5 papers
Macroscopic approaches to rotating neutron stars
A. A. Uleiev, A. G. Magner, S. P. Maydanyuk +6
The macroscopic model for a neutron star (NS) as a perfect liquid drop at equilibrium is extended to rotating systems with a small frequency within the effective-surface (ES)…
Rotating neutron stars within the macroscopic effective-surface approximation
A. G. Magner, S. P. Maydanyuk, A. Bonasera +6
The macroscopic model for a neutron star (NS) as a finite perfect fluid at the equilibrium is extended to rotating systems by incorporating the linear perturbation expansion over a…
On the High Excitation 7 De-exciting States in Si
J. B. Natowitz, X. G. Cao, A. Bonasera +1
A direct comparison and analysis of published spectra for the 7 disassembly of Si projectiles excited in collisions with C at 35 MeV/u reveals significant agreeme…
Leptodermic corrections to the TOV equations and nuclear astrophysics within the effective surface approximation
A. G. Magner, S. P. Maydanyuk, A. Bonasera +4
The macroscopic model for a neutron star (NS) as a liquid drop at the equilibrium is used to extend the Tolman-Oppenheimer-Volkoff (TOV) equations taking into account the gradient…
Neutron stars as a dense liquid drop at equilibrium within the effective surface approximation
A. G. Magner, S. P. Maydanyuk, A. Bonasera +4
The macroscopic model is formulated for a neutron star (NS) as a perfect liquid drop at the equilibrium. We use the leptodermic approximation , where is the crust thi…