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Opportunities for Nuclear Astrophysics at FRANZ

Published online by Cambridge University Press:  05 March 2013

R. Reifarth ,
L. P. Chau ,
M. Heil ,
F. Käppeler ,
O. Meusel ,
R. Plag ,
U. Ratzinger ,
A. Schempp  and
K. Volk
R. Reifarth*
Affiliation:
Gesellschaft für Schwerionenforschung mbH, Darmstadt, D-64291, Germany J.W. Goethe-Universität, Frankfurt a.M, D-60438, Germany
L. P. Chau
Affiliation:
J.W. Goethe-Universität, Frankfurt a.M, D-60438, Germany
M. Heil
Affiliation:
Gesellschaft für Schwerionenforschung mbH, Darmstadt, D-64291, Germany
F. Käppeler
Affiliation:
Forschungszentrum Karlsruhe, Karlsruhe, D-76021, Germany
O. Meusel
Affiliation:
J.W. Goethe-Universität, Frankfurt a.M, D-60438, Germany
R. Plag
Affiliation:
Gesellschaft für Schwerionenforschung mbH, Darmstadt, D-64291, Germany J.W. Goethe-Universität, Frankfurt a.M, D-60438, Germany
U. Ratzinger
Affiliation:
J.W. Goethe-Universität, Frankfurt a.M, D-60438, Germany
A. Schempp
Affiliation:
J.W. Goethe-Universität, Frankfurt a.M, D-60438, Germany
K. Volk
Affiliation:
J.W. Goethe-Universität, Frankfurt a.M, D-60438, Germany
*
DCorresponding author. Email: r.reifarth@gsi.de
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Abstract

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The ‘Frankfurter Neutronenquelle am Stern–Gerlach–Zentrum’ (FRANZ), which is currently under development, will be the strongest neutron source in the astrophysically interesting energy region in the world. It will be about three orders of magnitude more intense than the well-established neutron source at the Research Center Karlsruhe (FZK).

Keywords

nuclear reactions, nucleosynthesis, abundances
Type
s-Process and n Capture
Information
Publications of the Astronomical Society of Australia , Volume 26 , Issue 3 , 2009 , pp. 255 - 258
Copyright
Copyright © Astronomical Society of Australia 2009

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