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The CRESST-III experiment which is dedicated to low-mass dark matter search uses scintillating CaWO$_4$ crystals operated as cryogenic particle detectors. Background discrimination is achieved by exploiting the scintillating light signal of…

Directional detection is a promising dark matter search strategy. Indeed, weakly interacting massive particle (WIMP)-induced recoils would present a direction dependence toward the Cygnus constellation, while background-induced recoils…

Cosmology and Nongalactic Astrophysics · Physics 2011-04-22 J. Billard , F. Mayet , D. Santos

High light collection efficiency is an important requirement in any application of scintillation detectors. The purpose of this study is to investigate the possibility for improving this parameter in cryogenic scintillation bolometers,…

Instrumentation and Detectors · Physics 2014-02-11 F. A. Danevich , R. V. Kobychev , V. V. Kobychev , H. Kraus , V. B. Mikhailik , V. M. Mokina

There is currently vast evidence for Dark Matter (DM) from astronomical observations. However, in spite of tremendous efforts by large experimental groups, there is no confirmed direct detection of the dark matter in our galaxy. Recent…

Instrumentation and Methods for Astrophysics · Physics 2014-11-20 Juan Estrada

Small cryogenic detectors with efficient background rejection now best longer established and heavier direct dark matter searches. This paper reviews the experiments, results and prospects.

Astrophysics · Physics 2007-05-23 P. C. F. Di Stefano

It is an intriguing possibility that the cold dark matter of the Universe may consist of very light and very weakly interacting particles such as axion(-like particles) and hidden photons. This opens up (but also requires) new techniques…

High Energy Physics - Phenomenology · Physics 2015-06-16 Joerg Jaeckel , Javier Redondo

Direct detection of dark matter with directional sensitivity offers not only measurement of both recoil energy and direction of dark matter, but also a way to understand dark matter distribution in the Galaxy. Maxwell distribution is…

High Energy Physics - Phenomenology · Physics 2015-06-18 Keiko I. Nagao

Experiments based on noble liquids and solid state cryogenic detectors have had a leading role in the direct detection of dark matter. But smaller scale projects can help to explore the new dark matter landscape with advanced,…

Instrumentation and Methods for Astrophysics · Physics 2020-05-20 Susana Cebrián

We perform the first high-throughput search and evaluation of materials that can serve as excellent low-mass dark matter detectors. Using properties of close to one thousand materials from the Materials Project database, we project the…

High Energy Physics - Phenomenology · Physics 2025-06-26 Sinéad M. Griffin , Yonit Hochberg , Benjamin V. Lehmann , Rotem Ovadia , Kristin A. Persson , Bethany A. Suter , Ruo Xi Yang , Wayne Zhao

Among the many experimental techniques available, those providing directional information have the potential of yielding an unambiguous observation of WIMPs even in the presence of insidious backgrounds. A measurement of the distribution of…

Astrophysics · Physics 2014-11-18 Gabriella Sciolla

Recoil imaging entails the detection of spatially resolved ionization tracks generated by particle interactions. This is a highly sought-after capability in many classes of detector, with broad applications across particle and astroparticle…

