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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…

High Energy Physics - Phenomenology · Physics 2009-11-07 E. A. Baltz , L. Bergstrom

Magnetic monopoles are predicted in various unified gauge models and could be produced at intermediate mass scales. Their detection in a neutrino telescope is facilitated by the large amount of light emitted compared to that from muons.…

High Energy Astrophysical Phenomena · Physics 2012-08-30 ANTARES Collaboration , S. Adrián-Martínez , J. A. Aguilar , I. Al Samarai , A. Albert , M. André , M. Anghinolfi , G. Anton , S. Anvar , M. Ardid , A. C. Assis Jesus , T. Astraatmadja , J-J. Aubert , B. Baret , S. Basa , V. Bertin , S. Biagi , C. Bigongiari , C. Bogazzi , M. Bou-Cabo , B. Bouhou , M. C. Bouwhuis , J. Brunner , J. Busto , F. Camarena , A. Capone , C. Cârloganu , G. Carminati , J. Carr , S. Cecchini , Z. Charif , Ph. Charvis , T. Chiarusi , M. Circella , H. Costantini , P. Coyle , C. Curtil , M. P. Decowski , I. Dekeyser , A. Deschamps , C. Distefano , C. Donzaud , D. Dornic , Q. Dorosti , D. Drouhin , T. Eberl , U. Emanuele , A. Enzenhöfer , J-P. Ernenwein , S. Escoffier , P. Fermani , M. Ferri , V. Flaminio , F. Folger , U. Fritsch , J-L. Fuda , S. Galatà , P. Gay , G. Giacomelli , V. Giordano , J. P. Gómez-González , K. Graf , G. Guillard , G. Halladjian , G. Hallewell , H. van Haren , J. Hartman , A. J. Heijboer , Y. Hello , J. J. Hernández-Rey , B. Herold , J. Hößl , C. C. Hsu , M. de Jong , M. Kadler , O. Kalekin , A. Kappes , U. Katz , O. Kavatsyuk , P. Kooijman , C. Kopper , A. Kouchner , I. Kreykenbohm , V. Kulikovskiy , R. Lahmann , P. Lamare , G. Larosa , D. Lattuada , D. Lefèvre , G. Lim , D. Lo Presti , H. Loehner , S. Loucatos , S. Mangano , M. Marcelin , A. Margiotta , J. A. Martínez-Mora , A. Meli , T. Montaruli , M. Morganti , L. Moscoso , H. Motz , M. Neff , E. Nezri , D. Palioselitis , G. E. Păvălaş , K. Payet , P. Payre , J. Petrovic , P. Piattelli , N. Picot-Clemente , V. Popa , T. Pradier , E. Presani , C. Racca , C. Reed , G. Riccobene , C. Richardt , R. Richter , C. Rivière , A. Robert , K. Roensch , A. Rostovtsev , J. Ruiz-Rivas , M. Rujoiu , G. V. Russo , F. Salesa , P. Sapienza , F. Schöck , J-P. Schuller , F. Schüssler , T. Seitz , R. Shanidze , F. Simeone , A. Spies , M. Spurio , J. J. M. Steijger , Th. Stolarczyk , A. Sánchez-Losa , M. Taiuti , C. Tamburini , S. Toscano , B. Vallage , V. Van Elewyck , G. Vannoni , M. Vecchi , P. Vernin , S. Wagner , G. Wijnker , J. Wilms , E. de Wolf , H. Yepes , D. Zaborov , J. D. Zornoza , J. Zúñiga

We present updated results on the search for a neutrino signal from the core of the Earth and of the Sun induced by Weakly Interacting Massive Particles (WIMPs). In this paper we concentrate on neutralinos as WIMP candidates. The 971 and…

High Energy Physics - Experiment · Physics 2019-08-17 T. Montaruli , M. Ambriola et al

We present the results of a search for high energy neutrinos with the Baikal underwater Cherenkov detector NT-96. An upper limit to the flux of \nu_e + \nu_{\mu} + \bar{\nu_{\mu}} of E^2F_{\nu}(E)<1.4 10^{-5} cm^{-2} s^{-1} sr^{-1} GeV is…

Astrophysics · Physics 2007-05-23 BAIKAL Collaboration , V. Balkanov

A potential source of high energy neutrinos is the annihilation of Weakly Interacting Massive Particles (WIMPs) collecting in gravitational potential wells such as the centers of the Earth, the Sun, or the Galaxy. A search for such a WIMP…

High Energy Physics - Experiment · Physics 2019-08-14 A. Habig

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…

Searches for astronomical neutrino sources and weakly interactive massive particles (WIMPs) using the Super-Kamiokande detector have been performed. We select the neutrino-induced upward muon events for the first 4 years, which is already…

