Exploring the αp-process with Grand Raiden

S. O'Brien; T. Adachi; G. P.A. Berg; M. Couder; M. Dozono; H. Fujita; Y. Fujita; J. Görres; K. Hatanaka; D. Ishikawa; T. Kubo; H. Matsubara; Y. Namiki; Y. Ohkuma; H. Okamura; H. J. Ong; D. Patel; Y. Sakemis; K. Sault; Y. Shimbara; S. Suzuki; T. Suzuki; A. Tamii; T. Wakasa; R. Wantanabe; M. Wiescher; R. Yamada; J. Zenihiro

doi:10.1063/1.3087029

Exploring the αp-process with Grand Raiden

S. O'Brien, T. Adachi, G. P.A. Berg, M. Couder, M. Dozono, H. Fujita, Y. Fujita, J. Görres, K. Hatanaka, D. Ishikawa, T. Kubo, H. Matsubara, Y. Namiki, Y. Ohkuma, H. Okamura, H. J. Ong, D. Patel, Y. Sakemis, K. Sault, Y. ShimbaraS. Suzuki, T. Suzuki, A. Tamii, T. Wakasa, R. Wantanabe, M. Wiescher, R. Yamada, J. Zenihiro

Research output: Contribution to journal › Conference article › peer-review

7 Citations (Scopus)

Abstract

²²Mg, ³⁰S, ³⁴Ar and ³⁸Ca have been investigated using (p,t) reactions at RCNP with the intent of identifying energy levels in nuclei that determine the reaction rates along the pathway of the αp-process. These experiments exploit the high resolution and 0° capabilities of the Grand Raiden spectrometer and the WS beamline, which can deliver a fully dispersion matched beam to target. The level information is vital to understanding the nucleosynthesis occurring during explosive hydrogen burning, which, for example, is thought to occur during type I X-ray bursts. In the case of ²²Mg, new reaction rate calculations have been performed for the ¹⁸Ne(α,p)²¹Na reaction. The experimental technique will be discussed, and the experimental results will be presented.

Original language	English
Pages (from-to)	288-292
Number of pages	5
Journal	AIP Conference Proceedings
Volume	1090
DOIs	https://doi.org/10.1063/1.3087029
Publication status	Published - 2009
Externally published	Yes
Event	13th International Symposium on Capture Gamma-Ray Spectroscopy and Related Topics - Cologne, Germany Duration: 2009 Aug 25 → 2009 Aug 29

Keywords

Explosive hydrogen burning
Reaction rates
X-ray burst

ASJC Scopus subject areas

Physics and Astronomy(all)

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10.1063/1.3087029

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O'Brien, S., Adachi, T., Berg, G. P. A., Couder, M., Dozono, M., Fujita, H., Fujita, Y., Görres, J., Hatanaka, K., Ishikawa, D., Kubo, T., Matsubara, H., Namiki, Y., Ohkuma, Y., Okamura, H., Ong, H. J., Patel, D., Sakemis, Y., Sault, K., ... Zenihiro, J. (2009). Exploring the αp-process with Grand Raiden. AIP Conference Proceedings, 1090, 288-292. https://doi.org/10.1063/1.3087029

O'Brien, S, Adachi, T, Berg, GPA, Couder, M, Dozono, M, Fujita, H, Fujita, Y, Görres, J, Hatanaka, K, Ishikawa, D, Kubo, T, Matsubara, H, Namiki, Y, Ohkuma, Y, Okamura, H, Ong, HJ, Patel, D, Sakemis, Y, Sault, K, Shimbara, Y, Suzuki, S, Suzuki, T, Tamii, A, Wakasa, T, Wantanabe, R, Wiescher, M, Yamada, R & Zenihiro, J 2009, 'Exploring the αp-process with Grand Raiden', AIP Conference Proceedings, vol. 1090, pp. 288-292. https://doi.org/10.1063/1.3087029

