Astrophysical S factor for the B11(d,n)C12 reaction below 135 keV


Journal Article

The B11(d,n)C12 reaction was studied using deuteron beams of 120-160 keV to determine the absolute astrophysical S factors and cross sections for the n0 and n1 neutron groups. The slopes of the S factors are consistent with zero for both the n0 and n1 cases. The measured S factor for the sum of both neutron groups at c.m. energies below 135 keV is S=3180±480 keV b. A DWBA calculation is able to reproduce the ratio of the S factors found here to those obtained in a recent study of the Li7(d,n0,1)Be8 reaction. © 2006 The American Physical Society.

Full Text

Duke Authors

Cited Authors

  • Parpottas, Y; Ahmed, MW; Blackston, MA; Perdue, BA; Prior, RM; Sabourov, A; Spraker, MC; Weller, HR

Published Date

  • July 25, 2006

Published In

Volume / Issue

  • 74 / 1

Electronic International Standard Serial Number (EISSN)

  • 1089-490X

International Standard Serial Number (ISSN)

  • 0556-2813

Digital Object Identifier (DOI)

  • 10.1103/PhysRevC.74.015804

Citation Source

  • Scopus