Pulsed-neutron-source models for the astrophysical s-process

Details Pulsed-neutron-source models for the astrophysical s-process Pulsed-neutron-source models for the astrophysical s-process

May 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985remo.conf.....h&link_type=abstract

Presented at 20th Recontre de Moriond, Les Arcs, France, 10 Mar. 1985

Astronomy and Astrophysics

Astrophysics

Astrophysics, Beta Particles, Decay, Electrons, Heavy Elements, Neutron Sources, Positrons, Simulation, Abundance, Capture Effect, Electron Capture, Models, Solar System

Scientific paper

The astrophysical s-process is a sequence of neutron-capture and beta-decay reactions on a slow time scale compared to beta-decay lifetimes near the line of stability. This detailed sequence of neutron capture, continuum and bound-state beta decay, positron decay, and electron-capture reactions that comprise the s-process for a broad range of astrophysical environments was systematically studied. Results were then compared with the solar-system abundances of heavy elements to determine the range of physical conditions responsible for their nucleosynthesis.

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