Weak r-process component as a result of the neutrino interaction with the helium shell of a supernova

Details Weak r-process component as a result of the neutrino interaction with the helium shell of a supernova Weak r-process component as a result of the neutrino interaction with the helium shell of a supernova

Jun 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007astl...33..385n&link_type=abstract

Astronomy Letters, Volume 33, Issue 6, pp.385-389

Astronomy and Astrophysics

Astronomy

5

Scientific paper

Possibilities for the development of an r-process in the helium shell of a supernova under the action of free neutrons appearing as a result of inelastic neutrino scattering by 4He nuclei are investigated. The conditions in the outer part of the helium shell in metal-poor stars are shown to be favorable for the reproduction of a weak r-process component.

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