Searching for dark matter with paleo-detectors

被引:22
|
作者
Baum, Sebastian [1 ,2 ,3 ,4 ]
Drukier, Andrzej K. [1 ]
Freese, Katherine [1 ,2 ,3 ,5 ,6 ]
Gorski, Maciej [7 ]
Stengel, Patrick [1 ]
机构
[1] Stockholm Univ, Dept Phys, Oskar Klein Ctr Cosmoparticle Phys, S-10691 Stockholm, Sweden
[2] KTH Royal Inst Technol, Nordita, Roslagstullsbacken 23, S-10691 Stockholm, Sweden
[3] Stockholm Univ, Roslagstullsbacken 23, S-10691 Stockholm, Sweden
[4] Stanford Univ, Stanford Inst Theoret Phys, Dept Phys, Stanford, CA 94305 USA
[5] Univ Michigan, Leinweber Ctr Theoret Phys, Ann Arbor, MI 48109 USA
[6] Univ Texas Austin, Dept Phys, Austin, TX 78712 USA
[7] Natl Ctr Nucl Res, PL-05400 Otwock, Swierk, Poland
基金
瑞典研究理事会;
关键词
MAGNETIC MONOPOLES; ANCIENT MICA; LIMITS; MODULATION; EVAPORITES; SCATTERING; EVOLUTION; EXTENSION; ABUNDANCE; TRACKS;
D O I
10.1016/j.physletb.2020.135325
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
A large experimental program is underway to extend the sensitivity of direct detection experiments, searching for interaction of Dark Matter with nuclei, down to the neutrino floor. However, such experiments are becoming increasingly difficult and costly due to the large target masses and exquisite background rejection needed for the necessary improvements in sensitivity. We investigate an alternative approach to the detection of Dark Matter-nucleon interactions: Searching for the persistent traces left by Dark Matter scattering in ancient minerals obtained from much deeper than current underground laboratories. We estimate the sensitivity of paleo-detectors, which extends far beyond current upper limits for a wide range of Dark Matter masses. The sensitivity of our proposal also far exceeds the upper limits set by Snowden-Ifft et al. more than three decades ago using ancient Mica in an approach similar to paleo-detectors. (C) 2020 The Author(s). Published by Elsevier B.
引用
收藏
页数:7
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