Two experimental approaches in nuclear astrophysics using neutrons

Details Two experimental approaches in nuclear astrophysics using neutrons Two experimental approaches in nuclear astrophysics using neutrons

May 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1012..160p&link_type=abstract

FRONTIERS IN NUCLEAR STRUCTURE, ASTROPHYSICS, AND REACTIONS: FINUSTAR 2. AIP Conference Proceedings, Volume 1012, pp. 160-164 (

Astronomy and Astrophysics

Astrophysics

Atmospheres, Neutron Absorption, Transfer Reactions

Scientific paper

High resolution measurements using the (3He,n) reaction are used to determine excitation energies of astrophysically important states. Further, spins can be assigned to these states by comparing the measured differential cross sections to Hauser-Feshbach cross sections. The astrophysical reaction rates are then calculated using the experimental values. Reference [1] is an example of such measurements.
Absolute values of the astrophysical S factors and cross sections are calculated from measurements using the (d,n) reaction at low incident energies. Reference [2] is an example of such measurements.

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