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Coulomb excitation of 104Sn and the strength of the 100Sn shell closure.

Authors :
Guastalla G
DiJulio DD
Górska M
Cederkäll J
Boutachkov P
Golubev P
Pietri S
Grawe H
Nowacki F
Sieja K
Algora A
Ameil F
Arici T
Atac A
Bentley MA
Blazhev A
Bloor D
Brambilla S
Braun N
Camera F
Dombrádi Z
Domingo Pardo C
Estrade A
Farinon F
Gerl J
Goel N
Grȩbosz J
Habermann T
Hoischen R
Jansson K
Jolie J
Jungclaus A
Kojouharov I
Knoebel R
Kumar R
Kurcewicz J
Kurz N
Lalović N
Merchan E
Moschner K
Naqvi F
Nara Singh BS
Nyberg J
Nociforo C
Obertelli A
Pfützner M
Pietralla N
Podolyák Z
Prochazka A
Ralet D
Reiter P
Rudolph D
Schaffner H
Schirru F
Scruton L
Sohler D
Swaleh T
Taprogge J
Vajta Z
Wadsworth R
Warr N
Weick H
Wendt A
Wieland O
Winfield JS
Wollersheim HJ
Source :
Physical review letters [Phys Rev Lett] 2013 Apr 26; Vol. 110 (17), pp. 172501. Date of Electronic Publication: 2013 Apr 23.
Publication Year :
2013

Abstract

A measurement of the reduced transition probability for the excitation of the ground state to the first 2+ state in 104Sn has been performed using relativistic Coulomb excitation at GSI. 104Sn is the lightest isotope in the Sn chain for which this quantity has been measured. The result is a key point in the discussion of the evolution of nuclear structure in the proximity of the doubly magic nucleus 100Sn. The value B(E2; 0+ → 2+) = 0.10(4) e2b2 is significantly lower than earlier results for 106Sn and heavier isotopes. The result is well reproduced by shell model predictions and therefore indicates a robust N = Z = 50 shell closure.

Details

Language :
English
ISSN :
1079-7114
Volume :
110
Issue :
17
Database :
MEDLINE
Journal :
Physical review letters
Publication Type :
Academic Journal
Accession number :
23679711
Full Text :
https://doi.org/10.1103/PhysRevLett.110.172501