2007
DOI: 10.1016/j.nuclphysa.2006.12.020
|View full text |Cite
|
Sign up to set email alerts
|

The ELISe experiment at FAIR

Help me understand this report

Search citation statements

Order By: Relevance

Paper Sections

Select...
2
1
1
1

Citation Types

2
57
0
1

Year Published

2008
2008
2017
2017

Publication Types

Select...
6

Relationship

0
6

Authors

Journals

citations
Cited by 47 publications
(60 citation statements)
references
References 21 publications
2
57
0
1
Order By: Relevance
“…In Fig. 17(b), we see that the value of σ 2 remains almost constant between 22 8 O and 28 14 Si when mainly the 1d 5/2 shell is being filled. From 30 16 S on, the 2s 1/2 and 1d 3/2 levels start to be appreciably occupied and σ 2 starts increasing almost linearly with A until the proton-drip-line nucleus 34 20 Ca.…”
Section: N = 14 Isotonic Chainmentioning
confidence: 85%
See 4 more Smart Citations
“…In Fig. 17(b), we see that the value of σ 2 remains almost constant between 22 8 O and 28 14 Si when mainly the 1d 5/2 shell is being filled. From 30 16 S on, the 2s 1/2 and 1d 3/2 levels start to be appreciably occupied and σ 2 starts increasing almost linearly with A until the proton-drip-line nucleus 34 20 Ca.…”
Section: N = 14 Isotonic Chainmentioning
confidence: 85%
“…The N = 82 isotones below 132 Sn are believed to be in close relation with the peak of the solar r-process abundance distribution observed around the mass number A = 130 [43,44], whereas the N = 50 isotones near 78 Ni are thought to be responsible for producing the pronounced abundance peak observed around A = 80 [43,45]. On the other hand, scattering data for light nuclei, such as those of N = 14, are likely to be obtained in future electron scattering facilities such as SCRIT [19][20][21] and ELISe [22,23].…”
Section: Introductionmentioning
confidence: 82%
See 3 more Smart Citations