2005
DOI: 10.1016/j.nuclphysa.2005.05.106
|View full text |Cite
|
Sign up to set email alerts
|

The reaction rate for the destruction of fluorine in AGB stars

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
3
1

Citation Types

1
11
0

Year Published

2008
2008
2017
2017

Publication Types

Select...
2
1

Relationship

1
2

Authors

Journals

citations
Cited by 3 publications
(12 citation statements)
references
References 3 publications
1
11
0
Order By: Relevance
“…The differential cross section of the 19 F(α, p) 22 Ne reaction was determined relative to the differential cross section for elastic scattering measured at 160 • . It has been shown by Huang-sheng et al [22] and by Cseh et al [23] that below E lab = 2.5 MeV the elastic scattering of 4 He on 19 F follows the Rutherford law,…”
Section: Experimental Methodsmentioning
confidence: 94%
See 3 more Smart Citations
“…The differential cross section of the 19 F(α, p) 22 Ne reaction was determined relative to the differential cross section for elastic scattering measured at 160 • . It has been shown by Huang-sheng et al [22] and by Cseh et al [23] that below E lab = 2.5 MeV the elastic scattering of 4 He on 19 F follows the Rutherford law,…”
Section: Experimental Methodsmentioning
confidence: 94%
“…This study included the direct measurement of the 19 F(α, p) 22 Ne reaction by detecting both p 0 and p 1 protons (see Refs. [19,20]) as well as the additional measurement of the p 1 channel via the detection of the γ -ray transition [21] from the first excited state (2 + ) to the ground state (0 + ) of 22 Ne (see Fig. 1).…”
Section: Experimental Methodsmentioning
confidence: 99%
See 2 more Smart Citations
“…α + 0.0 (MeV) 23 Na FIG. 1: Energy level scheme for the 19 F(α,p) 22 Ne reaction. The entrance channel (α+ 19 F) has a threshold of 10.47 MeV with respect to the ground state of 23 Na.…”
mentioning
confidence: 99%