\bf Combustion Gasdynamics in Proto-Neutron Stars

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dc.creatorHorvath, J. E.
dc.date1993-05-12
dc.date.accessioned2026-07-07T02:18:46Z
dc.date.available2026-07-07T02:18:46Z
dc.descriptionThe 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.
dc.descriptionTalk 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
dc.identifierhttps://arxiv.org/abs/astro-ph/9305016
dc.identifierhttp://arxiv.org/abs/astro-ph/9305016
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/9619
dc.subjectAstrophysics
dc.title\bf Combustion Gasdynamics in Proto-Neutron Stars
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