Instrumentation and Detectors · Physics 2022-07-19 C. A. J. O'Hare , D. Loomba , K. Altenmüller , H. Álvarez-Pol , F. D. Amaro , H. M. Araújo , D. Aristizabal Sierra , J. Asaadi , D. Attié , S. Aune , C. Awe , Y. Ayyad , E. Baracchini , P. Barbeau , J. B. R. Battat , N. F. Bell , B. Biasuzzi , L. J. Bignell , C. Boehm , I. Bolognino , F. M. Brunbauer , M. Caamaño , C. Cabo , D. Caratelli , J. M. Carmona , J. F. Castel , S. Cebrián , C. Cogollos , D. Collison , E. Costa , T. Dafni , F. Dastgiri , C. Deaconu , V. De Romeri , K. Desch , G. Dho , F. Di Giambattista , D. Díez-Ibáñez , G. D'Imperio , B. Dutta , C. Eldridge , S. R. Elliott , A. C. Ezeribe , A. Fava , T. Felkl , B. Fernández-Domínguez , E. Ferrer Ribas , K. J. Flöthner , M. Froehlich , J. Galán , J. Galindo , F. García , J. A. García Pascual , B. P. Gelli , M. Ghrear , Y. Giomataris , K. Gnanvo , E. Gramellini , G. Grilli Di Cortona , R. Hall-Wilton , J. Harton , S. Hedges , S. Higashino , G. Hill , P. C. Holanda , T. Ikeda , I. G. Irastorza , P. Jackson , D. Janssens , B. Jones , J. Kaminski , I. Katsioulas , K. Kelly , N. Kemmerich , E. Kemp , H. B. Korandla , H. Kraus , A. Lackner , G. J. Lane , P. M. Lewis , M. Lisowska , G. Luzón , W. A. Lynch , G. Maccarrone , K. J. Mack , P. A. Majewski , R. D. P. Mano , C. Margalejo , D. Markoff , T. Marley , D. J. G. Marques , R. Massarczyk , G. Mazzitelli , C. McCabe , L. J. McKie , A. G. McLean , P. C. McNamara , Y. Mei , A. Messina , A. F. Mills , H. Mirallas , K. Miuchi , C. M. B. Monteiro , M. R. Mosbech , H. Muller , H. Natal da Luz , K. D. Nakamura , A. Natochii , T. Neep , J. L. Newstead , K. Nikolopoulos , L. Obis , E. Oliveri , G. Orlandini , A. Ortiz de Solórzano , J. von Oy , T. Papaevangelou , O. Pérez , Y. F. Perez-Gonzalez , D. Pfeiffer , N. S. Phan , S. Piacentini , E. Picatoste Olloqui , D. Pinci , S. Popescu , A. Prajapati , F. S. Queiroz , J. L. Raaf , F. Resnati , L. Ropelewski , R. C. Roque , E. Ruiz-Choliz , A. Rusu , J. Ruz , J. Samarati , E. M. Santos , J. M. F. dos Santos , F. Sauli , L. Scharenberg , T. Schiffer , S. Schmidt , K. Scholberg , M. Schott , J. Schueler , L. Segui , H. Sekiya , D. Sengupta , Z. Slavkovska , D. Snowden-Ifft , P. Soffitta , M. van Stenis , N. J. C. Spooner , L. Strigari , A. E. Stuchbery , X. Sun , S. Torelli , E. G. Tilly , A. W. Thomas , T. N. Thorpe , P. Urquijo , A. Utrobičić , S. E. Vahsen , R. Veenhof , J. K. Vogel , A. G. Williams , M. H. Wood , J. Zettlemoyer

Directional detection of non-baryonic Dark Matter is a promising search strategy for discriminating genuine WIMP events from background ones. However, carrying out such a strategy requires both a precise measurement of the energy down to a…

Instrumentation and Methods for Astrophysics · Physics 2010-09-20 C. Grignon , J. Billard , G. Bosson , O. Bourrion , O. Guillaudin , F. Mayet , J. P. Richer , D. Santos , E. Ferrer , I. Giomataris , J. P. Mols

Directional detection of galactic Dark Matter is a promising search strategy for discriminating genuine WIMP events from background ones. However, to take full advantage of this powerful detection method, one need to be able to extract…

Cosmology and Nongalactic Astrophysics · Physics 2010-04-15 J. Billard , F. Mayet , J. F. Macias-Perez , D. Santos , C. Grignon , O. Guillaudin

Directional detection of dark matter can provide unambiguous observation of dark matter interactions even in the presence of background. This article presents an experimental method to measure the direction tag ("head-tail") of the dark…

Directional detection of dark matter has sensitivity for both recoil energy and direction of nuclear recoil. It opens the way to measure local velocity distribution of dark matter. In this paper, we study possibility to discriminate…

High Energy Physics - Phenomenology · Physics 2020-04-02 Keiko I. Nagao , Tomonori Ikeda , Ryota Yakabe , Tatsuhiro Naka , Kentaro Miuchi

The CRESST experiment is a direct dark matter search which aims to measure interactions of potential dark matter particles in an earth-bound detector. With the current stage, CRESST-III, we focus on a low energy threshold for increased…

Liquid xenon-based direct detection dark matter experiments have recently expanded their searches to include high-energy nuclear recoil events as motivated by effective field theory dark matter and inelastic dark matter interaction models,…

Directional detection of nuclear recoils is broadly desirable in nuclear and particle physics. At low recoil energies, this capability may be used to confirm the cosmological origin of a dark matter signal, to penetrate the so-called…

Instrumentation and Detectors · Physics 2021-10-13 Majd Ghrear , Sven E. Vahsen , Cosmin Deaconu

Direction measurement of weakly interacting massive particles in time-projection chambers can provide definite evidence of their existence and help to determine their properties. This article demonstrates several concepts for charge…

Directional detection of Galactic Dark Matter is a promising search strategy for discriminating genuine WIMP events from background ones. Technical progress on gaseous detectors and read-outs has permitted the design and construction of…

Cosmology and Nongalactic Astrophysics · Physics 2014-11-20 J. Billard , F. Mayet , J. F. Macias-Perez , D. Santos