{ "id": "2107.07979", "version": "v1", "published": "2021-07-16T15:50:13.000Z", "updated": "2021-07-16T15:50:13.000Z", "title": "On the moment of inertia of PSR J0737-3039 A from LIGO/Virgo and NICER", "authors": [ "Zhiqiang Miao", "Ang Li" ], "comment": "9 pages, 5 figures, 2 tables", "categories": [ "astro-ph.HE", "astro-ph.SR", "nucl-th" ], "abstract": "We extend our previous study (Li et al. 2021) on neutron stars with a quark core to predict the moment of inertia of pulsar A in the double pulsar binary J0737-3039, assuming there is a phase transition in the pulsar inner core from the soft QMF or the stiff DD2 hadronic equation of state (EOS) to a high-density phase of quark matter modelled by the generic \"constant-sound-speed\" (CSS) parameterization. We perform a Bayesian analysis of the moment of inertia by incorporating observational data for the tidal deformability of the GW170817 and GW190425 binary neutron star mergers, as detected by LIGO/Virgo, and the mass and radius of PSR J0030+0451 and MSP J0740+6620, as detected by the Neutron Star Interior Composition Explorer. We find that the most probable values of the moment of inertia of PSR J0737-3039 A are $1.27_{-0.14}^{+0.18}\\times10^{45}\\,{\\rm g\\,cm^2}$ for QMF+CSS and similarly $1.29_{-0.15}^{+0.26}\\times10^{45}\\,{\\rm g\\,cm^2}$ for DD2+CSS at $90\\%$ credible interval. We also demonstrate how a moment of inertia measurement would improve our knowledge of the EOS and the mass-radius relation for hybrid stars and discuss whether a quark deconfinement phase transition is supported by the available data and forthcoming data that could be consistent with this hypothesis.", "revisions": [ { "version": "v1", "updated": "2021-07-16T15:50:13.000Z" } ], "analyses": { "keywords": [ "neutron star interior composition explorer", "ligo/virgo", "gw190425 binary neutron star mergers", "quark deconfinement phase transition", "stiff dd2 hadronic equation" ], "note": { "typesetting": "TeX", "pages": 9, "language": "en", "license": "arXiv", "status": "editable" } } }