Asosiy kontentga oʻtish
Maqola

Sub-Barrier Coulomb Excitation of [sup 106,108,110]Sn

A. EkströmNuclear physicsJ. CederkällNuclear physicsC. FahlanderNuclear physicsM. Hjorth‐JensenPhysics Department, University of Lund, Box 118, SE-221 00 Lund, SwedenF. AmesHeavy Ion Laboratory, Warsaw University, PolandP. A. ButlerOliver Lodge Laboratory, University of Liverpool, United KingdomT. DavinsonJ. EberthG. GeorgievEuropean Organization for Nuclear ResearchA. GörgenInstituut voor Kern-en Stralingsfysica, K.U. Leuven, BelgiumM. GórskaD. HabsDepartment of Physics, University of Oslo, NorwayM. HuyseOleg V. IvanovDepartment of Physics, University of Oslo, NorwayJ. IwanickiInstituut voor Kern-en Stralingsfysica, K.U. Leuven, BelgiumO. KesterGesellschaft für Schwerionenforschung, Darmstadt, GermanyU. KösterB. A. MarshP. ReiterMax Planck Institute for Nuclear PhysicsH. ScheitMax Planck Institute for Nuclear PhysicsD. SchwalmMax Planck Institute for Nuclear PhysicsS. SiemI. ŞtefânescuPhysics Department and Center of Mathematics for Applications, University of Oslo, NorwayG. M. TvetenJ. Van de WalleDepartment of Physics and Astronomy, University of Edingburg, United KingdomP. Van DuppenDepartment of Physics, University of Oslo, NorwayD. VoulotN. WarrTRIUMF, Vancouver, CanadaD. WeißhaarPhysics Department and Center of Mathematics for Applications, University of Oslo, NorwayF. WenanderTRIUMF, Vancouver, CanadaMagdalena ZielińskaAB Department, CERN 1211, Geneva 23, SwitzerlandP. DemetriouAB Department, CERN 1211, Geneva 23, SwitzerlandR. JulinTRIUMF, Vancouver, CanadaS. Harissopulos
ABI

Annotatsiya

The reduced transition probabilities between the first excited 2+ state and the 0+ ground state, B(E2;0+→2+), have been measured in 106,108,110Sn using sub‐barrier Coulomb excitation in inverse kinematics at REX‐ISOLDE. The results are, B(E2;0+→2+) = 0.220(22), 0.226(17), and 0.228(32)e2b2, for 110Sn, 108Sn, and 106Sn, respectively. The results for 106,108Sn are preliminary. De‐excitation γ‐rays were detected by the MINIBALL Ge‐array. The B(E2) reveals detailed information about the nuclear wave function. A shell model prediction based on an effective CD‐Bonn interaction in the ν(0g7/2,2s,1d,0h11/2) model space using eeffν = 1.0 e follows the experimental values for the neutron rich Sn isotopes, but fails to reproduce the results presented here.

Hali tarjima qilinmagan

Mavzular

Identifikatorlar

Iqtiboslar va manbalar

0 ta iqtibos0 ta foydalanilgan manba