First measurement of the 33Cl(p,α)30S reaction

C. M. Deibel; K. E. Rehm; J. M. Figueira; J. P. Greene; C. L. Jiang; B. P. Kay; H. Y. Lee; J. C. Lighthall; S. T. Marley; R. C. Pardo; N. Patel; M. Paul; C. Ugalde; A. Woodard; A. H. Wuosmaa; G. Zinkann

doi:10.1103/PhysRevC.84.045802

First measurement of the 33Cl(p,α)30S reaction

C. M. Deibel^*
, K. E. Rehm
, J. M. Figueira
, J. P. Greene
, C. L. Jiang
, B. P. Kay
, H. Y. Lee
, J. C. Lighthall
, S. T. Marley
, R. C. Pardo
, N. Patel
, M. Paul
, C. Ugalde
, A. Woodard
, A. H. Wuosmaa
, G. Zinkann

^*Corresponding author for this work

Racah Institute of Physics

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

20 Scopus citations

Abstract

The 30S(α,p)33Cl reaction may have a significant impact on final elemental abundances and energy output of type I X-ray bursts, as well as influencing observables such as double-peaked luminosity profiles, because it could bypass the 30S waiting point. This reaction has been studied experimentally for the first time in inverse kinematics via the time-inverse reaction 1H(33Cl,30S)α with a 33Cl radioactive ion beam produced at the Argonne Tandem Linac Accelerator System facility by the "in-flight" technique. This reaction was studied at three different beam energies. The experimental method used and the resulting data are discussed.

Original language	English
Article number	045802
Journal	Physical Review C - Nuclear Physics
Volume	84
Issue number	4
DOIs	https://doi.org/10.1103/PhysRevC.84.045802
State	Published - 6 Oct 2011

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Deibel, C. M., Rehm, K. E., Figueira, J. M., Greene, J. P., Jiang, C. L., Kay, B. P., Lee, H. Y., Lighthall, J. C., Marley, S. T., Pardo, R. C., Patel, N., Paul, M., Ugalde, C., Woodard, A., Wuosmaa, A. H., & Zinkann, G. (2011). First measurement of the 33Cl(p,α)30S reaction. Physical Review C - Nuclear Physics, 84(4), Article 045802. https://doi.org/10.1103/PhysRevC.84.045802

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title = "First measurement of the 33Cl(p,α)30S reaction",

abstract = "The 30S(α,p)33Cl reaction may have a significant impact on final elemental abundances and energy output of type I X-ray bursts, as well as influencing observables such as double-peaked luminosity profiles, because it could bypass the 30S waiting point. This reaction has been studied experimentally for the first time in inverse kinematics via the time-inverse reaction 1H(33Cl,30S)α with a 33Cl radioactive ion beam produced at the Argonne Tandem Linac Accelerator System facility by the {"}in-flight{"} technique. This reaction was studied at three different beam energies. The experimental method used and the resulting data are discussed.",

author = "Deibel, \{C. M.\} and Rehm, \{K. E.\} and Figueira, \{J. M.\} and Greene, \{J. P.\} and Jiang, \{C. L.\} and Kay, \{B. P.\} and Lee, \{H. Y.\} and Lighthall, \{J. C.\} and Marley, \{S. T.\} and Pardo, \{R. C.\} and N. Patel and M. Paul and C. Ugalde and A. Woodard and Wuosmaa, \{A. H.\} and G. Zinkann",

year = "2011",

month = oct,

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doi = "10.1103/PhysRevC.84.045802",

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AU - Deibel, C. M.

AU - Rehm, K. E.

AU - Figueira, J. M.

AU - Greene, J. P.

AU - Jiang, C. L.

AU - Kay, B. P.

AU - Lee, H. Y.

AU - Lighthall, J. C.

AU - Marley, S. T.

AU - Pardo, R. C.

AU - Patel, N.

AU - Paul, M.

AU - Ugalde, C.

AU - Woodard, A.

AU - Wuosmaa, A. H.

AU - Zinkann, G.

PY - 2011/10/6

Y1 - 2011/10/6

N2 - The 30S(α,p)33Cl reaction may have a significant impact on final elemental abundances and energy output of type I X-ray bursts, as well as influencing observables such as double-peaked luminosity profiles, because it could bypass the 30S waiting point. This reaction has been studied experimentally for the first time in inverse kinematics via the time-inverse reaction 1H(33Cl,30S)α with a 33Cl radioactive ion beam produced at the Argonne Tandem Linac Accelerator System facility by the "in-flight" technique. This reaction was studied at three different beam energies. The experimental method used and the resulting data are discussed.

AB - The 30S(α,p)33Cl reaction may have a significant impact on final elemental abundances and energy output of type I X-ray bursts, as well as influencing observables such as double-peaked luminosity profiles, because it could bypass the 30S waiting point. This reaction has been studied experimentally for the first time in inverse kinematics via the time-inverse reaction 1H(33Cl,30S)α with a 33Cl radioactive ion beam produced at the Argonne Tandem Linac Accelerator System facility by the "in-flight" technique. This reaction was studied at three different beam energies. The experimental method used and the resulting data are discussed.

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VL - 84

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First measurement of the 33Cl(p,α)30S reaction

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