Neutron single particle strengths from the (<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>d</mml:mi><mml:mo>,</mml:mo><mml:mi>p</mml:mi></mml:mrow></mml:math>) reaction on<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mmultiscripts><mml:mi mathvariant="normal">F</mml:mi><mml:mprescripts /><mml:none /><mml:mrow><mml:mn>18</mml:mn></mml:mrow></mml:mmultiscripts></mml:math>

Kozub, R. L.; Bardayan, D. W.; Batchelder, J. C.; Blackmon, J. C.; Brune, C. R.; Champagne, Arthur E; Cizewski, J. A.; Greife, U.; Gross, C. J.; Jewett, C.; Livesay, R. J.; Ma, Z.; Moazen, B. H.; Nesaraja, C. D.; Şahin, L.; Scott, J. P.; Shapira, D.; Smith, M. S.; Thomas, J. S.

doi:10.1103/physrevc.73.044307

Cited by 19 publications

(28 citation statements)

References 11 publications

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“…The observed excitation energies of 19 F compared reasonably well with the results from the 18 F(d, p) experiment of Kozub et al [6]. The experiment of Kozub et al was performed at a somewhat lower energy than the present one (E c.m.…”

Section: Results and Conclusionsupporting

confidence: 79%

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Astrophysically important 19Ne states studied with the 2H(18F, alpha+15O)n Reaction

Adekola¹,

Bardayan²,

Blackmon³

et al. 2009

Proceedings of 10th Symposium on Nuclei in the Cosmos — PoS(NIC X)

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Facility (HRIBF) of Oak Ridge National Laboratory (ORNL) by bombarding a 720-µg/cm 2 CD 2 target with a radioactive 18 F beam. The 19 Ne states of interest near the proton threshold decay by breakup into α and 15 O particles. These decay products were detected in coincidence with position-sensitive E−∆E silicon telescopes. The α and 15 N particles from the break up of the mirror nucleus 19 F were also measured with these detectors. Particle identification, coincidence, and Q-value requirements enable us to distinguish the reaction of interest from other reactions.

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Section: Results and Conclusionsupporting

confidence: 79%

“…al. [6] had earlier mentioned the possibility of l = 0 strength near the proton threshold in 19 Ne to be concentrated in a proton-bound state. We believe that the l = 0 strength in the 6.29-MeV state will make it relevant for the 18 F(p, α) 15 O process.…”

Section: Results and Conclusionmentioning

confidence: 99%

Astrophysically important 19Ne states studied with the 2H(18F, alpha+15O)n Reaction

Adekola¹,

Bardayan²,

Blackmon³

et al. 2009

Proceedings of 10th Symposium on Nuclei in the Cosmos — PoS(NIC X)

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“…Information about the nucleosynthesis and the ejection mechanism in novae can be essentially deduced from gamma-ray emission originating from electronpositron annihilations at 511 keV following the β + decay of 18 F. A precise interpretation of the measurements performed by γ-astronomy detectors relies on an accurate knowledge of the destruction modes of 18 F in novae. In this context, 18 F(p,α) 15 O is believed to be the most relevant reaction [1,2].…”

Section: Introductionmentioning

confidence: 99%

“…The typical temperature range in novae is of the order of (1 − 4) × 10 8 K. Consequently, 19 Ne resonances relevant in the burning process are located in an interval of about 1 MeV above the 18 F+p threshold (Q = 6.41 MeV) [1,3]. Many uncertainties remain on the determination of the 18 F(p,α) 15 O reaction rate at these energies.…”

Section: Introductionmentioning

confidence: 99%

The 18F(p, α) 15O low-energy S-factor: A microscopic approach

Dufour

Descouvemont

2007

Nuclear Physics A

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“…While these studies have contributed significantly to our understanding of the situation, there remains considerable uncertainty in the assignment of analog states between 19 F and 19 Ne [12,15]. Many of the observed states in 19 Ne do not have measured spins and parities, but are assigned based on their putative analog states in 19 F. The properties of these unobserved states and precise determination of isospin-mirror symmetry between these two nuclei will influence the 18 F + p reaction rates.…”

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confidence: 99%