Ahmed Hashem

Associate professor

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Microscopic calculations for fusion reactions involving stable and neutron-rich isotopes of C, O, Ne, Mg, and Si in the neutron star crust

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Citation:
M. Rashdan, R. Hussein, S. W. M., and A. S. Hashem, "Microscopic calculations for fusion reactions involving stable and neutron-rich isotopes of C, O, Ne, Mg, and Si in the neutron star crust", Physical Review C, vol. 112, no. 3: American Physical Society (APS), pp. 035803, 2025.
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Recent Publications

Tidal deformability and compactness of neutron stars and massive pulsars from semi-microscopic equations of state
Neutron star core-crust transition and crustal moment of inertia: Systematic investigation of implications of higher-order symmetry energy in the nuclear equation of state
Microscopic calculations for fusion reactions involving stable and neutron-rich isotopes of C, O, Ne, Mg, and Si in the neutron star crust
Density curvature, skewness, and kurtosis of the nuclear symmetry energy and their impact on the compactness and tidal deformability of neutron stars
Impact of the stiffness of equation of state on saturation properties of asymmetric nuclear matter and Urca cooling in neutron stars
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