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Related papers: WIMPs at High Energy Muon Colliders

200 papers

The WIMP dark matter (DM) hypothesis now is in an awkward position, owing to the stronger and stronger exclusion from DM direct detection. In this article we design a mechanism to evade this constraint.The idea is simple. DM has a…

High Energy Physics - Phenomenology · Physics 2022-01-12 Jun Guo , Zhaofeng Kang , Peng Zhang

Heavy Weakly Interacting Massive Particles (WIMPs) remain a prominent yet less constrained dark matter (DM) candidate, with the Galactic Centre (GC) serving as a prime target for indirect detection via gamma-ray signals. Extending our…

High Energy Astrophysical Phenomena · Physics 2026-01-06 Rajat Shinde , Julia Djuvsland , Davide Dapaoli , Jim Hinton

The standard model can be extended to include weakly-interacting light particle (WILP): real or complex singlet scalar, Majorana or Dirac neutral fermion, neutral or hidden-charged vector boson, etc. Imposing the $Z_2$ symmetry, these…

High Energy Physics - Phenomenology · Physics 2023-06-16 Huayang Song , Hao Sun , Jiang-Hao Yu

Solving the Dark Matter enigma represents one of the key objectives of contemporary physics. Recent astrophysical and cosmological measurements have unambiguously demonstrated that ordinary matter contributes to less than 5 % of the energy…

Astrophysics · Physics 2015-06-24 Gabriel Chardin

It was recently pointed out that direct detection signals from at least three different targets may be used to determine whether the Dark Matter (DM) particle is different from its antiparticle. In this work, we examine in detail the…

High Energy Physics - Phenomenology · Physics 2017-10-16 Bradley J. Kavanagh , Farinaldo S. Queiroz , Werner Rodejohann , Carlos E. Yaguna

We report on a dark matter search for a Weakly Interacting Massive Particle (WIMP) in the mass range $m_\chi \in [4, 30]\,\mathrm{GeV}/c^2$ with the EDELWEISS-III experiment. A 2D profile likelihood analysis is performed on data from eight…

The current state searches for dark matter in the form of Weakly Interacting Massive Particles (WIMPs) using both direct and indirect techniques is reviewed. Advances in recent years by various direct search experiments, utilising…

Astrophysics · Physics 2007-05-23 N. J. C. Spooner , V. A. Kudryavtsev

If Dark Matter is made of Weakly Interacting Massive Particles (WIMPs) with masses below $\sim$20 GeV, the corresponding nuclear recoils in mainstream WIMP experiments are of energies too close, or below, the experimental threshold. Gas…

Instrumentation and Detectors · Physics 2016-10-21 F. J. Iguaz , J. G. Garza , F. Aznar , J. F. Castel , S. Cebrián , T. Dafni , J. A. García , I. G. Irastorza , A. Lagraba , G. Luzón , A. Peiró

We enumerate the set of simplified models which match onto the complete set of gauge invariant effective operators up to dimension six describing interactions of a singlet-like Majorana fermion dark matter with the standard model. Tree…

High Energy Physics - Phenomenology · Physics 2016-10-05 Shigeki Matsumoto , Satyanarayan Mukhopadhyay , Yue-Lin Sming Tsai

The standard model (SM) plus a real gauge-singlet scalar field dubbed darkon (SM+D) is the simplest model possessing a weakly interacting massive particle (WIMP) dark-matter candidate. The upper limits for the WIMP-nucleon elastic…

High Energy Physics - Phenomenology · Physics 2010-04-21 Xiao-Gang He , Tong Li , Xue-Qian Li , Jusak Tandean , Ho-Chin Tsai

We consider the proposal that dark matter (DM) is composed of a spin-3/2 particle that is a singlet of the standard model (SM). Its leading effective interactions with ordinary matter involve a pair of their fields and a pair of SM…

High Energy Physics - Phenomenology · Physics 2013-05-31 Ran Ding , Yi Liao , Ji-Yuan Liu , Kai Wang

The WIMP proposed here yields the observed abundance of dark matter, and is consistent with the current limits from direct detection, indirect detection, and collider experiments, if its mass is $\sim 72$ GeV/$c^2$. It is also consistent…

High Energy Physics - Phenomenology · Physics 2021-08-02 Reagan Thornberry , Maxwell Throm , Gabriel Frohaug , John Killough , Dylan Blend , Michael Erickson , Brian Sun , Brett Bays , Roland E. Allen

The underlaying assumptions and uncertainties involved in the derivation of WIMP exclusion limits from XENON10 and XENON100 detectors are examined. In view of these, recent claims of sensitivity to light-mass Weakly Interacting Massive…

Cosmology and Nongalactic Astrophysics · Physics 2011-06-15 J. I. Collar

New limits are presented on the cross section for Weakly Interacting Massive Particle (WIMP) nucleon scattering in the KIMS CsI(T) detector array at the Yangyang Underground Laboratory. The exposure used for these results is 24524.3…

