High precision measurements along the rp-process path

D. Galaviz, M. Amthor, D. Bazin, B. A. Brown, A. Cole, T. Elliot, A. Estrade, Zs. S. Fülöp, A. Gade, T. Glasmacher, R. Kessler, G. Lorusso, M. Matos, F. Montes, W. Müller, J. Pereira, H. Schatz, B. Sherrill, F. Schertz, Y. Shimbara & 4 others E. Smith, A. Tamii, M. Wallace, R. Zegers

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

The level structure of 30S and 31Cl was studied at the NSCL by using neutron removal reactions with a radioactive 31S and 32Cl beam, respectively. The γ -decay from excited states in 30S and 31Cl was measured in a Ge-detector array. The results discussed for this work may reduce the uncertainties in the determination of the 29P(p,γ )30S and 30S(p,γ )31Cl astrophysical reaction rates under rp-process conditions.

Original languageEnglish
Title of host publicationProceedings of Science
Publication statusPublished - 2006
Event9th International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos, NIC 2006 - Geneva, Switzerland
Duration: Jun 25 2006Jun 30 2006

Other

Other9th International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos, NIC 2006
CountrySwitzerland
CityGeneva
Period6/25/066/30/06

Fingerprint

astrophysics
reaction kinetics
neutrons
detectors
decay
excitation

ASJC Scopus subject areas

  • General

Cite this

Galaviz, D., Amthor, M., Bazin, D., Brown, B. A., Cole, A., Elliot, T., ... Zegers, R. (2006). High precision measurements along the rp-process path. In Proceedings of Science

High precision measurements along the rp-process path. / Galaviz, D.; Amthor, M.; Bazin, D.; Brown, B. A.; Cole, A.; Elliot, T.; Estrade, A.; Fülöp, Zs. S.; Gade, A.; Glasmacher, T.; Kessler, R.; Lorusso, G.; Matos, M.; Montes, F.; Müller, W.; Pereira, J.; Schatz, H.; Sherrill, B.; Schertz, F.; Shimbara, Y.; Smith, E.; Tamii, A.; Wallace, M.; Zegers, R.

Proceedings of Science. 2006.

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Galaviz, D, Amthor, M, Bazin, D, Brown, BA, Cole, A, Elliot, T, Estrade, A, Fülöp, ZS, Gade, A, Glasmacher, T, Kessler, R, Lorusso, G, Matos, M, Montes, F, Müller, W, Pereira, J, Schatz, H, Sherrill, B, Schertz, F, Shimbara, Y, Smith, E, Tamii, A, Wallace, M & Zegers, R 2006, High precision measurements along the rp-process path. in Proceedings of Science. 9th International Symposium on Nuclear Astrophysics - Nuclei in the Cosmos, NIC 2006, Geneva, Switzerland, 6/25/06.
Galaviz D, Amthor M, Bazin D, Brown BA, Cole A, Elliot T et al. High precision measurements along the rp-process path. In Proceedings of Science. 2006
Galaviz, D. ; Amthor, M. ; Bazin, D. ; Brown, B. A. ; Cole, A. ; Elliot, T. ; Estrade, A. ; Fülöp, Zs. S. ; Gade, A. ; Glasmacher, T. ; Kessler, R. ; Lorusso, G. ; Matos, M. ; Montes, F. ; Müller, W. ; Pereira, J. ; Schatz, H. ; Sherrill, B. ; Schertz, F. ; Shimbara, Y. ; Smith, E. ; Tamii, A. ; Wallace, M. ; Zegers, R. / High precision measurements along the rp-process path. Proceedings of Science. 2006.
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abstract = "The level structure of 30S and 31Cl was studied at the NSCL by using neutron removal reactions with a radioactive 31S and 32Cl beam, respectively. The γ -decay from excited states in 30S and 31Cl was measured in a Ge-detector array. The results discussed for this work may reduce the uncertainties in the determination of the 29P(p,γ )30S and 30S(p,γ )31Cl astrophysical reaction rates under rp-process conditions.",
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AU - Galaviz, D.

AU - Amthor, M.

AU - Bazin, D.

AU - Brown, B. A.

AU - Cole, A.

AU - Elliot, T.

AU - Estrade, A.

AU - Fülöp, Zs. S.

AU - Gade, A.

AU - Glasmacher, T.

AU - Kessler, R.

AU - Lorusso, G.

AU - Matos, M.

AU - Montes, F.

AU - Müller, W.

AU - Pereira, J.

AU - Schatz, H.

AU - Sherrill, B.

AU - Schertz, F.

AU - Shimbara, Y.

AU - Smith, E.

AU - Tamii, A.

AU - Wallace, M.

AU - Zegers, R.

PY - 2006

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AB - The level structure of 30S and 31Cl was studied at the NSCL by using neutron removal reactions with a radioactive 31S and 32Cl beam, respectively. The γ -decay from excited states in 30S and 31Cl was measured in a Ge-detector array. The results discussed for this work may reduce the uncertainties in the determination of the 29P(p,γ )30S and 30S(p,γ )31Cl astrophysical reaction rates under rp-process conditions.

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