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ZENODO
Dataset . 2022
License: CC BY
Data sources: Datacite
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ZENODO
Dataset . 2022
License: CC BY
Data sources: Datacite
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Light Axion Emission and the Formation of Merging Black Holes Binaries

Authors: Croon, Djuna; Sakstein, Jeremy;

Light Axion Emission and the Formation of Merging Black Holes Binaries

Abstract

# Reproduction Package for the Paper "Light axion emission and the formation of merging binary black holes" ## Authors: Djuna Croon (djuna.l.croon@durham.ac.uk) Jeremy Sakstein (sakstein@hawaii.edu) ## Software MESA version 15140 (http://mesa.sourceforge.net/) MESASDK version 20210401 (http://www.astro.wisc.edu/~townsend/static.php?ref=mesasdk) GFORTRAN GCC version 9.2.0 ## Example Directories **work:** Contains inlists, run\_star\_extras, and run\_binary_\extras needed to reproduce our results. These were adapted from the reproduction package of A&A 650, A107 (2021). A small number of models did not converge using the default controls. These can be made to complete by either setting the control make\_gradr\_sticky\_in\_solver\_iters = .true. (see inlist1, this works for models with small initial periods) or by relaxing delta\_HR\_limit and delta\_HR\_hard\_limit (see run\_binary\_extras line 900). ## Citation Policy If you use any part of this reproduction package for independent work we recommend you cite the following papers: - https://arxiv.org/abs/2208.01110 - Phys.Dark Univ. 32 (2021) 100801 - Phys.Rev.D 102 (2020) 11, 115024 - Phys.Rev.Lett. 125 (2020) 26, 261105 - Astrophys.J.Lett. 916 (2021) 2, L16 - Phys.Rev.D 105 (2022) 095038 - A&A 650, A107 (2021) - Astrophys. J. Suppl. 192, 3 (2011) - Astrophys. J. Suppl. 208, 4 (2013) - Astrophys. J. Suppl. 234, 34 (2018) - ApJS 243, 10 (2019)

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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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This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
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