57 citations · 102 across the 6 of their papers we have counts for
7 papers
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…
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…
What neutron stars tell about the hadron-quark phase transition: a Bayesian study
János Takátsy, Péter Kovács, György Wolf +1
The existence of quark matter inside the heaviest neutron stars has been the topic of numerous recent studies, many of them suggesting that a phase transition to strongly interacti…
Hybrid star properties from an extended linear sigma model
János Takátsy, Péter Kovács, György Wolf
The equation of state provided by effective models of strongly interacting matter should comply with the restrictions imposed by current astrophysical observations on compact stars…
Hybrid star construction with the extended linear sigma model: preliminary results
Péter Kovács, János Takátsy
The interior of compact stars is usually divided into two major parts, the outer part called crust and the inner part called core. There are several possibilities for the compositi…
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…