Investigating the influence of the full-kinematics treatment for charged-current processes in binary neutron star mergers

arXiv:2609.19922 · astro-ph.HE · Submitted 2026-09-17 · Read on arXiv

astro-ph.HE

Submitted: 2026-09-17

Updated: 2026-09-17

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Core — 15× in this paper · explained in 2 episodes
• Abundance — 10× in this paper · explained in 1 episode
• Degeneracy — 2× in this paper · explained in 3 episodes
• Gravitational Wave Emission — 2× in this paper · explained in 2 episodes
• alpha — 2× in this paper · explained in 1 episode
• Accuracy — 1× in this paper · explained in 1 episode
• Calibration — 1× in this paper · explained in 7 episodes
• Momentum transfer — 1× in this paper · explained in 2 episodes
• Regularization — 1× in this paper · explained in 3 episodes
• Robustness — 1× in this paper · explained in 5 episodes
• Unified Framework — 1× in this paper · explained in 5 episodes

Sources

• Transient Events from Neutron Star Mergers
• Electromagnetic Counterparts of Compact Object Mergers Powered by the Radioactive Decay of R-process Nuclei
• Optical emission from a kilonova following a gravitational-wave-detected neutron-star merger
• Swope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source
• Swift and NuSTAR observations of GW170817: detection of a blue kilonova
• Spectroscopic identification of r-process nucleosynthesis in a double neutron star merger
• A kilonova as the electromagnetic counterpart to a gravitational-wave source
• The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/Virgo GW170817. I. Dark Energy Camera Discovery of the Optical Counterpart
• The Emergence of a Lanthanide-Rich Kilonova Following the Merger of Two Neutron Stars
• The discovery of the electromagnetic counterpart of GW170817: kilonova AT 2017gfo/DLT17ck
• GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
• Electromagnetic Evidence that SSS17a is the Result of a Binary Neutron Star Merger
• Identification of strontium in the merger of two neutron stars
• Effect of a High Opacity on the Light Curves of Radioactively Powered Transients from Compact Object Mergers
• Red or blue? A potential kilonova imprint of the delay until black hole formation following a neutron star merger
• Nucleosynthesis and observation of the heaviest elements
• Truncated Moment Formalism for Radiation Hydrodynamics in Numerical Relativity
• Charged current neutrino interactions in hot and dense matter
• Charged-Current Muonic Reactions in Core-Collapse Supernovae
• Neutrino signal from proto-neutron star evolution: Effects of opacities from charged-current-neutrino interactions and inverse neutron decay

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• XRISM Resolve Spectroscopy of GX 5-1: Constraints on Iron Spectral Features in a Luminous Neutron-Star Binary
• SN 1006: A Cosmic Laboratory for Investigating Shock Acceleration Physics
• Neutrino Spectral Pinching in 3D Core-Collapse Supernovae: Late-Time Convergence, Failed-Explosion Signatures, and Viewing-Angle Dispersion