Astrometric deflections from gravitational wave memory accumulation over cosmological scales

We study the impact of gravitational wave memory on the distribution of far away light sources in the sky. For the first time, we compute the buildup of small, but permanent tensor distortions of the metric over cosmological timescales using realistic models of compact binary coalescences whose rate of occurrence is extrapolated at $z\ensuremath{\sim}\mathcal{O}(1)$. This allows for a consistent computation of the random-walk-like evolution of gravitational wave memory which, in turn, is used to estimate the overall shape and magnitude of astrometric deflections of far away sources of light. We find that, for pulsar or quasar proper motions, the near-Earth contribution to the astrometric deflections dominates the result and the deflection is analogous to a stochastic gravitational wave memory background that is generally subdominant to the primary stochastic gravitational wave background. We find that this contribution can be within the reach of future surveys such as Theia. Finally, we also study the deviation of the presently observed angular distribution of quasars from perfect isotropy, which arises from the slow buildup of gravitational wave memory over the entire history of the Universe. In this case, we find that astrometric deflections depend on the entire light trajectory from the source to Earth, yielding a quadrupole pattern whose magnitude is unlikely to be within reach of the next generation of astrometric surveys due to shot noise and cosmic variance limitations.