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A large-scale magnetic field produced by a solar-like dynamo in binary neutron star mergers
The merger of two neutron stars launches a relativistic jet, which must be driven by a strong large-scale magnetic field. However, the...
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Binary Neutron Star Mergers
In this Chapter, we discuss how neutron stars are probed using gravitational waves. The discovery of the first neutron star binary in 1974 by H. A....
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Measurement errors of neutron star tidal deformability for binary neutron star mergers
We investigate the measurement errors of the neutron star tidal deformability in gravitational wave parameter estimation for merging binary neutron...
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Neutrino emission from binary neutron star mergers: characterising light curves and mean energies
Neutrinos are copiously emitted by neutron star mergers, due to the high temperatures reached by dense matter during the merger and its aftermath....
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Black Hole-Neutron Star Mergers
Pushed by the rapid rise of gravitational wave astronomy, the study of compact binary mergers has made significant progress over the last 5 years....
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Dynamically screened strongly quantized electron transport in binary neutron-star merger
We examine electron-transport coefficients in magnetized hot and dense electron-ion plasma relevant in binary neutron star merger simulation. We...
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Search for Pre-Burst Emission from Binary Neutron Star Mergers with Spectrum–Roentgen–Gamma
AbstractClose binary systems consisting of two neutron stars (BNS) emit gravitational waves, that allow them to merge on timescales shorter than...
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End-to-end study of the host galaxy and genealogy of the first binary neutron star merger
Binary neutron star mergers are one of the ultimate events of massive binary star evolution, and our understanding of their parent systems is still...
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The production of actinides in neutron star mergers
Although the multimessenger detection of the neutron star merger event GW170817 confirmed that mergers are promising sites producing the majority of...
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Universal Relations for Binary Neutron Star Mergers with Long-lived Remnants
In the last 25 years, an extensive body of work has developed various equation of state independent - or (approximately) universal - relations that...
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Nuclear astrophysics in our time: supernovae, neutron stars and binary neutron star mergers
This volume focuses on topical issues in nuclear astrophysics, particularly supernovae, neutron stars, and binary neutron star mergers. An overview...
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Turbulence modelling in neutron star merger simulations
Observations of neutron star mergers have the potential to unveil detailed physics of matter and gravity in regimes inaccessible by other...
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Simulating neutron star mergers with the Lagrangian Numerical Relativity code SPHINCS_BSSN
We present the first neutron star merger simulations performed with the newly developed Numerical Relativity code
SPHINCS_BSSN . This code evolves the...
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The use of hypermodels to understand binary neutron star collisions
Gravitational waves from the collision of binary neutron stars provide a unique opportunity to study the behaviour of supranuclear matter, the...
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An assessment of the association between a fast radio burst and binary neutron star merger
Fast radio bursts (FRBs) are bright millisecond-duration radio bursts at cosmological distances. While young magnetars are the leading source...
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Neutrino transport in general relativistic neutron star merger simulations
Numerical simulations of neutron star–neutron star and neutron star–black hole binaries play an important role in our ability to model...
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Interpreting binary neutron star mergers: describing the binary neutron star dynamics, modelling gravitational waveforms, and analyzing detections
Gravitational waves emitted from the coalescence of neutron star binaries open a new window to probe matter and fundamental physics in unexplored,...
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Impact of quark deconfinement in neutron star mergers and hybrid star mergers
We describe an unambiguous gravitational-wave signature to identify the occurrence of a strong phase transition from hadronic matter to deconfined...
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Black Hole-Neutron Star Mergers
Pushed by the rapid rise of gravitational wave astronomy, the study of compact binary mergers has made significant progress over the last 5 years....
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The evolution of binary neutron star post-merger remnants: a review
Two neutron stars merge somewhere in the Universe approximately every 10 to 100 s, creating violent explosions potentially observable in...
