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Rapid stellar and binary population synthesis with COMPAS: Methods paper II

Mandel, I., Riley, J., Boesky, A., Brček, A., Hirai, R., Kapil, V., Lau, M. Y. M., Merritt, J. D., Rodríguez-Segovia, N., Romero-Shaw, I., Song, Y., Stevenson, S., Vajpeyi, A., van Son, L. A. C., Vigna-Gómez, A. and Willcox, R. 2025. Rapid stellar and binary population synthesis with COMPAS: Methods paper II. The Astrophysical Journal Supplement 280 (1) , 43. 10.3847/1538-4365/adf8d0

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Abstract

The COMPAS (https://compas.science) public rapid binary population synthesis code has undergone a number of key improvements since the original COMPAS methods paper was published. These include more sophisticated and robust treatments of binary interactions: mass transfer physics; common-envelope events; tides and gravitational-wave radiation reaction; and updated prescriptions for stellar evolution, winds, and supernovae. The code structure and outputs have also been updated, with a focus on improving resolution without sacrificing computational speed. This paper describes the substantive changes in the code between the previous methods paper and COMPAS v03.22.01.

Item Type: Article
Date Type: Publication
Status: Published
Schools: Schools > Physics and Astronomy
Publisher: IOP
Date of First Compliant Deposit: 19 February 2026
Last Modified: 19 Feb 2026 12:00
URI: https://orca.cardiff.ac.uk/id/eprint/185041

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