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The problems of simple elementary weakly interacting massive particles (WIMPs) appeal to extend the physical basis for nonbaryonic dark matter. Such extension involves more sophisticated dark matter candidates from physics beyond the…

High Energy Physics - Phenomenology · Physics 2019-04-30 Vitaly Beylin , Maxim Yu. Khlopov , Vladimir Kuksa , Nikolay Volchanskiy

Dark Matter is one of the most intriguing riddles of modern astrophysics. The Standard Cosmological Model implies that only 4.5% of the mass-energy of the Universe is baryonic matter and the remaining 95% is unknown. Of this remainder, 22%…

Instrumentation and Methods for Astrophysics · Physics 2010-11-19 Andrzej M. Szelc

Dark matter plays a crucial role in our comprehension of the universe, but its mysterious nature poses challenges for direct detection. A primary obstacle in detecting dark matter is distinguishing genuine signals from the prevailing…

High Energy Physics - Experiment · Physics 2025-03-05 M. Mirzakhani , S. Maludze

Since the daring intuition by Fritz Zwicky in 1933 about the existence of dark matter in the Universe, in spite of the extensive investigations pursued over a very long lapse of time, the nature of this matter and of its (other than…

High Energy Physics - Phenomenology · Physics 2019-10-30 Alessandro Bottino

Several aspects of the motivation for particle dark matter search are introduced. The experimental principles and present state of the most important experiments are presented. Direct searches for WIMPs are explained in some detail,…

Astrophysics · Physics 2007-05-23 Martin Loidl

Assuming that cosmological dark matter consists of weakly interacting massive particles, we use the recent precise measurement of cosmological parameters to predict the guaranteed rates of production of such particles in association with…

High Energy Physics - Phenomenology · Physics 2009-10-09 Andreas Birkedal , Konstantin Matchev , Maxim Perelstein

The next generation of dark matter (DM) direct detection experiments and neutrino telescopes will probe large swaths of dark matter parameter space. In order to interpret the signals in these experiments, it is necessary to have good models…

High Energy Astrophysical Phenomena · Physics 2009-07-30 Annika H. G. Peter

Direct detection experiments aim at the detection of dark matter in the form of weakly interacting massive particles (WIMPs) by searching for signals from elastic dark matter nucleus scattering. Additionally, inelastic scattering in which…

High Energy Physics - Phenomenology · Physics 2020-01-08 G. Arcadi , C. Döring , C. Hasterok , S. Vogl

The search for dark matter is a very wide an active field of research, and I necessarily concentrate here only in some aspects of it. I will review the prospects for direct and indirect dark matter searches of Weakly Interacting Massive…

High Energy Physics - Phenomenology · Physics 2009-01-23 Graciela B. Gelmini

It is shown that weakly interacting massive particles (WIMPs), which are possible cold dark matter candidates, can be studied by exclusive measurements of X-rays following WIMPs nuclear interactions. Inner-shell atomic electrons are ionized…

High Energy Physics - Phenomenology · Physics 2009-11-11 H. Ejiri , Ch. C. Moustakidis , J. D. Vergados

We review several current aspects of dark matter theory and experiment. We overview the present experimental status, which includes current bounds and recent claims and hints of a possible signal in a wide range of experiments: direct…

High Energy Physics - Phenomenology · Physics 2018-06-13 Leszek Roszkowski , Enrico Maria Sessolo , Sebastian Trojanowski

The search for weakly-interacting massive particle (WIMP) dark matter is multi-pronged. Ultimately, the WIMP-dark-matter picture will only be confirmed if different classes of experiments see consistent signals and infer the same WIMP…

Cosmology and Nongalactic Astrophysics · Physics 2013-10-29 Annika H. G. Peter , Vera Gluscevic , Anne M. Green , Bradley J. Kavanagh , Samuel K. Lee

Dark Matter is a hypothetical particle proposed to explain the missing matter expected from the cosmological observation. The motivation of Dark Matter is overwhelming however as it is mainly deduced from its gravitational interaction, for…

High Energy Physics - Experiment · Physics 2016-02-04 Siew Yan Hoh , Jyothsna Komaragiri , Wan Ahmad Tajuddin Bin Wan Abdullah

The hierarchical clustering observed in cold dark matter simulations results in highly clumped galactic halos. If the dark matter in our halo is made of weakly interacting massive particles (WIMPs), their annihilation products should be…

Astrophysics · Physics 2009-11-07 P. Blasi , A. V. Olinto , C. Tyler

Weakly Interacting Massive Particle (WIMP) direct detection event rate calculations usually rely on fairly simple, essentially static, analytic halo models. This is largely since the resolution of numerical simulations is not yet large…

Astrophysics · Physics 2009-12-31 Anne M Green

We present a search for an excess of neutrino interactions due to dark matter in the form of Weakly Interacting Massive Particles (WIMPs) annihilating in the galactic center or halo based on the data set of Super-Kamiokande-I, -II, -III and…

