The investigation of strongly interacting systems ranges from matter inside
atomic nuclei to matter under extreme conditions in astrophysics. These systems
require the introduction of nuclear forces and a systematic many-body
approach to solve the strong interaction particles. Understanding the behavior
of infinite nuclear matter provides a path to predict the properties of
neutron stars and gives insights to astrophysical phenomena. Three-nucleon
forces have to be considered when studying nuclear systems, because their
impact is necessary to reproduce properties of nuclei and to correctly obtain
the neutron drip line. Moreover, they are needed to predict the empirical saturation
properties of infinite nuclear matter. The self-consistent Green’s
Function approach paves the way for an improved Ab initio analysis of nuclear
matter, thereby providing the basis for the equation of state of neutron
stars and supernova explosions.
References
[1]
Gad, Kh. (2018) Temperature Effects on the Equation of State and Symmetry Energy at Low and High Densities. Physics of Atomic Nuclei, 81, 429-441.
https://doi.org/10.1134/S1063778818040038
[2]
Hassaneen, K.S. and Mansour, H. (2017) The Thermal Properties of Asymmetric Nuclear Matter within the Extended Brueckner-Hartree-Fock Approach. Journal of the Physical Society of Japan, 86, Article ID: 024201.
https://doi.org/10.7566/JPSJ.86.024201
[3]
Mansour, H. and Hassaneen, K.S. (2014) The Properties of Nuclear Matter at Zero and Finite Temperatures. Physics of Atomic Nuclei, 77, 290-298.
https://doi.org/10.1134/S1063778814020124
[4]
Hassaneen, K.S., Abo-Elsebaa, H.M., Sultan, E.A. and Mansour, H.M.M. (2011) Nuclear Binding Energy and Symmetry Energy of Nuclear Matter with Modern Nucleon-Nucleon Potentials. Annals of Physics, 326, 566-577.
https://doi.org/10.1016/j.aop.2010.11.010
[5]
Mansour, H.M.M., El-Zohry, M. and Elmeshneb, A.E. (2018) A Study of the Three-Body Force Effect on the EOS Properties of Asymmetric Nuclear Matter. Armenian Journal of Physics, 11, 1-10.
