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Readout technologies for directional WIMP Dark Matter detection

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arxiv 1610.02396 v1 pith:XZCCIMC4 submitted 2016-10-06 physics.ins-det astro-ph.COastro-ph.IMhep-ex

J. B. R. Battat , I. G. Irastorza , A. Aleksandrov , M. Ali Guler , T. Asada , E. Baracchini , J. Billard , G. Bosson
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O. Bourrion J. Bouvier A. Buonaura K. Burdge S. Cebrian P. Colas L. Consiglio T. Dafni N. D'Ambrosio C. Deaconu G. De Lellis T. Descombes A. Di Crescenzo N. Di Marco G. Druitt R. Eggleston E. Ferrer-Ribas T. Fusayasu J. Galan G. Galati J. A. Garcia J. G. Garza V. Gentile M. Garcia-Sciveres Y. Giomataris N. Guerrero O. Guillaudin J. Harton T. Hashimoto M. T. Hedges F. Iguaz T. Ikeda I. Jaegle J. A. Kadyk T. Katsuragawa S. Komura H. Kubo K. Kuge J. Lamblin A. Lauria E. R. Lee P. Lewis M. Leyton D. Loomba J. P. Lopez G. Luzon F. Mayet H. Mirallas K. Miuchi T. Mizumoto Y. Mizumura P. Monacelli J. Monroe M. C. Montesi T. Naka K. Nakamura H. Nishimura A. Ochi T. Papevangelou J. D. Parker N. S. Phan F. Pupilli J. P. Richer Q. Riffard G. Rosa D. Santos T. Sawano H. Sekiya I. S. Seong D. P. Snowden-Ifft N. J. C. Spooner A. Sugiyama R. Taishaku A. Takada A. Takeda M. Tanaka T. Tanimori T. N. Thorpe V. Tioukov H. Tomita A. Umemoto S. E. Vahsen Y. Yamaguchi M. Yoshimoto E. Zayas
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classification physics.ins-detastro-ph.COastro-ph.IMhep-ex
keywords directionaltechnologiesdetectionreadoutdarkdetectorsmatternuclear
verification ladder T0 review T1 audit T2 compute T3 formal
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The measurement of the direction of WIMP-induced nuclear recoils is a compelling but technologically challenging strategy to provide an unambiguous signature of the detection of Galactic dark matter. Most directional detectors aim to reconstruct the dark-matter-induced nuclear recoil tracks, either in gas or solid targets. The main challenge with directional detection is the need for high spatial resolution over large volumes, which puts strong requirements on the readout technologies. In this paper we review the various detector readout technologies used by directional detectors. In particular, we summarize the challenges, advantages and drawbacks of each approach, and discuss future prospects for these technologies.

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  1. Simulations of 3-Dimensional Recoil Response to Coherent Elastic Neutrino-Nucleus Scattering Events in Directional Direct Dark Matter Detectors

    astro-ph.HE 2026-06 unverdicted novelty 4.0 of 10

    Simulations of solar CEvNS events produce annually varying ring-like 3D recoil distributions in directional detectors that lack target dependence and contrast with fixed WIMP signals.

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