Was GW170817 a canonical neutron star merger? Bayesian analysis with a third family of compact stars

Abstract

We investigate the possibility that GW170817 has not been the merger of two conventional neutron stars (NS) but involved at least one if not two hybrid stars with a quark matter core which might even belong to a third family of compact stars. To this end, we develop a Bayesian analysis method for selecting the most probable equation of state (EoS) under a set of constraints from compact star physics, which now also include the tidal deformability from GW170817 and the first result for the mass and radius determination for PSR J0030+0451 by NICER. We apply this method for the first time to a two-parameter family of hybrid EoS based on the DD2 model with nucleonic excluded volume for hadronic matter and the color superconducting generalized nlNJL model for quark matter. The model has a variable onset of deconfinement and can mimic the effects of pasta phases with the possibility of a third family of hybrid stars in the mass-radius ($M-R$) diagram. The main findings of this study are that: 1) the presence of multiple configurations for a given mass (twins) corresponds to a set of disconnected lines in the diagram of tidal deformabilities for binary mergers, so that merger events from the same mass range may result in a probability landscape with different peak positions; 2) the Bayesian analysis with the above observational constraints favors an early onset of the deconfinement transition, at masses of $M_{\mathrm{onset}}\le 0.8M_{\odot }$ with a $M-R$ relationship that in the range of observed neutron star masses is almost indistinguishable from that of a soft hadronic APR EoS; 3) a few yet fictitious measurements of the NICER experiment with a $1\sigma$ range that is half of the present value and different mass and radius would change the posterior likelihood so that hybrid EoS with a phase transition onset in the range $M_{\mathrm{onset}}=1.1-1.6M_{\odot }$ would be favored.

22 pages, 11 figures

References in corpus (19)

• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Shapiro delay measurement of a two solar mass neutron star
• A Massive Pulsar in a Compact Relativistic Binary
• PSR J0030+0451 Mass and Radius from NICER Data and Implications for the Properties of Neutron Star Matter
• A NICER View of PSR J0030+0451: Millisecond Pulsar Parameter Estimation
• Tidal Love numbers of neutron stars
• Hyperon Puzzle: Hints from Quantum Monte Carlo Calculations
• A new quark-hadron hybrid equation of state for astrophysics - I. High-mass twin compact stars
• Reconstructing the neutron-star equation of state with gravitational-wave detectors from a realistic population of inspiralling binary neutron stars
• Neutron star mass and radius measurements from atmospheric model fits to X-ray burst cooling tail spectra
• Inner crust of neutron stars with mass-fitted Skyrme functionals
• Analytical representations of unified equations of state of neutron-star matter
• Compact stars with sequential QCD phase transitions
• Confronting gravitational-wave observations with modern nuclear physics constraints
• Studying strong phase transitions in neutron stars with gravitational waves
• Hybrid stars within a covariant, nonlocal chiral quark model
• Consequences of a strong phase transition in the dense matter equation of state for the rotational evolution of neutron stars
• Special point on the mass radius diagram of hybrid stars
• Hybrid neutron stars based on a modified PNJL model

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• Constraints on the dense matter equation of state and neutron star properties from NICER's mass-radius estimate of PSR J0740+6620 and multimessenger observations
• Variation of delta baryon mass and hybrid star properties in static and rotating conditions
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