Do Pulsar Timing Datasets Favor Massive Gravity?

TL;DR

This paper investigates how massive gravity theories affect gravitational wave propagation and pulsar timing array observations, finding that massive GWs fit current data better and could be constrained further with future measurements.

Contribution

It analyzes the impact of massive gravity on GW signals and pulsar timing data, providing new insights into graviton mass constraints from PTA observations.

Findings

Massive GWs improve fit to pulsar timing data.

Future PTA data could detect additional polarization modes.

PTA observations can constrain graviton mass effectively.

Abstract

Several observational phenomena suggest that the standard model of cosmology and particle physics requires revision. To address this, we consider the extension of general relativity known as massive gravity (MG). In this Letter, we explore the imprints of MG on the propagation of gravitational waves (GWs): their modified dispersion relation and their additional (two vector and one scalar) polarization modes on the stochastic GW background (SGWB) detected by pulsar timing arrays (PTAs). We analyze the effects of massive GWs on the Hellings-Downs curve induced by modification of the overlap reduction function. Our study consists of analyzing observational data from the NANOGrav 15-year dataset and the Chinese PTA Data Release I, and is independent of the origin of the SGWB (astrophysical or cosmological). By considering the bound on the graviton mass imposed through the dispersion relation, we scrutinize the possibility of detecting traces of MG in the PTA observational data. We find that massive GWs predict better fits for the observed pulsar correlations. Future PTA missions with more precise data will hopefully be able to detect the GW additional polarization modes and might be effectively used to constrain the graviton mass.