POSYDON: A General-Purpose Population Synthesis Code with Detailed Binary-Evolution Simulations

Autor: Tassos Fragos, Jeff J. Andrews, Simone S. Bavera, Christopher P. L. Berry, Scott Coughlin, Aaron Dotter, Prabin Giri, Vicky Kalogera, Aggelos Katsaggelos, Konstantinos Kovlakas, Shamal Lalvani, Devina Misra, Philipp M. Srivastava, Ying Qin, Kyle A. Rocha, Jaime Román-Garza, Juan Gabriel Serra, Petter Stahle, Meng Sun, Xu Teng, Goce Trajcevski, Nam Hai Tran, Zepei Xing, Emmanouil Zapartas, Michael Zevin

Publikováno v: Fragos, T, Andrews, J J, Bavera, S S, Berry, C P L, Coughlin, S, Dotter, A, Giri, P, Kalogera, V, Katsaggelos, A, Kovlakas, K, Lalvani, S, Misra, D, Srivastava, P M, Qin, Y, Rocha, K A, Roman-Garza, J, Serra, J G, Stahle, P, Sun, M, Teng, X, Trajcevski, G, Tran, N H, Xing, Z, Zapartas, E & Zevin, M 2023, ' POSYDON : A General-purpose Population Synthesis Code with Detailed Binary-evolution Simulations ', Astrophysical Journal, Supplement Series, vol. 264, no. 2, 45 . https://doi.org/10.3847/1538-4365/ac90c1
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Most massive stars are members of a binary or a higher-order stellar systems, where the presence of a binary companion can decisively alter their evolution via binary interactions. Interacting binaries are also important astrophysical laboratories fo

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