The impact of isomers on a kilonova associated with neutron star mergers
arXiv:2001.10668 · doi:10.1093/mnrasl/slaa016
Abstract
We investigate the significance of isomers on a kilonova associated with neutron star mergers (NSMs) for the first time. We calculate the evolution of abundances and energy generation rates () of ejecta from NSMs, taking into account decay through isomers. We find that for ejecta with electron fraction () of , is appreciably changed from those without isomers, due to the large change in timing of decay through the isomeric states of and . In particular, the effects of the isomers on are prominent for ejecta of , which could emit a fraction of an early, blue component of a kilonova observed in GW170817. When the excitation from a ground state to its isomeric state is important, the isomers of and also cause additional and appreciable change in . Furthermore, we demonstrate that larger amounts of lanthanide-free ejecta result in a better fit of an observed light curve of the kilonova in GW170817 if the isomers are taken into account.
6 pages, 4 figures. Accepted for publication in MNRAS
References in corpus (10)
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- Origin of the heavy elements in binary neutron-star mergers from a gravitational wave event
- The Electromagnetic Counterpart of the Binary Neutron Star Merger LIGO/VIRGO GW170817. II. UV, Optical, and Near-IR Light Curves and Comparison to Kilonova Models
- A kilonova as the electromagnetic counterpart to a gravitational-wave source
- The Emergence of a Lanthanide-Rich Kilonova Following the Merger of Two Neutron Stars
- Comprehensive nucleosynthesis analysis for ejecta of compact binary mergers
- The Combined Ultraviolet, Optical, and Near-Infrared Light Curves of the Kilonova Associated with the Binary Neutron Star Merger GW170817: Unified Data Set, Analytic Models, and Physical Implications
- Kilonova from post-merger ejecta as an optical and near-infrared counterpart of GW170817
- Nucleosynthesis in Magnetically Driven Jets from Collapsars
- Heavy element nucleosynthesis in a collapsar
Cited by in corpus (13)
- Kilonovae across the nuclear physics landscape: The impact of nuclear physics uncertainties on r-process-powered emission
- Modeling Kilonova Light Curves: Dependence on Nuclear Inputs
- Atlas of Nuclear Isomers -- Second Edition
- Astromers: Nuclear Isomers in Astrophysics
- Astromers in the radioactive decay of r-process nuclei
- Isochronic evolution and the radioactive decay of r-process nuclei
- High-precision measurements of low-lying isomeric states in In with JYFLTRAP double Penning trap
- Alpha decay law of excited nuclei and its role in stellar decay rates
- Neutron transfer reactions on the ground state and isomeric state of a 130Sn beam
- How Do Nuclear Isomers Influence the Gamma-Ray Bursts in Binary Neutron Star Mergers?
- Gamma-ray emission from decays of boosted nuclei in protomagnetar jets
- Sensitivity of Neutron-Rich Nuclear Isomer Behavior to Uncertainties in Direct Transitions
- Exploration for Astromers near Sn with the Canadian Penning Trap