skip to main content
OSTI.GOV title logo U.S. Department of Energy
Office of Scientific and Technical Information

Title: SUGGEL: A Program Suggesting the Orbital Angular Momentum of a Neutron Resonance from the Magnitude of its Neutron Width

Technical Report ·
DOI:https://doi.org/10.2172/777661· OSTI ID:777661

The SUGGEL computer code has been developed to suggest a value for the orbital angular momentum of a neutron resonance that is consistent with the magnitude of its neutron width. The suggestion is based on the probability that a resonance having a certain value of g{Gamma}{sub n} is an l-wave resonance. The probability is calculated by using Bayes' theorem on the conditional probability. The probability density functions (pdf's) of g{Gamma}{sub n} for up to d-wave (l=2) have been derived from the {chi}{sup 2} distribution of Porter and Thomas. The pdf's take two possible channel spins into account. This code is a tool which evaluators will use to construct resonance parameters and help to assign resonance spin. The use of this tool is expected to reduce time and effort in the evaluation procedure, since the number of repeated runs of the fitting code (e.g., SAMMY) may be reduced.

Research Organization:
Oak Ridge National Lab. (ORNL), Oak Ridge, TN (United States)
Sponsoring Organization:
US Department of Energy (US)
DOE Contract Number:
AC05-96OR22464
OSTI ID:
777661
Report Number(s):
ORNL/TM-2000/314; TRN: US0102047
Resource Relation:
Other Information: PBD: 2 Feb 2001
Country of Publication:
United States
Language:
English

Similar Records

Statistical Assignment of Neutron Orbital Angular Momentum to a Resonance
Journal Article · Wed Sep 15 00:00:00 EDT 2004 · Nuclear Science and Engineering · OSTI ID:777661

Neutron resonance parameters of /sup 68//sub 30/Zn+n and statistical distributions of level spacings and widths
Journal Article · Thu Apr 01 00:00:00 EST 1982 · Phys. Rev. C; (United States) · OSTI ID:777661

Neutron resonance spectroscopy. XII. The separated isotopes of W
Journal Article · Thu Nov 01 00:00:00 EST 1973 · Phys. Rev., C, v. 8, no. 5, pp. 1813-1826 · OSTI ID:777661