Astrophysics · Physics 2007-05-23 Kamiokande Collaboration

The Weakly Interacting Massive Particle (WIMP) is the main candidate for the relic dark matter. A set of exclusion curves currently obtained for cross sections of the spin-dependent WIMP-proton and WIMP-neutron interaction is given. A…

High Energy Physics - Phenomenology · Physics 2009-11-10 V. A. Bednyakov

I review the essentials of ultrahigh-energy neutrino interactions, show how neutral-current detection and flavor tagging can enhance the scientific potential of neutrino telescopes, and sketch new studies on neutrino encounters with dark…

Astrophysics · Physics 2007-05-23 Chris Quigg

The nature of Dark Matter (DM) remains one of the most important unresolved questions of fundamental physics. Many models, including Weakly Interacting Massive Particles (WIMPs), assume DM to be a particle and predict a weak coupling with…

High Energy Astrophysical Phenomena · Physics 2021-07-26 Giovanni Renzi

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…

High Energy Physics - Phenomenology · Physics 2008-02-03 Marc Kamionkowski

The Weakly Interacting Massive Particle (WIMP) is a popular particle physics candidate for the dark matter (DM). It can annihilate and/or decay to neutrino and antineutrino pair. The proposed 50 kt Magnetized Iron CALorimeter (MagICAL)…

High Energy Physics - Phenomenology · Physics 2018-03-09 Sanjib Kumar Agarwalla , Amina Khatun , Ranjan Laha

The dense energy deposition from a low-energy nuclear recoil produces, via the thermoacoustic effect, a brief yet intense pressure pulse that can be used for WIMP or neutrino detection in some fiber-optic devices sensitive to acoustooptic…

High Energy Physics - Experiment · Physics 2007-05-23 J. I. Collar

We review various issues related to the direct detection of constituents of dark matter, which are assumed to be Weakly Interacting Massive Particles (WIMPs). We specifically consider heavy WIMPs such as: 1) The lightest supersymmetric…

Nuclear Theory · Physics 2017-08-23 J. D. Vergados

We present the results of indirect searches for Weakly Interacting Massive Particles (WIMPs) with 1679.6 live days of data from the Super-Kamiokande detector using neutrino-induced upward through-going muons. The search is performed by…

High Energy Physics - Experiment · Physics 2012-08-27 Kamiokande Collaboration , S. Desai , Y. Ashie , S. Fukuda , Y. Fukuda , K. Ishihara , Y. Itow , Y. Koshio , A. Minamino , M. Miura , S. Moriyama , M. Nakahata , T. Namba , R. Nambu , Y. Obayashi , N. Sakurai , M. Shiozawa , Y. Suzuki , H. Takeuchi , Y. Takeuchi , S. Yamada , M. Ishitsuka , T. Kajita , K. Kaneyuki , S. Nakayama , A. Okada , T. Ooyabu , C. Saji , M. Earl , E. Kearns , J. L. Stone , L. R. Sulak , C. W. Walter , W. Wang , M. Goldhaber , T. Barszczak , D. Casper , J. P. Cravens , W. Gajewski , W. R. Kropp , S. Mine , D. W. Liu , M. B. Smy , H. W. Sobel , C. W. Sterner , M. R. Vagins , K. S. Ganezer , J. Hill , W. E. Keig , J. Y. Kim , I. T. Lim , R. W. Ellsworth , S. Tasaka , G. Guillian , A. Kibayashi , J. G. Learned , S. Matsuno , D. Takemori , M. D. Messier , Y. Hayato , A. K. Ichikawa , T. Ishida , T. Ishii , T. Iwashita , J. Kameda , T. Kobayashi , T. Maruyama , K. Nakamura , K. Nitta , Y. Oyama , M. Sakuda , Y. Totsuka , A. T. Suzuki , M. Hasegawa , K. Hayashi , T. Inagaki , I. Kato , H. Maesaka , T. Morita , T. Nakaya , K. Nishikawa , T. Sasaki , S. Ueda , S. Yamamoto , T. J. Haines , S. Dazeley , S. Hatakeyama , R. Svoboda , E. Blaufuss , J. A. Goodman , G. W. Sullivan , D. Turcan , K. Scholberg , A. Habig , C. K. Jung , T. Kato , K. Kobayashi , M. Malek , C. Mauger , C. McGrew , A. Sarrat , E. Sharkey , C. Yanagisawa , T. Toshito , C. Mitsuda , K. Miyano , T. Shibata , Y. Kajiyama , Y. Nagashima , M. Takita , M. Yoshida , H. I. Kim , H. Okazawa , T. Ishizuka , Y. Choi , H. K. Seo , Y. Gando , T. Hasegawa , K. Inoue , J. Shirai , A. Suzuki , M. Koshiba , T. Hashimoto , Y. Nakajima , K. Nishijima , T. Harada , H. Ishino , M. Morii , R. Nishimura , Y. Watanabe , D. Kielczewska , J. Zalipska , R. Gran , K. K. Shiraishi , K. Washburn , R. J. Wilkes

