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:
-
- 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. https://doi.org/10.2172/1164790
Brown, D. 2014.
"Averaging cross section data so we can fit it". United States. https://doi.org/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},
url = {https://www.osti.gov/biblio/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}
}
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