Surrogate light curve models for kilonovae with comprehensive wind ejecta outflows and parameter estimation for AT2017gfo
astro-ph.HE
Submitted: 2022-11-08
Updated: 2023-03-13
Comments: 15 pages, 6 figures, data available in Zenodo (https://zenodo.org/record/7335961) and GitHub (https://github.com/markoris/surrogate_kne)
Journal ref: Phys. Rev. Res. 5, 013168 (2023)
DOI: 10.1103/PhysRevResearch.5.013168
Code: https://github.com/markoris/surrogate_kne
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- 3D radiative transfer kilonova modelling for binary neutron star merger simulations
- A study of the agreement between binary neutron star ejecta models derived from numerical relativity simulations
- Using Neural Networks to Perform Rapid High-Dimensional Kilonova Parameter Inference
- Constraining inputs to realistic kilonova simulations through comparison to observed $r$-process abundances
- An updated nuclear-physics and multi-messenger astrophysics framework for binary neutron star mergers
- General relativistic simulations of collapsing binary neutron star mergers with Monte-Carlo neutrino transport
Related papers
- Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
- Collisionless Accretion of Finite-Angular-Momentum Plasma onto a Spinning Black Hole
- Impact of Magnetic Field Topology on Electromagnetic and Gravitational Waves from Binary Neutron Star Merger Remnants
- 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