Ayık, S.Yılmaz, O.Acar, F.Danışman, B.Er, Nuray2021-06-232021-06-2320110375-9474https://doi.org/10.1016/j.nuclphysa.2011.04.004https://hdl.handle.net/20.500.12491/6939The 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.eninfo:eu-repo/semantics/closedAccessSpinodal InstabilityStochastic Mean-fieldArticle10.1016/j.nuclphysa.2011.04.004859173862-s2.0-79957790662Q2WOS:000292430300007Q3