A unified spin-harmonic framework for correlating pulsar timing, astrometric deflection, and shimmering gravitational wave observations

Mentasti, Giorgio; Contaldi, Carlo

doi:10.48550/arXiv.2507.16906

OA Location

https://doi.org/10.48550/arXiv.2507.16906

Author(s)

Mentasti, Giorgio

Contaldi, Carlo

Type

preprint

Abstract

We present a unified spin-weighted harmonic framework that delivers analytic, diagonal expressions for the overlap (correlation) functions of three low frequency gravitational wave observables-pulsar timing redshifts, astrometric deflections, and time-dependent image distortions (``shimmering''). Writing each response in spin-s spherical harmonics and rotating to a basis in which the wave tensor has definite helicity, we obtain compact closed-form series for every auto- and cross-correlation, recovering the Hellings-Downs curve as the s = 0 limit and deriving its astrometric (s = 1) and shimmering ( ) analogues. The formalism naturally extends to non-standard scalar-breathing, longitudinal, and vector polarisation modes, clarifying when higher-spin observables are (and are not) sourced and providing a complete set of harmonic spectra ready for parameter estimation pipelines. These results supply the common theoretical language needed to combine upcoming pulsar timing, Gaia-class astrometric, and high resolution imaging data sets, enabling coherent, multi probe searches for stochastic gravitational wave backgrounds, tests of general relativity and its alternatives across the nano- to micro-hertz gravitational wave band.