The impact of hyperons on neutron star mergers: gravitational waves, mass ejection and black hole formation
arXiv:2501.12905 · doi:10.1103/vrnr-lf6k
Abstract
We study the influence of hyperons in binary neutron star (NS) mergers considering a total of 14 temperature dependent equations of state (EoSs) models which include hyperonic degrees of freedom and partly delta resonances. Thermally produced hyperons induce a higher heat capacity and a lower thermal index, i.e. a reduced thermal pressure for a given amount of thermal energy, compared to purely nucleonic models. We run a large set of relativistic hydrodynamics simulations of NS mergers to explore the impact on observables of these events. In symmetric binaries, we describe a characteristic increase of the dominant postmerger gravitational-wave (GW) frequency by a few per cent, which is specifically linked to the occurrence of hyperons and can thus be potentially used as a discriminator between purely nucleonic and hyperonic systems. We corroborate that this effect occurs similarly for asymmetric binaries and becomes more prominent with increasing total binary mass. Hyperonic models tend to stick out in relations between the dominant postmerger GW frequency and the tidal deformability of massive stars providing a signature to identify the presence of hyperons. Distinct secondary postmerger GW spectral features are differently affected by the presence of hyperons, in the sense that one feature exhibits a characteristic frequency shift due to the specific thermal properties of hyperonic EoSs while the other does not. The dynamical mass ejection of mergers is tentatively enhanced for hyperonic models in comparison to nucleonic EoSs which yield roughly the same stellar properties of cold NSs. This may serve useful to identify exotic degrees of freedom in these systems by kilonova observations. Also, for hyperonic EoSs the threshold mass for prompt black hole formation is reduced by about 0.05 in comparison to nucleonic systems with the same stellar parameters of cold NSs.
31 pages, 28 figures, accepted for publication in PRD
References in corpus (59)
- 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
- Multi-messenger Observations of a Binary Neutron Star Merger
- Neutron Star Observations: Prognosis for Equation of State Constraints
- Exploring the Sensitivity of Next Generation Gravitational Wave Detectors
- PSR J0952-0607: The Fastest and Heaviest Known Galactic Neutron Star
- Neutron-star radius constraints from GW170817 and future detections
- Kilonovae
- Hyperon Puzzle: Hints from Quantum Monte Carlo Calculations
- Spectral properties of the post-merger gravitational-wave signal from binary neutron stars
- Neutron Stars and the Nuclear Equation of State
- Relativistic neutron star merger simulations with non-zero temperature equations of state I. Variation of binary parameters and equation of state
- Merger and Mass Ejection of Neutron-Star Binaries
- New Hyperon Equations of State for Supernovae and Neutron Stars in Density-dependent Hadron Field Theory
- Testing Approximations of Thermal Effects in Neutron Star Merger Simulations
- Strangeness in Nuclei and Neutron Stars
- The Dynamics of Binary Neutron Star Mergers and of GW170817
- Nuclear equation of state for core-collapse supernova simulations with realistic nuclear forces
- Estimation of the effect of hyperonic three-body forces on the maximum mass of neutron stars
- Hyperon mixing and universal many-body repulsion in neutron stars
- The electromagnetic counterparts of compact binary mergers
- A General-relativistic Determination of the Threshold Mass to Prompt Collapse in Binary Neutron Star Mergers
- A New Open-Source Nuclear Equation of State Framework based on the Liquid-Drop Model with Skyrme Interaction
- Equation of State for Nucleonic and Hyperonic Neutron Stars with Mass and Radius Constraints
- A new temperature dependent hyperonic equation of state: application to rotating neutron star models and I-Q-relations
- Constraining hypernuclear density functional with -hypernuclei and compact stars
- Hyperon-nucleon three-body forces and strangeness in neutron stars
- The evolution of binary neutron star post-merger remnants: a review
- Heavy Baryons in Compact Stars
- The Equation of State for the Nucleonic and Hyperonic Core of Neutron Stars
- Constraining the onset density of the hadron-quark phase transition with gravitational-wave observations
- Nuclear equation of state for arbitrary proton fraction and temperature based on chiral effective field theory and a Gaussian process emulator
- Confronting GW190814 with hyperonization in dense matter and hypernuclear compact stars
- Systematics of prompt black-hole formation in neutron star mergers
- Inferring prompt black-hole formation in neutron star mergers from gravitational-wave data
- A new equation of state for core-collapse supernovae based on realistic nuclear forces and including a full nuclear ensemble
- Neutron Star Mergers and How to Study Them
- Relativistic hypernuclear compact stars with calibrated equations of state
- Numerical relativity simulations of prompt collapse mergers: threshold mass and phenomenological constraints on neutron star properties after GW170817
- Quasi-universal behaviour of the threshold mass in unequal-mass, spinning binary neutron-star mergers
- Microscopic equation of state of hot nuclear matter for numerical relativity simulations
- Neutron matter at finite temperature based on chiral effective field theory interactions
- Equations of state for hot neutron stars -- II. The role of exotic particle degrees of freedom
- Massive -resonance admixed hypernuclear stars with anti-kaon condensations
- Thermal Effects in Binary Neutron Star Mergers
- Frequency deviations in universal relations of isolated neutron stars and postmerger remnants
- Spectral analysis of gravitational waves from binary neutron star merger remnants
- EoS for hot neutron stars
- Delta-resonances and hyperons in proto-neutron stars and merger remnants
- Equation of State table with hyperon and antikaon for supernova and neutron star merger
- Effects of hyperons on the nuclear equation of state in a Dirac-Brueckner-Hartree-Fock model
- Thermal behavior as indicator for hyperons in binary neutron star merger remnants
- Equation of state and composition of proto-neutron stars and merger remnants with hyperons
- The Role of Baryon Structure in Neutron Stars
- Quick Guides for Use of the CompOSE Data Base
- Frequencies of - and -oscillation modes in cold and hot compact stars
- Hot and Dense Matter Equation of State Probability Distributions for Astrophysical Simulations
- Hyperonic uncertainties in neutron stars, mergers and supernovae
Cited by in corpus (4)
- Investigating the Impact of Higher-Order Phase Transitions in Binary Neutron-Star Mergers
- Probing Strange Dark Matter through -mode Oscillations of Neutron Stars with Hyperons and Quark Matter
- Hyperons in Neutron Stars across the observed mass range: Insights from realistic -N and - interactions within a Microscopic Framework
- Renormalization-Group Invariant Parity-Doublet Model for Nuclear and Neutron-Star Matter