Improving the nuclear physics input along the rp-process path

D. Galaviz; M. Amthor; D. Bazin; B. A. Brown; A. Cole; T. Elliot; A. Estrade; Zs 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; E. Smith; A. Tamii; M. Wallace; R. Zegers

doi:10.1016/j.nuclphysa.2007.01.067

Improving the nuclear physics input along the rp-process path

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

Physics

Research output: Contribution to journal › Article › peer-review

2 Scopus citations

Abstract

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

Original language	English
Pages (from-to)	381-384
Number of pages	4
Journal	Nuclear Physics A
Volume	788
Issue number	1-4
DOIs	https://doi.org/10.1016/j.nuclphysa.2007.01.067
State	Published - May 15 2007

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Galaviz, D., Amthor, M., Bazin, D., Brown, B. A., Cole, A., Elliot, T., Estrade, A., Fülöp, Z., Gade, A., Glasmacher, T., Kessler, R., Lorusso, G., Matos, M., Montes, F., Müller, W., Pereira, J., Schatz, H., Sherrill, B., Schertz, F., ... Zegers, R. (2007). Improving the nuclear physics input along the rp-process path. Nuclear Physics A, 788(1-4), 381-384. https://doi.org/10.1016/j.nuclphysa.2007.01.067

@article{e56ebd3712eb4c058a1577df9c593a19,

title = "Improving the nuclear physics input along the rp-process path",

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

author = "D. Galaviz and M. Amthor and D. Bazin and Brown, {B. A.} and A. Cole and T. Elliot and A. Estrade and Zs F{\"u}l{\"o}p and A. Gade and T. Glasmacher and R. Kessler and G. Lorusso and M. Matos and F. Montes and W. M{\"u}ller and J. Pereira and H. Schatz and B. Sherrill and F. Schertz and Y. Shimbara and E. Smith and A. Tamii and M. Wallace and R. Zegers",

note = "Funding Information: ∗This work was supported by the U.S. National Science Foundation Grants No. PHY-01-10253 (NSCL) and No. PHY-02-016783 (JINA)",

year = "2007",

month = may,

day = "15",

doi = "10.1016/j.nuclphysa.2007.01.067",

language = "English",

volume = "788",

pages = "381--384",

journal = "Nuclear Physics A",

issn = "0375-9474",

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Galaviz, D, Amthor, M, Bazin, D, Brown, BA, Cole, A, Elliot, T, Estrade, A, Fülöp, Z, 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 2007, 'Improving the nuclear physics input along the rp-process path', Nuclear Physics A, vol. 788, no. 1-4, pp. 381-384. https://doi.org/10.1016/j.nuclphysa.2007.01.067

TY - JOUR

T1 - Improving the nuclear physics input along the rp-process path

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

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.

N1 - Funding Information: ∗This work was supported by the U.S. National Science Foundation Grants No. PHY-01-10253 (NSCL) and No. PHY-02-016783 (JINA)

PY - 2007/5/15

Y1 - 2007/5/15

N2 - The level structure of 30S was studied at the NSCL by using neutron removal reactions with a radioactive 31S beam. The γ-decay from excited states in 30S was measured in a Ge-detector array. The results discussed for this work will reduce the uncertainties in the determination of the astrophysical 29P(p,γ)30S reaction rate under rp-process conditions.

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

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U2 - 10.1016/j.nuclphysa.2007.01.067

DO - 10.1016/j.nuclphysa.2007.01.067

M3 - Article

AN - SCOPUS:34248140234

SN - 0375-9474

VL - 788

SP - 381

EP - 384

JO - Nuclear Physics A

JF - Nuclear Physics A

IS - 1-4

ER -

Improving the nuclear physics input along the rp-process path

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