A recoil separator for nuclear astrophysics SECAR

Authors

G. P.A. Berg, University of Notre Dame
D. W. Bardayan, University of Notre Dame
J. C. Blackmon, Louisiana State University
K. A. Chipps, ORNL Physics Division
M. Couder, University of Notre Dame
U. Greife, Colorado School of Mines
U. Hager, Michigan State University
F. Montes, Michigan State University
K. E. Rehm, Argonne National Laboratory
H. Schatz, Michigan State University
M. S. Smith, ORNL Physics Division
M. Wiescher, University of Notre Dame
C. Wrede, Michigan State University
A. Zeller, Michigan State University

Document Type

Article

Publication Date

6-1-2016

Abstract

A recoil separator SECAR has been designed to study radiative capture reactions relevant for the astrophysical rp-process in inverse kinematics for the Facility for Rare Isotope Beams (FRIB). We describe the design, layout, and ion optics of the recoil separator and present the status of the project.

Publication Source (Journal or Book title)

Nuclear Instruments and Methods in Physics Research, Section B: Beam Interactions with Materials and Atoms

First Page

165

Last Page

167

Recommended Citation

Berg, G., Bardayan, D., Blackmon, J., Chipps, K., Couder, M., Greife, U., Hager, U., Montes, F., Rehm, K., Schatz, H., Smith, M., Wiescher, M., Wrede, C., & Zeller, A. (2016). A recoil separator for nuclear astrophysics SECAR. Nuclear Instruments and Methods in Physics Research, Section B: Beam Interactions with Materials and Atoms, 376, 165-167. https://doi.org/10.1016/j.nimb.2016.02.009