Dark matter astrometry at underground detectors with multiscatter events
Abstract
We show that current and imminent underground detectors are capable of precision astrometry of dark matter. First, we show that Galactic dark matter velocity distributions can be obtained from reconstructed tracks of dark matter scattering on multiple nuclei during transit; using the liquid scintillator neutrino detector as an example, we find that the dark matter velocity vector can be reconstructed event by event with such a small uncertainty that the precision of dark matter astrometry will be limited mainly by statistics. We then determine the number of dark matter events required to determine the dispersion speed, escape speed, and velocity anisotropies of the local dark matter halo and also find that with as few as events dark matter signals may be discriminated from potential backgrounds arising as power-law distributions. Finally, we discuss the prospects of dark matter astrometry at other liquid scintillator detectors, dark matter experiments, and the recently proposed MATHUSLA detector.
- Authors:
- Publication Date:
- Research Org.:
- Univ. of Hawaii, Honolulu, HI (United States). High Energy Physics Group
- Sponsoring Org.:
- USDOE Office of Science (SC), High Energy Physics (HEP); National Science Foundation (NSF); Natural Sciences and Engineering Research Council of Canada (NSERC); National Research Council Canada
- OSTI Identifier:
- 1579587
- Alternate Identifier(s):
- OSTI ID: 1597498; OSTI ID: 1780921
- Grant/Contract Number:
- SC0010504; PHY-1607611
- Resource Type:
- Published Article
- Journal Name:
- Physical Review. D.
- Additional Journal Information:
- Journal Name: Physical Review. D. Journal Volume: 100 Journal Issue: 12; Journal ID: ISSN 2470-0010
- Publisher:
- American Physical Society (APS)
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
Citation Formats
Bramante, Joseph, Kumar, Jason, and Raj, Nirmal. Dark matter astrometry at underground detectors with multiscatter events. United States: N. p., 2019.
Web. doi:10.1103/PhysRevD.100.123016.
Bramante, Joseph, Kumar, Jason, & Raj, Nirmal. Dark matter astrometry at underground detectors with multiscatter events. United States. https://doi.org/10.1103/PhysRevD.100.123016
Bramante, Joseph, Kumar, Jason, and Raj, Nirmal. Tue .
"Dark matter astrometry at underground detectors with multiscatter events". United States. https://doi.org/10.1103/PhysRevD.100.123016.
@article{osti_1579587,
title = {Dark matter astrometry at underground detectors with multiscatter events},
author = {Bramante, Joseph and Kumar, Jason and Raj, Nirmal},
abstractNote = {We show that current and imminent underground detectors are capable of precision astrometry of dark matter. First, we show that Galactic dark matter velocity distributions can be obtained from reconstructed tracks of dark matter scattering on multiple nuclei during transit; using the liquid scintillator neutrino detector SNO+ as an example, we find that the dark matter velocity vector can be reconstructed event by event with such a small uncertainty that the precision of dark matter astrometry will be limited mainly by statistics. We then determine the number of dark matter events required to determine the dispersion speed, escape speed, and velocity anisotropies of the local dark matter halo and also find that with as few as O(10) events dark matter signals may be discriminated from potential backgrounds arising as power-law distributions. Finally, we discuss the prospects of dark matter astrometry at other liquid scintillator detectors, dark matter experiments, and the recently proposed MATHUSLA detector.},
doi = {10.1103/PhysRevD.100.123016},
journal = {Physical Review. D.},
number = 12,
volume = 100,
place = {United States},
year = {Tue Dec 17 00:00:00 EST 2019},
month = {Tue Dec 17 00:00:00 EST 2019}
}
https://doi.org/10.1103/PhysRevD.100.123016
Web of Science
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