Relativistic hybrid stars with sequential first-order phase transitions in light of multimessenger constraints
arXiv:2301.10940 · doi:10.3847/1538-4357/acb688
Abstract
In this work, we consider the properties of compact stars in which quark matter has low- and high-density phases that are separated by a first-order phase transition. Thus, unlike the commonly considered case of a single phase transition from hadronic to quark matter, our models of hybrid stars contain sequential phase transitions from hadronic matter to low- and then to high-density quark matter phases. We extend our previous study of the parameter space of hybrid stars with a single phase transition to those with sequential phase transitions, taking into account the constraints on the mass and radius of neutron stars from the NICER experiment, the experimental inferences of the neutron skin thickness of the lead nucleus by the PREX-II experiment, and constraints on the tidal deformability from the gravitational-wave event GW170817. We determine the range of the masses for which both twin and triplet configurations, i.e., identical-mass stars with two and three different values of radii, arise.
v2: matches published version, 11 pages, 11 figures
References in corpus (17)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- GW190814: Gravitational Waves from the Coalescence of a 23 M Black Hole with a 2.6 M Compact Object
- 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
- Color superconductivity in dense quark matter
- Impact of the PSR J0740+6620 radius constraint on the properties of high-density matter
- Compact stars with sequential QCD phase transitions
- Confronting GW190814 with hyperonization in dense matter and hypernuclear compact stars
- Quark-nuclear hybrid equation of state for neutron stars under modern observational constraints
- Delta baryons and diquark formation in the cores of neutron stars
- Constraints on the phase transition and nuclear symmetry parameters from PSR and multimessenger data of other neutron stars
- The Radius of PSR J0740+6620 from NICER and XMM-Newton Data
- Holographic QCD in the NICER era
- QCD phase transition drives supernova explosion of a very massive star
- Impact of slow conversions on hybrid stars with sequential QCD phase transitions
- Strong first-order phase transition in a rotating neutron star core and the associated energy release
- Energy release from hadron-quark phase transition in neutron stars and the axial -mode of gravitational waves
Cited by in corpus (17)
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- New covariant density functionals of nuclear matter for compact star simulations
- Universal relations for compact stars with exotic degrees of freedom
- Impact of the nuclear equation of state on the formation of twin stars
- Confronting new NICER mass-radius measurements with phase transition in dense matter and twin compact stars
- Hybrid stars with large quark cores within the parity doublet model and modified NJL model
- Comprehensive Analysis of Constructing Hybrid Stars with an RG-consistent NJL Model
- Higgs-Confinement Transitions in QCD from Symmetry Protected Topological Phases
- Analyzing the dense matter equation of states in the light of the compact object HESS J1731-347
- Observational Probes of the Neutron Star Equation of State with Hyperons, Bosonic Dark Matter, and Quark Matter
- Confronting recent light compact star observations with color-flavor locked quark matter
- How Neutron Star Observations Point Towards Exotic Matter: Existing Explanations and a Prospective Proposal
- The mixed phase quark core in massive hybrid stars
- Constraining the competition between the deconfinement and chiral phase transitions in light of the multimessenger era
- Scalarized Hybrid Neutron Stars in Scalar Tensor Gravity
- Investigating Universal Relations in Compact Stars featuring Admixed Exotic Dense Matter