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Phys. Rev. Lett. 83, 4025–4028 (1999)

Sub-Coulomb α Transfers on 12C and the 12C(α,γ)16O S Factor

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C. R. Brune1, W. H. Geist1,*, R. W. Kavanagh2, and and K. D. Veal1,†
1University of North Carolina, Chapel Hill, North Carolina 27599-3255and Triangle Universities Nuclear Laboratory, Durham, North Carolina 27708-0308
2W. K. Kellogg Radiation Laboratory, California Institute of Technology, Pasadena, California 91125

Received 17 June 1999; published in the issue dated 15 November 1999

The 12C(α,γ)16O reaction is crucial for the understanding of He burning in massive stars, but the low-energy cross section is highly uncertain. To address this problem we have measured at sub-Coulomb energies total cross sections for the 12C(6Li,d)16O and 12C(7Li,t)16O reactions to the bound 2+ and 1- states of 16O. The data are analyzed to obtain the reduced α widths of these states. Together with capture and phase-shift data, these results provide for a more accurate determination of the low-energy 12C(α,γ)16O S factor: SE1(0.3MeV) = 101±17keVb and SE2(0.3MeV) = 42-23+16keVb for the E1 and E2 multipole components of the reaction.

© 1999 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevLett.83.4025
DOI:
10.1103/PhysRevLett.83.4025
PACS:
24.30.-v, 21.10.Pc, 25.70.Hi, 26.20.+f

*Present address: Los Alamos National Laboratory, Los Alamos, NM 87545.