Web4Desktop, a Framework for Improving the Usability of Web Applications

Carstoiu, Bogdan; Carstoiu, Dorin

doi:10.1007/978-3-642-16419-4_47

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2010

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“…Both real and imaginary potentials were obtained from folding. The elastic scattering fit was carried out with OPTJLM1 [41]. The optical parameters obtained are shown in Table V.…”

Section: Mgmentioning

confidence: 99%

Giant resonances inMg24andSi28from 240 MeV
Chen
¹
,
Lui
²
,
Clark
³

et al. 2009
Phys. Rev. C
61
19
88
2
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“…Both real and imaginary potentials were obtained from folding. The elastic scattering fit was carried out with OPTJLM1 [41]. The optical parameters obtained are shown in Table V.…”

Section: Mgmentioning

confidence: 99%

Giant resonances inMg24andSi28from 240 MeV
Chen
¹
,
Lui
²
,
Clark
³

et al. 2009
Phys. Rev. C
61
19
88
2
View full text Add to dashboard Cite

“…The fits in both cases were made using the code OPTIMINIX [31]. The Coulomb component in the optical potential was calculated by folding the appropriate Hartree-Fock charge densities with the proton-proton Coulomb interaction.…”

Section: -3mentioning

confidence: 99%

Stellar reaction rate forMg22+p→
Al-Abdullah
¹
,
Cârstoiu
²
,
Chen
³

et al. 2010
Phys. Rev. C
27
3
16
0
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The production of 22 Na in ONe novae can be influenced by the 22 Mg(p,γ ) 23 Al reaction. To investigate this reaction rate at stellar energies, we have determined the asymptotic normalization coefficient (ANC) for 22 Mg + p → 23 Al through measurements of the ANCs in the mirror nuclear system 22 Ne + n → 23 Ne. The peripheral neutron-transfer reactions 13 C( 12 C, 13 C) 12 C and 13 C( 22 Ne, 23 Ne) 12 C were studied. The identical entrance and exit channels of the first reaction make it possible to extract independently the ground-state ANC in 13 C. Our experiment gives C 2 p 1/2 ( 13 C) = 2.24 ± 0.11 fm −1 , which agrees with the value obtained from several previous measurements. The weighted average for all the obtained C 2 p 1/2 is 2.31 ± 0.08 fm −1 . This value is adopted to be used in obtaining the ANCs in 23 Ne. The differential cross sections for the reaction 13 C( 22 Ne, 23 Ne) 12 C leading to the J π = 5/2 + and 1/2 + states in 23 Ne have been measured at 12 MeV/u. Optical model parameters for use in the DWBA calculations were obtained from measurements of the elastic scatterings 22 Ne + 13 C and 22 Ne + 12 C. The extracted ANC for the ground state in 23 Ne, C 2 d 5/2 = 0.86 ± 0.08 ± 0.12 fm −1 , is converted to its corresponding value in 23 Al using mirror symmetry to give C 2 d 5/2 ( 23 Al) = (4.63 ± 0.77) × 10 3 fm −1 . The astrophysical S factor S(0) for the 22 Mg(p,γ ) reaction was determined to be 0.96 ± 0.11 keV b. The consequences for nuclear astrophysics are discussed.

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Web4Desktop, a Framework for Improving the Usability of Web Applications

Cited by 2 publications

References 0 publications

Giant resonances inMg24andSi28from 240 MeV
Chen
¹
,
Lui
²
,
Clark
³

et al. 2009
Phys. Rev. C
61
19
88
2
View full text Add to dashboard Cite

Giant resonances inMg24andSi28from 240 MeV
Chen
¹
,
Lui
²
,
Clark
³

et al. 2009
Phys. Rev. C
61
19
88
2
View full text Add to dashboard Cite

Stellar reaction rate forMg22+p→
Al-Abdullah
¹
,
Cârstoiu
²
,
Chen
³

et al. 2010
Phys. Rev. C
27
3
16
0
View full text Add to dashboard Cite

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Web4Desktop, a Framework for Improving the Usability of Web Applications

Cited by 2 publications

References 0 publications

Giant resonances inMg24andSi28from 240 MeVChen1, Lui2, Clark3 et al. 2009Phys. Rev. C6119882View full textAdd to dashboardCite

Giant resonances inMg24andSi28from 240 MeVChen1, Lui2, Clark3 et al. 2009Phys. Rev. C6119882View full textAdd to dashboardCite

Stellar reaction rate forMg22+p→Al-Abdullah1, Cârstoiu2, Chen3 et al. 2010Phys. Rev. C273160View full textAdd to dashboardCite

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Giant resonances inMg24andSi28from 240 MeV
Chen
¹
,
Lui
²
,
Clark
³

et al. 2009
Phys. Rev. C
61
19
88
2
View full text Add to dashboard Cite

Giant resonances inMg24andSi28from 240 MeV
Chen
¹
,
Lui
²
,
Clark
³

et al. 2009
Phys. Rev. C
61
19
88
2
View full text Add to dashboard Cite

Stellar reaction rate forMg22+p→
Al-Abdullah
¹
,
Cârstoiu
²
,
Chen
³

et al. 2010
Phys. Rev. C
27
3
16
0
View full text Add to dashboard Cite