1 Ocak 2011 Dergi makalesi Açık Erişim

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

Dublin Core

<?xml version='1.0' encoding='utf-8'?>
<oai_dc:dc xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
  <dc:creator>Ayik, S.</dc:creator>
  <dc:creator>Yilmaz, O.</dc:creator>
  <dc:creator>Acar, F.</dc:creator>
  <dc:creator>Danisman, B.</dc:creator>
  <dc:creator>Er, N.</dc:creator>
  <dc:creator>Gokalp, A.</dc:creator>
  <dc:date>2011-01-01</dc:date>
  <dc:description>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.</dc:description>
  <dc:identifier>https://aperta.ulakbim.gov.trrecord/20601</dc:identifier>
  <dc:identifier>oai:zenodo.org:20601</dc:identifier>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>http://www.opendefinition.org/licenses/cc-by</dc:rights>
  <dc:source>NUCLEAR PHYSICS A 859(1) 73-86</dc:source>
  <dc:title>Investigations of instabilities in nuclear matter in stochastic relativistic models</dc:title>
  <dc:type>info:eu-repo/semantics/article</dc:type>
  <dc:type>publication-article</dc:type>
</oai_dc:dc>