Light Curves and Event Rates of Axion Instability Supernovae

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

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

- Summary
- Metrics

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

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

Impact byBIP!

	selected citations These citations are derived from selected sources. This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	0
	popularity This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.	Average
	influence This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).	Average
	impulse This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.	Average