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Novel Model of an Ultra-stripped Supernova Progenitor of a Double Neutron Star

appsOther research productkeyboard_double_arrow_right Other ORP type 17 Sep 2021Publisher:Zenodo
Authors: Jiang, Long; Tauris, Thomas; Chen, Wen-Cong; Fuller, Jim;

doi: 10.5281/zenodo.5516837 , 10.5281/zenodo.5513810

Novel Model of an Ultra-stripped Supernova Progenitor of a Double Neutron Star

Abstract

(Inlist_2NS.tar.gz =inlist_2NS.zip) Recent discoveries of double neutron star (DNS) mergers and ultra-stripped supernovae (SNe) raise the questions of their origin and connection. We present the 1D model of a DNS progenitor system which is calculated self-consistently until an ultra-stripped iron core collapse. We apply the MESA code starting from a post-common envelope binary consisting of a NS and a zero-age main-sequence helium star and continue the modelling via Case BB Roche-lobe over ow until the infall velocity of the collapsing iron core exceeds 1000 kms^-1. Depending on the initial conditions, this family of systems is anticipated to reproduce the DNS mergers detected by the LIGO-network.

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This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
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