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Title: Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres

Abstract

We show that axion dark matter may be detectable through narrow radio lines emitted from neutron stars. Neutron star magnetospheres host both a strong magnetic field and a plasma frequency that increases towards the neutron star surface. As the axions pass through the magnetosphere, they can resonantly convert into radio photons when the plasma frequency matches the axion mass. We solve the axion-photon mixing equations, including a full treatment of the magnetized plasma, to obtain the conversion probability. We discuss possible neutron star targets and how they may probe the QCD-axion parameter space in the mass range of ~ 0.2–40 μeV.

Authors:
; ; ;
Publication Date:
Research Org.:
Univ. of Michigan, Ann Arbor, MI (United States)
Sponsoring Org.:
USDOE Office of Science (SC)
OSTI Identifier:
1485744
Alternate Identifier(s):
OSTI ID: 1613150
Grant/Contract Number:  
de-sc0019225; SC0019225
Resource Type:
Published Article
Journal Name:
Physical Review Letters
Additional Journal Information:
Journal Name: Physical Review Letters Journal Volume: 121 Journal Issue: 24; Journal ID: ISSN 0031-9007
Publisher:
American Physical Society
Country of Publication:
United States
Language:
English
Subject:
79 ASTRONOMY AND ASTROPHYSICS; Physics; Dark matter; Radio, microwave, & sub-mm astronomy; Axions; Neutron stars & pulsars

Citation Formats

Hook, Anson, Kahn, Yonatan, Safdi, Benjamin R., and Sun, Zhiquan. Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres. United States: N. p., 2018. Web. doi:10.1103/PhysRevLett.121.241102.
Hook, Anson, Kahn, Yonatan, Safdi, Benjamin R., & Sun, Zhiquan. Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres. United States. https://doi.org/10.1103/PhysRevLett.121.241102
Hook, Anson, Kahn, Yonatan, Safdi, Benjamin R., and Sun, Zhiquan. Thu . "Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres". United States. https://doi.org/10.1103/PhysRevLett.121.241102.
@article{osti_1485744,
title = {Radio Signals from Axion Dark Matter Conversion in Neutron Star Magnetospheres},
author = {Hook, Anson and Kahn, Yonatan and Safdi, Benjamin R. and Sun, Zhiquan},
abstractNote = {We show that axion dark matter may be detectable through narrow radio lines emitted from neutron stars. Neutron star magnetospheres host both a strong magnetic field and a plasma frequency that increases towards the neutron star surface. As the axions pass through the magnetosphere, they can resonantly convert into radio photons when the plasma frequency matches the axion mass. We solve the axion-photon mixing equations, including a full treatment of the magnetized plasma, to obtain the conversion probability. We discuss possible neutron star targets and how they may probe the QCD-axion parameter space in the mass range of ~ 0.2–40 μeV.},
doi = {10.1103/PhysRevLett.121.241102},
journal = {Physical Review Letters},
number = 24,
volume = 121,
place = {United States},
year = {Thu Dec 13 00:00:00 EST 2018},
month = {Thu Dec 13 00:00:00 EST 2018}
}

Journal Article:
Free Publicly Available Full Text
Publisher's Version of Record
https://doi.org/10.1103/PhysRevLett.121.241102

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Cited by: 97 works
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