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

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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Friedrich Röpke

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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 (pp. 4420–4426). 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

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

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