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相关论文: Collider Signatures of SuperWIMP Warm Dark Matter

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Dark matter may be composed of superWIMPs, superweakly-interacting massive particles produced in the late decays of other particles. We focus here on the well-motivated supersymmetric example of gravitino LSPs. Gravitino superWIMPs share…

高能物理 - 唯象学 · 物理学 2007-05-23 Jonathan L. Feng , Arvind Rajaraman , Bryan T. Smith , Shufang Su , Fumihiro Takayama

We investigate a new class of dark matter: superweakly-interacting massive particles (superWIMPs). As with conventional WIMPs, superWIMPs appear in well-motivated particle theories with naturally the correct relic density. In contrast to…

高能物理 - 唯象学 · 物理学 2010-11-11 Jonathan L. Feng , Arvind Rajaraman , Fumihiro Takayama

Super-weakly interacting massive particles produced in the late decays of weakly interacting massive particles (WIMPs) are generic in large regions of supersymmetric parameter space and other frameworks for physics beyond the standard…

高能物理 - 唯象学 · 物理学 2013-08-08 Jose A. R. Cembranos , Manoj Kaplinghat

Extremely weakly interacting massive particles (E-WIMPs) are intriguing candidates for cold dark matter in the Universe. We review two well motivated E-WIMPs, an axino and a gravitino, and point out their cosmological and phenomenological…

高能物理 - 唯象学 · 物理学 2011-02-19 Ki-Young Choi , Leszek Roszkowski

The heavy gravitinos in minimal supergravity (mSUGRA) models couple gravitionally and can naturally be the Superweakly Interacting Massive Particle (SuperWIMP). As plausible candidates for the cold dark matter in the universe, such…

高能物理 - 唯象学 · 物理学 2009-11-10 Fei Wang , Jin Min Yang

SuperWIMPs are extremely weakly interacting massive particles that inherit their relic abundance from late decays of frozen-out parent particles. Within supersymmetric models, gravitinos and axinos represent two of the most well-motivated…

高能物理 - 唯象学 · 物理学 2023-09-13 Meera Deshpande , Jan Hamann , Dipan Sengupta , Martin White , Anthony G. Williams , Yvonne Y. Y. Wong

Cold dark matter may be made of superweakly-interacting massive particles, superWIMPs, that naturally inherit the desired relic density from late decays of metastable WIMPs. Well-motivated examples are weak-scale gravitinos in supergravity…

高能物理 - 唯象学 · 物理学 2008-11-26 Jonathan L. Feng , Arvind Rajaraman , Fumihiro Takayama

Collisionless, cold dark matter in the form of weakly-interacting massive particles (WIMPs) is well-motivated in particle physics, naturally yields the observed relic density, and successfully explains structure formation on large scales.…

高能物理 - 唯象学 · 物理学 2008-11-26 Jose A. R. Cembranos , Jonathan L. Feng , Arvind Rajaraman , Fumihiro Takayama

We investigate the superWIMP scenario in the framework of supersymmetry, in which the lightest supersymmetric particle is a stable gravitino. We consider slepton, sneutrino or neutralino being the next-lightest supersymmetric particle, and…

高能物理 - 唯象学 · 物理学 2007-05-23 Jonathan L. Feng , Shufang Su , Fumihiro Takayama

The axino and the gravitino are extremely weakly interacting candidates for the lightest supersymmetric particle (LSP). We demonstrate that either of them could provide the right amount of cold dark matter. Assuming that a charged slepton…

高能物理 - 唯象学 · 物理学 2007-05-23 Frank Daniel Steffen

Gravitinos and axinos produced in the late decays of other supersymmetric particles are well-motivated dark matter (DM) candidates, whose experimental evidences are very distinctive and different from other standard candidates, as thermal…

高能物理 - 唯象学 · 物理学 2008-11-26 J. A. R. Cembranos , Jonathan L. Feng , A. Rajaraman , F. Takayama

Weakly Interacting Massive Particles (WIMPs) are among the best-motivated dark matter candidates. In light of no conclusive detection signal yet despite an extensive search program that combines, often in a complementary way, direct,…

Weakly interacting massive particles (WIMPs) are among the favored candidates for cold dark matter in the universe. The phenomenology of supersymmetric WIMPs has been quite developed during recent years. However, there are other…

高能物理 - 唯象学 · 物理学 2009-11-07 E. A. Baltz , L. Bergstrom

In supergravity theories, a natural possibility is that neutralinos or sleptons freeze out at their thermal relic density, but then decay to gravitinos after about a year. The resulting gravitinos are then superWIMPs --…

高能物理 - 唯象学 · 物理学 2007-05-23 Jonathan L. Feng

Light WIMPs are dark matter particle candidates with weak scale interaction with the known particles, and mass in the GeV to 10's of GeV range. Hints of light WIMPs have appeared in several dark matter searches in the last decade. The…

高能物理 - 唯象学 · 物理学 2017-12-13 Graciela B. Gelmini

Models in which the dark matter is very weakly coupled to the observable sector may explain the observed dark matter density, either as a "superWIMP" or as "asymmetric dark matter." Both types of models predict displaced vertices at…

高能物理 - 唯象学 · 物理学 2009-06-30 Spencer Chang , Markus A. Luty

Several ideas for new physics beyond the standard model may provide particle candidates for the dark matter in the Galactic halo. The two leading candidates are an axion and a weakly-interacting massive particle (WIMP), such as the…

高能物理 - 唯象学 · 物理学 2008-02-03 Marc Kamionkowski

We describe two natural scenarios in which both dark matter WIMPs (weakly interacting massive particles) and a variety of supersymmetric partners should be discovered in the foreseeable future. In the first scenario, the WIMPs are…

高能物理 - 唯象学 · 物理学 2019-02-20 Maxwell Throm , Reagan Thornberry , John Killough , Brian Sun , Gentill Abdulla , Roland E. Allen

This article gives an overview on the status of experimental searches for dark matter at the end of 2014. The main focus is on direct searches for weakly interacting massive particles (WIMPs) using underground-based low-background…

宇宙学与河外天体物理 · 物理学 2015-07-29 Marc Schumann

Weakly Interacting Massive Particles (WIMPs) continue to be considered some of the best-motivated Dark Matter (DM) candidates. No conclusive signal, despite an extensive search program that combines, often in a complementary way, direct,…

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