 John F. Beacom , Nicole F. Bell , Gregory D. Mack

It is shown that a decaying neutralino in a supergravity unified framework is a viable candidate for dark matter. Such a situation arises in the presence of a hidden sector with ultraweak couplings to the visible sector where the neutralino…

高能物理 - 唯象学 · 物理学 2021-08-18 Amin Aboubrahim , Tarek Ibrahim , Michael Klasen , Pran Nath

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

It is shown that the combined constraints on the amount of cold dark matter and of proton stability produce a stringent upper limit on the gluino mass $m_{\tilde g}$ (and hence on the lightest neutralino mass $m_{\chi_1^0}\simeq m_{\tilde…

高能物理 - 唯象学 · 物理学 2008-11-26 R. Arnowitt , Pran Nath