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Investigations of instabilities in nuclear matter in stochastic relativistic models

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


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        "affiliation": "Tennessee Technol Univ, Dept Phys, Cookeville, TN 38505 USA", 
        "name": "Ayik, S."
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        "affiliation": "Middle E Tech Univ, Dept Phys, TR-06531 Ankara, Turkey", 
        "name": "Yilmaz, O."
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        "affiliation": "Middle E Tech Univ, Dept Phys, TR-06531 Ankara, Turkey", 
        "name": "Acar, F."
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      {
        "affiliation": "Middle E Tech Univ, Dept Phys, TR-06531 Ankara, Turkey", 
        "name": "Danisman, B."
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      {
        "affiliation": "Abant Izzet Baysal Univ, Dept Phys, Bolu, Turkey", 
        "name": "Er, N."
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      {
        "affiliation": "Middle E Tech Univ, Dept Phys, TR-06531 Ankara, Turkey", 
        "name": "Gokalp, A."
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    "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.", 
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      "issue": "1", 
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