Neutron Resonance Spectroscopy of 103Rh from 30 eV to 2 keV

Authors

D A. Smith, Los Alamos National LaboratoryFollow
J D. Bowman, Los Alamos National LaboratoryFollow
Bret E. Crawford, Gettysburg CollegeFollow
C A. Grossmann, North Carolina State UniversityFollow
T Haseyama, Kyoto UniversityFollow
A Masaike, Kyoto UniversityFollow
Y Matsuda, Kyoto UniversityFollow
G E. Mitchell, North Carolina State UniversityFollow
S I. Penttila, Los Alamos National LaboratoryFollow
N R. Roberson, Duke UniversityFollow
S J. Seestrom, Los Alamos National LaboratoryFollow
E I. Sharapov, Joint Institute for Nuclear ResearchFollow
Sharon L. Stephenson, Gettysburg CollegeFollow
V W. Yuan, Los Alamos National LaboratoryFollow

Document Type

Article

Publication Date

9-1999

Department 1

Physics

Abstract

Neutron resonances in ¹⁰³Rh have been measured for neutron energies from 30 to 2000 eV using the time-of-flight method and the (n,γ) reaction. The rhodium resonance spectroscopy is essential for the analysis of parity violation measurements recently performed on neutron resonances in ¹⁰³Rh. Neutron scattering and radiative widths were determined, and orbital angular momentum assignments made with a Bayesian analysis. The s-wave and p-wave strength functions and average level spacings were determined.

Copyright Note

This is the publisher's version of the work. This publication appears in Gettysburg College's institutional repository by permission of the copyright owner for personal use, not for redistribution.

Recommended Citation

Smith, D. A., Bowman, J. D., Crawford, B. E., Grossmann, C. A., Haseyama, T., Masaike, A., Matsuda, Y., Mitchell, G. E., Penttila, S. I., Roberson, N. R., Seestrom, S. J., Sharapov, E. I., Stephenson, S., & Yuan, V. W. (1999). Neutron Resonance Spectroscopy of 103Rh from 30 eV to 2 keV. Physical Review C, 60(045502). http://dx.doi.org/10.1103/PhysRevC.60.045502

Required Publisher's Statement

Copyright held by American Physical Society. First published as DA Smith et al, Neutron Resonance Spectroscopy of 103Rh from 30 eV to 2 keV, Physical Review C, 60, 045502, doi: 10.1103/PhysRevC.60.045502.