Danchev, I. C.Antonov, A. N.Kadrev, D. N.Gaidarov, M. K.Sarriguren, P.Moya de Guerra, Elvira2023-06-162023-06-162020-06-160556-281310.1103/PhysRevC.101.064315https://hdl.handle.net/20.500.14352/6391©2020 American Physical Society. I.C.D. thanks Prof. F. Myhrer and Prof. K. Kubodera for numerous discussions and valuable advice and Prof. R. Machleidt and Prof. M. Hjorth-Jensen for their help in developing his computer code. I.C.D. also acknowledges partial financial support from the University of Mount Olive Professional Development Fund. A.N.A., D.N.K., and M.K.G. are grateful for the support of the Bulgarian National Science Fund under Contract No. KP-06-N38/1. P.S. acknowledges support from Ministerio de Ciencia, Innovación y Universidades MCIU/AEI/FEDER,UE (Spain) under Contract No. PGC2018-093636-B-I00.We derive the values of nuclear symmetry energy, its components, as well as pressure in finite nuclei at saturation density from their corresponding values in nuclear matter obtained in nonrelativistic Brueckner-Hartree-Fock calculations with the realistic Bonn B and Bonn CD potentials using the coherent density fluctuation model in the framework of a self-consistent Skyrme-Hartree-Fock plus BCS method. We focus on three isotopic chains of spherical nuclei (Ni, Sn, and Pb) and compare our results with those obtained with an effective Brueckner density-dependent potential. The role of the three-body forces on the considered quantities is also studied and discussed.engjournal articlehttps://doi.org/10.1103/PhysRevC.101.064315https://journals.aps.org/open access539.1Strongly interacting particlesMany-body problemStatistical-theorySpin-isospinStateDependenceEquation2-bodyParametrizationSaturationFísica nuclear2207 Física Atómica y Nuclear