Turbulent magnetic field amplification from spiral SASI modes: Implications for core-collapse supernovae and proto-neutron star magnetization

Eirik Endeve, Christian Y. Cardall, Reuben D. Budiardja, Samuel W. Beck, Alborz Bejnood, Ross J. Toedte, Anthony Mezzacappa, John M. Blondin

Research output: Contribution to journalArticlepeer-review

79 Scopus citations

Fingerprint

Dive into the research topics of 'Turbulent magnetic field amplification from spiral SASI modes: Implications for core-collapse supernovae and proto-neutron star magnetization'. Together they form a unique fingerprint.

Physics