First measurement of the 18O(p,α)15N cross section at astrophysical energies

M. La Cognata; C. Spitaleri; A. Mukhamedzhanov; R. E. Tribble; T. Al-Abdullah; A. Banu; S. Cherubini; A. Coc; V. Crucill; V. Goldberg; M. Gulino; B. Irgaziev; G. Kiss; L. Lamia; J. Mrazek; R. G. Pizzone; S. M.R. Puglia; G. G. Rapisarda; S. Romano; M. L. Sergi; G. Tabacaru; L. Trache; W. Trzaska; S. Tudisco; A. Tumino

doi:10.1088/1742-6596/202/1/012019

First measurement of the ¹⁸O(p,α)¹⁵N cross section at astrophysical energies

M. La Cognata^*
, C. Spitaleri
, A. Mukhamedzhanov
, R. E. Tribble
, T. Al-Abdullah
, A. Banu
, S. Cherubini
, A. Coc
, V. Crucill
, V. Goldberg
, M. Gulino
, B. Irgaziev
, G. Kiss
, L. Lamia
, J. Mrazek
, R. G. Pizzone
, S. M.R. Puglia
, G. G. Rapisarda
, S. Romano
, M. L. Sergi

G. Tabacaru, L. Trache, W. Trzaska, S. Tudisco, A. Tumino

^*Corresponding author for this work

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

1 Scopus citations

Abstract

The ¹⁸O(p,α)¹⁵N reaction rate has been deduced by means of the Trojan horse method. For the first time the contribution of the 20 keV resonance has been directly evaluated, giving a value about 35% larger than the one in the literature. Moreover, the present approach has allowed to improve the accuracy by a factor 8.5, as it is based on the measured strength instead of spectroscopic measurements. The contribution of the 90 keV resonance has been also determined, which turned out to be of negligible importance to astrophysics.

Original language	English
Article number	012019
Journal	Journal of Physics: Conference Series
Volume	202
DOIs	https://doi.org/10.1088/1742-6596/202/1/012019
State	Published - 2010
Externally published	Yes

ASJC Scopus subject areas

General Physics and Astronomy

Access to Document

10.1088/1742-6596/202/1/012019

Cite this

La Cognata, M., Spitaleri, C., Mukhamedzhanov, A., Tribble, R. E., Al-Abdullah, T., Banu, A., Cherubini, S., Coc, A., Crucill, V., Goldberg, V., Gulino, M., Irgaziev, B., Kiss, G., Lamia, L., Mrazek, J., Pizzone, R. G., Puglia, S. M. R., Rapisarda, G. G., Romano, S., ... Tumino, A. (2010). First measurement of the ¹⁸O(p,α)¹⁵N cross section at astrophysical energies. Journal of Physics: Conference Series, 202, Article 012019. https://doi.org/10.1088/1742-6596/202/1/012019

@article{125c1d11db9e41d1bca9a65ee8282e5f,

title = "First measurement of the 18O(p,α)15N cross section at astrophysical energies",

abstract = "The 18O(p,α)15N reaction rate has been deduced by means of the Trojan horse method. For the first time the contribution of the 20 keV resonance has been directly evaluated, giving a value about 35\% larger than the one in the literature. Moreover, the present approach has allowed to improve the accuracy by a factor 8.5, as it is based on the measured strength instead of spectroscopic measurements. The contribution of the 90 keV resonance has been also determined, which turned out to be of negligible importance to astrophysics.",

author = "\{La Cognata\}, M. and C. Spitaleri and A. Mukhamedzhanov and Tribble, \{R. E.\} and T. Al-Abdullah and A. Banu and S. Cherubini and A. Coc and V. Crucill and V. Goldberg and M. Gulino and B. Irgaziev and G. Kiss and L. Lamia and J. Mrazek and Pizzone, \{R. G.\} and Puglia, \{S. M.R.\} and Rapisarda, \{G. G.\} and S. Romano and Sergi, \{M. L.\} and G. Tabacaru and L. Trache and W. Trzaska and S. Tudisco and A. Tumino",

year = "2010",

doi = "10.1088/1742-6596/202/1/012019",

language = "English",

volume = "202",

journal = "Journal of Physics: Conference Series",

issn = "1742-6588",

publisher = "IOP Publishing Ltd.",

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La Cognata, M, Spitaleri, C, Mukhamedzhanov, A, Tribble, RE, Al-Abdullah, T, Banu, A, Cherubini, S, Coc, A, Crucill, V, Goldberg, V, Gulino, M, Irgaziev, B, Kiss, G, Lamia, L, Mrazek, J, Pizzone, RG, Puglia, SMR, Rapisarda, GG, Romano, S, Sergi, ML, Tabacaru, G, Trache, L, Trzaska, W, Tudisco, S & Tumino, A 2010, 'First measurement of the ¹⁸O(p,α)¹⁵N cross section at astrophysical energies', Journal of Physics: Conference Series, vol. 202, 012019. https://doi.org/10.1088/1742-6596/202/1/012019

TY - JOUR

T1 - First measurement of the 18O(p,α)15N cross section at astrophysical energies

AU - La Cognata, M.

AU - Spitaleri, C.

AU - Mukhamedzhanov, A.

AU - Tribble, R. E.

AU - Al-Abdullah, T.

AU - Banu, A.

AU - Cherubini, S.

AU - Coc, A.

AU - Crucill, V.

AU - Goldberg, V.

AU - Gulino, M.

AU - Irgaziev, B.

AU - Kiss, G.

AU - Lamia, L.

AU - Mrazek, J.

AU - Pizzone, R. G.

AU - Puglia, S. M.R.

AU - Rapisarda, G. G.

AU - Romano, S.

AU - Sergi, M. L.

AU - Tabacaru, G.

AU - Trache, L.

AU - Trzaska, W.

AU - Tudisco, S.

AU - Tumino, A.

PY - 2010

Y1 - 2010

N2 - The 18O(p,α)15N reaction rate has been deduced by means of the Trojan horse method. For the first time the contribution of the 20 keV resonance has been directly evaluated, giving a value about 35% larger than the one in the literature. Moreover, the present approach has allowed to improve the accuracy by a factor 8.5, as it is based on the measured strength instead of spectroscopic measurements. The contribution of the 90 keV resonance has been also determined, which turned out to be of negligible importance to astrophysics.

AB - The 18O(p,α)15N reaction rate has been deduced by means of the Trojan horse method. For the first time the contribution of the 20 keV resonance has been directly evaluated, giving a value about 35% larger than the one in the literature. Moreover, the present approach has allowed to improve the accuracy by a factor 8.5, as it is based on the measured strength instead of spectroscopic measurements. The contribution of the 90 keV resonance has been also determined, which turned out to be of negligible importance to astrophysics.

UR - https://www.scopus.com/pages/publications/77950513107

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DO - 10.1088/1742-6596/202/1/012019

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