A strongly interacting massive particle (SIMP) is an interesting candidate for dark matter (DM) because its self-interaction cross section can be naturally strong enough to address the astrophysical problem of small-scale structure…

High Energy Physics - Phenomenology · Physics 2020-10-14 Ayuki Kamada , Masaki Yamada , Tsutomu T. Yanagida

A multi-TeV muon collider offers a spectacular opportunity in the direct exploration of the energy frontier. Offering a combination of unprecedented energy collisions in a comparatively clean leptonic environment, a high energy muon…

High Energy Physics - Experiment · Physics 2023-08-10 K. M. Black , S. Jindariani , D. Li , F. Maltoni , P. Meade , D. Stratakis , D. Acosta , R. Agarwal , K. Agashe , C. Aime , D. Ally , A. Apresyan , A. Apyan , P. Asadi , D. Athanasakos , Y. Bao , E. Barzi , N. Bartosik , L. A. T. Bauerdick , J. Beacham , S. Belomestnykh , J. S. Berg , J. Berryhill , A. Bertolin , P. C. Bhat , M. E. Biagini , K. Bloom , T. Bose , A. Bross , E. Brost , N. Bruhwiler , L. Buonincontri , D. Buttazzo , V. Candelise , A. Canepa , L. Carpenter , M. Casarsa , F. Celiberto , C. Cesarotti , G. Chachamis , Z. Chacko , P. Chang , S. V. Chekanov , T. Y. Chen , M. Chiesa , T. Cohen , M. Costa , N. Craig , A. Crivellin , C. Curatolo , D. Curtin , G. Da Molin , S. Dasu , A. de Gouvea , D. Denisov , R. Dermisek , K. F. Di Petrillo , T. Dorigo , J. M. Duarte , V. D. Elvira , R. Essig , P. Everaerts , J. Fan , M. Felcini , G. Fiore , D. Fiorina , M. Forslund , R. Franceschini , M. V. Garzelli , C. E. Gerber , L. Giambastiani , D. Giove , S. Guiducci , T. Han , K. Hermanek , C. Herwig , J. Hirschauer , T. R. Holmes , S. Homiller , L. A. Horyn , A. Ivanov , B. Jayatilaka , H. Jia , C. K. Jung , Y. Kahn , D. M. Kaplan , M. Kaur , M. Kawale , P. Koppenburg , G. Krintiras , K. Krizka , B. Kuchma , L. Lee , L. Li , P. Li , Q. Li , W. Li , R. Lipton , Z. Liu , S. Lomte , Q. Lu , D. Lucchesi , T. Luo , K. Lyu , Y. Ma , P. A. N. Machado , C. Madrid , D. J. Mahon , A. Mazzacane , N. McGinnis , C. McLean , B. Mele , F. Meloni , S. C. Middleton , R. K. Mishra , N. Mokhov , A. Montella , M. Morandin , S. Nagaitsev , F. Nardi , M. S. Neubauer , D. V. Neuffer , H. Newman , R. Ogaz , I. Ojalvo , I. Oksuzian , T. Orimoto , B. Ozek , K. Pachal , S. Pagan Griso , P. Panci , V. Papadimitriou , N. Pastrone , K. Pedro , F. Pellemoine , A. Perloff , D. Pinna , F. Piccinini , Marc-Andre Pleier , S. Posen , K. Potamianos , S. Rappoccio , M. Reece , L. Reina , A. Reinsvold Hall , C. Riccardi , L. Ristori , T. Robens , R. Ruiz , P. Sala , D. Schulte , L. Sestini , V. Shiltsev , P. Snopok , G. Stark , J. Stupak , S . Su , R. Sundrum , M. Swiatlowski , M. J. Syphers , A. Taffard , W. Thompson , Y. Torun , C. G. Tully , I. Vai , M. Valente , U. van Rienen , R. van Weelderen , G. Velev , N. Venkatasubramanian , L. Vittorio , C. Vuosalo , X. Wang , H. Weber , R. Wu , Y. Wu , A. Wulzer , K. Xie , S. Xie , R. Yohay , K. Yonehara , F. Yu , A. V. Zlobin , D. Zuliani , J. Zurita

In this work we show that from the spectrum of particles of a 3-3-1 gauge model with heavy sterile neutrinos we can have up to three Cold Dark Matter candidates as WIMPs. We obtain their relic abundance and analyze their compatibility with…

High Energy Physics - Phenomenology · Physics 2015-03-17 J. K. Mizukoshi , C. A. de S. Pires , F. S. Queiroz , P. S. Rodrigues da Silva

A possible connection between the abundances of baryonic and dark matter (DM) has been explored so far mostly in the context of the so-called asymmetric DM. Recently, a very different mechanism, dubbed "WIMPy baryogenesis", has been…

High Energy Physics - Phenomenology · Physics 2015-06-11 Nicolas Bernal , Francois-Xavier Josse-Michaux , Lorenzo Ubaldi