Investigations of instabilities in nuclear matter in stochastic relativistic models

Ayik S., YILMAZ O., ACAR F. P., Danisman B., Er N., Gokalp A.

NUCLEAR PHYSICS A, cilt.859, sa.1, ss.73-86, 2011 (SCI-Expanded) identifier identifier

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 859 Sayı: 1
  • Basım Tarihi: 2011
  • Doi Numarası: 10.1016/j.nuclphysa.2011.04.004
  • Dergi Adı: NUCLEAR PHYSICS A
  • Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Sayfa Sayıları: ss.73-86
  • Atatürk Üniversitesi Adresli: Hayır

Özet

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.