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title = "Exploring the αp-process with Grand Raiden",

abstract = "22Mg, 30S, 34Ar and 38Ca have been investigated using (p,t) reactions at RCNP with the intent of identifying energy levels in nuclei that determine the reaction rates along the pathway of the αp-process. These experiments exploit the high resolution and 0° capabilities of the Grand Raiden spectrometer and the WS beamline, which can deliver a fully dispersion matched beam to target. The level information is vital to understanding the nucleosynthesis occurring during explosive hydrogen burning, which, for example, is thought to occur during type I X-ray bursts. In the case of 22Mg, new reaction rate calculations have been performed for the 18Ne(α,p)21Na reaction. The experimental technique will be discussed, and the experimental results will be presented.",

keywords = "Explosive hydrogen burning, Reaction rates, X-ray burst",

author = "S. O'Brien and T. Adachi and Berg, {G. P.A.} and M. Couder and M. Dozono and H. Fujita and Y. Fujita and J. G{\"o}rres and K. Hatanaka and D. Ishikawa and T. Kubo and H. Matsubara and Y. Namiki and Y. Ohkuma and H. Okamura and Ong, {H. J.} and D. Patel and Y. Sakemis and K. Sault and Y. Shimbara and S. Suzuki and T. Suzuki and A. Tamii and T. Wakasa and R. Wantanabe and M. Wiescher and R. Yamada and J. Zenihiro",

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doi = "10.1063/1.3087029",

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pages = "288--292",

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T1 - Exploring the αp-process with Grand Raiden

AU - O'Brien, S.

AU - Adachi, T.

AU - Berg, G. P.A.

AU - Couder, M.

AU - Dozono, M.

AU - Fujita, H.

AU - Fujita, Y.

AU - Görres, J.

AU - Hatanaka, K.

AU - Ishikawa, D.

AU - Kubo, T.

AU - Matsubara, H.

AU - Namiki, Y.

AU - Ohkuma, Y.

AU - Okamura, H.

AU - Ong, H. J.

AU - Patel, D.

AU - Sakemis, Y.

AU - Sault, K.

AU - Shimbara, Y.

AU - Suzuki, S.

AU - Suzuki, T.

AU - Tamii, A.

AU - Wakasa, T.

AU - Wantanabe, R.

AU - Wiescher, M.

AU - Yamada, R.

AU - Zenihiro, J.

PY - 2009

Y1 - 2009

N2 - 22Mg, 30S, 34Ar and 38Ca have been investigated using (p,t) reactions at RCNP with the intent of identifying energy levels in nuclei that determine the reaction rates along the pathway of the αp-process. These experiments exploit the high resolution and 0° capabilities of the Grand Raiden spectrometer and the WS beamline, which can deliver a fully dispersion matched beam to target. The level information is vital to understanding the nucleosynthesis occurring during explosive hydrogen burning, which, for example, is thought to occur during type I X-ray bursts. In the case of 22Mg, new reaction rate calculations have been performed for the 18Ne(α,p)21Na reaction. The experimental technique will be discussed, and the experimental results will be presented.

AB - 22Mg, 30S, 34Ar and 38Ca have been investigated using (p,t) reactions at RCNP with the intent of identifying energy levels in nuclei that determine the reaction rates along the pathway of the αp-process. These experiments exploit the high resolution and 0° capabilities of the Grand Raiden spectrometer and the WS beamline, which can deliver a fully dispersion matched beam to target. The level information is vital to understanding the nucleosynthesis occurring during explosive hydrogen burning, which, for example, is thought to occur during type I X-ray bursts. In the case of 22Mg, new reaction rate calculations have been performed for the 18Ne(α,p)21Na reaction. The experimental technique will be discussed, and the experimental results will be presented.

KW - Explosive hydrogen burning

KW - Reaction rates

KW - X-ray burst

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Y2 - 25 August 2009 through 29 August 2009

ER -

Exploring the αp-process with Grand Raiden

Abstract

Keywords

ASJC Scopus subject areas

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