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Nuclear equation of state constraints from tidal deformability of neutron stars

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Hellenic Nuclear Physics Society   

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Nuclear equation of state constraints from tidal deformability of neutron stars (EN)
Moustakidis, Ch. C.
info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
2019-03-08
We study the effect of nuclear equation of state on the tidal polarizability of neutron stars. The predicted equations of state for the β-stable nuclear matter are parameterized by varying the slope L of the symmetry energy at saturation density on the interval 65 MeV≤L≤115 MeV. The effects of the density dependence of the nuclear symmetry energy on the neutron star tidal polarizability are presented and analyzed. A comparison of theoretical predictions with the recent observation predictions is also performed and analyzed. (EN)
Annual Symposium of the Hellenic Nuclear Physics Society
English
Hellenic Nuclear Physics Society (HNPS) (EN)
2654-0088
2654-007X
Annual Symposium of the Hellenic Nuclear Physics Society; Τόμ. 21 (2013): HNPS2013; 44-49 (EL)
HNPS Advances in Nuclear Physics; Vol. 21 (2013): HNPS2013; 44-49 (EN)
Πνευματική ιδιοκτησία (c) 2019 Ch. C. Moustakidis (EL)
Hellenic Nuclear Physics Society
Annual Symposium of the Hellenic Nuclear Physics Society
Oral contributions



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