On the sensitivity of present direct detection experiments to WIMP-quark and WIMP-gluon effective interactions: A systematic assessment and new model-independent approaches

被引：9

作者：

Kang, Sunghyun ^{[1
]}

Scopel, Stefano ^{[1
]}

Tomar, Gaurav ^{[1
]}

Yoon, Jong-Hyun ^{[1
]}

机构：

[1] Sogang Univ, Dept Phys, Seoul 121742, South Korea

来源：

ASTROPARTICLE PHYSICS | 2020年 / 114卷

基金：

新加坡国家研究基金会;

关键词：

Dark matter; Weakly interacting massive particles; Direct detection; Effective theories; DARK-MATTER; DAMA/LIBRA;

D O I：

10.1016/j.astropartphys.2019.07.001

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Assuming for Weakly Interacting Massive Particles (WIMPs) a Maxwellian velocity distribution in the Galaxy we provide an assessment of the sensitivity of existing Dark Matter (DM) direct detection (DD) experiments to operators up to dimension 7 of the relativistic effective field theory describing dark matter interactions with quarks and gluons. In particular we focus on a systematic approach, including an extensive set of experiments and large number of couplings, both exceeding for completeness similar analyses in the literature. The relativistic effective theory requires to fix one coupling for each quark flavor, so in principle for each different combination the bounds should be recalculated starting from direct detection experimental data. To address this problem we propose an approximate model-independent procedure that allows to directly calculate the bounds for any combination of couplings in terms of model-independent limits on the Wilson coefficients of the non-relativistic theory expressed in terms of the WIMP mass and of the neutron-to-proton coupling ratio C-n/C-p. We test the result of the approximate procedure against that of a full calculation, and discuss its possible pitfalls and limitations. We also provide a simple interpolating interface in Python that allows to apply our method quantitatively. (C) 2019 Elsevier B.V. All rights reserved.

引用

页码：80 / 91

页数：12

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