\bf Combustion Gasdynamics in Proto-Neutron Stars
Astrophysics
2007-05-23 v1
Abstract
The possible conversion of neutron matter to strange matter and its relevance to astrophysical problems are discussed. Particular attention is paid to the {\it form} in which this hypothetical burning process should be propagated in dense matter and to the {\it moment} when it should start.
Cite
@article{arxiv.astro-ph/9305016,
title = {\bf Combustion Gasdynamics in Proto-Neutron Stars},
author = {J. E. Horvath},
journal= {arXiv preprint arXiv:astro-ph/9305016},
year = {2007}
}
Comments
Talk given at the VI J.A.Swieca School on Nuclear Physics (Campos do Jordao, Brazil, Feb93), PlainTeX, 9 p., 2 fig. available upon request, IAG/USP - 93 -014