Indirect study of the astrophysically important 15O(α,γ)19Ne reaction through 2H(18Ne,19Ne)1H

A.M. Laird; S. Cherubini; A.N. Ostrowski; M. Aliotta; T. Davinson; A. Di Pietro; P. Figuera; D. Groombridge; W. Galster; J.S. Graulich; J. Hinnefeld; M. Lattuada; P. Leleux; L. Michel; A. Musumarra; A. Ninane; M.G. Pellegriti; A.C. Shotter; A. Spitaleri; A. Tumino; J. Vervier; P. Woods

doi:10.1103/PhysRevC.66.048801

Indirect study of the astrophysically important 15O(α,γ)19Ne reaction through 2H(18Ne,19Ne)1H

A.M. Laird, S. Cherubini, A.N. Ostrowski, M. Aliotta, T. Davinson, A. Di Pietro, P. Figuera, D. Groombridge, W. Galster, J.S. Graulich, J. Hinnefeld, M. Lattuada, P. Leleux, L. Michel, A. Musumarra, A. Ninane, M.G. Pellegriti, A.C. Shotter, A. Spitaleri, A. TuminoJ. Vervier, P. Woods

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

21 Citations (Scopus)

Abstract

The 15O(α,γ)19Ne reaction is generally considered as a potential breakout reaction from the hot CNO cycle. Under nova conditions, the reaction rate is dominated by a single sub-Coulomb resonance at Ec.m.=504 keV which corresponds to a 19Ne excitation energy of ER=4.033 MeV. Results from a d(18Ne,19Ne)p experiment show that states of astrophysical interest are populated in this reaction. An upper limit for the α-branching ratio of the 4.033 MeV state was identified and branching ratios for other states in 19Ne were found to be in good agreement with stable beam based results.

Original language	English
Article number	048801
Pages (from-to)	1-4
Number of pages	4
Journal	Physical Review C: Nuclear Physics
Volume	66
Issue number	4
DOIs	https://doi.org/10.1103/PhysRevC.66.048801
Publication status	Published - Oct 2002

Keywords

astrophysics
branching ratios
plasmas

Access to Document

10.1103/PhysRevC.66.048801

Cite this

Laird, A. M., Cherubini, S., Ostrowski, A. N., Aliotta, M., Davinson, T., Di Pietro, A., Figuera, P., Groombridge, D., Galster, W., Graulich, J. S., Hinnefeld, J., Lattuada, M., Leleux, P., Michel, L., Musumarra, A., Ninane, A., Pellegriti, M. G., Shotter, A. C., Spitaleri, A., ... Woods, P. (2002). Indirect study of the astrophysically important 15O(α,γ)19Ne reaction through 2H(18Ne,19Ne)1H. Physical Review C: Nuclear Physics, 66(4), 1-4. Article 048801. https://doi.org/10.1103/PhysRevC.66.048801

@article{f9576c3d140241b698d4783be15577bd,

title = "Indirect study of the astrophysically important 15O(α,γ)19Ne reaction through 2H(18Ne,19Ne)1H",

abstract = "The 15O(α,γ)19Ne reaction is generally considered as a potential breakout reaction from the hot CNO cycle. Under nova conditions, the reaction rate is dominated by a single sub-Coulomb resonance at Ec.m.=504 keV which corresponds to a 19Ne excitation energy of ER=4.033 MeV. Results from a d(18Ne,19Ne)p experiment show that states of astrophysical interest are populated in this reaction. An upper limit for the α-branching ratio of the 4.033 MeV state was identified and branching ratios for other states in 19Ne were found to be in good agreement with stable beam based results.",

keywords = "astrophysics, branching ratios, plasmas",

author = "A.M. Laird and S. Cherubini and A.N. Ostrowski and M. Aliotta and T. Davinson and {Di Pietro}, A. and P. Figuera and D. Groombridge and W. Galster and J.S. Graulich and J. Hinnefeld and M. Lattuada and P. Leleux and L. Michel and A. Musumarra and A. Ninane and M.G. Pellegriti and A.C. Shotter and A. Spitaleri and A. Tumino and J. Vervier and P. Woods",

year = "2002",

month = oct,

doi = "10.1103/PhysRevC.66.048801",

language = "English",

volume = "66",

pages = "1--4",

journal = "Physical Review C: Nuclear Physics",

issn = "0556-2813",

publisher = "American Physical Society",

number = "4",

}

Laird, AM, Cherubini, S, Ostrowski, AN, Aliotta, M, Davinson, T, Di Pietro, A, Figuera, P, Groombridge, D, Galster, W, Graulich, JS, Hinnefeld, J, Lattuada, M, Leleux, P, Michel, L, Musumarra, A, Ninane, A, Pellegriti, MG, Shotter, AC, Spitaleri, A, Tumino, A, Vervier, J & Woods, P 2002, 'Indirect study of the astrophysically important 15O(α,γ)19Ne reaction through 2H(18Ne,19Ne)1H', Physical Review C: Nuclear Physics, vol. 66, no. 4, 048801, pp. 1-4. https://doi.org/10.1103/PhysRevC.66.048801

TY - JOUR

T1 - Indirect study of the astrophysically important 15O(α,γ)19Ne reaction through 2H(18Ne,19Ne)1H

AU - Laird, A.M.

AU - Cherubini, S.

AU - Ostrowski, A.N.

AU - Aliotta, M.

AU - Davinson, T.

AU - Di Pietro, A.

AU - Figuera, P.

AU - Groombridge, D.

AU - Galster, W.

AU - Graulich, J.S.

AU - Hinnefeld, J.

AU - Lattuada, M.

AU - Leleux, P.

AU - Michel, L.

AU - Musumarra, A.

AU - Ninane, A.

AU - Pellegriti, M.G.

AU - Shotter, A.C.

AU - Spitaleri, A.

AU - Tumino, A.

AU - Vervier, J.

AU - Woods, P.

PY - 2002/10

Y1 - 2002/10

N2 - The 15O(α,γ)19Ne reaction is generally considered as a potential breakout reaction from the hot CNO cycle. Under nova conditions, the reaction rate is dominated by a single sub-Coulomb resonance at Ec.m.=504 keV which corresponds to a 19Ne excitation energy of ER=4.033 MeV. Results from a d(18Ne,19Ne)p experiment show that states of astrophysical interest are populated in this reaction. An upper limit for the α-branching ratio of the 4.033 MeV state was identified and branching ratios for other states in 19Ne were found to be in good agreement with stable beam based results.

AB - The 15O(α,γ)19Ne reaction is generally considered as a potential breakout reaction from the hot CNO cycle. Under nova conditions, the reaction rate is dominated by a single sub-Coulomb resonance at Ec.m.=504 keV which corresponds to a 19Ne excitation energy of ER=4.033 MeV. Results from a d(18Ne,19Ne)p experiment show that states of astrophysical interest are populated in this reaction. An upper limit for the α-branching ratio of the 4.033 MeV state was identified and branching ratios for other states in 19Ne were found to be in good agreement with stable beam based results.

KW - astrophysics

KW - branching ratios

KW - plasmas

U2 - 10.1103/PhysRevC.66.048801

DO - 10.1103/PhysRevC.66.048801

M3 - Article

SN - 0556-2813

VL - 66

SP - 1

EP - 4

JO - Physical Review C: Nuclear Physics

JF - Physical Review C: Nuclear Physics

IS - 4

M1 - 048801

ER -

Indirect study of the astrophysically important 15O(α,γ)19Ne reaction through 2H(18Ne,19Ne)1H

Abstract

Keywords

Access to Document

Fingerprint

Cite this