95 citations · 131 across the 4 of their papers we have counts for
8 papers
Neutron Stars and Gravitational Waves: the Key Role of Nuclear Equation of State
P. S. Koliogiannis, A. Kanakis-Pegios, Ch. C. Moustakidis
Neutron stars are the densest known objects in the universe and an ideal laboratory for the strange physics of super-condensed matter. Theoretical studies in connection with recent…
Thermal effects on tidal deformability of a coalescing binary neutron star system
A. Kanakis-Pegios, P. S. Koliogiannis, Ch. C. Moustakidis
The study of neutron star mergers by the detection of the emitted gravitational waves is one of the most promised tools to study the properties of dense nuclear matter at high dens…
Speed of sound constraints from tidal deformability of neutron stars
A. Kanakis-Pegios, P. S. Koliogiannis, Ch. C. Moustakidis
The upper bound of the speed of sound in dense nuclear matter is one of the most interesting but still unsolved problems in Nuclear Physics. Theoretical studies in connection with…
Speed of sound constraints on maximally rotating neutron stars
Ch. Margaritis, P. S. Koliogiannis, Ch. C. Moustakidis
The observation of maximally rotating neutron stars (in comparison to nonrotating ones) may provide more information on the behavior of nuclear matter at high densities. We provide…
Effects of the equation of state on the bulk properties of maximally-rotating neutron stars
P. S. Koliogiannis, Ch. C. Moustakidis
Neutron stars are among the densest known objects in the universe and an ideal laboratory for the strange physics of super-condensed matter. While the simultaneously measurements o…
Constraints on the equation of state from the stability condition of neutron stars
P. S. Koliogiannis, Ch. C. Moustakidis
The stellar equilibrium and collapse, including mainly white dwarfs, neutron stars and supper massive stars, is an interplay between general relativistic effects and the equation o…