Turbulence and nuclear reactions in 3D hydrodynamics simulations of massive stars

Our knowledge of massive star evolution and nucleosynthesis is limited by uncertainties related to multi-dimensional processes taking place in stellar interiors. Recently, theoretical works have started to improve 1D stellar evolution codes through the implementation of results from 3D hydrodynamics...

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Bibliographic Details
Main Authors: Rizzuti Federico, Hirschi Raphael, Georgy Cyril, Arnett David, Meakin Casey, Murphy Alexander
Format: Article
Language:English
Published: EDP Sciences 2023-01-01
Series:EPJ Web of Conferences
Online Access:https://www.epj-conferences.org/articles/epjconf/pdf/2023/05/epjconf_npa-x2023_05001.pdf