scholarly journals Nuclear energy density functionals from empirical ground-state densities

2021 ◽  
Vol 103 (4) ◽  
Author(s):  
Giacomo Accorto ◽  
Tomoya Naito ◽  
Haozhao Liang ◽  
Tamara Nikšić ◽  
Dario Vretenar
2010 ◽  
Vol 19 (04) ◽  
pp. 548-557 ◽  
Author(s):  
D. VRETENAR ◽  
T. NIKŠIĆ ◽  
P. RING

A class of relativistic nuclear energy density functionals is explored, in which only nucleon degrees of freedom are explicitly used in the construction of effective interaction terms. Short-distance correlations, as well as intermediate and long-range dynamics, are encoded in the nucleon-density dependence of the strength functionals of an effective interaction Lagrangian. The resulting phenomenological effective interaction, adjusted to experimental binding energies of a large set of axially deformed nuclei, together with a new separable pairing interaction adjusted to reproduce the pairing gap in nuclear matter calculated with the Gogny force, is applied in triaxial relativistic Hartree-Bogoliubov calculations of sequences of heavy nuclei: Th , U , Pu , Cm , Cf , Fm , and No .


2011 ◽  
Vol 83 (3) ◽  
Author(s):  
N. Nikolov ◽  
N. Schunck ◽  
W. Nazarewicz ◽  
M. Bender ◽  
J. Pei

2020 ◽  
Vol 224 ◽  
pp. 145-165
Author(s):  
Derk Pieter Kooi ◽  
Paola Gori-Giorgi

We analyse a path to construct density functionals for the dispersion interaction energy from an expression in terms of the ground state densities and exchange–correlation holes of the isolated fragments.


2010 ◽  
Vol 81 (6) ◽  
Author(s):  
Ch. C. Moustakidis ◽  
T. Nikšić ◽  
G. A. Lalazissis ◽  
D. Vretenar ◽  
P. Ring

2020 ◽  
Vol 51 (3) ◽  
pp. 611
Author(s):  
P. Bączyk ◽  
M. Konieczka ◽  
K.M.L. Martinez ◽  
S. Antić ◽  
P.A.M. Guichon ◽  
...  

2019 ◽  
Vol 18 ◽  
pp. 107
Author(s):  
Ch. C. Moustakidis ◽  
T. Niksic ◽  
G. A. Lalazissis ◽  
D. Vretenar ◽  
P. Ring

The transition density nt and pressure Pt at the inner edge between the liquid core and the solid crust of a neutron star are analyzed using the thermodynami- cal method and the framework of relativistic nuclear energy density functionals. Starting from a functional that has been carefully adjusted to experimental binding energies of finite nuclei, and varying the density dependence of the cor- responding symmetry energy within the limits determined by isovector prop- erties of finite nuclei, we estimate the constraints on the core-crust transition density and pressure of neutron stars: 0.086 fm−3 ≤ nt < 0.090 fm−3 and 0.3 MeV fm−3 < Pt ≤ 0.76 MeV fm−3 [1].


2020 ◽  
Vol 56 (6) ◽  
Author(s):  
Young-Min Kim ◽  
Kyujin Kwak ◽  
Chang Ho Hyun ◽  
Hana Gil ◽  
Chang-Hwan Lee

2014 ◽  
Vol 89 (2) ◽  
Author(s):  
L. M. Robledo ◽  
R. N. Bernard ◽  
G. F. Bertsch

2016 ◽  
Vol 724 ◽  
pp. 012041
Author(s):  
X. Roca-Maza ◽  
G. Colò ◽  
H. Z. Liang ◽  
J. Meng ◽  
P. Ring ◽  
...  

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