2015
DOI: 10.1051/epjconf/20159502004
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Direct dark matter searches review

Abstract: Abstract. Direct Dark Matter Searches are experiments looking for the energetic recoils due to the scattering of Weakly Interacting Massive Particles (WIMPs) from our galactic halo on nuclei in a terrestrial target. The principles of these type of searches is described, and the status and results of the leading experiments in that field are presented, as well as their prospects in the coming years.

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Cited by 16 publications
(11 citation statements)
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“…On the other hand, dark matter is one of the main known problems of physics. Many astrophysical searches are being carried out (see, e.g., [15][16][17][18][19][20][21] for reviews). The possible production of dark matter particles by accelerators (see, e.g., [22,23] for reviews) is also actively considered.…”
Section: Introductionmentioning
confidence: 99%
“…On the other hand, dark matter is one of the main known problems of physics. Many astrophysical searches are being carried out (see, e.g., [15][16][17][18][19][20][21] for reviews). The possible production of dark matter particles by accelerators (see, e.g., [22,23] for reviews) is also actively considered.…”
Section: Introductionmentioning
confidence: 99%
“…Dark matter is a very old problem. On the experimental side, it is being actively searched for, by direct detection (see, e.g., [1][2][3] for reviews), by indirect detection (see, e.g., [4][5][6] for reviews), and by accelerator production (see, e.g., [7,8] for reviews). Many "little anomalies" are known, from the Fermi excess of GeV gamma-rays [9] to the PAMELA and AMS-02 over-abundance of positrons [10][11][12].…”
Section: Introductionmentioning
confidence: 99%
“…For reviews on DM and on its detection searches see e.g. [5][6][7][8][9] The collisionless DM paradigm based on weakly interacting massive particles 10 works very well on large (cosmological) scales (≥ M pc), but encounters several problems at low (galactic) scales, like the core-cusp problem, the diversity problem, the missing satellites problem and the too-big-to-fail problem. 11 Self-interacting DM was introduced long time ago 12 in an effort to resolve, or at least to alleviate, the small scale crisis of collisionless DM.…”
Section: Introductionmentioning
confidence: 99%