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A Search for Axionic Dark Matter Using the Magnetar PSR J1745-2900
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A Search for Axionic Dark Matter Using the Magnetar PSR J1745-2900
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We report on a search for dark matter axion conversion photons from the magnetosphere of the Galactic Center magnetar PSR J1745-2900 using spectra obtained from the Karl G. Jansky Very Large Array. No significant spectral features are detected. Using a hybrid model for PSR J1745-2900 and canonical assumptions about the dark matter density profile, we exclude axion models with axion-photon coupling $g_{a\gamma\gamma}$ > 6-34 x 10$^{-12}$ GeV$^{-1}$ with 95% confidence over the mass ranges 4.2-8.4, 18.6-26.9, 33.0-41.4, 53.7-62.1, and 126.0-159.3 $\mu$eV. If there is a dark matter cusp, the limits reduce to $g_{a\gamma\gamma}$ > 6-34 x 10$^{-14}$ GeV$^{-1}$, which overlap some axion models for the observed mass ranges > 33 $\mu$eV. These limits may be improved by modeling the stimulated emission that can boost the axion-photon conversion process.
Forward citations
Cited by 3 Pith papers
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Constraining meV Axion Dark Matter with ALMA Observations of the Galactic Center Magnetar SGR 1745-2900
ALMA observations of the magnetar SGR 1745-2900 exclude axion-photon couplings down to ~2e-13 GeV^-1 in the 0.55-0.62 meV mass range, reaching the QCD axion window under a dark-matter spike model.
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Galactic Centre Pulsars with the SKAO
Updated SKA-MID sensitivity and multi-beam search strategies can detect up to ~84% of Galactic Centre pulsars (and ~60% of MSPs) under magnetar-like scattering, unlocking precision tests around Sgr A*.
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DALI sensitivity to streaming axion dark matter
DALI has sensitivity to axion streams spanning two decades in mass that matches photon coupling strengths of representative axion models.
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