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astro-ph.HE2026
Orbital eccentricity can make neutron star g-mode resonances observable with current gravitational-wave detectors
János Takátsy, Lorenz Zwick, Pankaj Saini +1
Dynamical tides can provide us vital information about the properties of neutron star (NS) matter. This is particularly true for g-modes, whose frequency and tidal coupling are hig…
astro-ph.HE2025
Astrophysical constraints on the cold equation of state of the strongly interacting matter
Gábor Kasza, János Takátsy, György Wolf
At present, the only experimental access to the properties of cold, dense strongly interacting matter is provided by astrophysical observations. Neutron stars are the only known sy…
astro-ph.HE2020
Comment on "Tidal Love numbers of neutron and self-bound quark stars"
János Takátsy, Péter Kovács
We comment on the paper of S. Postnikov et al. in Phys. Rev. D 82, 024016 (2010) and give a modified formula that needs to be taken into account when calculating the tidal Love num…