Relic neutralinos produced after the Big Bang are favoured candidates for Dark Matter. They can accumulate at the centre of massive celestial objects like our Sun. Their annihilation can result in a high-energy neutrino flux that could be…

Astrophysics · Physics 2019-08-13 Gordon Lim

An ever-increasing body of evidence suggests that weakly interacting massive particles (WIMPs) constitute the bulk of the matter in the Universe. Experimental data, dimensional analysis and Standard Model particle physics are sufficient to…

High Energy Physics - Phenomenology · Physics 2007-05-23 F. Halzen

After a short introduction on some general implications of recent cosmological observations, we discuss the properties of relic neutralinos in connection with present experimental strategies for detecting WIMPs.

High Energy Physics - Phenomenology · Physics 2009-11-07 A. Bottino , F. Donato , N. Fornengo , S. Scopel

There should be not doubt by now that neutrino telescopes are competitive instruments when it comes to searches for dark matter. Their large detector volumes collect hundreds of neutrinos per day. They scrutinize the whole sky continuously,…

High Energy Astrophysical Phenomena · Physics 2018-08-27 Carlos Pérez de los Heros

A search for high-energy neutrinos coming from the direction of the Sun has been performed using the data recorded by the ANTARES neutrino telescope during 2007 and 2008. The neutrino selection criteria have been chosen to maximize the…

High Energy Astrophysical Phenomena · Physics 2015-06-15 ANTARES Collaboration , S. Adrián-Martinez , I. Al Samarai , A. Albert , M. André , M. Anghinolfi , G. Anton , L. Anton , S. Anvar , M. Ardid , T. Astraatmadjaote , J-J. Aubert , B. Baret , S. Basa , V. Bertin , S. Biagi , C. Bigongiari , C. Bogazzi , B. Bouhou , M. C. Bouwhuis , J. Brünner , J. Busto , A. Capone , C. Cârloganu , J. Carr , S. Cecchini , Z. Charif , Ph. Charvis , T. Chiarusi , M. Circella , F. Classen , R. Coniglione , L. Core , H. Costantini , P. Coyle , A. Creusot , C. Curtil , G. De Bonis , M. P. Decowski , I. Dekeyser , A. Deschamps , C. Distefano , C. Donzaud , D. Dornic , Q. Dorosti , D. Drouhin , A. Dumas , T. Eberl , U. Emanuele , A. Enzenhöfer , J-P. Ernenwein , S. Escoffier , K. Fehn , P. Fermani , S. Ferry , V. Flaminio , F. Folger , U. Fritsch , J-L. Fuda , S. Galatà , P. Gay , S. Geisselsöder , K. Geyer , G. Giacomelli , V. Giordano , A. Gleixner , J. P. Gómez-González , K. Graf , G. Guillard , G. Hallewell , M. Hamal , H. van Haren , A. J. Heijboer , Y. Hello , J. J. Hernández-Rey , B. Herold , J. Hössl , C. C. Hsu , C. James , M. de Jong , M. Kadler , O. Kalekin , A. Kappesote , U. Katz , P. Kooijman , C. Kopper , A. Kouchner , I. Kreykenbohm , V. Kulikovskiy , R. Lahmann , G. Lambardote , G. Larosa , D. Lattuada , D. Lefèvre , E. Leonora , D. Lo Presti , H. Loehner , S. Loucatos , F. Louis , S. Mangano , M. Marcelin , A. Margiotta , J. A. Martinez-Mora , S. Martini , T. Montaruli , M. Morgantiote , H. Motz , C. Mueller , M. Neff , E. Nezri , D. Palioselitis , G. E. Pavalas , J. Petrovic , P. Piattelli , V. Popa , T. Pradier , C. Racca , C. Reed , G. Riccobene , R. Richter , C. Rivière , A. Robert , K. Roensch , A. Rostovtsev , M. Rujoiu , D. F. E. Samtleben , A. Sánchez-Losa , P. Sapienza , J. Schmid , J. Schnabel , S. Schulte , F. Schüssler , T. Seitz , R. Shanidze , F. Simeone , A. Spies , M. Spurio , J. J. M. Steijger , Th. Stolarczyk , M. Taiuti , C. Tamburini , A. Trovato , B. Vallage , C. Vallée , V. Van Elewyck , P. Vernin , E. Visser , S. Wagner , G. Wijnker , J. Wilms , E. de Wolf , K. Yatkin , H. Yepes , D. Zaborov , J. D. Zornoza , J. Zúñiga