On the stability of slow neutron combustion in astrophysical objects

Details On the stability of slow neutron combustion in astrophysical objects On the stability of slow neutron combustion in astrophysical objects

Nov 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988phlb..213..516h&link_type=abstract

Physics Letters B, Volume 213, Issue 4, p. 516-520.

Physics

58

Scientific paper

The problem of slow neutron combustion in astrophysical objects is studied from the hydrodynamical point of of view, showing that unless the existence of unknown stabilizing effects, the process seems to be absolutely unstable. It is shown that the slow combustion is likely to become a fast combustion mode called detonation. Some possible consequences of this instability for neutron stars and type II supernovae are presented and discussed.
Fellow of the Comisión de Investigaciones Científicas de la Provincia de Buenos Aires.

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