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DARWIN (dark matter wimp search with noble liquids) is a design study for a next-generation, multi-ton dark matter detector in Europe. Liquid argon and/or liquid xenon are the target media for the direct detection of dark matter candidates…

天体物理仪器与方法 · 物理学 2019-08-14 Laura Baudis

We briefly discuss the expected level of supersymmetric dark matter cross-sections as a reference for dark matter detectors. We then discuss the current ZEPLIN II program as a prototype of large liquid Xenon detectors. Cryoarray is a…

天体物理学 · 物理学 2007-05-23 David B. Cline

The observable signal of higher-spin particles is rare in current particle collider experiments. In the meantime, there have no evident constraints on the spin of the dark matter particles. And thereby it is natural to consider the…

高能物理 - 唯象学 · 物理学 2022-03-28 Ke-yun Wu , Acckin Lee

A search for dark matter particles is performed using events with a Z boson candidate and large missing transverse momentum. The analysis is based on proton-proton collision data at a center-of-mass energy of 13 TeV, collected by the CMS…

高能物理 - 实验 · 物理学 2021-04-21 CMS Collaboration

Spin-dependent fifth-forces are associated with particles beyond the standard model. In particular, light pseudo-scalar bosons mediate long-range forces, allowing mass to interact with spins. The search of these interactions can be…

高能物理 - 实验 · 物理学 2022-03-07 N. Crescini , G. Carugno , P. Falferi , A. Ortolan , G. Ruoso , C. C. Speake

The search for direct interactions of dark matter particles remains one of the most pressing challenges of contemporary experimental physics. A variety of different approaches is required to probe the available parameter space and to meet…

天体物理仪器与方法 · 物理学 2009-10-19 Rafael F. Lang , Wolfgang Seidel

We study current constraints and search prospects for a GeV scale vector boson at a range of low energy experiments. It couples to the Standard Model charged particles with a strength <= 10^-3 to 10^-4 of that of the photon. The possibility…

高能物理 - 唯象学 · 物理学 2010-02-23 Matthew Reece , Lian-Tao Wang

LUX-ZEPLIN (LZ) collaboration has achieved the strongest constraint on weak-scale dark matter (DM)-nucleon spin-independent (SI) scattering cross section in a large region of parameter space. In this paper, we take a complementary approach…

高能物理 - 唯象学 · 物理学 2024-02-08 Tarak Nath Maity , Ranjan Laha

The NuMI facility at Fermilab produces a high-intensity beam of muon neutrinos and antineutrinos, designed to study neutrino oscillations. This beam may also be a source of dark matter particles produced through a light mediator. We search…

