Open AccessR-mode constraints from neutron star equation of state
Author(s) -
Ch. C. Moustakidis,
M. C. Papazoglou
Publication year - 2019
Publication title -
hnps advances in nuclear physics
Language(s) - English
Resource type - Journals
eISSN - 2654-0088
pISSN - 2654-007X
DOI - 10.12681/hnps.1913
Subject(s) - neutron star , physics , equation of state , astrophysics , gravitational wave , mode (computer interface) , instability , gravitation , stars , astronomy , mechanics , computer science , quantum mechanics , operating system
The gravitational radiation has been proposed a long time before, as an explana- tion for the observed relatively low spin frequencies of young neutron stars and of accreting neutron stars in low-mass X-ray binaries as well. In the present work we studied the effects of the neutron star equation of state on the r-mode instability window of rotating neutron stars.
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