Maity, TN and Laha, R (2024) Cosmic-ray boosted dark matter in Xe-based direct detection experiments. In: European Physical Journal C, 84 (2).
|
PDF
Eur_phy_jou__84_2.pdf.pdf - Published Version Download (662kB) | Preview |
Abstract
LUX-ZEPLIN (LZ) collaboration has achieved the strongest constraint on weak-scale dark matter (DM)-nucleon spin-independent (SI) scattering cross section in a large region of parameter space. In this paper, we take a complementary approach and study the prospect of detecting cosmic-ray boosted sub-GeV DM in LZ. In the absence of a signal for DM, we improve upon the previous constraints by a factor of (Formula presented.) using the LZ result for some regions of the parameter space. We also show that upcoming XENONnT and future Darwin experiments will be sensitive to cross sections smaller by factors of (Formula presented.) and (Formula presented.) compared to the current LZ limit, respectively. © The Author(s) 2024.
Item Type: | Journal Article |
---|---|
Publication: | European Physical Journal C |
Publisher: | Institute for Ionics |
Additional Information: | The copyright for this article belongs to Authors. |
Keywords: | Cosmic rays; Galaxies, 'current; Dark matter; Detection experiments; Direct-detection; Independent scattering; Large regions; Parameter spaces; Scattering cross section, Dark Matter |
Department/Centre: | Division of Physical & Mathematical Sciences > Centre for High Energy Physics |
Date Deposited: | 01 Mar 2024 09:53 |
Last Modified: | 01 Mar 2024 09:53 |
URI: | https://eprints.iisc.ac.in/id/eprint/84153 |
Actions (login required)
View Item |