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Time-Scales of the s Process: from Minutes to Ages

Published online by Cambridge University Press:  05 March 2013

F. Käppeler ,
S. Bisterzo ,
R. Gallino ,
M. Heil ,
M. Pignatari ,
R. Reifarth ,
O. Straniero ,
S. Walter ,
N. Winckler  and
K. Wisshak
F. Käppeler*
Affiliation:
Forschungszentrum Karlsruhe, Institut für Kernphysik, P.O. Box 3640, D-76021 Karlsruhe, Germany
S. Bisterzo
Affiliation:
Dipartimento di Fisica Generale, Universitá di Torino, Via P. Giuria 1, I-10125 Torino, Italy
R. Gallino
Affiliation:
Dipartimento di Fisica Generale, Universitá di Torino, Via P. Giuria 1, I-10125 Torino, Italy
M. Heil
Affiliation:
GSI Darmstadt, Planckstr. 1, D-64291 Darmstadt, Germany
M. Pignatari
Affiliation:
Keele University, Keele, Staffordshire ST5 5BG, UK Joint Institute for Nuclear Astrophysics, University of Notre Dame, Notre Dame, IN 46556, USA
R. Reifarth
Affiliation:
GSI Darmstadt, Planckstr. 1, D-64291 Darmstadt, Germany
O. Straniero
Affiliation:
Osservatorio Astronomico di Collurania, I-64100 Teramo, Italy
S. Walter
Affiliation:
Forschungszentrum Karlsruhe, Institut für Kernphysik, P.O. Box 3640, D-76021 Karlsruhe, Germany
N. Winckler
Affiliation:
GSI Darmstadt, Planckstr. 1, D-64291 Darmstadt, Germany
K. Wisshak
Affiliation:
Forschungszentrum Karlsruhe, Institut für Kernphysik, P.O. Box 3640, D-76021 Karlsruhe, Germany
*
CCorresponding author. Email: [email protected]
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Abstract

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The time scales in the s process appears to be an approriate aspect to discuss at the occasion of Roberto's 70th anniversary, the more as this subject has been repeatedly addressed during the 20 years of collaboration between Torino and Karlsruhe. The two chronometers presented in this text were selected to illustrate the intense mutual stimulation of both groups. Based on a reliable set of accurate stellar (n, γ) cross sections determined mostly at FZK, the Torino group succeeded to develop a comprehensive picture of the various s-process scenarios, which are most valuable for understanding the composition of the solar system as well as for the interpretation of an increasing number of astronomical observations.

Keywords

stars: AGBnuclear reactions, nucleosynthesis, abundancestime
Type
s-Process and n Capture
Information
Publications of the Astronomical Society of Australia , Volume 26 , Issue 3 , 2009 , pp. 209 - 216
Copyright
Copyright © Astronomical Society of Australia 2009

