Electron charge form factors and static properties of extremely light 1p-shell nuclei within the anisotropic-oscillator model involving projections

2000 ◽  
Vol 63 (5) ◽  
pp. 739-751
Author(s):  
A. L. Savchenko ◽  
V. K. Tartakovsky ◽  
A. V. Fursaev
2019 ◽  
Vol 28 (03) ◽  
pp. 1950015
Author(s):  
Xiaoyong Guo ◽  
Zaijun Wang ◽  
Tianjing Li ◽  
Jian Liu

We construct a scheme to calculate the charge form factors for the elastic electron scattering. Our calculation is based on the relativistic eikonal approximation and the Skyrme–Hartree–Fock equation. To perform our calculation and benchmark the results, eight model nuclei with available experimental data: [Formula: see text], [Formula: see text], [Formula: see text], [Formula: see text], [Formula: see text], [Formula: see text], [Formula: see text], and [Formula: see text] are considered. For the comparison, the charge form factors calculated by the relativistic mean-field (RMF) model are also provided. Parameter set SLy5 is utilized for the Skyrme force, and the set NL3 is applied for the RMF model. It has been confirmed that combining of a nonrelativistic treatment for the target nucleus with a relativistic treatment for the incident electron may work better to reach highly descriptive and predictive results similar to the pure relativistic treatment. The results of this work are also useful for future experiments to test different inputs of densities for a specific nucleus.


1978 ◽  
Vol 17 (3) ◽  
pp. 874-878 ◽  
Author(s):  
C. Y. Hu ◽  
S. A. Moszkowski ◽  
D. L. Shannon

1990 ◽  
Vol 41 (5) ◽  
pp. 1568-1577 ◽  
Author(s):  
N. Barik ◽  
S. N. Jena ◽  
D. P. Rath

1986 ◽  
Vol 459 (3-4) ◽  
pp. 645-662 ◽  
Author(s):  
Leonard S. Kisslinger ◽  
Ma Wei-Hsing ◽  
Pervez Hoodbhoy

2011 ◽  
Vol 26 (03n04) ◽  
pp. 677-678
Author(s):  
MARTA ŁUSZCZAK ◽  
ANTONI SZCZUREK

The cross sections for exclusive D+D- meson pair production in nucleus - nucleus collisions are calculated and differential distributions are shown. Realistic (Fourier transform of the charge density) charge form factors of nuclei are used. Absorption effects are included. Predictions for the STAR and PHENIX collaboration measurements at RHIC are presented.


1995 ◽  
Vol 351 (1-3) ◽  
pp. 24-28 ◽  
Author(s):  
W.W. Buck ◽  
R.A. Williams ◽  
Hiroshi Ito
Keyword(s):  

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