Optimized statistical approach for comparing multi-messenger neutron star data

Carolyn A. Raithel, Feryal Özel, Dimitrios Psaltis

Research output: Contribution to journalArticlepeer-review

Abstract

The neutron star equation of state is now being constrained from a diverse set of multi-messenger data, including gravitational waves from binary neutron star mergers, X-ray observations of the neutron star radius, and many types of laboratory nuclear experiments. These measurements are often mapped to a common domain for comparison with one another or are used to constrain the predictions of theoretical equations of state. We explore here the statistical biases that can arise when such multi-messenger data are compared or combined across different domains. We find that placing Bayesian priors individually in each domain of measurement can lead to biased constraints. We present a new prescription for defining Bayesian priors consistently across different experiments, which will allow for robust cross-domain comparisons. Using the first two binary neutron star mergers as an example, we show that a uniform prior in the tidal deformability can produce inflated evidence for large radii, while a uniform prior in the radius points toward smaller radii. Finally, using this new prescription, we provide a status update on multi-messenger constraints on the neutron star radius.

Original languageEnglish (US)
Article number10pp
JournalAstrophysical Journal
Volume908
Issue number1
DOIs
StatePublished - Feb 10 2021

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint

Dive into the research topics of 'Optimized statistical approach for comparing multi-messenger neutron star data'. Together they form a unique fingerprint.

Cite this