Search for Non-Tensorial Gravitational-Wave Backgrounds in the NANOGrav 15-Year Data Set

Abstract

The recent detection of a stochastic signal in the NANOGrav 15-year data set has aroused great interest in uncovering its origin. However, the evidence for the Hellings-Downs correlations, a key signature of the gravitational-wave background (GWB) predicted by general relativity, remains inconclusive. In this letter, we search for an isotropic non-tensorial GWB, allowed by general metric theories of gravity, in the NANOGrav 15-year data set. Our analysis reveals a Bayes factor of approximately 2.5, comparing the quadrupolar (tensor transverse, TT) correlations to the scalar transverse (ST) correlations, suggesting that the ST correlations provide a comparable explanation for the observed stochastic signal in the NANOGrav data. We obtain the median and the $90\%$ equal-tail amplitudes as ${\mathcal{A}}_{\mathrm{ST}}=7.8_{-3.5}^{+5.1}\times 10^{-15}$ at the frequency of 1/year. Furthermore, we find that the vector longitudinal (VL) and scalar longitudinal (SL) correlations are weakly and strongly disfavoured by data, respectively, yielding upper limits on the amplitudes: ${\mathcal{A}}_{\mathrm{VL}}^{95\%}\lesssim 1.7\times 10^{-15}$ and ${\mathcal{A}}_{\mathrm{SL}}^{95\%}\lesssim 7.4\times 10^{-17}$. Lastly, we fit the NANOGrav data with the general transverse (GT) correlations parameterized by a free parameter $\alpha$. Our analysis yields $\alpha =1.74_{-1.41}^{+1.18}$, thus excluding both the TT ($\alpha =3$) and ST ($\alpha =0$) models at the $90\%$ confidence level.

Comments: 9 pages, 4 figures, 3 tables; match the published version