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

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(0.3 MeV)  =  101±17 keV b and SE2(0.3 MeV)  =  42-23+16 keV b 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.

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