Measurement of the Li-8(a,n)B-11 reaction cross section at energies of astrophysical interest

Details Measurement of the Li-8(a,n)B-11 reaction cross section at energies of astrophysical interest Measurement of the Li-8(a,n)B-11 reaction cross section at energies of astrophysical interest

Mar 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992phrvl..68.1283b&link_type=abstract

Physical Review Letters (ISSN 0031-9007), vol. 68, March 2, 1992, p. 1283-1286. Research supported by Institute for Physical and

Astronomy and Astrophysics

Astrophysics

42

Boron, Lithium Isotopes, Nuclear Astrophysics, Nuclear Fusion, Nuclear Reactions, Cross Sections, Ground State, Helium Isotopes

Scientific paper

The cross section for the Li-8(a,n)B-11 reaction - which is crucial to
predictions of primordial nucleosynthesis in inhomogeneous models - is
measured using a radioactive-beam facility. The reaction cross section
to all allowed B-11 states was found to be larger than that to just the
B-11 ground state by about a factor of 5.

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