1997
DOI: 10.1103/physrevlett.79.3837
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Halo Properties of the First1/2+State inF17

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Cited by 184 publications
(228 citation statements)
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“…Experimental data on excitation functions are from [35,[37][38][39]. Our results are in a good agreement with obtained earlier phase shifts from [26,30] that are shown in Figure 1 by squares and rhombs at energies above 1.5 MeV.…”
Section: Phase Shift Analysissupporting
confidence: 81%
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“…Experimental data on excitation functions are from [35,[37][38][39]. Our results are in a good agreement with obtained earlier phase shifts from [26,30] that are shown in Figure 1 by squares and rhombs at energies above 1.5 MeV.…”
Section: Phase Shift Analysissupporting
confidence: 81%
“…(4) from 2 P scattering waves with potentials of zero depth in comparison with experimental data are shown in Figure 2 by the green solid line. The measurement results of the total cross sections in the range from 0.4 to 2.5 MeV [37] are shown by black squares, and circles are data from [50] at 0.5 -2.5 MeV. Triangles show results of work [45], which lead to S-factor at zero energy of 0.4 keVb.…”
Section: The Astrophysical S-factormentioning
confidence: 99%
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“…These measurements have prompted interest in the determination of reliable opticalmodel potentials for 17 F. The proton radiative capture reaction 16 O(p, γ ) 17 F has been measured at stellar energies by Morlock et al [10]. The extracted astrophysical S factors are in excellent agreement with those obtained with the asymptotic normalization coefficient (ANC) method by use of the transfer reaction 16 O( 3 He,d) 17 F by Gagliardi et al [11], and the halo properties of the first excited state (J π = 1/2 + , E x = 495 keV) were well established.…”
Section: Introductionmentioning
confidence: 99%