Rapid stellar and binary population synthesis with COMPAS

Autor:	COMPAS, Team, Riley, Jeff, Agrawal, Poojan, Barrett, Jim W., Boyett, Kristan N. K., Broekgaarden, Floor S., Chattopadhyay, Debatri, Gaebel, Sebastian M., Gittins, Fabian, Hirai, Ryosuke, Howitt, George, Justham, Stephen, Khandelwal, Lokesh, Kummer, Floris, Lau, Mike Y. M., Mandel, Ilya, de Mink, Selma E., Neijssel, Coenraad, Riley, Tim, van Son, Lieke, Stevenson, Simon, Vigna-Gomez, Alejandro, Vinciguerra, Serena, Wagg, Tom, Willcox, Reinhold
Rok vydání:	2021
Předmět:	Astrophysics - Instrumentation and Methods for Astrophysics Astrophysics - High Energy Astrophysical Phenomena Astrophysics - Solar and Stellar Astrophysics
Druh dokumentu:	Working Paper
DOI:	10.3847/1538-4365/ac416c
Popis:	Compact Object Mergers: Population Astrophysics and Statistics (COMPAS; https://compas.science) is a public rapid binary population synthesis code. COMPAS generates populations of isolated stellar binaries under a set of parametrized assumptions in order to allow comparisons against observational data sets, such as those coming from gravitational-wave observations of merging compact remnants. It includes a number of tools for population processing in addition to the core binary evolution components. COMPAS is publicly available via the github repository https://github.com/TeamCOMPAS/COMPAS/, and is designed to allow for flexible modifications as evolutionary models improve. This paper describes the methodology and implementation of COMPAS. It is a living document which will be updated as new features are added to COMPAS; the current document describes COMPAS v02.21.00. Comment: Code publicly available via https://compas.science . Minor updates to match version accepted to ApJS
Databáze:	arXiv
Externí odkaz:	http://arxiv.org/abs/2109.10352 Zobrazit plný text záznamu View this record from Arxiv