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From 3D hydrodynamic simulations of common-envelope interaction to gravitational-wave mergers

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Modeling the evolution of progenitors of gravitational-wave merger events in binary stars faces two major uncertainties: the common-envelope phase and supernova kicks. These two processes are critical for the final orbital configuration of double compact-object systems with neutron stars and black h...

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Main Authors: Moreno, Melvin M. (Author) , Schneider, Fabian (Author) , Röpke, Friedrich (Author) , Ohlmann, Sebastian T. (Author) , Pakmor, Rüdiger (Author) , Podsiadlowski, Philipp (Author) , Sand, Christian (Author)
Format: Article (Journal) Chapter/Article
Language:English
Published: 23 Nov 2021
In: Arxiv
Year: 2021, Pages: 1-16
DOI:10.48550/arXiv.2111.12112
Online Access:Verlag, kostenfrei, Volltext: https://doi.org/10.48550/arXiv.2111.12112
Verlag, kostenfrei, Volltext: http://arxiv.org/abs/2111.12112
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Author Notes:Melvin M. Moreno, Fabian R.N. Schneider, Friedrich K. Röpke, Sebastian T. Ohlmann, Rüdiger Pakmor, Philipp Podsiadlowski, and Christian Sand
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From 3D hydrodynamic simulations of common-envelope interaction to gravitational-wave mergers by Moreno, Melvin M. (Author) , Schneider, Fabian (Author) , Röpke, Friedrich (Author) , Ohlmann, Sebastian T. (Author) , Pakmor, Rüdiger (Author) , Podsiadlowski, Philipp (Author) , Sand, Christian (Author) ,


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