<?xml version="1.0" encoding="UTF-8"?><?xml-stylesheet type="text/xsl" href="static/style.xsl"?><OAI-PMH xmlns="http://www.openarchives.org/OAI/2.0/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/ http://www.openarchives.org/OAI/2.0/OAI-PMH.xsd"><responseDate>2026-10-15T00:09:49Z</responseDate><request verb="GetRecord" identifier="oai:docta.ucm.es:20.500.14352/6391" metadataPrefix="qdc">https://docta.ucm.es/rest/oai/request</request><GetRecord><record><header><identifier>oai:docta.ucm.es:20.500.14352/6391</identifier><datestamp>2023-08-04T02:28:25Z</datestamp><setSpec>com_20.500.14352_14</setSpec><setSpec>col_20.500.14352_15</setSpec></header><metadata><qdc:qualifieddc xmlns:qdc="http://dspace.org/qualifieddc/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:dcterms="http://purl.org/dc/terms/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns:doc="http://www.lyncode.com/xoai" xsi:schemaLocation="http://purl.org/dc/elements/1.1/ http://dublincore.org/schemas/xmls/qdc/2006/01/06/dc.xsd http://purl.org/dc/terms/ http://dublincore.org/schemas/xmls/qdc/2006/01/06/dcterms.xsd http://dspace.org/qualifieddc/ http://www.ukoln.ac.uk/metadata/dcmi/xmlschema/qualifieddc.xsd">
   <dc:title>Symmetry energy properties of neutron-rich nuclei from the coherent density fluctuation model applied to nuclear matter calculations with Bonn potentials</dc:title>
   <dc:creator>Danchev, I. C.</dc:creator>
   <dc:creator>Antonov, A. N.</dc:creator>
   <dc:creator>Kadrev, D. N.</dc:creator>
   <dc:creator>Gaidarov, M. K.</dc:creator>
   <dc:creator>Sarriguren, P.</dc:creator>
   <dc:creator>Moya de Guerra, Elvira</dc:creator>
   <dcterms:abstract>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.</dcterms:abstract>
   <dcterms:dateAccepted>2023-06-16T15:20:08Z</dcterms:dateAccepted>
   <dcterms:available>2023-06-16T15:20:08Z</dcterms:available>
   <dcterms:created>2023-06-16T15:20:08Z</dcterms:created>
   <dcterms:issued>2020-06-16</dcterms:issued>
   <dc:type>journal article</dc:type>
   <dc:identifier>https://hdl.handle.net/20.500.14352/6391</dc:identifier>
   <dc:identifier>0556-2813</dc:identifier>
   <dc:identifier>10.1103/PhysRevC.101.064315</dc:identifier>
   <dc:language>eng</dc:language>
   <dc:relation>PGC2018-093636-B-I00</dc:relation>
   <dc:relation>KP-06-N38/1</dc:relation>
   <dc:rights>open access</dc:rights>
   <dc:publisher>Amer Physical Soc</dc:publisher>
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