95 citations · 581 across the 27 of their papers we have counts for
9 papers · 1 filter
Hybrid Stars with a Crossover Equation of State
G. A. Tsalis, Ch. C. Moustakidis
The possible occurrence of a phase transition in superdense nuclear matter remains an open problem in nuclear physics. In particular, the transition from purely hadronic matter to…
Hadron-quark phase transitions along proto-neutron-star evolution
P. Laskos-Patkos, P. S. Koliogiannis, Ch. C. Moustakidis
The new era of multi-messenger astronomy requires the accurate and self-consistent derivation of the nuclear equation of state at high temperature. In the present work, we focused…
Constraints on the isovector properties of finite nuclei from neutron stars observations
M. Divaris, A. Kanakis-Pegios, Ch. C. Moustakidis
The nuclear symmetry energy plays important role on the structure of finite nuclei as well as on the bulk properties of neutron stars. However, its values at high densities are com…
Signatures of quark deconfinement through the r-modes of twin stars
P. Laskos-Patkos, Ch. C. Moustakidis
The observation and distinction of two compact stars with an identical mass but a different radius would be a clear sign of hadron-quark phase transition in nuclear matter. Motivat…
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…
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…