Relativistic mean field approach with density dependent couplings for finite nuclei

1997 ◽  
Vol 55 (3) ◽  
pp. 1211-1217 ◽  
Author(s):  
H. Shen ◽  
Y. Sugahara ◽  
H. Toki
Keyword(s):  
Mean Field ◽  
Density Dependent ◽  
Field Approach ◽  
Relativistic Mean Field ◽  
Finite Nuclei

ELECTROMAGNETIC AND ISOVECTOR TERMS IN STANDARD RELATIVISTIC MEAN FIELD MODEL

2011 ◽  
Vol 20 (09) ◽  
pp. 1983-2010 ◽  
Author(s):  
A. SULAKSONO
Keyword(s):  
Nuclear Matter ◽  
Field Model ◽  
Local Density ◽  
Mean Field ◽  
Binding Energies ◽  
Particle Spectrum ◽  
Mean Field Model ◽  
Density Dependent ◽  
Relativistic Mean Field ◽  
Finite Nuclei

The effects of auxiliary contribution in forms of electromagnetic tensors and relativistic electromagnetic exchange in local density approximation as well as δ meson and isovector density-dependent nonlinear terms in standard relativistic mean field model constrained by nuclear matter stability criteria in some selected finite nuclei and nuclear matter properties are studied. It is found that in the case of finite nuclei, the electromagnetic tensors play the most dominant part compared to other auxiliary terms. Due to the presence of electromagnetic tensors, the binding energies prediction of the model can be improved quite significantly. However, these terms do not yield demanded effects for rms radii prediction. In the case of nuclear matter properties, the isovector density-dependent nonlinear term plays the most crucial role in providing predictions which are quite compatible with experimental constraints. We have also shown these auxiliary contributions are indeed unable to improve the single particle spectrum results of the model.

THE INNER CRUST OF NEUTRON STARS IN RELATIVISTIC MEAN FIELD APPROACH

2008 ◽  
Vol 17 (09) ◽  
pp. 1765-1773 ◽  
Author(s):  
JIGUANG CAO ◽  
ZHONGYU MA ◽  
NGUYEN VAN GIAI
Keyword(s):  
Boundary Conditions ◽  
Neutron Stars ◽  
Mean Field ◽  
Bcs Theory ◽  
Neutron Density ◽  
Field Approach ◽  
Hartree Fock ◽  
Relativistic Mean Field ◽  
Density Distributions ◽  
Rmf Model

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.

Relativistic mean-field approach for Λ,Ξ , and Σ hypernuclei

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

scholarly journals ENDPOINT OF rp PROCESS USING RELATIVISTIC MEAN FIELD APPROACH AND A NEW MASS FORMULA

2012 ◽  
Vol 21 (08) ◽  
pp. 1250074 ◽  
Author(s):  
CHIRASHREE LAHIRI ◽  
G. GANGOPADHYAY
Keyword(s):  
Mass Formula ◽  
Optical Potential ◽  
Mean Field ◽  
Proton Capture ◽  
Density Profiles ◽  
X Ray ◽  
Field Approach ◽  
Relativistic Mean Field ◽  
Rapid Proton ◽  
Rp Process

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.

Dimensional effects in a relativistic mean-field approach

1998 ◽  
Vol 57 (2) ◽  
pp. 857-865 ◽  
Author(s):  
A. Delfino ◽  
Lizardo H. C. M. Nunes ◽  
J. S. Sá Martins
Keyword(s):  
Mean Field ◽  
Field Approach ◽  
Relativistic Mean Field ◽  
Dimensional Effects
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