1975
DOI: 10.1103/physrevc.12.1730
|View full text |Cite
|
Sign up to set email alerts
|

Angular distribution measurements forC14(d, p)C

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2

Citation Types

9
68
1

Year Published

1981
1981
2015
2015

Publication Types

Select...
5
3

Relationship

0
8

Authors

Journals

citations
Cited by 73 publications
(78 citation statements)
references
References 9 publications
9
68
1
Order By: Relevance
“…Since this channel contributes less than 5% to the total capture cross section at the relevant energies, the final result is not very sensitive to the particular choice of this spectroscopic factor. A fit to the experimental data, weighted by the relative error bar of each data point, was then performed and resulted in a best-fit spectroscopic factor of C 2 S 0 = 0.95 ± 0.05 for the ground state 1s 1/2 single-particle configuration, which is in good agreement with 0.88 as derived from (d, p) data [31]. The final calculated cross section, convoluted with the different neutron spectra, is compared with the experimental data in Table V.…”
Section: B Theoretical Modeling Of Direct Radiative Capturesupporting
confidence: 52%
See 1 more Smart Citation
“…Since this channel contributes less than 5% to the total capture cross section at the relevant energies, the final result is not very sensitive to the particular choice of this spectroscopic factor. A fit to the experimental data, weighted by the relative error bar of each data point, was then performed and resulted in a best-fit spectroscopic factor of C 2 S 0 = 0.95 ± 0.05 for the ground state 1s 1/2 single-particle configuration, which is in good agreement with 0.88 as derived from (d, p) data [31]. The final calculated cross section, convoluted with the different neutron spectra, is compared with the experimental data in Table V.…”
Section: B Theoretical Modeling Of Direct Radiative Capturesupporting
confidence: 52%
“…3 to facilitate a direct comparison with the data from the activation measurement. The calculated capture to the first excited state of 15 C was normalized by the spectroscopic factor C 2 S 1 = 0.69, extracted from experimental neutron transfer 14 C(d, p) 15 C * data [31]. Since this channel contributes less than 5% to the total capture cross section at the relevant energies, the final result is not very sensitive to the particular choice of this spectroscopic factor.…”
Section: B Theoretical Modeling Of Direct Radiative Capturementioning
confidence: 99%
“…] it was shown that the 14 C(n, γ) 15 C radiative capture at astrophysically relevant energies is peripheral reaction, i.e. the overall normalization of its cross section is determined by the asymptotic normalization coefficient (ANC) for 15 …”
mentioning
confidence: 99%
“…the overall normalization of its cross section is determined by the asymptotic normalization coefficient (ANC) for 15 …”
mentioning
confidence: 99%
“…For the magnitude of its tail to be determined by C mir , the single-particle wave function should be multiplied by a spectroscopic amplitude S 1=2 mir C mir =b s:p: , where b s:p: is the single-particle ANC obtained in such a model. Table II were used in the analysis of the 14 Cd; p 15 C reaction within the distorted wave Born approximation [19], direct (n; ) calculations [5], time-dependent [20], and distorted [21] and from knockout [22], are smaller than C 2 mir and S mir by 25%. This discrepancy may originate due to either insufficient understanding of one-nucleon removal reactions, or to underestimating the R ÿ .…”
mentioning
confidence: 99%