2024/09/21 by James M. Cline, Cline, James M. · 2 voices
Computer Science · Physics and Astronomy · Earth and Planetary Sciences · #Computational Physics and Python Applications #Scientific Research and Discoveries #Geophysics and Gravity Measurements
paper · pdf · doi:10.48550/arxiv.2409.13692
It was recently claimed (arXiv:2405.05410 [gr-qc]) that evidence for a stochastic gravitational wave background observed by pulsar timing arrays can be attributed instead to random perturbations of the Sun's motion by transiting asteroids. I show that that this would lead to a large dipole component accompanying a much smaller quadrupolar perturbation of pulsar timing signals, which would not be confused with a gravitational wave signal. Such an anomalous dipole would have been detected and identified as a spurious background by the PTA collaborations, if it existed.