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Light Curves and Event Rates of Axion Instability Supernovae

Research datakeyboard_double_arrow_right Dataset 04 Nov 2022 English Publisher:ZenodoFunded by:NSF | WoU-MMA: Collaborative Re..., NSF | Collaborative Research: W...

Authors: Mori, Kanji; Moriya, Takashi J.; Takiwaki, Tomoya; Kotake, Kei; Horiuchi, Shunsaku; Blinnikov, Sergei I.;

doi: 10.5281/zenodo.7288159 , 10.5281/zenodo.7288158

Light Curves and Event Rates of Axion Instability Supernovae

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Abstract

These files are MESA (Modules for Experiments in Stellar Astrophysics) inlists that can reproduce results in Mori et al. (2022) (https://arxiv.org/abs/2209.03517). MESA version 12778 and MESA SDK version x86_64-linux-20.3.2 are used. Before running the code, the user should edit MESA following the instruction in Sakstein, Croon & McDermott (https://doi.org/10.5281/zenodo.6347632). PISN.tar.gz includes inlists for standard pair-instability supernovae while AISN_0.5.tar.gz and AISN_2.0.tar.gz are for axion instability supernovae with f=0.5 (i.e. ALP mass = 511 keV) and f=2.0 (i.e. ALP mass = 511*4 keV), respectively. Each directory consists of directories like "heavy_new_particle_100". The three digit number indicates the initial stellar mass. The users are encouraged to cite the following papers when they write a paper using these inlists. Mori et al. (2022), arXiv:2209.03517 Sakstein, Croon & McDermott (2022) Phys. Rev. D 105, 095038 Croon, McDermott & Sakstein (2020) Phys. Rev. D 102, 115024 MESA instrumental papers

Related Organizations

Kurchatov Institute
Russian Federation
Virginia Tech
United States
National Astronomical Observatory of Japan
Japan
Fukuoka University
Japan

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Light Curves and Event Rates of Axion Instability Supernovae
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Funded by

NSF| WoU-MMA: Collaborative Research: A Next-Generation SuperNova Early Warning System for Multimessenger Astronomy, NSF| Collaborative Research: WoU-MMA: Revealing the Fate of Heavy Nuclei in Stellar Explosions and Pathways to Cosmic Rays

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NEANIAS Space Research Community