Literature DB >> 33408377

Core-collapse supernova explosion theory.

A Burrows1, D Vartanyan2.   

Abstract

Most supernova explosions accompany the death of a massive star. These explosions give birth to neutron stars and black holes, and eject solar masses of heavy elements. However, determining the mechanism of explosion has been a half-century journey of great numerical and physical complexity. Here we present the status of this theoretical quest and the physics and astrophysics upon which its resolution seems to depend. The delayed neutrino-heating mechanism is emerging as the key driver of supernova explosions, but there remain many issues to address, such as the chaos of the involved dynamics.

Entities:  

Year:  2021        PMID: 33408377     DOI: 10.1038/s41586-020-03059-w

Source DB:  PubMed          Journal:  Nature        ISSN: 0028-0836            Impact factor:   49.962


  7 in total

1.  Pulsar recoil and gravitational radiation due to asymmetrical stellar collapse and explosion.

Authors: 
Journal:  Phys Rev Lett       Date:  1996-01-15       Impact factor: 9.161

2.  Pulsar recoil by large-scale anisotropies in supernova explosions.

Authors:  L Scheck; T Plewa; H-Th Janka; K Kifonidis; E Müller
Journal:  Phys Rev Lett       Date:  2004-01-09       Impact factor: 9.161

3.  Electron capture rates on nuclei and implications for stellar core collapse.

Authors:  K Langanke; G Martínez-Pinedo; J M Sampaio; D J Dean; W R Hix; O E B Messer; A Mezzacappa; M Liebendörfer; H-Th Janka; M Rampp
Journal:  Phys Rev Lett       Date:  2003-06-19       Impact factor: 9.161

4.  A large-scale dynamo and magnetoturbulence in rapidly rotating core-collapse supernovae.

Authors:  Philipp Mösta; Christian D Ott; David Radice; Luke F Roberts; Erik Schnetter; Roland Haas
Journal:  Nature       Date:  2015-11-30       Impact factor: 49.962

5.  Neutrino-induced nucleosynthesis of A>64 nuclei: the nu p process.

Authors:  C Fröhlich; G Martínez-Pinedo; M Liebendörfer; F-K Thielemann; E Bravo; W R Hix; K Langanke; N T Zinner
Journal:  Phys Rev Lett       Date:  2006-04-10       Impact factor: 9.161

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

Authors:  John M Blondin; Anthony Mezzacappa
Journal:  Nature       Date:  2007-01-04       Impact factor: 49.962

7.  Discovery of an Exceptionally Strong β-Decay Transition of ^{20}F and Implications for the Fate of Intermediate-Mass Stars.

Authors:  O S Kirsebom; S Jones; D F Strömberg; G Martínez-Pinedo; K Langanke; F K Röpke; B A Brown; T Eronen; H O U Fynbo; M Hukkanen; A Idini; A Jokinen; A Kankainen; J Kostensalo; I Moore; H Möller; S T Ohlmann; H Penttilä; K Riisager; S Rinta-Antila; P C Srivastava; J Suhonen; W H Trzaska; J Äystö
Journal:  Phys Rev Lett       Date:  2019-12-31       Impact factor: 9.161

  7 in total
  2 in total

1.  High-entropy ejecta plumes in Cassiopeia A from neutrino-driven convection.

Authors:  Toshiki Sato; Keiichi Maeda; Shigehiro Nagataki; Takashi Yoshida; Brian Grefenstette; Brian J Williams; Hideyuki Umeda; Masaomi Ono; John P Hughes
Journal:  Nature       Date:  2021-04-21       Impact factor: 69.504

2.  Nuclear astrophysics in our time: supernovae, neutron stars and binary neutron star mergers.

Authors:  Debades Bandyopadhyay
Journal:  Eur Phys J Spec Top       Date:  2021-05-17       Impact factor: 2.707

  2 in total

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