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We develop a Bayesian analysis method for selecting the most probable equation of state under a set of constraints from compact star physics, which now include the tidal deformability from GW170817.
Static solutions of Einstein’s field equations for spheres of fluid
Tolman, R.C · 1939
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On Massive neutron cores
Oppenheimer, J.R.; Volkoff, G.M · 1939
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Equation of State at Supranuclear Densities and the Existence of a Third Family of Superdense Stars
Gerlach, U.H · 1968
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The Stability of a Star with a Phase Change in General Relativity Theory
Seidov, Z.F · 1971
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Nonidentical neutron star twins
Glendenning, N.K.; Kettner, C · 2000
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Relativistic mean-field models with effective hadron masses and coupling constants, and rho- condensation
Kolomeitsev, E.E.; Voskresensky, D.N · 2005
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The Equation of State from Observed Masses and Radii of Neutron Stars
Steiner, A.W.; Lattimer, J.M.; Brown, E.F · 2010
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Tidal deformability of neutron stars with realistic equations of state and their gravitational wave signatures in binary inspiral
Hinderer, T.; Lackey, B.D.; Lang, R.N.; Read, J.S · 2010
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Generic conditions for stable hybrid stars
Alford, M.G.; Han, S.; Prakash, M · 2013
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Proving the CEP with compact stars?
Alvarez-Castillo, D.E.; Blaschke, D · 2013
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Mass-radius constraints for compact stars and a critical endpoint
Blaschke, D.; Alvarez-Castillo, D.E.; Benic, S · 2013
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A Massive Pulsar in a Compact Relativistic Binary
Antoniadis, J.; others · 2013
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A new quark-hadron hybrid equation of state for astrophysics - I. High-mass twin compact stars
Benic, S.; Blaschke, D.; Alvarez-Castillo, D.E.; Fischer, T.; Typel, S · 2015
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High-mass twins & resolution of the reconfinement, masquerade and hyperon puzzles of compact star interiors
Blaschke, D.; Alvarez-Castillo, D.E · 2016
Cited alongside, same era.
Universal symmetry energy contribution to the neutron star equation of state 2016
Blaschke, D.; Alvarez-Castillo, D.E.; Klahn, T · 2016
Cited alongside, same era.
New class of hybrid EoS and Bayesian M-R data analysis
Alvarez-Castillo, D.; Ayriyan, A.; Benic, S.; Blaschke, D.; Grigorian, H.; Typel, S · 2016
Cited alongside, same era.
Relativistic Mean-Field Models with Scaled Hadron Masses and Couplings: Hyperons and Maximum Neutron Star Mass
Maslov, K.A.; Kolomeitsev, E.E.; Voskresensky, D.N · 2016
Cited alongside, same era.
High-mass twin stars with a multipolytrope equation of state
Alvarez-Castillo, D.E.; Blaschke, D.B · 2017
Cited alongside, same era.
Bayesian parameter constraints for neutron star masses and radii using X-ray timing observations of accretion-powered millisecond pulsars
Salmi, T.; Nättilä, J.; Poutanen, J · 2018
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Equation of state for dense nucleonic matter from metamodeling. II. Predictions for neutron star properties
Margueron, J.; Hoffmann Casali, R.; Gulminelli, F · 2018
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Third family of compact stars within a nonlocal chiral quark model equation of state 2018
Alvarez-Castillo, D.E.; Blaschke, D.B.; Grunfeld, A.G.; Pagura, V.P · 2018
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New constraints on radii and tidal deformabilities of neutron stars from GW170817
Most, E.R.; Weih, L.R.; Rezzolla, L.; Schaffner-Bielich, J · 2018
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Constraining twin stars with GW170817 2018
Montana, G.; Tolos, L.; Hanauske, M.; Rezzolla, L · 2018
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Abbott, B.; others · 2017
Cited alongside, same era.
Neutron-star radius constraints from GW170817 and future detections
Bauswein, A.; Just, O.; Janka, H.T.; Stergioulas, N · 2017
Cited alongside, same era.
From Neutron Star Observables to the Equation of State. II. Bayesian Inference of Equation of State Pressures
Raithel, C.A.; Özel, F.; Psaltis, D · 2017
Cited alongside, same era.
Quark-nuclear hybrid star equation of state with excluded volume effects
Kaltenborn, M.A.R.; Bastian, N.U.F.; Blaschke, D.B · 2017
Cited alongside, same era.
Implications from GW170817 and I-Love-Q relations for relativistic hybrid stars
Paschalidis, V.; Yagi, K.; Alvarez-Castillo, D.; Blaschke, D.B.; Sedrakian, A · 2018
Cited alongside, same era.
Gravitational-wave constraints on the neutron-star-matter Equation of State
Annala, E.; Gorda, T.; Kurkela, A.; Vuorinen, A · 2018
Cited alongside, same era.
Using gravitational-wave observations and quasi-universal relations to constrain the maximum mass of neutron stars
Rezzolla, L.; Most, E.R.; Weih, L.R · 2018
Cited alongside, same era.
Tidal deformability and other global parameters of compact stars with phase transitions 2018
Sieniawska, M.; Turczanski, W.; Bejger, M.; Zdunik, J.L · 2018
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Robustness of third family solutions for hybrid stars against mixed phase effects
Ayriyan, A.; Bastian, N.U.; Blaschke, D.; Grigorian, H.; Maslov, K.; Voskresensky, D.N · 2018
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Model of the Phase Transition Mimicking the Pasta Phase in Cold and Dense Quark-Hadron Matter
Ayriyan, A.; Grigorian, H · 2018
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Two Novel Approaches to the Hadron-Quark Mixed Phase in Compact Stars
Abgaryan, V.; Alvarez-Castillo, D.; Ayriyan, A.; Blaschke, D.; Grigorian, H · 2018
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Hybrid equation of state with pasta phases and third family of compact stars I: Pasta phases and effective mixed phase model 2018
Maslov, K.; Yasutake, N.; Ayriyan, A.; Blaschke, D.; Grigorian, H.; Maruyama, T.; Tatsumi, T.; Voskresensky, D.N · 2018
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GW170817: Measurements of neutron star radii and equation of state
Abbott, B.P.; others · 2018
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GW170817: Measurements of neutron star radii and equation of state
LIGO Scientific Collaboration and Virgo Collaboration · 2018
Closest in time.
Signals in the tidal deformability for phase transitions in compact stars with constraints from GW170817
Christian, J.E.; Zacchi, A.; Schaffner-Bielich, J · 2019
Closest in time.