First direct measurement of the 17f(p,γ)18ne cross section

K. A. Chipps; D. W. Bardayan; J. C. Blackmon; K. Y. Chae; U. Greife; R. Hatarik; R. L. Kozub; C. Matei; B. H. Moazen; C. D. Nesaraja; S. D. Pain; W. A. Peters; S. T. Pittman; J. F. Shriner; M. S. Smith

doi:10.1063/1.3087067

First direct measurement of the ¹⁷f(p,γ)¹⁸ne cross section

K. A. Chipps, D. W. Bardayan, J. C. Blackmon, K. Y. Chae, U. Greife, R. Hatarik, R. L. Kozub, C. Matei, B. H. Moazen, C. D. Nesaraja, S. D. Pain, W. A. Peters, S. T. Pittman, J. F. Shriner, M. S. Smith

Nuclear Structure and Nuclear Astrophysi

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

Abstract

The rate of the ¹⁷F(p,γ) ¹⁸Ne reaction is of significant importance in astrophysical events like novae and x-ray bursts. A 3⁺ state in ¹⁸Ne predicted to dominate the rate was found at 599.8 keV using the ¹⁷F(p,p)¹⁷F reaction [1], but the resonance strength was nknown. For the first time, the ^F17 ¹⁸Ne reaction has been measured directly with the Daresbury Recoil Separator, using a mixed beam of radioactive ¹⁷F and stable ¹⁷O from the HRIBF at ORNL. A γ width was found for the 599.8 keV resonance in ¹⁸Ne, and an upper limit on the direct capture S factor was determined at an intermediate energy of 800 keV.

Original language	English
Pages (from-to)	471-475
Number of pages	5
Journal	AIP Conference Proceedings
Volume	1090
DOIs	https://doi.org/10.1063/1.3087067
State	Published - 2009
Event	13th International Symposium on Capture Gamma-Ray Spectroscopy and Related Topics - Cologne, Germany Duration: Aug 25 2009 → Aug 29 2009

Keywords

F
Ne
Novae
Proton capture

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@article{a7b33b3ee6054d319d2acc97c768d593,

title = "First direct measurement of the 17f(p,γ)18ne cross section",

abstract = "The rate of the 17F(p,γ) 18Ne reaction is of significant importance in astrophysical events like novae and x-ray bursts. A 3+ state in 18Ne predicted to dominate the rate was found at 599.8 keV using the 17F(p,p)17F reaction [1], but the resonance strength was nknown. For the first time, the F17 18Ne reaction has been measured directly with the Daresbury Recoil Separator, using a mixed beam of radioactive 17F and stable 17O from the HRIBF at ORNL. A γ width was found for the 599.8 keV resonance in 18Ne, and an upper limit on the direct capture S factor was determined at an intermediate energy of 800 keV.",

keywords = "F, Ne, Novae, Proton capture",

author = "Chipps, {K. A.} and Bardayan, {D. W.} and Blackmon, {J. C.} and Chae, {K. Y.} and U. Greife and R. Hatarik and Kozub, {R. L.} and C. Matei and Moazen, {B. H.} and Nesaraja, {C. D.} and Pain, {S. D.} and Peters, {W. A.} and Pittman, {S. T.} and Shriner, {J. F.} and Smith, {M. S.}",

year = "2009",

doi = "10.1063/1.3087067",

language = "English",

volume = "1090",

pages = "471--475",

journal = "AIP Conference Proceedings",

issn = "0094-243X",

publisher = "American Institute of Physics",

note = "13th International Symposium on Capture Gamma-Ray Spectroscopy and Related Topics ; Conference date: 25-08-2009 Through 29-08-2009",

}

TY - JOUR

T1 - First direct measurement of the 17f(p,γ)18ne cross section

AU - Chipps, K. A.

AU - Bardayan, D. W.

AU - Blackmon, J. C.

AU - Chae, K. Y.

AU - Greife, U.

AU - Hatarik, R.

AU - Kozub, R. L.

AU - Matei, C.

AU - Moazen, B. H.

AU - Nesaraja, C. D.

AU - Pain, S. D.

AU - Peters, W. A.

AU - Pittman, S. T.

AU - Shriner, J. F.

AU - Smith, M. S.

PY - 2009

Y1 - 2009

N2 - The rate of the 17F(p,γ) 18Ne reaction is of significant importance in astrophysical events like novae and x-ray bursts. A 3+ state in 18Ne predicted to dominate the rate was found at 599.8 keV using the 17F(p,p)17F reaction [1], but the resonance strength was nknown. For the first time, the F17 18Ne reaction has been measured directly with the Daresbury Recoil Separator, using a mixed beam of radioactive 17F and stable 17O from the HRIBF at ORNL. A γ width was found for the 599.8 keV resonance in 18Ne, and an upper limit on the direct capture S factor was determined at an intermediate energy of 800 keV.

AB - The rate of the 17F(p,γ) 18Ne reaction is of significant importance in astrophysical events like novae and x-ray bursts. A 3+ state in 18Ne predicted to dominate the rate was found at 599.8 keV using the 17F(p,p)17F reaction [1], but the resonance strength was nknown. For the first time, the F17 18Ne reaction has been measured directly with the Daresbury Recoil Separator, using a mixed beam of radioactive 17F and stable 17O from the HRIBF at ORNL. A γ width was found for the 599.8 keV resonance in 18Ne, and an upper limit on the direct capture S factor was determined at an intermediate energy of 800 keV.

KW - F

KW - Ne

KW - Novae

KW - Proton capture

UR - http://www.scopus.com/inward/record.url?scp=64849103143&partnerID=8YFLogxK

U2 - 10.1063/1.3087067

DO - 10.1063/1.3087067

M3 - Conference article

AN - SCOPUS:64849103143

SN - 0094-243X

VL - 1090

SP - 471

EP - 475

JO - AIP Conference Proceedings

JF - AIP Conference Proceedings

T2 - 13th International Symposium on Capture Gamma-Ray Spectroscopy and Related Topics

Y2 - 25 August 2009 through 29 August 2009

ER -

First direct measurement of the ¹⁷f(p,γ)¹⁸ne cross section

Abstract

Keywords

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