Dergi makalesi Açık Erişim
Ayik, S.; Yilmaz, O.; Acar, F.; Danisman, B.; Er, N.; Gokalp, A.
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.
Dosya adı | Boyutu | |
---|---|---|
bib-b81f0c8e-f349-4555-9538-6a198f55743b.txt
md5:cd29b70f700b253d3fbf5368d3379dd0 |
192 Bytes | İndir |
Görüntülenme | 14 |
İndirme | 5 |
Veri hacmi | 960 Bytes |
Tekil görüntülenme | 14 |
Tekil indirme | 5 |