Self-consistent 3D Supernova Models From −7 Minutes to +7 s: A 1-bethe Explosion of a ∼19 M ⊙ Progenitor-Reference-Cited by-同舟云学术

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Self-consistent 3D Supernova Models From −7 Minutes to +7 s: A 1-bethe Explosion of a ∼19 M ⊙ Progenitor

Published:2021-06-30 Issue:1 Volume:915 Page:28
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Bollig Robert^ORCID,Yadav Naveen^ORCID,Kresse Daniel^ORCID,Janka Hans-Thomas^ORCID,Müller Bernhard^ORCID,Heger Alexander^ORCID

Funder

EC ∣ European Research Council

Deutsche Forschungsgemeinschaft

Department of Education and Training ∣ Australian Research Council

Australian Research Council Centre for Excellence for Gravitational Wave Discovery

Australian Research Council Centre of Excellence for All Sky Astrophysics in 3 Dimensions

National Science Foundation

Gauss Centre for Supercomputing

Leibniz Supercomputing Centre

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/abf82e/pdf

Reference116 articles.

1. GRAVITATIONAL COLLAPSE AND WEAK INTERACTIONS

2. TOWARD REALISTIC PROGENITORS OF CORE-COLLAPSE SUPERNOVAE

3. Revival of a stalled supernova shock by neutrino heating

4. Pulsar spins from an instability in the accretion shock of supernovae

5. Stability of Standing Accretion Shocks, with an Eye toward Core‐Collapse Supernovae

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1. Muon-induced collisional flavor instability in core-collapse supernova;Physical Review D;2024-08-27

2. Interplay between neutrino kicks and hydrodynamic kicks of neutron stars and black holes;Astrophysics and Space Science;2024-08

3. The gravitational-wave emission from the explosion of a 15 solar mass star with rotation and magnetic fields;Monthly Notices of the Royal Astronomical Society;2024-07-23

4. Two-dimensional models of core-collapse supernova explosions assisted by heavy sterile neutrinos;Physical Review D;2024-07-22

5. Fate of supernova progenitors in massive binary systems;Monthly Notices of the Royal Astronomical Society;2024-07-12

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