Pulsar Timing Noise from Brownian Motion of the Sun

Abstract

Recently, pulsar timing arrays (PTAs) reported a signal at nanohertz frequencies consistent with a stochastic gravitational-wave background. Here, I show that the Brownian motion of the Sun as a result of its random gravitational interactions with the cluster of thousands of unmodeled main-belt asteroids of diameters ≲80 km, combined with small inaccuracies in the estimated masses of larger asteroids, introduces timing noise for pulsars, which is up to 20% of the reported signal at frequencies of ∼1 few years ^–1 . The asteroid contribution needs to be modeled better in order to obtain accurate inferences from the PTA signal.

Keywords

• Asteroid belt
• Gravitational wave astronomy