Effects of core polarization and exchange currents on the magnetic form factors of 0f 7/2 and 0g 9/2-shell nuclei

1979 ◽  
Vol 293 (1) ◽  
pp. 5-8 ◽  
Author(s):  
T. Suzuki ◽  
H. Hyuga ◽  
A. Arima
Keyword(s):  
Form Factors ◽  
Core Polarization ◽  
Magnetic Form Factors

Core polarization effects on the magnetic form factors of15N and17O

1992 ◽  
Vol 105 (5) ◽  
pp. 695-702 ◽  
Author(s):  
A. Gökalp ◽  
O. Yilmaz
Keyword(s):  
Form Factors ◽  
Core Polarization ◽  
Polarization Effects ◽  
Magnetic Form Factors

Core-polarization effects on magnetic form factors ofPb207,Pb208, andBi209

1982 ◽  
Vol 26 (2) ◽  
pp. 750-753 ◽  
Author(s):  
Toshio Suzuki ◽  
Makoto Oka ◽  
Hiroyuki Hyuga ◽  
Akito Arima
Keyword(s):  
Form Factors ◽  
Core Polarization ◽  
Polarization Effects ◽  
Magnetic Form Factors

scholarly journals High-precision determination of the electric and magnetic form factors of the proton

2011 ◽  
Author(s):  
Jan C. Bernauer ◽  
Atsushi Hosaka ◽  
Kanchan Khemchandani ◽  
Hideko Nagahiro ◽  
Kanabu Nawa ◽  
...  
Keyword(s):  
High Precision ◽  
Form Factors ◽  
Precision Determination ◽  
Magnetic Form Factors ◽  
High Precision Determination

Theoretical Magnetic Form Factors ofCo++andFe++in Their Monoxides

1971 ◽  
Vol 4 (11) ◽  
pp. 3901-3911 ◽  
Author(s):  
A. Mahendra ◽  
D. C. Khan
Keyword(s):  
Form Factors ◽  
Magnetic Form Factors

scholarly journals O2 State in 18 O by using Core – Polarization effects

2008 ◽  
pp. 66-72
Keyword(s):  
Perturbation Theory ◽  
Experimental Studies ◽  
Form Factors ◽  
Wave Model ◽  
Collective Model ◽  
Core Polarization ◽  
Polarization Effects ◽  
The Core ◽  
The Subject ◽  
Space Wave

Coulomb form factors for E0 transition in 18O are discussed taking into account core-polarization effects. These effects are taken into account through the collective model of Tassie and also through a microscopic perturbation theory including excitations up to 2p1f shell. Space wave model functions defined for the orbits 1 and 2125O nucleus has been the subject of extensive theoretical and experimental studies, which received much attention in last decade [Alex Brown et.al.2005]. The 18O system contains two neutrons in addition to the16O core distributed in the sd – shell. d1 are obtained from the diagonalization of the interaction Hamilonian of Wildenthal. The calculations include the 0 2state with excitation energies3.6337MeV. The core – polarization effects which incorporate the ollective model of Tassei describe the data very well for this state.

scholarly journals Precise neutron magnetic form factors

2002 ◽  
Vol 524 (1-2) ◽  
pp. 26-32 ◽  
Author(s):  
G Kubon ◽  
H Anklin ◽  
P Bartsch ◽  
D Baumann ◽  
W.U Boeglin ◽  
...  
Keyword(s):  
Form Factors ◽  
Magnetic Form Factors
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