An instability in neutron stars at birth

Adam Burrows, Bruce A. Fryxell

Research output: Contribution to journalArticlepeer-review

99 Scopus citations


Calculations with a two-dimensional hydrodynamic simulation show that a generic Raleigh-Taylor-like instability occurs in the mantles of nascent neutron stars, that it is possibly violent, and that the standard spherically symmetric models of neutron star birth and supernova explosion may be inadequate. Whether this "convective" instability is pivotal to the supernova mechanism, pulsar magnetic fields, or a host of other important issues that attend stellar collapse remains to be seen, but its existence promises to modify all questions concerning this most energetic of astronomical phenomena.

Original languageEnglish (US)
Pages (from-to)430-434
Number of pages5
Issue number5081
StatePublished - 1992
Externally publishedYes

All Science Journal Classification (ASJC) codes

  • General


Dive into the research topics of 'An instability in neutron stars at birth'. Together they form a unique fingerprint.

Cite this