高能物理 - 实验 · 物理学 2025-11-13 S. Abubakar , M. Acero , B. Acharya , P. Adamson , N. Anfimov , A. Antoshkin , E. Arrieta-Diaz , L. Asquith , A. Aurisano , A. Back , N. Balashov , P. Baldi , B. A. Bambah , E. F. Bannister , A. Barros , A. Bat , T. Bezerra , V. Bhatnagar , B. Bhuyan , J. Bian , A. C. Booth , R. Bowles , B. Brahma , C. Bromberg , N. Buchanan , A. Butkevich , T. J. Carroll , E. Catano-Mur , J. P. Cesar , R. Chirco , S. Choate , B. C. Choudhary , O. T. K. Chow , A. Christensen , M. F. Cicala , T. E. Coan , T. Contreras , A. Cooleybeck , D. Coveyou , L. Cremonesi , G. S. Davies , P. F. Derwent , Z. Djurcic , K. Dobbs , D. Duenas Tonguino , E. C. Dukes , R. Ehrlich , E. Ewart , P. Filip , M. J. Frank , H. R. Gallagher , A. Giri , R. A. Gomes , M. C. Goodman , R. Group , A. Habig , F. Hakl , J. Hartnell , R. Hatcher , J. M. Hays , M. He , K. Heller , V Hewes , A. Himmel , T. Horoho , X. Huang , A. Ivanova , I. Kakorin , A. Kalitkina , D. M. Kaplan , A. Khanam , B. Kirezli , J. Kleykamp , O. Klimov , L. W. Koerner , L. Kolupaeva , R. Kralik , A. Kumar , C. D. Kuruppu , V. Kus , T. Lackey , K. Lang , J. Lesmeister , A. Lister , J. A. Lock , S. Magill , W. A. Mann , M. T. Manoharan , M. Manrique Plata , M. L. Marshak , M. Martinez-Casales , V. Matveev , A. Medhi , B. Mehta , M. D. Messier , H. Meyer , T. Miao , W. H. Miller , S. R. Mishra , R. Mohanta , A. Moren , A. Morozova , W. Mu , L. Mualem , M. Muether , C. Murthy , D. Myers , J. Nachtman , D. Naples , J. K. Nelson , O. Neogi , R. Nichol , E. Niner , A. Norman , A. Norrick , H. Oh , A. Olshevskiy , T. Olson , A. Pal , J. Paley , L. Panda , R. B. Patterson , G. Pawloski , R. Petti , L. R. Prais , A. Rafique , V. Raj , M. Rajaoalisoa , B. Ramson , B. Rebel , C. Reynolds , E. Robles , P. Roy , O. Samoylov , M. C. Sanchez , S. Sanchez Falero , P. Shanahan , P. Sharma , A. Sheshukov , Shivam , A. Shmakov , W. Shorrock , S. Shukla , I. Singh , V. Singh , S. Singh Chhibra , J. Smolik , P. Snopok , N. Solomey , A. Sousa , K. Soustruznik , M. Strait , C. Sullivan , L. Suter , A. Sutton , S. Swain , A. Sztuc , N. Talukdar , P. Tas , J. Thomas , E. Tiras , M. Titus , Y. Torun , D. Tran , J. Trokan-Tenorio , J. Urheim , B. Utt , P. Vahle , Z. Vallari , K. J. Vockerodt , A. V. Waldron , M. Wallbank , C. Weber , M. Wetstein , D. Whittington , D. A. Wickremasinghe , J. Wolcott , S. Wu , W. Wu , Y. Xiao , B. Yaeggy , A. Yahaya , A. Yankelevich , K. Yonehara , S. Zadorozhnyy , J. Zalesak , R. Zwaska

The EDELWEISS II experiment is devoted to the search for Weakly Interacting Massive Particles (WIMP) that would constitute the Dark Matter halo of our Galaxy. For this purpose, the experiment uses cryogenic germanium detectors, cooled down…

宇宙学与河外天体物理 · 物理学 2014-11-20 Veronique Sanglard

As experimental null results increase the pressure on heavy weakly interacting massive particles (WIMPs) as an explanation of thermal dark matter (DM), it seems timely to explore previously overlooked regions of the WIMP parameter space. In…

高能物理 - 唯象学 · 物理学 2019-02-13 Patrick Foldenauer

If the dark matter particle has spin 0, only two types of WIMP-nucleon interaction can arise from the non-relativistic reduction of renormalisable single-mediator models for dark matter-quark interactions. Based on this crucial observation,…

高能物理 - 唯象学 · 物理学 2018-01-17 Riccardo Catena , Jan Conrad , Christian Döring , Alfredo Davide Ferella , Martin B. Krauss

Some extensions of the Standard Model provide Dark Matter candidate particles with sub-GeV mass. These Light Dark Matter particles have been considered for example in Warm Dark Matter scenarios (e.g. the keV scale sterile neutrino, axino or…

The Cryogenic Dark Matter Search (CDMS) employs low-temperature Ge and Si detectors to search for Weakly Interacting Massive Particles (WIMPs) via their elastic-scattering interactions with nuclei while discriminating against interactions…

天体物理学 · 物理学 2012-08-27 CDMS Collaboration

We investigate the velocity and recoil momentum dependence of dark matter interactions with ordinary matter. In particular we focus on the single-electron resolution semiconductor detectors, which allow experimental assessment of sub-GeV…

高能物理 - 唯象学 · 物理学 2019-06-05 Matti Heikinheimo , Kai Nordlund , Kimmo Tuominen , Nader Mirabolfathi

Direct detection experiments aimed at uncovering the elusive nature of dark matter (DM) have made significant progress in probing ever lower cross-sections for DM-nucleon interactions. At the same time, an upper limit in the cross-section…

