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Related papers: New Limits on Dark Matter from Super-Kamiokande

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Weakly Interacting Massive Particles (WIMPs) are one of the leading candidates for Dark Matter. For understanding the nature of WIMPs and identifying them among new particles produced at colliders (hopefully in the near future),…

High Energy Physics - Phenomenology · Physics 2011-08-17 Chung-Lin Shan

The recent results of the EDGES collaboration indicate that during the era of reionization, the primordial gas was much colder than expected. The cooling of the gas could be explained by interactions between dark matter (DM) and particles…

High Energy Physics - Phenomenology · Physics 2018-11-14 Niki Klop , Shin'ichiro Ando

Indirect detection of dark matter via its annihilation products is a key technique in the search for dark matter in the form of weakly interacting massive particles (WIMPs). Strong constraints exist on the annihilation of WIMPs to highly…

High Energy Physics - Phenomenology · Physics 2020-09-10 Nicole F. Bell , Matthew J. Dolan , Sandra Robles

The PICASSO experiment at SNOLAB reports new results for spin-dependent WIMP interactions on $^{19}$F using the superheated droplet technique. A new generation of detectors and new features which enable background discrimination via the…

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

We study whether spin-independent scattering of weakly-interacting massive particles (WIMPs) with nuclei can account for the annual modulation signal reported by DAMA. We consider both elastic and inelastic scattering processes. We find…

High Energy Physics - Phenomenology · Physics 2009-05-29 Frank Petriello , Kathryn M. Zurek

Neutrino telescopes are looking to detect neutrinos produced by the annihilation of weakly interacting massive particle (WIMP) dark matter in the sun. The event rate depends on the dark matter density in the sun, which in turn is dictated…

High Energy Physics - Phenomenology · Physics 2010-03-31 Prateek Agrawal , Zackaria Chacko , Can Kilic , Rashmish K. Mishra

We report new results from the Cryogenic Dark Matter Search (CDMS II) at the Soudan Underground Laboratory. Two towers, each consisting of six detectors, were operated for 74.5 live days, giving spectrum-weighted exposures of 34 kg-d for…

Astrophysics · Physics 2012-08-27 CDMS Collaboration

A search for muon neutrinos originating from dark matter annihilations in the Sun is performed using the data recorded by the ANTARES neutrino telescope from 2007 to 2012. In order to obtain the best possible sensitivities to dark matter…

High Energy Astrophysical Phenomena · Physics 2016-06-13 ANTARES collaboration , S. Adrián-Martínez , A. Albert , M. André , G. Anton , M. Ardid , J. -J. Aubert , T. Avgitas , B. Baret , J. Barrios-Martí , S. Basa , V. Bertin , S. Biagi , R. Bormuth , M. C. Bouwhuis , R. Bruijn , J. Brunner , J. Busto , A. Capone , L. Caramete , J. Carr , S. Celli , T. Chiarusi , M. Circella , A. Coleiro , R. Coniglione , H. Costantini , P. Coyle , A. Creusot , A. Deschamps , G. De Bonis , C. Distefano , C. Donzaud , D. Dornic , D. Drouhin , T. Eberl , I. El Bojaddaini , D. Elsässer , A. Enzenhöfer , K. Fehn , I. Felis , L. A. Fusco , S. Galatà , P. Gay , S. Geißelsöder , K. Geyer , V. Giordano , A. Gleixner , H. Glotin , R. Gracia-Ruiz , K. Graf , S. Hallmann , H. van Haren , A. J. Heijboer , Y. Hello , J. J. Hernández-Rey , J. Hößl , J. Hofestädt , C. Hugon , G. Illuminati , C. W James , M. de Jong , M. Jongen , M. Kadler , O. Kalekin , U. Katz , D. Kießling , A. Kouchner , M. Kreter , I. Kreykenbohm , V. Kulikovskiy , C. Lachaud , R. Lahmann , D. Lefèver , E. Leonora , S. Loucatos , M. Marcelin , A. Margiotta , A. Marinelli , J. A. Martínez-Mora , A. Mathieu , K. Melis , T. Michael , P. Migliozzi , A. Moussa , C. Mueller , E. Nezri , G. E. Păvălaş , C. Pellegrino , C. Perrina , P. Piattelli , V. Popa , T. Pradier , C. Racca , G. Riccobene , K. Roensch , M. Saldana , D. F. E. Samtleben , A. Sánchez-Losa , M. Sanguineti , P. Sapienza , J. Schnabel , F. Schüssler , T. Seitz , C. Sieger , M. Spurio , Th. Stolarczyk , M. Taiuti , C. Tönnis , A. Trovato , M. Tselengidou , D. Turpin , B. Vallage , C. Vallée , V. Van Elewyck , D. Vivolo , S. Wagner , J. Wilms , J. D. Zornoza , J. Zúñiga

The observation of GeV neutrinos coming from the Sun would be an unmistakable signal of dark matter. Current neutrino detectors have so far failed to detect such a signal, however, and bounds from direct and indirect dark matter searches…

High Energy Physics - Phenomenology · Physics 2017-12-20 Nicolao Fornengo , Antonio Masiero , Farinaldo S. Queiroz , Carlos E. Yaguna

