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Limits on Dark Matter Effective Field Theory Parameters with CRESST-II

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arxiv 1809.03753 v1 pith:AL27LZEG submitted 2018-09-11 hep-ph

Limits on Dark Matter Effective Field Theory Parameters with CRESST-II

G. Angloher , P. Bauer , A. Bento , E. Bertoldo , C. Bucci , L. Canonica , A. D'Addabbo , X. Defay
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S. Di Lorenzo A. Erb F. v. Feilitzsch N. Ferreiro Iachellini P. Gorla D. Hauff J. Jochum M. Kiefer H. Kluck H. Kraus A. Langenk\"amper M. Mancuso V. Mokina E. Mondragon V. Morgalyuk A. M\"unster M. Olmi C. Pagliarone F. Petricca W. Potzel F. Pr\"obst F. Reindl J. Rothe K. Sch\"affner J. Schieck V. Schipperges S. Sch\"onert M. Stahlberg L. Stodolsky C. Strandhagen R. Strauss C. T\"urkoglu I. Usherov M. Willers M. W\"ustrich V. Zema R. Catena
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classification hep-ph
keywords darkmattercresst-iieffectivefieldlimitstheoryaiming
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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CRESST is a direct dark matter search experiment, aiming for an observation of nuclear recoils induced by the interaction of dark matter particles with cryogenic scintillating calcium tungstate crystals. Instead of confining ourselves to standard spin-independent and spin-dependent searches, we re-analyze data from CRESST-II using a more general effective field theory (EFT) framework. On many of the EFT coupling constants, improved exclusion limits in the low-mass region (< 3-4 GeV) are presented.

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