MESA-QUEST: Modeling Quasi-Stars in MESA

Fuente: arXiv
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Auteurs principaux: Campbell, Claire B., Santarelli, Andrew D., Caplan, Matthew E.
Format: Preprint
Publié: 2025
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author Campbell, Claire B.
Santarelli, Andrew D.
Caplan, Matthew E.
author_facet Campbell, Claire B.
Santarelli, Andrew D.
Caplan, Matthew E.
contents Supermassive black hole formation remains an unsolved problem. Quasi-stars have been suggested as a viable heavy-seeding mechanism. In this work, we implement methods for modeling quasi-stars previously used with the Cambridge STARS code into the 1D stellar evolution code MESA. The computational capabilities of MESA allow for more detailed simulations of quasi-star evolution due to its modularity and the ease of implementing of new physical processes and controls. Our implementation, the MESA Quasi-star Evolutionary Simulation Toolkit (MESA-QUEST), is available in a publicly accessible repository.
format Preprint
id arxiv_https___arxiv_org_abs_2507_12651
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle MESA-QUEST: Modeling Quasi-Stars in MESA
Campbell, Claire B.
Santarelli, Andrew D.
Caplan, Matthew E.
High Energy Astrophysical Phenomena
Supermassive black hole formation remains an unsolved problem. Quasi-stars have been suggested as a viable heavy-seeding mechanism. In this work, we implement methods for modeling quasi-stars previously used with the Cambridge STARS code into the 1D stellar evolution code MESA. The computational capabilities of MESA allow for more detailed simulations of quasi-star evolution due to its modularity and the ease of implementing of new physical processes and controls. Our implementation, the MESA Quasi-star Evolutionary Simulation Toolkit (MESA-QUEST), is available in a publicly accessible repository.
title MESA-QUEST: Modeling Quasi-Stars in MESA
topic High Energy Astrophysical Phenomena
url https://arxiv.org/abs/2507.12651