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

Title: Averaging cross section data so we can fit it

Abstract

The 56Fe cross section we are interested in have a lot of fluctuations. We would like to fit the average of the cross section with cross sections calculated within EMPIRE. EMPIRE is a Hauser-Feshbach theory based nuclear reaction code, requires cross sections to be smoothed using a Lorentzian profile. The plan is to fit EMPIRE to these cross sections in the fast region (say above 500 keV).

Authors:
 [1]
  1. Brookhaven National Lab. (BNL), Upton, NY (United States). NNDC
Publication Date:
Research Org.:
Brookhaven National Lab. (BNL), Upton, NY (United States). National Nuclear Data Center (NNDC)
Sponsoring Org.:
USDOE Office of Science (SC)
OSTI Identifier:
1164790
Report Number(s):
BNL-106328-2014-IR
R&D Project: EST-003-NEFA; KB0301041; TRN: US1500129
DOE Contract Number:  
AC02-98CH10886
Resource Type:
Technical Report
Country of Publication:
United States
Language:
English
Subject:
73 NUCLEAR PHYSICS AND RADIATION PHYSICS; CROSS SECTIONS; IRON 56 TARGET; HAUSER-FESHBACH THEORY; MEV RANGE 01-10; NEUTRON REACTIONS; ELASTIC SCATTERING; INELASTIC SCATTERING; CAPTURE; GAMMA RADIATION; IRON 57; TOTAL CROSS SECTIONS; DATA ANALYSIS; national nuclear data center

Citation Formats

Brown, D. Averaging cross section data so we can fit it. United States: N. p., 2014. Web. doi:10.2172/1164790.
Brown, D. Averaging cross section data so we can fit it. United States. doi:10.2172/1164790.
Brown, D. Thu . "Averaging cross section data so we can fit it". United States. doi:10.2172/1164790. https://www.osti.gov/servlets/purl/1164790.
@article{osti_1164790,
title = {Averaging cross section data so we can fit it},
author = {Brown, D.},
abstractNote = {The 56Fe cross section we are interested in have a lot of fluctuations. We would like to fit the average of the cross section with cross sections calculated within EMPIRE. EMPIRE is a Hauser-Feshbach theory based nuclear reaction code, requires cross sections to be smoothed using a Lorentzian profile. The plan is to fit EMPIRE to these cross sections in the fast region (say above 500 keV).},
doi = {10.2172/1164790},
journal = {},
number = ,
volume = ,
place = {United States},
year = {Thu Oct 23 00:00:00 EDT 2014},
month = {Thu Oct 23 00:00:00 EDT 2014}
}

Technical Report:

Save / Share: