@article{54f7c1a359164d7c9f329ad082670ee0,
title = "Extending the discovery potential for inelastic-dipole dark matter with FASER",
abstract = "Neutral particles are notoriously difficult to observe through electromagnetic interactions. As a result, they naturally elude detection in most collider detectors. In this paper, we point out that neutral particles that interact through a dipole interaction can nevertheless be detected in far-forward detectors designed to search for long-lived particles (LLPs). In contrast to previous analyses that focused on neutral particles with elastic interactions, we consider inelastic interactions. This naturally leads to LLPs, and we demonstrate that FASER (and future experiments at the Forward Physics Facility) will be able to probe substantial regions of the associated parameter space. In particular, we find that FASER is capable of probing the region of parameter space wherein thermal freeze-out gives rise to an O(GeV) dark-matter candidate with the appropriate relic abundance, as well as regions of parameter space that are difficult to probe at fixed-target experiments. FASER and its successor experiments may therefore play a critical role in the discovery of such a dark-matter candidate.",
author = "Dienes, {Keith R.} and Feng, {Jonathan L.} and Max Fieg and Fei Huang and Lee, {Seung J.} and Brooks Thomas",
note = "Funding Information: We thank Daniele Barducci, Enrico Bertuzzo, David Casper, Xiaoyong Chu, Patrick deNiverville, Andrei Golutvin, Felix Kling, Dominik K{\"o}hler, Jui-Lin Kuo, Gopolang Mohlabeng, Marco Taoso, Claudio Toni, and Sebastian Trojanowski for discussions. The research activities of K. R. D. were supported in part by the U.S. Department of Energy under Grant DE-FG02-13ER41976/DE-SC0009913, and by the U.S. National Science Foundation (NSF) through its employee IR/D program. The work of J. L. F., M. F., and F. H. was supported in part by NSF Grants PHY-1915005 and PHY-2210283. The work of J. L. F. was also supported in part by NSF Grant PHY-2111427, Simons Investigator Award No. 376204, Simons Foundation Grant 623683, and Heising-Simons Foundation Grants No. 2019-1179 and No. 2020-1840. The work of M. F. was also supported in part by NSF Graduate Research Fellowship Award No. DGE-1839285. The work of F. H. was also supported in part by the International Postdoctoral Exchange Fellowship Program. The research activities of S. L. were supported in part by the National Research Foundation of Korea (NRF) grant funded by the Korean government (MEST) (No. NRF-2021R1A2C1005615) and the Samsung Science & Technology Foundation under Project Number SSTF-BA2201-06. The research activities of B. T. were supported in part by the National Science Foundation under Grant PHY-2014104. The opinions and conclusions expressed herein are those of the authors and do not represent any funding agencies. Publisher Copyright: {\textcopyright} 2023 authors. Published by the American Physical Society.",
year = "2023",
month = jun,
day = "1",
doi = "10.1103/PhysRevD.107.115006",
language = "English (US)",
volume = "107",
journal = "Physical Review D",
issn = "2470-0010",
publisher = "American Physical Society",
number = "11",
}