1. Home page
  2. Search

Nuclear equation of state effects on the r-mode instability of neutron stars

This item is provided by the institution :
Hellenic Nuclear Physics Society   

Repository :
Annual Symposium of the Hellenic Nuclear Physics Society  | ΕΚΤ eProceedings   

see the original item page
in the repository's web site and access all digital files if the item*



Nuclear equation of state effects on the r-mode instability of neutron stars (EN)
Moustakidis, Ch. C.
info:eu-repo/semantics/article
info:eu-repo/semantics/publishedVersion
2012-12-01
We study the effect of nuclear equation of state on the r-mode instability of a rotating neutron star. We consider the case where the crust of the neutron star is perfectly rigid and we employ the related theory. The effects of the density dependence of the nuclear symmetry energy on r-mode instability properties are presented and analyzed. A comparison of theoretical predictions with observed neutron stars in low-mass X-ray binaries is also performed and analyzed. (EN)
Nuclear symmetry energy (EN)
Neutron stars (EN)
Gravitational waves (EN)
Nuclear equation of state (EN)
r-mode instability (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. 20 (2012): HNPS2012; 27-34 (EL)
HNPS Advances in Nuclear Physics; Vol. 20 (2012): HNPS2012; 27-34 (EN)
Πνευματική ιδιοκτησία (c) 2019 Ch. C. Moustakidis (EL)
Hellenic Nuclear Physics Society
Annual Symposium of the Hellenic Nuclear Physics Society
Oral contributions



*Institutions are responsible for keeping their URLs functional (digital file, item page in repository site)