Nonresonant capture cross sections of 11 B (n,γ) and 12 C (n,γ) at stellar energies

Details Nonresonant capture cross sections of 11 B (n,γ) and 12 C (n,γ) at stellar energies Nonresonant capture cross sections of 11 B (n,γ) and 12 C (n,γ) at stellar energies

Oct 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003phrvc..68d7601l&link_type=abstract

Physical Review C, vol. 68, Issue 4, id. 047601

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3

Radiative Capture, Hydrostatic Stellar Nucleosynthesis, Nucleosynthesis In Novae, Supernovae, And Other Explosive Environments, 6<=A<=19

Scientific paper

The nonresonant direct radiative capture (DRC) cross sections of 11 B (n,γ) and 12 C (n,γ) at stellar energies are deduced by means of the asymptotic normalization coefficient (ANC) method. The ANC factors were extracted from the peripheral transfer reactions of 11 B (d,p) and 12 C (d,p) . The deduced DRC cross sections of 12 C (n,γ) are in good agreement with experimental results of direct measurement. The DRC cross sections of 11 B (n,γ) at low energies are obtained for the first time.

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