References

Allen, B. J., Lowenthal, G. C. & de Laeter, J. R., 1981, JPhGS, 7, 1271 Google Scholar
Arlandini, C., Käppeler, F., Wisshak, K., Gallino, R., Lugaro, M., Busso, M. & Straniero, O., 1999, ApJ, 525, 886 Google Scholar
Arnould, M., 1973, A&A, 22, 311 Google Scholar
Arnould, M. & Goriely, S., 2003, PhR, 384, 1 Google Scholar
Arnould, M., Takahashi, K. & Yokoi, K., 1984, A&A, 137, 51 Google Scholar
Audouze, J., Fowler, W. A. & Schramm, D. N., 1972, NPhS, 238, 8 Google Scholar
Bao, Z. Y., Beer, H., Käppeler, F., Voss, F., Wisshak, K. & Rauscher, T., 2000, ADNDT, 76, 70 Google Scholar
Beer, H. & Käppeler, F., 1980, PhRvC, 21, 534 Google Scholar
Beer, H. & Walter, G., 1984, Ap&SS, 100, 243 Google Scholar
Beer, H. & Penzhorn, R.-D., 1987, A&A, 174, 323 Google Scholar
Beer, H., Käppeler, F., Wisshak, K. & Ward, R. A., 1981, ApJS, 46, 295 Google Scholar
Beer, H., Walter, G., Macklin, R. L. & Patchett, P. J., 1984, PhRvC, 30, 464 Google Scholar
Best, J., Stoll, H., Arlandini, C., Jaag, S., Käppeler, F., Wisshak, K., Mengoni, A., Reffo, G. & Rauscher, T., 2001, PhRvC, 64, 15801 Google Scholar
Busso, M., Lambert, D. L., Beglio, L., Gallino, R., Raiteri, C. M. & Smith, V. V., 1995, ApJ, 446, 775 CrossRefGoogle Scholar
Busso, M., Gallino, R. & Wasserburg, G. J., 1999, ARA&A, 37, 239 Google Scholar
Chieffi, A. & Straniero, O., 1989, ApJS, 71, 47 CrossRefGoogle Scholar
Cowan, J. J., Pfeiffer, B., Kratz, K.-L., Thielemann, F.-K., Sneden, C., Burles, S., Tytler, D. & Beers, T. C., 1999, ApJ, 521, 194 CrossRefGoogle Scholar
Doll, C., Börner, H., Jaag, S. & Käppeler, F., 1999, PhRvC, 59, 492 Google Scholar
Gallino, R., Busso, M., Picchio, G., Raiteri, C. M. & Renzini, A., 1988, ApJ, 334, L45 CrossRefGoogle Scholar
Gallino, R., Arlandini, C., Busso, M., Lugaro, M., Travaglio, C., Straniero, O., Chieffi, A. & Limongi, M., 1998, ApJ, 497, 388 Google Scholar
Heil, M., Winckler, N., Dababneh, S., Käppeler, F., Wisshak, K., Bisterzo, S., Gallino, R., Davis, A. M. & Rauscher, T., 2008, ApJ, 673, 434 CrossRefGoogle Scholar
Klay, N., Käppeler, F., Beer, H. & Schatz, G., 1991, PhRvC, 44, 2839 Google Scholar
Klay, N. et al., 1991, PhRvC, 44, 2801 Google Scholar
Kneissl, U., 2005, Bulg. Nucl. Sci. Trans., 10, 55 Google Scholar
Mathews, G. J., Takahashi, K., Ward, R. A. & Howard, W. M., 1986, ApJ, 302, 410 Google Scholar
Mohr, P., 2008, PoS, NIC X, 081Google Scholar
Mosconi, M. et al., 2007, PrPNP, 59, 165 Google Scholar
Pagel, B. E. J., 1990, in Astrophysical Ages and Dating Meth-ods, Eds. Vangioni-Flam, E., Cassé, M., Audouze, J. & Tran Thanh Van, J. (Gif surYvette: Editions Frontières), 493 Google Scholar
Pepin, R. O., Becker, R. H. & Rider, P. E., 1995, GeCoA, 59, 4997 Google Scholar
Reifarth, R. & Käppeler, F., 2002, PhRvC, 66, 054605Google Scholar
Reifarth, R. et al., 2002, PhRvC, 66, 064603Google Scholar
Reifarth, R., Käppeler, F., Voss, F., Wisshak, K., Gallino, R., Pignatari, M. & Straniero, O., 2004, ApJ, 614, 363 Google Scholar
Schatz, G., 1983, A&A, 122, 327 Google Scholar
Smith, V. V. & Lambert, D. L., 1988, ApJ, 333, 219 CrossRefGoogle Scholar
Stecher-Rasmussen, F., Abrahams, K., Kopecky, J., Lindner, J. & Polak, P., 1988, in Inst. Phys. Conf. Ser. 88, Capture Gamma-Ray Spectroscopy 1987, Eds. Abrahams, K. & Van Assche, P. (Bristol: Institute of Physics), 754 Google Scholar
Straniero, O., Gallino, R., Busso, M., Chieffi, A., Raiteri, C. M., Limongi, M. & Salaris, M., 1995, ApJ, 440, L85 Google Scholar
Straniero, O., Chieffi, A., Limongi, M., Busso, M., Gallino, R. & Arlandini, C., 1997, ApJ, 478, 332 Google Scholar
Straniero, O., Domínguez, I., Cristallo, R. & Gallino, R., 2003, PASA, 20, 389 Google Scholar
Straniero, O., Gallino, R. & Cristallo, S., 2006, NPhA, 777, 311 Google Scholar
Takahashi, K. & Yokoi, K., 1987, ADNDT, 36, 375 Google Scholar
Vanhorenbeek, J., Lagrange, J. M., Pautrat, M., Dionisio, J. S. & Vieu, Ch., 2000, PhRvC, 62, 015801Google Scholar
Ward, R. A. & Fowler, W. A., 1980, ApJ, 238, 266 Google Scholar
Wisshak, K. et al., 2001, PhRvL, 87, 251102Google Scholar
Wisshak, K., Voss, F., Käppeler, F. & Kazakov, L., 2006, PhRvC, 73, 015807Google Scholar
Yokoi, K., Takahashi, K. & Arnould, M., 1983, A&A, 117, 65 Google Scholar
Yokoi, K., Takahashi, K. & Arnould, M., 1985, A&A, 145, 339 Google Scholar
Zhao, W. R. & Käppeler, F., 1991, PhRvC, 44, 506 Google Scholar