The quest for new physics beyond the Standard Model is boosted by the recently observed deviation in the anomalous magnetic moments of muon and electron from their respective theoretical prediction. In the present work, we have proposed a…

高能物理 - 唯象学 · 物理学 2022-07-08 Anirban Biswas , Sarif Khan

Multiple viable theoretical models predict heavy dark matter particles with a mass close to the Planck mass, a range relatively unexplored by current experimental measurements. We use 219.4 days of data collected with the XENON1T experiment…

高能物理 - 实验 · 物理学 2023-07-06 E. Aprile , K. Abe , S. Ahmed Maouloud , L. Althueser , B. Andrieu , E. Angelino , J. R. Angevaare , V. C. Antochi , D. Antón Martin , F. Arneodo , L. Baudis , A. L. Baxter , M. Bazyk , L. Bellagamba , R. Biondi , A. Bismark , E. J. Brookes , A. Brown , S. Bruenner , G. Bruno , R. Budnik , T. K. Bui , C. Cai , J. M. R. Cardoso , D. Cichon , A. P. Cimental Chavez , M. Clark , A. P. Colijn , J. Conrad , J. J. Cuenca-García , J. P. Cussonneau , V. D'Andrea , M. P. Decowski , P. Di Gangi , S. Di Pede , S. Diglio , K. Eitel , A. Elykov , S. Farrell , A. D. Ferella , C. Ferrari , H. Fischer , M. Flierman , W. Fulgione , C. Fuselli , P. Gaemers , R. Gaior , A. Gallo Rosso , M. Galloway , F. Gao , R. Glade-Beucke , L. Grandi , J. Grigat , H. Guan , M. Guida , R. Hammann , A. Higuera , C. Hils , L. Hoetzsch , N. F. Hood , J. Howlett , M. Iacovacci , Y. Itow , J. Jakob , F. Joerg , A. Joy , N. Kato , M. Kara , P. Kavrigin , S. Kazama , M. Kobayashi , G. Koltman , A. Kopec , F. Kuger , H. Landsman , R. F. Lang , L. Levinson , I. Li , S. Li , S. Liang , S. Lindemann , M. Lindner , K. Liu , J. Loizeau , F. Lombardi , J. Long , J. A. M. Lopes , Y. Ma , C. Macolino , J. Mahlstedt , A. Mancuso , L. Manenti , F. Marignetti , T. Marrodán Undagoitia , K. Martens , J. Masbou , D. Masson , E. Masson , S. Mastroianni , M. Messina , K. Miuchi , K. Mizukoshi , A. Molinario , S. Moriyama , K. Morå , Y. Mosbacher , M. Murra , J. Müller , K. Ni , U. Oberlack , B. Paetsch , J. Palacio , Q. Pellegrini , R. Peres , C. Peters , J. Pienaar , M. Pierre , V. Pizzella , G. Plante , T. R. Pollmann , J. Qi , J. Qin , D. Ramírez García , R. Singh , L. Sanchez , J. M. F. dos Santos , I. Sarnoff , G. Sartorelli , J. Schreiner , D. Schulte , P. Schulte , H. Schulze Eißing , M. Schumann , L. Scotto Lavina , M. Selvi , F. Semeria , P. Shagin , S. Shi , E. Shockley , M. Silva , H. Simgen , A. Takeda , P. -L. Tan , A. Terliuk , D. Thers , F. Toschi , G. Trinchero , C. Tunnell , F. Tönnies , K. Valerius , G. Volta , C. Weinheimer , M. Weiss , D. Wenz , C. Wittweg , T. Wolf , V. H. S. Wu , Y. Xing , D. Xu , Z. Xu , M. Yamashita , L. Yang , J. Ye , L. Yuan , G. Zavattini , M. Zhong , T. Zhu

We present prospects for discovering dark matter scattering in gravitational wave detectors. The focus of this work is on light, particle dark matter with masses below 1 GeV/c$^{2}$. We investigate how a potential signal compares to typical…

高能物理 - 唯象学 · 物理学 2020-12-08 Chun-Hao Lee , Chrisna Setyo Nugroho , Martin Spinrath