scholarly journals Above-barrier heavy-ion fusion cross-sections using the relativistic mean-field approach: Case of spherical colliding nuclei

2020 ◽  
Vol 994 ◽  
pp. 121657 ◽  
Author(s):  
M.V. Chushnyakova ◽  
M. Bhuyan ◽  
I.I. Gontchar ◽  
N.A. Khmyrova
2004 ◽  
Vol 13 (01) ◽  
pp. 309-313 ◽  
Author(s):  
A. DOBROWOLSKI ◽  
K. POMORSKI ◽  
J. BARTEL

Using the collective potential between colliding ions based on the effective nucleon-nucleon interactions of the Skyrme type and the semi-classical Extended Thomas-Fermi approach we describe heavy-ion fusion cross sections applying a Monte-Carlo sampling method of trajectories with the Langevin formalism using friction as described in the so-called Surface-Friction Model.


2008 ◽  
Vol 17 (09) ◽  
pp. 1765-1773 ◽  
Author(s):  
JIGUANG CAO ◽  
ZHONGYU MA ◽  
NGUYEN VAN GIAI

The microscopic properties and superfluidity of the inner crust in neutron stars are investigated in the framework of the relativistic mean field(RMF) model and BCS theory. The Wigner-Seitz(W-S) cell of inner crust is composed of neutron-rich nuclei immersed in a sea of dilute, homogeneous neutron gas. The pairing properties of nucleons in the W-S cells are treated in BCS theory with Gogny interaction. In this work, we emphasize on the choice of the boundary conditions in the RMF approach and superfluidity of the inner crust. Three kinds of boundary conditions are suggested. The properties of the W-S cells with the three kinds of boundary conditions are investigated. The neutron density distributions in the RMF and Hartree-Fock-Bogoliubov(HFB) models are compared.


2018 ◽  
Vol 98 (2) ◽  
Author(s):  
Z.-X. Liu ◽  
C.-J. Xia ◽  
W.-L. Lu ◽  
Y.-X. Li ◽  
J. N. Hu ◽  
...  

1975 ◽  
Vol 248 (2) ◽  
pp. 356-376 ◽  
Author(s):  
R. Broda ◽  
M. Ishihara ◽  
B. Herskind ◽  
H. Oeschler ◽  
S. Ogaza ◽  
...  

2012 ◽  
Vol 21 (08) ◽  
pp. 1250074 ◽  
Author(s):  
CHIRASHREE LAHIRI ◽  
G. GANGOPADHYAY

Densities from relativistic mean field calculations are applied to construct the optical potential and, hence calculate the endpoint of the rapid proton capture (rp) process. Mass values are taken from a new phenomenological mass formula. Endpoints are calculated for different temperature-density profiles of various X-ray bursters. We find that the rp process can produce significant quantities of nuclei upto around mass 95. Our results differ from existing works to some extent.


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