Modeling Type Ia supernovae with explosions in white dwarfs near and below the Chandrasekhar mass

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Abstract:

The progenitor evolution and the explosion mechanism of Type Ia supernovae remain unexplained. Nonetheless, substantial progress has been made over the past years with three-dimensional hydrodynamic simulations of different scenarios. Here, we review some recent work pertaining to the leading paradigms of modeling: thermonuclear explosions of white dwarf stars near and below the Chandrasekhar mass limit. We discuss implications of the different explosion channels and their predictions of observables.

SEEK ID: https://publications.h-its.org/publications/1610

SEEK ID: https://publications.h-its.org/publications/1610

DOI: 10.1142/9789811269776_0373

Research Groups: Physics of Stellar Objects

Publication type: Journal

Journal: The Sixteenth Marcel Grossmann Meeting

Book Title: The Sixteenth Marcel Grossmann Meeting

Citation: The Sixteenth Marcel Grossmann Meeting,pp.4420-4426,WORLD SCIENTIFIC

Date Published: 1st Feb 2023

URL: https://www.worldscientific.com/doi/abs/10.1142/9789811269776_0373

Registered Mode: imported from a bibtex file

Authors: Friedrich K. Röpke, Florian Lach, Sabrina Gronow, Stuart A. Sim, Fionntan P. Callan, Christine E. Collins

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Citation
Röpke, F. K., Lach, F., Gronow, S., Sim, S. A., Callan, F. P., & Collins, C. E. (2023). Modeling Type Ia supernovae with explosions in white dwarfs near and below the Chandrasekhar mass. In The Sixteenth Marcel Grossmann Meeting. Proceedings of the MG16 Meeting on General Relativity. WORLD SCIENTIFIC. https://doi.org/10.1142/9789811269776_0373
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Created: 13th Feb 2023 at 15:04

Last updated: 5th Mar 2024 at 21:25

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