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Supplying angular momentum to the jittering jets explosion mechanism using convection in inner star layers

Published online by Cambridge University Press:  29 August 2024

Dmitry Shishkin Open the ORCID record for Dmitry Shishkin [Opens in a new window]
Dmitry Shishkin*
Affiliation:
Department of Physics, Technion, Haifa, 3200003, Israel
*
email:s.dmitry@campus.technion.ac.il
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Abstract

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The jittering jets explosion mechanism of core collapse supernovae proposes that stochastic convective motion, amplified by instabilities, results in intermittent accretion disk that launches jittering jets that explode the star. We conduct one-dimensional simulations of a wide range of stellar masses and show that the convective motion in the pre-collapse stellar core, when scaled to corresponding three-dimensional simulations, supply sufficient angular momentum fluctuation to form the intermittent accretion disk the launches the jittering jets. The resulting neutron star masses are consistent with observations.

Keywords

supernovae: general
Type
Poster Paper
Information
Proceedings of the International Astronomical Union , Volume 18 , Symposium S361: Massive Stars Near and Far , May 2022 , pp. 607 - 609
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Creative Commons
Creative Common License - CCCreative Common License - BY
This is an Open Access article, distributed under the terms of the Creative Commons Attribution licence (https://creativecommons.org/licenses/by/4.0/), which permits unrestricted re-use, distribution, and reproduction in any medium, provided the original work is properly cited.
Copyright
© The Author(s), 2024. Published by Cambridge University Press on behalf of International Astronomical Union

References

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Shishkin, D., & Soker, N. 2021, MNRAS: Letters, 508, L43 Google Scholar
Shishkin, D., & Soker, N. 2022, MNRAS, 513, 4224 Google Scholar
Soker, N. 2019, Research in Astronomy and Astrophysics, 19, 095 Google Scholar
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