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The 41Ca(n,α)38Ar cross section up to 100 keV neutron energy

Cyrillus Wagemans UGent, Sofie Vermote UGent and J Van Gils (2010) POS PROCEEDINGS OF SCIENCE.
abstract
The 41Ca(n,alpha)38Ar reaction cross section has been studied with resonance neutrons at the GELINA neutron facility of the Institute for Reference Materials and Measurements in Geel (Belgium) from a few eV up to 100 keV. A Frisch-gridded ionization chamber with methane as detector gas was installed at a 30 meter long flight path. About 20 resonances have been identified. From the cross section data obtained, the Maxwellian averaged cross section (MACS) as a function of stellar temperature has been calculated by numerical integration.
Please use this url to cite or link to this publication:
author
organization
alternative title
The 41Ca(n,alpha)38Ar cross section up to 100 keV neutron energy
year
type
conference
publication status
published
subject
in
POS PROCEEDINGS OF SCIENCE
PoS Proc. Sci.
article number
PoS(NIC XI)199
pages
6 pages
conference name
11th Symposium on Nuclei in the Cosmos (NIC XI)
conference location
Heidelberg, Germany
conference start
2010-07-19
conference end
2010-07-23
ISSN
1824-8039
language
English
UGent publication?
yes
classification
C1
copyright statement
I have retained and own the full copyright for this publication
id
1105947
handle
http://hdl.handle.net/1854/LU-1105947
alternative location
http://pos.sissa.it/archive/conferences/100/199/NIC%20XI_199.pdf
date created
2011-01-20 14:10:04
date last changed
2016-12-21 15:40:42
@inproceedings{1105947,
  abstract     = {The 41Ca(n,alpha)38Ar reaction cross section has been studied with resonance neutrons at the GELINA neutron facility of the Institute for Reference Materials and Measurements in Geel (Belgium) from a few eV up to 100 keV. A Frisch-gridded ionization chamber with methane as detector gas was installed at a 30 meter long flight path. About 20 resonances have been identified. From the cross section data obtained, the Maxwellian averaged cross section (MACS) as a function of stellar temperature has been calculated by numerical integration.},
  articleno    = {PoS(NIC XI)199},
  author       = {Wagemans, Cyrillus and Vermote, Sofie and Van Gils, J},
  booktitle    = {POS PROCEEDINGS OF SCIENCE},
  issn         = {1824-8039},
  language     = {eng},
  location     = {Heidelberg, Germany},
  pages        = {6},
  title        = {The 41Ca(n,\ensuremath{\alpha})38Ar cross section up to 100 keV neutron energy},
  url          = {http://pos.sissa.it/archive/conferences/100/199/NIC\%20XI\_199.pdf},
  year         = {2010},
}

Chicago
Wagemans, Cyrillus, Sofie Vermote, and J Van Gils. 2010. “The 41Ca(n,α)38Ar Cross Section up to 100 keV Neutron Energy.” In Pos Proceedings of Science.
APA
Wagemans, Cyrillus, Vermote, S., & Van Gils, J. (2010). The 41Ca(n,α)38Ar cross section up to 100 keV neutron energy. POS PROCEEDINGS OF SCIENCE. Presented at the 11th Symposium on Nuclei in the Cosmos (NIC XI).
Vancouver
1.
Wagemans C, Vermote S, Van Gils J. The 41Ca(n,α)38Ar cross section up to 100 keV neutron energy. POS PROCEEDINGS OF SCIENCE. 2010.
MLA
Wagemans, Cyrillus, Sofie Vermote, and J Van Gils. “The 41Ca(n,α)38Ar Cross Section up to 100 keV Neutron Energy.” Pos Proceedings of Science. 2010. Print.