Detecting Axion-like Dark Matter with Linearly Polarized Pulsar Light
arXiv:1901.10981 · doi:10.1103/PhysRevD.101.063012
Abstract
Non-relativistic QCD axions or axion-like particles are among the most popular candidates for cold Dark Matter (DM) in the universe. We proposed to detect axion-like DM, using linearly polarized pulsar light as a probe. Because of birefringence effect potentially caused by an oscillating galactic axion DM background, when pulsar light travels across the galaxy, its linear polarization angle may vary with time. With a soliton+NFW galactic DM density profile, we show that this strategy can potentially probe an axion-photon coupling as small as GeV for axion mass eV, given the current measurement accuracy. An exclusion limit stronger than CAST ( GeV) and SN1987A ( GeV) could be extended up to eV and eV, respectively.
6 pages, 1 figure; calculation corrected, main conclusions unchanged, references added
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