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Neutron exposure and neutron flux in Asymptotic Giant Branch stars: a study of neutron capture cross sections of Zr isotopes

Giuseppe Tagliente UGent (2011)
abstract
Nuclear astrophysics is an interdisciplinary branch of physics involving close collaboration among researchers in various subfields of nuclear physics and astrophysics, with significant emphasis in areas such as stellar modeling, measurement and theoretical estimation of nuclear reaction rates, cosmology, cosmochemistry, gamma ray, optical and X-ray astronomy. In general terms, nuclear astrophysics aims to understand the origin of the chemical elements and the energy generation in stars. This work concerns the measurements of the neutron capture cross sections of 90,91,92,93,94,96Zr isotopes, performed at the time-of-flight facilities n_TOF at CERN and GELINA at IRMM and their implication in stellar modeling.
Please use this url to cite or link to this publication:
author
promoter
UGent and UGent
organization
year
type
dissertation
publication status
published
subject
keyword
Nuclear Physics, Astrophysics
pages
191 pages
publisher
Ghent University. Faculty of Sciences
place of publication
Ghent, Belgium
defense location
Gent : Het Pand (zaal rector Blancquaert)
defense date
2011-04-28 17:00
language
English
UGent publication?
yes
classification
D1
copyright statement
I have retained and own the full copyright for this publication
id
1211593
handle
http://hdl.handle.net/1854/LU-1211593
date created
2011-04-22 12:34:49
date last changed
2017-01-16 10:38:02
@phdthesis{1211593,
  abstract     = {Nuclear astrophysics is an interdisciplinary branch of physics involving close collaboration among researchers in various subfields of nuclear physics and astrophysics, with significant emphasis in areas such as stellar modeling, measurement and theoretical estimation of nuclear reaction rates, cosmology, cosmochemistry, gamma ray, optical and X-ray astronomy. In general terms, nuclear astrophysics aims to understand the origin of the chemical elements and the energy generation in stars.
This work concerns the measurements of the neutron capture cross sections of 90,91,92,93,94,96Zr isotopes, performed at the time-of-flight facilities n\_TOF at CERN and GELINA at IRMM and their implication in stellar modeling.},
  author       = {Tagliente, Giuseppe},
  keyword      = {Nuclear Physics,Astrophysics},
  language     = {eng},
  pages        = {191},
  publisher    = {Ghent University. Faculty of Sciences},
  school       = {Ghent University},
  title        = {Neutron exposure and neutron flux in Asymptotic Giant Branch stars: a study of neutron capture cross sections of Zr isotopes},
  year         = {2011},
}

Chicago
Tagliente, Giuseppe. 2011. “Neutron Exposure and Neutron Flux in Asymptotic Giant Branch Stars: a Study of Neutron Capture Cross Sections of Zr Isotopes”. Ghent, Belgium: Ghent University. Faculty of Sciences.
APA
Tagliente, G. (2011). Neutron exposure and neutron flux in Asymptotic Giant Branch stars: a study of neutron capture cross sections of Zr isotopes. Ghent University. Faculty of Sciences, Ghent, Belgium.
Vancouver
1.
Tagliente G. Neutron exposure and neutron flux in Asymptotic Giant Branch stars: a study of neutron capture cross sections of Zr isotopes. [Ghent, Belgium]: Ghent University. Faculty of Sciences; 2011.
MLA
Tagliente, Giuseppe. “Neutron Exposure and Neutron Flux in Asymptotic Giant Branch Stars: a Study of Neutron Capture Cross Sections of Zr Isotopes.” 2011 : n. pag. Print.