Inelastic dark matter, in which WIMP-nucleus scatterings occur through a transition to an excited WIMP state ~ 100 keV above the ground state, provides a compelling explanation of the DAMA annual modulation signal. We demonstrate that the…

High Energy Physics - Phenomenology · Physics 2009-05-22 Spencer Chang , Graham D. Kribs , David Tucker-Smith , Neal Weiner

In experiments for direct dark matter searches, neutrinos coherently scattering off nuclei can produce similar events as Weakly Interacting Massive Particles (WIMPs). To reach sensitivities better than about 10^-10 pb for the elastic WIMP…

Dark matter and neutrinos provide the two most compelling pieces of evidence for new physics beyond the Standard Model of Particle Physics but they are often treated as two different sectors. In this paper, we consider how neutrino…

High Energy Physics - Phenomenology · Physics 2018-05-28 Andres Olivares-Del Campo , Sergio Palomares-Ruiz , Silvia Pascoli

Weakly Interacting Massive Particles (WIMPs), which are among the best motivated dark matter (DM) candidates, could make up all or only a fraction of the total DM budget. We consider a scenario in which WIMPs are a sub-dominant DM…

Cosmology and Nongalactic Astrophysics · Physics 2017-03-01 Sebastian Baum , Luca Visinelli , Katherine Freese , Patrick Stengel

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…

Astrophysics · Physics 2012-08-27 CDMS Collaboration

It is usually assumed that WIMPs interact through spin-independent and spin-dependent interactions. Interactions which carry additional powers of the momentum transfer, q^2, are assumed to be too small to be relevant. In theories with new…

High Energy Physics - Phenomenology · Physics 2010-08-18 Spencer Chang , Aaron Pierce , Neal Weiner

Signals broadly compatible with light (7-10 GeV) dark matter have been reported in three direct detection experiments: CoGeNT, DAMA/LIBRA, and CDMS-II silicon. These possible signals have been interpreted in the context of spin-independent…

High Energy Physics - Phenomenology · Physics 2013-09-11 Matthew R. Buckley , W. Hugh Lippincott

The Korea Invisible Mass Search(KIMS) experiment presents new limits on WIMP-nucleon cross section using the data from an exposure of 3409 kgd taken with low background CsI(Tl) crystals at Yangyang underground laboratory. The most stringent…

We discuss the neutrino constraints from solar and terrestrial dark matter (DM) annihilations in the inelastic dark matter (iDM) scenario after the recent CDMS II results. To reconcile the DAMA/LIBRA data with constraints from all other…

High Energy Physics - Phenomenology · Physics 2014-11-20 Jing Shu , Peng-fei Yin , Shou-hua Zhu

We present the result of an indirect search for high energy neutrinos from WIMP annihilation in the Sun using upward-going muon (upmu) events at Super-Kamiokande. Datasets from SKI-SKIII (3109.6 days) were used for the analysis. We looked…

High Energy Astrophysical Phenomena · Physics 2015-05-30 Kamiokande Collaboration , T. Tanaka , K. Abe , Y. Hayato , T. Iida , J. Kameda , Y. Koshio , Y. Kouzuma , M. Miura , S. Moriyama , M. Nakahata , S. Nakayama , Y. Obayashi , H. Sekiya , M. Shiozawa , Y. Suzuki , A. Takeda , Y. Takenaga , K. Ueno , K. Ueshima , S. Yamada , T. Yokozawa , C. Ishihara , S. Hazama , H. Kaji , T. Kajita , K. Kaneyuki , T. McLachlan , K. Okumura , Y. Shimizu , N. Tanimoto , F. Dufour , E. Kearns , M. Litos3 , J. L. Raaf , J. L. Stone , L. R. Sulak , J. P. Cravens , K. Bays , W. R. Kropp , S. Mine , C. Regis , M. B. Smy , H. W. Sobel , K. S. Ganezer , J. Hill , W. E. Keig , J. S. Jang , J. Y. Kim , I. T. Lim , J. B. Albert , K. Scholberg , C. W. Walter , R. Wendell , T. Wongjirad , T. Ishizuka , S. Tasaka , J. G. Learned , S. Matsuno , S. Smith , K. Martens , M. Vagins , Y. Watanabe , T. Hasegawa , T. Ishida , T. Ishii , T. Kobayashi , T. Nakadaira , K. Nakamura , K. Nishikawa , H. Nishino , Y. Oyama , K. Sakashita , T. Sekiguchi , T. Tsukamoto , A. T. Suzuki , Y. Takeuchi , M. Ikeda , A. Minamino , T. Nakaya , L. Labarga , Y. Fukuda , Y. Itow , G. Mitsuka , C. K. Jung , C. McGrew , G. Lopez , C. Yanagisawa , N. Tamura , H. Ishino , A. Kibayashi , M. Sakuda , Y. Kuno , M. Yoshida , S. B. Kim , B. S. Yang , H. Okazawa , Y. Choi , K. Nishijima , Y. Yokosawa , M. Koshiba , Y. Totsuka , M. Yokoyama , S. Chen , Y. Heng , Z. Yang , H. Zhang , D. Kielczewska , P. Mijakowski , K. Connolly , M. Dziomba , E. Thrane , R. J. Wilkes