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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: [email protected]
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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

References

Bao, Z.Y., Beer, H., Käppeler, F., Voss, F., Wisshak, K. & Rauscher, T., 2000, ADNDT, 76, 70 CrossRefGoogle Scholar
Beer, H., 1991, ApJ, 375, 823 Google Scholar
Couture, A. & Reifarth, R., 2007, ADNDT, 93, 807 Google Scholar
Jaag, S. & Käppeler, F., 1996, PhRvC, 53, 2474 Google Scholar
Käppeler, F., Beer, H. & Wisshak, K., 1989, RPPh, 52, 945 Google Scholar
Knie, K., Korschinek, G., Faestermann, T., Dorfi, E. A., Rugel, G. & Wallner, A., 2004, PhRvL, 93, 171103Google Scholar
Koehler, P. E., 2001, NIMPA, 460, 352 Google Scholar
Lugaro, M., Herwig, F., Lattanzio, J. C., Gallino, R. & Straniero, O., 2003, ApJ, 586, 1305 Google Scholar
Ratynski, W. & Käppeler, F., 1988, PhRvC, 37, 595 Google Scholar
Reifarth, R. et al., 2002, PhRvC, 666, 064603Google Scholar
Reifarth, R. et al., 2003, ApJ, 582, 1251 Google Scholar
Reifarth, R., Haight, R. C., Heil, M., Käppeler, F. & Vieira, D. J., 2004, NIMPA, 524, 215 Google Scholar
Uberseder, E. et al., 2009, PhRvL, 102, 151101Google Scholar
Walter, S., Heil, M., Käppeler, F., Plag, R. & Reifarth, R., 2006, AIPC, 819, 307 Google Scholar
Wisshak, K., Guber, K., Käppeler, F., Krisch, J., Müller, H., Rupp, G. & Voss, F., 1990, NIMPA, 292, 595 Google Scholar