High Energy Physics - Experiment · Physics 2020-10-14 Kamiokande Collaboration , K. Abe , C. Bronner , Y. Haga , Y. Hayato , M. Ikeda , S. Imaizumi , H. Ito , K. Iyogi , J. Kameda , Y. Kataoka , Y. Kato , Y. Kishimoto , Ll. Marti , M. Miura , S. Moriyama , T. Mochizuki , Y. Nagao , M. Nakahata , Y. Nakajima , T. Nakajima , S. Nakayama , T. Okada , K. Okamoto , A. Orii , G. Pronost , H. Sekiya , M. Shiozawa , Y. Sonoda , A. Takeda , A. Takenaka , H. Tanaka , S. Tasaka , T. Tomura , K. Ueno , T. Yano , T. Yokozawa , R. Akutsu , S. Han , T. Irvine , T. Kajita , I. Kametani , K. P. Lee , T. McLachlan , K. Okumura , E. Richard , T. Tashiro , R. Wang , J. Xia , D. Bravo-Berguño , L. Labarga , P. Fernandez , F. d. M. Blaszczyk , J. Gustafson , C. Kachulis , E. Kearns , J. L. Raaf , J. L. Stone , L. R. Sulak , S. Sussman , L. Wan , T. Wester , S. Berkman , S. Tobayama , J. Bian , G. Carminati , M. Elnimr , N. J. Griskevich , W. R. Kropp , S. Locke , S. Mine , A. Renshaw , M. B. Smy , H. W. Sobel , V. Takhistov , P. Weatherly , B. L. Hartfiel , J. Hill , W. E. Keig , N. Hong , J. Y. Kim , I. T. Lim , R. G. Park , T. Akiri , B. Bodur , A. Himmel , Z. Li , E. O'Sullivan , K. Scholberg , C. W. Walter , T. Wongjirad , A. Coffani , O. Drapier , S. El Hedri , A. Giampaolo , M. Gonin , J. Imber , Th. A. Mueller , P. Paganini , B. Quilain , T. Ishizuka , T. Nakamura , J. S. Jang , K. Choi , J. G. Learned , S. Matsuno , S. N. Smith , J. Amey , L. H. V. Anthony , R. P. Litchfield , W. Y. Ma , A. A. Sztuc , Y. Uchida , M. O. Wascko , V. Berardi , M. G. Catanesi , R. A. Intonti , E. Radicioni , N. F. Calabria , L. N. Machado , G. De Rosa , G. Collazuol , F. Iacob , M. Lamoureux , N. Ospina , L. Ludovici , T. Boschi , F. Di Lodovico , S. Molina Sedgwick , S. Zsoldos , Y. Nishimura , S. Cao , M. Friend , T. Hasegawa , T. Ishida , T. Ishii , T. Kobayashi , T. Nakadaira , K. Nakamura , Y. Oyama , K. Sakashita , T. Sekiguchi , T. Tsukamoto , KE. Abe , M. Hasegawa , Y. Isobe , H. Miyabe , Y. Nakano , T. Shiozawa , T. Sugimoto , A. T. Suzuki , Y. Takeuchi , S. Yamamoto , A. Ali , Y. Ashida , T. Hayashino , T. Hiraki , S. Hirota , K. Huang , K. Ieki , M. Jiang , T. Kikawa , M. Mori , A. Murakami , KE. Nakamura , T. Nakaya , N. D. Patel , K. Suzuki , S. Takahashi , K. Tateishi , R. A. Wendell , N. McCauley , P. Mehta , A. Pritchard , K. M. Tsui , Y. Fukuda , Y. Itow , H. Menjo , G. Mitsuka , M. Murase , F. Muto , T. Niwa , K. Sato , T. Suzuki , M. Taani , z M. Tsukada , P. Mijakowski , K. Frankiewicz , J. Hignight , C. K. Jung , X. Li , J. L. Palomino , G. Santucci , C. Vilela , M. J. Wilking , C. Yanagisawa , D. Fukuda , K. Hagiwara , M. Harada , T. Horai , H. Ishino , S. Ito , T. Kayano , A. Kibayashi , Y. Koshio , W. Ma , T. Mori , H. Nagata , N. Piplani , M. Sakuda , S. Seiya , Y. Takahira , C. Xu , R. Yamaguchi , Y. Kuno , G. Barr , D. Barrow , L. Cook , C. Simpson , D. Wark , F. Nova , R. Tacik , J. Y. Yang , A. Cole , S. J. Jenkins , J. McElwee , M. Thiesse , L. Thompson , H. Okazawa , S. B. Kim , Y. Choi , K. Ito , K. Nishijima , K. Iwamoto , M. Koshiba , Y. Suda , M. Yokoyama , R. G. Calland , A. Goldsack , K. Martens , M. Murdoch , Y. Suzuki , M. R. Vagins , D. Hamabe , M. Kuze , Y. Okajima , M. Tanaka , T. Yoshida , M. Inomoto , M. Ishitsuka , R. Matsumoto , K. Ohta , M. Shinoki , J. F. Martin , C. M. Nantais , H. A. Tanaka , T. Towstego , M. Hartz , A. Konaka , P. de Perio , N. W. Prouse , S. Chen , B. D. Xu , Y. Zhang , B. Richards , K. Connolly , R. J. Wilkes , B. Jamieson , J. Walker , P. Giorgio , A. Minamino , K. Okamoto , G. Pintaudi

WIMP direct detection experiments are just reaching the sensitivity required to detect galactic dark matter in the form of neutralinos. Data from these experiments are usually analysed under the simplifying assumption that the Milky Way…

Astrophysics · Physics 2008-11-26 Anne M Green

Direct searches for Dark Matter are experiment dedicated to the observation of the energetic recoiling ions produced by the scattering of WIMP particles from our galactic halo on terrestrial targets. The status and prospects of some…

High Energy Astrophysical Phenomena · Physics 2009-06-24 J. Gascon

Although a discovery of wimps either at colliders or in direct experiments would have enormous implications for our understanding of particle physics, it would imply less than one would like about our understanding of the dark matter in the…

High Energy Physics - Phenomenology · Physics 2007-05-23 Jacob L. Bourjaily , Gordon L. Kane

The majority of the matter in the universe is still unidentified and under investigation by both direct and indirect means. Many experiments searching for the recoil of dark-matter particles off target nuclei in underground laboratories…

High Energy Physics - Phenomenology · Physics 2015-10-28 Michael Klasen , Martin Pohl , Günter Sigl
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