Multimessenger Binary Mergers Containing Neutron Stars: Gravitational Waves, Jets, and -Ray Bursts
arXiv:2102.03366 · doi:10.3389/fspas.2021.656907
Abstract
Neutron stars (NSs) are extraordinary not only because they are the densest form of matter in the visible Universe but also because they can generate B-fields ten orders of magnitude larger than those currently constructed on Earth. The combination of extreme gravity with the enormous electromagnetic (EM) fields gives rise to spectacular phenomena like those observed on August 2017 with the merger of a binary neutron star (NSNS) system, an event that generated a gravitational wave (GW) signal, a short -ray burst (sGRB), and a kilonova. This event serves as the highlight so far of the era of multimessenger astronomy. In this review, we present the current state of our theoretical understanding of compact binary mergers containing NSs as gleaned from the latest general relativistic magnetohydrodynamic simulations. Such mergers can lead to events like the one on August 2017, GW170817, and its EM counterparts, GRB 170817 and AT 2017gfo. In addition to exploring the GW emission from binary black hole-neutron star and NSNS mergers, we also focus on their counterpart EM signals. In particular, we are interested in identifying the conditions under which a relativistic jet can be launched following these mergers. Such a jet is an essential feature of most sGRB models and provides the main conduit of energy from the central object to the outer radiation regions. Jet properties, including their lifetimes and Poynting luminosities, the effects of the initial B-field geometries and spins of the coalescing NSs, as well as their governing equation of state, are discussed. Lastly, we present our current understanding of how the Blandford-Znajek mechanism arises from merger remnants as the trigger for launching jets, if, when and how a horizon is necessary for this mechanism, and the possibility that it can turn on in magnetized neutron ergostars, which contain ergoregions, but no horizons.
Invited review for the Research Topic: "Neutron Star Physics in the Multi-Messenger Discourse", Frontiers Astronomy and Space Sciences. 22pages, 12 figures. Matches published version
References in corpus (66)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Multi-messenger Observations of a Binary Neutron Star Merger
- Gravitational Waves and Gamma-rays from a Binary Neutron Star Merger: GW170817 and GRB 170817A
- A bright millisecond radio burst of extragalactic origin
- 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
- Origin of the heavy elements in binary neutron-star mergers from a gravitational wave event
- Constraints on a phenomenologically parameterized neutron-star equation of state
- Illuminating Gravitational Waves: A Concordant Picture of Photons from a Neutron Star Merger
- Constraining the Maximum Mass of Neutron Stars From Multi-Messenger Observations of GW170817
- Formation of Double Neutron Star Systems
- GW170817: Joint Constraint on the Neutron Star Equation of State from Multimessenger Observations
- Neutron-star radius constraints from GW170817 and future detections
- A Radio Counterpart to a Neutron Star Merger
- Modeling GW170817 based on numerical relativity and its implications
- Producing ultra-strong magnetic fields in neutron star mergers
- Accurate evolutions of inspiralling neutron-star binaries: prompt and delayed collapse to black hole
- Merger of binary neutron stars to a black hole: Disk mass, short gamma-ray bursts, and quasinormal mode ringing
- The dynamical mass ejection from binary neutron star mergers: Radiation-hydrodynamics study in general relativity
- Binary Neutron Star Mergers: Dependence on the Nuclear Equation of State
- The Influence of Magnetic Field Geometry on the Evolution of Black Hole Accretion Flows: Similar Disks, Drastically Different Jets
- Relativistic neutron star merger simulations with non-zero temperature equations of state I. Variation of binary parameters and equation of state
- A decade of Gamma-Ray Bursts observed by -LAT: The 2 GRB catalog
- Testing Approximations of Thermal Effects in Neutron Star Merger Simulations
- Black Hole-Neutron Star Mergers: Disk Mass Predictions
- Estimating the Contribution of Dynamical Ejecta in the Kilonova Associated with GW170817
- Magnetized Neutron Star Mergers and Gravitational Wave Signals
- General relativistic simulations of magnetized binary neutron star mergers
- Binary-black-hole initial data with nearly-extremal spins
- Fully General Relativistic Simulations of Black Hole-Neutron Star Mergers
- Properties of hypermassive neutron stars formed in mergers of spinning binaries
- Relativistic simulations of black hole-neutron star coalescence: the jet emerges
- Evolving black hole-neutron star binaries in general relativity using pseudospectral and finite difference methods
- Gravitational Wave Signatures of Highly Compact Boson Star Binaries
- Relativistic Simulations of Black Hole-Neutron Star Mergers: Effects of black-hole spin
- A lower bound on the maximum mass if the secondary in GW190814 was once a rapidly spinning neutron star
- Longterm general relativistic simulation of binary neutron stars collapsing to a black hole
- General relativistic simulations of compact binary mergers as engines of short gamma-ray bursts
- Numerical relativity simulations of neutron star merger remnants using conservative mesh refinement
- First 100 ms of a long-lived magnetized neutron star formed in a binary neutron star merger
- Merger of black hole-neutron star binaries in full general relativity
- Black hole-neutron star mergers: effects of the orientation of the black hole spin
- Merger of black hole-neutron star binaries: nonspinning black hole case
- Black Hole Spin Evolution: Implications for Short-hard Gamma Ray Bursts and Gravitational Wave Detection
- Sub-radian-accuracy gravitational waveforms of coalescing binary neutron stars in numerical relativity
- Gravitational waves and mass ejecta from binary neutron star mergers: Effect of the stars' rotation
- Initial data for black hole-neutron star binaries: a flexible, high-accuracy spectral method
- Mergers of Magnetized Neutron Stars with Spinning Black Holes: Disruption, Accretion and Fallback
- Advanced LIGO Constraints on Neutron Star Mergers and R-Process Sites
- Binary Neutron Star Mergers and Short Gamma-Ray Bursts: Effects of Magnetic Field Orientation, Equation of State, and Mass Ratio
- General Relativistic Binary Merger Simulations and Short Gamma Ray Bursts
- Neutrino transport in black hole-neutron star binaries: neutrino emission and dynamical mass ejection
- GRMHD simulations of prompt-collapse neutron star mergers: the absence of jets
- General relativistic simulations of black hole-neutron star mergers: Effects of tilted magnetic fields
- Dynamical Capture Binary Neutron Star Mergers
- Mergers of Black Hole -- Neutron Star binaries. I. Methods and First Results
- Quasiequilibrium black hole-neutron star binaries in general relativity
- A brief overview of black hole-neutron star mergers
- Effects of spin on magnetized binary neutron star mergers and jet launching
- Binary Neutron Star Merger Simulations with a Calibrated Turbulence Model
- Black holes, disks and jets following binary mergers and stellar collapse: The narrow range of EM luminosities and accretion rates
- Eccentric mergers of black holes with spinning neutron stars
- The role of the ergosphere in the Blandford-Znajek process
- Black hole-neutron star coalescence: effects of the neutron star spin on jet launching and dynamical ejecta mass
- Great Impostors: Extremely Compact, Merging Binary Neutron Stars in the Mass Gap Posing as Binary Black Holes
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- Prospects for the inference of inertial modes from hypermassive neutron stars with future gravitational-wave detectors
- Fast Neutrino Conversion in Hydrodynamic Simulations of Neutrino-Cooled Accretion Disks