Convection, type II supernovae, and the early evolution of neutron stars

Adam Burrows, James M. Lattimer

Research output: Contribution to journalArticlepeer-review

43 Scopus citations

Abstract

We discuss some of the issues attending the study of the early evolution of neutron stars. In particular, the effect of convection during the protoneutron star stage is investigated. We conclude that convection not only affects a young neutron star's first seconds in interesting ways, but also that it makes the long-term mechanism for Type II supernova explosions more viable and energetic.

Original languageEnglish (US)
Pages (from-to)51-62
Number of pages12
JournalPhysics Reports
Volume163
Issue number1-3
DOIs
StatePublished - Jun 1988
Externally publishedYes

All Science Journal Classification (ASJC) codes

  • Physics and Astronomy(all)

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