Neutron Star Core-Crust Transition and Crustal Moment of Inertia: Systematic Implications of Higher-Order Symmetry Energy in the Nuclear Equation of State
W. M. Seif🇪🇬 · A. S. Hashem🇪🇬
Jul 25, 20252507.18384nucl-thPRC4 citations
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Hashem, A.S.
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Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state
W. M. Seif🇪🇬 · A. S. Hashem🇪🇬
Jul 16, 20252507.11379nucl-thAnnals Phys.1 citation
Constraints on the nuclear symmetry energy and its density slope from the {\alpha} decay process
Apr 13, 20181804.04336nucl-thCPC16 citations
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