Abstract
The cross section for is calculated at energies relevant to big-bang nucleosynthesis using the recently developed effective field theory that describes the two-nucleon sector. The amplitude is computed up to and depends only upon nucleon-nucleon phase shift data. In contrast, the contribution is computed up to next-to-leading order, and the four-nucleon-one-magnetic-photon counterterm that enters is determined by the cross section for cold neutron capture. The uncertainty in the calculation for nucleon energies up to is estimated to be
- Received 27 July 1999
DOI:https://doi.org/10.1103/PhysRevC.60.065205
©1999 American Physical Society