#### Title

Kinematically complete measurement of the [Formula Presented] excitation function for the astrophysically important 7.08-MeV state in [Formula Presented]

#### Document Type

Article

#### Publication Date

1-1-2000

#### Abstract

Knowledge of the astrophysical [Formula Presented] rate is important for understanding gamma-ray emission from novae and heavy-element production in x-ray bursts. A state with [Formula Presented] in [Formula Presented] provides an s-wave resonance and, depending on its properties, could dominate the [Formula Presented] rate. By measuring a kinematically complete [Formula Presented] excitation function with a radioactive [Formula Presented] beam at the ORNL Holifield Radioactive Ion Beam Facility, we find that the [Formula Presented] state lies at a center-of-mass energy of [Formula Presented] has a total width of [Formula Presented] and a proton partial-width of [Formula Presented]. © 2000 The American Physical Society.

#### Publication Source (Journal or Book title)

Physical Review C - Nuclear Physics

#### First Page

4

#### Recommended Citation

Bardayan, D., Blackmon, J., Bradfield-Smith, W., Brune, C., Champagne, A., Davinson, T., Johnson, B., Kozub, R., Lee, C., Lewis, R., Parker, P., Shotter, A., Smith, M., Visser, D., & Woods, P.
(2000). Kinematically complete measurement of the [Formula Presented] excitation function for the astrophysically important 7.08-MeV state in [Formula Presented].* Physical Review C - Nuclear Physics**, 62* (4), 4.
https://doi.org/10.1103/PhysRevC.62.042802