Spinodal instabilities in nuclear matter in a stochastic relativistic mean-field approach


Creative Commons License

Ayik S., YILMAZ TÜZÜN Ö., Er N., Gokalp A., Ring P.

PHYSICAL REVIEW C, cilt.80, sa.3, 2009 (SCI İndekslerine Giren Dergi) identifier identifier

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 80 Konu: 3
  • Basım Tarihi: 2009
  • Doi Numarası: 10.1103/physrevc.80.034613
  • Dergi Adı: PHYSICAL REVIEW C

Özet

Spinodal instabilities and early growth of baryon density fluctuations in symmetric nuclear matter are investigated in the basis of the stochastic extension of the relativistic mean-field approach in the semiclassical approximation. Calculations are compared with the results of nonrelativistic calculations based on Skyrme-type effective interactions under similar conditions. A qualitative difference appears in the unstable response of the system: the system exhibits most unstable behavior at higher baryon densities around rho(b) = 0.4 rho(0) in the relativistic approach while most unstable behavior occurs at lower baryon densities around rho(b) = 0.2 rho(0) in the nonrelativistic calculations