NEUTRON DENSITY DISTRIBUTIONS IN SPHERICALLY SYMMETRIC LEAD ISOTOPES

2010 ◽  
Vol 25 (24) ◽  
pp. 2071-2076
Author(s):  
S. HADDAD
Keyword(s):  
Density Distribution ◽  
Lead Isotopes ◽  
Neutron Density ◽  
Spherically Symmetric ◽  
Fermi Model ◽  
Thomas Fermi ◽  
Density Distributions ◽  
Fermi Distribution ◽  
Neutron Density Distribution ◽  
Two Parameter

Based on a relativistic Thomas–Fermi model, it is shown that a two-parameter Fermi distribution can be used for describing the neutron density distribution in the 208 Pb nucleus.

Ratio of pion-nucleus reaction cross sections and the neutron density distribution for lead

1972 ◽  
Vol 41 (5) ◽  
pp. 577-580 ◽  
Author(s):  
B.W. Allardyce ◽  
C.J. Batty ◽  
D.J. Baugh ◽  
E. Friedman ◽  
G. Heymann ◽  
...  
Keyword(s):  
Density Distribution ◽  
Cross Sections ◽  
Reaction Cross ◽  
Neutron Density ◽  
Neutron Density Distribution ◽  
Reaction Cross Sections

scholarly journals Average CsI Neutron Density Distribution from COHERENT Data

2018 ◽  
Vol 120 (7) ◽  
Author(s):  
M. Cadeddu ◽  
C. Giunti ◽  
Y. F. Li ◽  
Y. Y. Zhang
Keyword(s):  
Density Distribution ◽  
Neutron Density ◽  
Neutron Density Distribution

ISOSPIN EFFECT AND ISOSCALING PHENOMENON IN PROJECTILE FRAGMENTATION

2008 ◽  
Vol 17 (09) ◽  
pp. 1669-1680 ◽  
Author(s):  
C. W. MA ◽  
Y. FU ◽  
D. Q. FANG ◽  
Y. G. MA ◽  
X. Z. CAI ◽  
...  
Keyword(s):  
Excitation Energy ◽  
Projectile Fragmentation ◽  
Skin Thickness ◽  
Neutron Density ◽  
Neutron Skin ◽  
Density Distributions ◽  
Neutron Rich Nucleus ◽  
Neutron Skin Thickness ◽  
Neutron Density Distribution ◽  
The Relationship

We have studied the isospin effect and isoscaling behavior in projectile fragmentation using a modified statistical abrasion-ablation (SAA) model. The relationship between neutron skin thickness (δnp) and neutron abrasion cross section (σ nabr ) has also been investigated. We find the normalized peak differences and reduced isoscaling parameters decrease with (Z proj - Z)/Z proj or the excitation energy per nucleon and have no significant dependence on the size of the reaction systems. The excitation energy dependence of the symmetry energy coefficients are tentatively extracted from α and β. Assuming Fermi-type density distributions for proton and neutron and introducing a parameter to adjust the diffuseness of the neutron density distribution for neutron-rich nucleus, δnp and σ nabr for neutron-rich nucleus were found to have a linear correlation. It is suggested that σ nabr could be used as an observable to extract the neutron skin thickness for neutron-rich nucleus.

Neutron density distribution and the halo structure ofC22

2011 ◽  
Vol 83 (3) ◽  
Author(s):  
Manjari Sharma ◽  
A. Bhagwat ◽  
Z. A. Khan ◽  
W. Haider ◽  
Y. K. Gambhir
Keyword(s):  
Density Distribution ◽  
Neutron Density ◽  
Halo Structure ◽  
Neutron Density Distribution

scholarly journals Average CsI neutron density distribution from COHERENT data

2019 ◽  
Author(s):  
Matteo Cadeddu ◽  
Carlo Giunti ◽  
Yufeng Li ◽  
Yiyu Zhang
Keyword(s):  
Density Distribution ◽  
Neutron Density ◽  
Neutron Density Distribution
Sign in / Sign up

Export Citation Format

Share Document