Production and Detection of an Axion Dark Matter Echo
Abstract
Electromagnetic radiation with angular frequency equal to half the axion mass stimulates the decay of cold dark matter axions and produces an echo, i.e., faint electromagnetic radiation traveling in the opposite direction. We propose to search for axion dark matter by sending out to space a powerful beam of microwave radiation and listening for its echo. We estimate the sensitivity of this technique in the isothermal and caustic ring models of the Milky Way halo and find it to be a promising approach to axion, or axionlike, dark matter detection.
- Authors:
- Publication Date:
- Research Org.:
- Univ. of Florida, Gainesville, FL (United States)
- Sponsoring Org.:
- USDOE Office of Science (SC)
- OSTI Identifier:
- 1566936
- Alternate Identifier(s):
- OSTI ID: 1611380
- Grant/Contract Number:
- SC0010296
- Resource Type:
- Published Article
- Journal Name:
- Physical Review Letters
- Additional Journal Information:
- Journal Name: Physical Review Letters Journal Volume: 123 Journal Issue: 13; Journal ID: ISSN 0031-9007
- Publisher:
- American Physical Society
- Country of Publication:
- United States
- Language:
- English
- Subject:
- 79 ASTRONOMY AND ASTROPHYSICS; Physics; Axions; Particle astrophysics; Particle dark matter
Citation Formats
Arza, Ariel, and Sikivie, Pierre. Production and Detection of an Axion Dark Matter Echo. United States: N. p., 2019.
Web. doi:10.1103/PhysRevLett.123.131804.
Arza, Ariel, & Sikivie, Pierre. Production and Detection of an Axion Dark Matter Echo. United States. https://doi.org/10.1103/PhysRevLett.123.131804
Arza, Ariel, and Sikivie, Pierre. Fri .
"Production and Detection of an Axion Dark Matter Echo". United States. https://doi.org/10.1103/PhysRevLett.123.131804.
@article{osti_1566936,
title = {Production and Detection of an Axion Dark Matter Echo},
author = {Arza, Ariel and Sikivie, Pierre},
abstractNote = {Electromagnetic radiation with angular frequency equal to half the axion mass stimulates the decay of cold dark matter axions and produces an echo, i.e., faint electromagnetic radiation traveling in the opposite direction. We propose to search for axion dark matter by sending out to space a powerful beam of microwave radiation and listening for its echo. We estimate the sensitivity of this technique in the isothermal and caustic ring models of the Milky Way halo and find it to be a promising approach to axion, or axionlike, dark matter detection.},
doi = {10.1103/PhysRevLett.123.131804},
journal = {Physical Review Letters},
number = 13,
volume = 123,
place = {United States},
year = {2019},
month = {9}
}
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https://doi.org/10.1103/PhysRevLett.123.131804
https://doi.org/10.1103/PhysRevLett.123.131804
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Cited by: 3 works
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