The NANOGrav 12.5-year data set: Search for Non-Einsteinian Polarization Modes in theGravitational-Wave Background
Zaven Arzoumanian, Paul T. Baker, Harsha Blumer, Bence Becsy, Adam, Brazier, Paul R. Brook, Sarah Burke-Spolaor, Maria Charisi, Shami Chatterjee,, Siyuan Chen, James M. Cordes, Neil J. Cornish, Fronefield Crawford, H., Thankful Cromartie, Megan E. DeCesar, Dallas M. DeGan

TL;DR
This study analyzes 12.5 years of NANOGrav data to search for non-Einsteinian polarization modes in the gravitational-wave background, finding no significant evidence but setting upper limits on their amplitudes.
Contribution
It provides the first constraints on scalar polarization modes in the gravitational-wave background using pulsar timing data.
Findings
No substantial evidence for non-Einsteinian polarization modes.
Scalar-transverse correlations are slightly favored but not statistically significant.
Upper limits are placed on polarization mode amplitudes for various metric theories.
Abstract
We search NANOGrav's 12.5-year data set for evidence of a gravitational wave background (GWB) with all the spatial correlations allowed by general metric theories of gravity. We find no substantial evidence in favor of the existence of such correlations in our data. We find that scalar-transverse (ST) correlations yield signal-to-noise ratios and Bayes factors that are higher than quadrupolar (tensor transverse, TT) correlations. Specifically, we find ST correlations with a signal-to-noise ratio of 2.8 that are preferred over TT correlations (Hellings and Downs correlations) with Bayesian odds of about 20:1. However, the significance of ST correlations is reduced dramatically when we include modeling of the Solar System ephemeris systematics and/or remove pulsar J00300451 entirely from consideration. Even taking the nominal signal-to-noise ratios at face value, analyses of simulated…
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Taxonomy
TopicsPulsars and Gravitational Waves Research · Cosmology and Gravitation Theories · Radio Astronomy Observations and Technology
