Joint SKA PTA and astrometry analysis improves gravitational wave background detection sensitivity by 10-50%.
Astrophysical Sources of Stochastic Gravitational-Wave Background
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abstract
We review the spectral properties of stochastic backgrounds of astrophysical origin and discuss how they may differ from the primordial contribution by their statistical properties. We show that stochastic searches with the next generation of terrestrial interferometers could put interesting constrains on the physical properties of astrophysical populations, such as the ellipticity and magnetic field of magnetars, or the coalescence rate of compact binaries.
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astro-ph.IM 1years
2026 1verdicts
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Synergies Between Pulsar Timing Array and Astrometry
Joint SKA PTA and astrometry analysis improves gravitational wave background detection sensitivity by 10-50%.