Measurement of the O-17(p,gamma)F-18 reaction rate at astrophysically relevant energies

U. Hager; L. Buchmann; B. Davids; J. Fallis; B. R. Fulton; N. Galinski; U. Greife; D. A. Hutcheon; D. Ottewell; A. Rojas; C. Ruiz; K. Setoodehnia

doi:10.1103/PhysRevC.85.035803

Measurement of the O-17(p,gamma)F-18 reaction rate at astrophysically relevant energies

U. Hager, L. Buchmann, B. Davids, J. Fallis, B. R. Fulton, N. Galinski, U. Greife, D. A. Hutcheon, D. Ottewell, A. Rojas, C. Ruiz, K. Setoodehnia

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Abstract

The O-17( p, gamma)F-18 reaction plays an important role in hydrogen- burning nucleosynthesis. Conflicting values for the low- energy behavior of its cross section exist in the literature. We present direct measurements of the astrophysical S factor of the O-17( p, gamma)F-18 reaction at center- of- mass energies between 250 and 500 keV. These measurements were conducted in inverse kinematics at the DRAGON recoil separator.

Original language	English
Article number	035803
Pages (from-to)	-
Number of pages	7
Journal	Physical Review C
Volume	85
Issue number	3
DOIs	https://doi.org/10.1103/PhysRevC.85.035803
Publication status	Published - 14 Mar 2012

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10.1103/PhysRevC.85.035803

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abstract = "The O-17( p, gamma)F-18 reaction plays an important role in hydrogen- burning nucleosynthesis. Conflicting values for the low- energy behavior of its cross section exist in the literature. We present direct measurements of the astrophysical S factor of the O-17( p, gamma)F-18 reaction at center- of- mass energies between 250 and 500 keV. These measurements were conducted in inverse kinematics at the DRAGON recoil separator.",

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AU - Hager, U.

AU - Buchmann, L.

AU - Davids, B.

AU - Fallis, J.

AU - Fulton, B. R.

AU - Galinski, N.

AU - Greife, U.

AU - Hutcheon, D. A.

AU - Ottewell, D.

AU - Rojas, A.

AU - Ruiz, C.

AU - Setoodehnia, K.

PY - 2012/3/14

Y1 - 2012/3/14

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AB - The O-17( p, gamma)F-18 reaction plays an important role in hydrogen- burning nucleosynthesis. Conflicting values for the low- energy behavior of its cross section exist in the literature. We present direct measurements of the astrophysical S factor of the O-17( p, gamma)F-18 reaction at center- of- mass energies between 250 and 500 keV. These measurements were conducted in inverse kinematics at the DRAGON recoil separator.

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Measurement of the O-17(p,gamma)F-18 reaction rate at astrophysically relevant energies

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