New Constraints on Macroscopic Dark Matter Using Radar Meteor Detectors
Pawan Dhakal, Steven Prohira, Christopher V. Cappiello, John F. Beacom, Scott Palo, John Marino
· Physical Review D 107, 043026
Plain-language summary
Macroscopic dark matter candidates — hypothetical massive particles that interact with ordinary matter — would leave ionisation trails in Earth's upper atmosphere similar to the trails left by meteors. This paper shows that radar systems designed to detect meteors can also search for these dark matter candidates. It is a novel application of existing observational infrastructure, directly relevant to HICS's meteor radar programme.
Cite
APA
Pawan Dhakal, Steven Prohira, Christopher V. Cappiello, John F. Beacom, Scott Palo, John Marino. (2023). New Constraints on Macroscopic Dark Matter Using Radar Meteor Detectors. Physical Review D 107, 043026. https://doi.org/10.1103/PhysRevD.107.043026
BibTeX
@article{HICS2023_1,
author = {Pawan Dhakal, Steven Prohira, Christopher V. Cappiello, John F. Beacom, Scott Palo, John Marino},
title = {New Constraints on Macroscopic Dark Matter Using Radar Meteor Detectors},
journal = {Physical Review D 107, 043026},
year = {2023},
doi = {10.1103/PhysRevD.107.043026},
url = {https://doi.org/10.1103/PhysRevD.107.043026},
}