Physics
Scientific paper
Apr 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993injpb..67..109p&link_type=abstract
Indian J. Phys., Part B, Vol. 67, No. 2, p. 109 - 131
Physics
Scientific paper
A neutron star is one of the possible endpoints of stellar evolution. High mass stars become neutron stars after suffering a supernovae explosion. In this paper, the author has discussed various neutron producing reactions (i.e. neutron sources) in nucleosynthesis during different evolving stages i.e. main sequence stage, red giant stage, supernova stage and neutron star stage. Neutrons produced in one stage come into the next stage as remnant and play an active role to begin nucleosynthesis in the next stage, and ultimately the formation of a neutron star.
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