{ "id": "2001.10668", "version": "v1", "published": "2020-01-29T02:37:34.000Z", "updated": "2020-01-29T02:37:34.000Z", "title": "The impact of isomers on a kilonova associated with neutron star mergers", "authors": [ "Shin-ichiro Fujimoto", "Masa-aki Hashimoto" ], "comment": "6 pages, 4 figures. Accepted for publication in MNRAS", "categories": [ "astro-ph.HE", "nucl-th" ], "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 ($\\dot{\\epsilon}_{\\rm nuc}$) of ejecta from NSMs, taking into account $\\beta^-$ decay through isomers. We find that for ejecta with electron fraction ($Y_e$) of $0.2-0.3$, $\\dot{\\epsilon}_{\\rm nuc}$ is appreciably changed from those without isomers, due to the large change in timing of $\\beta^-$ decay through the isomeric states of ${}^{123, 125, 127} \\rm Sn$ and ${}^{128} \\rm Sb$. In particular, the effects of the isomers on $\\dot{\\epsilon}_{\\rm nuc}$ are prominent for ejecta of $Y_e \\sim 0.25$, 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 ${}^{129} \\rm Sb$ and ${}^{129, 131} \\rm Te$ also cause additional and appreciable change in $\\dot{\\epsilon}_{\\rm nuc}$. 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.", "revisions": [ { "version": "v1", "updated": "2020-01-29T02:37:34.000Z" } ], "analyses": { "keywords": [ "neutron star mergers", "isomeric state", "lanthanide-free ejecta result", "energy generation rates", "larger amounts" ], "note": { "typesetting": "TeX", "pages": 6, "language": "en", "license": "arXiv", "status": "editable" } } }