Cross-correlating pulsar timing and polarimetry isolates the circular polarization of isotropic stochastic GW backgrounds and shares the Hellings-Downs angular pattern.
Title resolution pending
2 Pith papers cite this work. Polarity classification is still indexing.
2
Pith papers citing it
verdicts
UNVERDICTED 2representative citing papers
No axion conversion lines detected from two X-ray dim isolated neutron stars with FAST, setting g_aγγ ≲ 5×10^{-12} GeV^{-1} for masses 4.14-6.20 μeV, the tightest ACL-method constraint in this range.
citing papers explorer
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Detecting Parity-Violating Gravitational Wave Backgrounds with Pulsar Polarization Arrays
Cross-correlating pulsar timing and polarimetry isolates the circular polarization of isotropic stochastic GW backgrounds and shares the Hellings-Downs angular pattern.
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Searching for axion dark matter conversion spectral lines in neutron star magnetospheres with FAST
No axion conversion lines detected from two X-ray dim isolated neutron stars with FAST, setting g_aγγ ≲ 5×10^{-12} GeV^{-1} for masses 4.14-6.20 μeV, the tightest ACL-method constraint in this range.