R-mode constraints from neutron star equation of state

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Δημοσιευμένα: Mar 8, 2019
DOI: https://doi.org/10.12681/hnps.1913
Ch. C. Moustakidis
Department of Physics, Aristotle University of Thessaloniki
M. C. Papazoglou
Department of Physics, Aristotle University of Thessaloniki
Περίληψη

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.

Λεπτομέρειες άρθρου
  • Ενότητα
  • Oral contributions
Αναφορές
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