Research Article Open Access

THE PROPERTIES OF NUCLEAR MATTER

Khaled Hassaneen1, Hesham Mansour2 and Khaled Hassaneen3
  • 1 Department of Physics, Faculty of Science, Sohag University, Sohag, Egypt
  • 2 Department of Physics, Faculty of Science, Cairo University, Gizza, Egypt
  • 3 Department of Physics, Faculty of Science, Taif University, Taif, Saudi Arabia

Abstract

The microscopic and bulk properties of nuclear matter at zero and finite temperatures are studied in the frame of the Brueckner theory. The results for the symmetry energy are also obtained using different potentials. The calculations are based on realistic nucleon-nucleon interactions which reproduce the nucleon-nucleon phase shifts. These microscopic approaches are supplemented by a density-dependent contact interaction to achieve the empirical saturation property of symmetric nuclear matter. Special attention is paid to behavior of the effective mass in asymmetric nuclear matter. The nuclear symmetry potential at fixed nuclear density is also calculated and its value decreases with increasing the nucleon energy. The hot properties of nuclear matter are also calculated using T2-approximation at low temperatures. Good agreement is obtained in comparison with previous works around the saturation point.

Physics International
Volume 4 No. 1, 2013, 37-59

DOI: https://doi.org/10.3844/pisp.2013.37.59

Submitted On: 3 September 2012 Published On: 17 July 2013

How to Cite: Hassaneen, K. & Mansour, H. (2013). THE PROPERTIES OF NUCLEAR MATTER. Physics International, 4(1), 37-59. https://doi.org/10.3844/pisp.2013.37.59

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Keywords

  • Brueckner-Hartree-Fock Approximation
  • Self-Consistent Greens Function (SCGF) Method
  • Three-Body Forces
  • Symmetry Energy
  • Symmetry Potential
  • Effective Mass and T2-Approximation Method