1 Ocak 2011 Dergi makalesi Açık Erişim

Ayik, S.; Yilmaz, O.; Acar, F.; Danisman, B.; Er, N.; Gokalp, A.

DataCite XML

<?xml version='1.0' encoding='utf-8'?>
<resource xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://datacite.org/schema/kernel-4" xsi:schemaLocation="http://datacite.org/schema/kernel-4 http://schema.datacite.org/meta/kernel-4.1/metadata.xsd">
  <identifier identifierType="URL">https://aperta.ulakbim.gov.tr/record/20601</identifier>
  <creators>
    <creator>
      <creatorName>Ayik, S.</creatorName>
      <givenName>S.</givenName>
      <familyName>Ayik</familyName>
      <affiliation>Tennessee Technol Univ, Dept Phys, Cookeville, TN 38505 USA</affiliation>
    </creator>
    <creator>
      <creatorName>Yilmaz, O.</creatorName>
      <givenName>O.</givenName>
      <familyName>Yilmaz</familyName>
      <affiliation>Middle E Tech Univ, Dept Phys, TR-06531 Ankara, Turkey</affiliation>
    </creator>
    <creator>
      <creatorName>Acar, F.</creatorName>
      <givenName>F.</givenName>
      <familyName>Acar</familyName>
      <affiliation>Middle E Tech Univ, Dept Phys, TR-06531 Ankara, Turkey</affiliation>
    </creator>
    <creator>
      <creatorName>Danisman, B.</creatorName>
      <givenName>B.</givenName>
      <familyName>Danisman</familyName>
      <affiliation>Middle E Tech Univ, Dept Phys, TR-06531 Ankara, Turkey</affiliation>
    </creator>
    <creator>
      <creatorName>Er, N.</creatorName>
      <givenName>N.</givenName>
      <familyName>Er</familyName>
      <affiliation>Abant Izzet Baysal Univ, Dept Phys, Bolu, Turkey</affiliation>
    </creator>
    <creator>
      <creatorName>Gokalp, A.</creatorName>
      <givenName>A.</givenName>
      <familyName>Gokalp</familyName>
      <affiliation>Middle E Tech Univ, Dept Phys, TR-06531 Ankara, Turkey</affiliation>
    </creator>
  </creators>
  <titles>
    <title>Investigations Of Instabilities In Nuclear Matter In Stochastic Relativistic Models</title>
  </titles>
  <publisher>Aperta</publisher>
  <publicationYear>2011</publicationYear>
  <dates>
    <date dateType="Issued">2011-01-01</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Journal article</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://aperta.ulakbim.gov.tr/record/20601</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1016/j.nuclphysa.2011.04.004</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="http://www.opendefinition.org/licenses/cc-by">Creative Commons Attribution</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="Abstract">The spinodal instabilities for symmetric nuclear matter at finite temperature are studied within different relativistic mean-field models in the semi-classical approximation and the relativistic results are compared with Skyrme type non-relativistic calculations. Qualitatively similar results appear in the unstable response of the system in both non-relativistic and relativistic descriptions. Furthermore, the early growth of baryon, scalar and current density correlation functions are calculated for hot symmetric nuclear matter. (C) 2011 Elsevier B.V. All rights reserved.</description>
  </descriptions>
</resource>