First experimental limit on the Ne(p, γ)Na resonance strength, of astrophysical interest

R.D. Page; G. Vancraeynest; A.C. Shotter; M. Huyse; C.R. Bain; F. Binon; R. Coszach; T. Davinson; P. Decrock; Th. Delbar; P. Duhamel; M. Gaelens; W. Galster; P. Leleux; I. Licot; E. Lienard; P. Lipnik; C. Michotte; A. Ninane; P.J. Seilin; Cs. Sükösd; P. Van Duppen; J. Vanhorenbeeck; J. Vervier; M. Wiescher; P.J. Woods

First experimental limit on the Ne(p, γ)Na resonance strength, of astrophysical interest

R.D. Page
, G. Vancraeynest
, A.C. Shotter
, M. Huyse
, C.R. Bain
, F. Binon
, R. Coszach
, T. Davinson
, P. Decrock
, Th. Delbar
, P. Duhamel
, M. Gaelens
, W. Galster
, P. Leleux
, I. Licot
, E. Lienard
, P. Lipnik
, C. Michotte
, A. Ninane
, P.J. Seilin

Cs. Sükösd, P. Van Duppen, J. Vanhorenbeeck, J. Vervier, M. Wiescher, P.J. Woods

School of Physics and Astronomy

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

Abstract

The Ne(p, γ)Na reaction may influence considerably the reaction flow between the CNO and NeNa mass regions in high temperature hydrogen burning conditions. The 447 keV resonance has been studied by exploiting radioactive Ne beams with novel detection techniques to measure β -delayed α radioactivity of Na nuclei produced in reactions with polyethylene targets. A 90% C.L. upper limit of 18 meV for the resonance strength has been determined and implications for the spin assignment of the 2.646 MeV state in Na and the stellar reaction rate are discussed.

Original language	English
Pages (from-to)	3066-3069
Number of pages	4
Journal	Physical Review Letters
Volume	73
Issue number	23
Publication status	Published - 1 Jan 1994

Cite this

Page, R. D., Vancraeynest, G., Shotter, A. C., Huyse, M., Bain, C. R., Binon, F., Coszach, R., Davinson, T., Decrock, P., Delbar, T., Duhamel, P., Gaelens, M., Galster, W., Leleux, P., Licot, I., Lienard, E., Lipnik, P., Michotte, C., Ninane, A., ... Woods, P. J. (1994). First experimental limit on the Ne(p, γ)Na resonance strength, of astrophysical interest. Physical Review Letters, 73(23), 3066-3069.

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title = "First experimental limit on the Ne(p, γ)Na resonance strength, of astrophysical interest",

abstract = "The Ne(p, γ)Na reaction may influence considerably the reaction flow between the CNO and NeNa mass regions in high temperature hydrogen burning conditions. The 447 keV resonance has been studied by exploiting radioactive Ne beams with novel detection techniques to measure β -delayed α radioactivity of Na nuclei produced in reactions with polyethylene targets. A 90\% C.L. upper limit of 18 meV for the resonance strength has been determined and implications for the spin assignment of the 2.646 MeV state in Na and the stellar reaction rate are discussed.",

author = "R.D. Page and G. Vancraeynest and A.C. Shotter and M. Huyse and C.R. Bain and F. Binon and R. Coszach and T. Davinson and P. Decrock and Th. Delbar and P. Duhamel and M. Gaelens and W. Galster and P. Leleux and I. Licot and E. Lienard and P. Lipnik and C. Michotte and A. Ninane and P.J. Seilin and Cs. S{\"u}k{\"o}sd and \{Van Duppen\}, P. and J. Vanhorenbeeck and J. Vervier and M. Wiescher and P.J. Woods",

year = "1994",

month = jan,

day = "1",

language = "English",

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pages = "3066--3069",

journal = "Physical Review Letters",

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Page, RD, Vancraeynest, G, Shotter, AC, Huyse, M, Bain, CR, Binon, F, Coszach, R, Davinson, T, Decrock, P, Delbar, T, Duhamel, P, Gaelens, M, Galster, W, Leleux, P, Licot, I, Lienard, E, Lipnik, P, Michotte, C, Ninane, A, Seilin, PJ, Sükösd, C, Van Duppen, P, Vanhorenbeeck, J, Vervier, J, Wiescher, M & Woods, PJ 1994, 'First experimental limit on the Ne(p, γ)Na resonance strength, of astrophysical interest', Physical Review Letters, vol. 73, no. 23, pp. 3066-3069.

TY - JOUR

T1 - First experimental limit on the Ne(p, γ)Na resonance strength, of astrophysical interest

AU - Page, R.D.

AU - Vancraeynest, G.

AU - Shotter, A.C.

AU - Huyse, M.

AU - Bain, C.R.

AU - Binon, F.

AU - Coszach, R.

AU - Davinson, T.

AU - Decrock, P.

AU - Delbar, Th.

AU - Duhamel, P.

AU - Gaelens, M.

AU - Galster, W.

AU - Leleux, P.

AU - Licot, I.

AU - Lienard, E.

AU - Lipnik, P.

AU - Michotte, C.

AU - Ninane, A.

AU - Seilin, P.J.

AU - Sükösd, Cs.

AU - Van Duppen, P.

AU - Vanhorenbeeck, J.

AU - Vervier, J.

AU - Wiescher, M.

AU - Woods, P.J.

PY - 1994/1/1

Y1 - 1994/1/1

N2 - The Ne(p, γ)Na reaction may influence considerably the reaction flow between the CNO and NeNa mass regions in high temperature hydrogen burning conditions. The 447 keV resonance has been studied by exploiting radioactive Ne beams with novel detection techniques to measure β -delayed α radioactivity of Na nuclei produced in reactions with polyethylene targets. A 90% C.L. upper limit of 18 meV for the resonance strength has been determined and implications for the spin assignment of the 2.646 MeV state in Na and the stellar reaction rate are discussed.

AB - The Ne(p, γ)Na reaction may influence considerably the reaction flow between the CNO and NeNa mass regions in high temperature hydrogen burning conditions. The 447 keV resonance has been studied by exploiting radioactive Ne beams with novel detection techniques to measure β -delayed α radioactivity of Na nuclei produced in reactions with polyethylene targets. A 90% C.L. upper limit of 18 meV for the resonance strength has been determined and implications for the spin assignment of the 2.646 MeV state in Na and the stellar reaction rate are discussed.

UR - https://www.scopus.com/pages/publications/0001317603

M3 - Article

AN - SCOPUS:0001317603

SN - 0031-9007

VL - 73

SP - 3066

EP - 3069

JO - Physical Review Letters

JF - Physical Review Letters

IS - 23

ER -

First experimental limit on the Ne(p, γ)Na resonance strength, of astrophysical interest

Abstract

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