Orbital eccentricity can make neutron star g-mode resonances observable with current gravitational-wave detectors
János Takátsy🇭🇺 · Lorenz Zwick🇩🇰 · Pankaj Saini🇩🇰 · Johan Samsing🇩🇰
Feb 18, 20262602.15111↳ astro-ph.HEPRD4 citations
Author
Takátsy, János
Affiliationsfrom papers in this corpus
Collaboratorsmost frequent first
Astrophysical constraints on the cold equation of state of the strongly interacting matter
Gábor Kasza🇭🇺 · János Takátsy🇭🇺 · György Wolf🇭🇺
Dec 24, 20252512.19907↳ astro-ph.HE2 citations
Observability of dynamical tides in merging eccentric neutron star binaries
János Takátsy🇭🇺 · Bence Kocsis🇬🇧 · Péter Kovács🇭🇺
Jul 26, 20242407.17560↳ astro-ph.HEPRD8 citations
What neutron stars tell about the hadron-quark phase transition: a Bayesian study
János Takátsy🇭🇺 · Péter Kovács🇭🇺 · György Wolf🇭🇺 · Jürgen Schaffner-Bielich🇩🇪
Mar 2, 20232303.00013↳ astro-ph.HEPRD66 citations
Neutron star properties with careful parameterization in the (axial)vector meson extended linear sigma model
Péter Kovács🇭🇺 · János Takátsy🇭🇺 · Jürgen Schaffner-Bielich🇩🇪 · György Wolf🇭🇺
Nov 12, 20212111.06127nucl-thPRD22 citations
Hybrid star properties from an extended linear sigma model
János Takátsy🇭🇺 · Péter Kovács🇭🇺 · György Wolf🇭🇺
Feb 25, 20212102.12426nucl-thAstron.Nachr.0 citations
Comment on "Tidal Love numbers of neutron and self-bound quark stars"
János Takátsy🇭🇺 · Péter Kovács🇭🇺
Jul 3, 20202007.01139↳ astro-ph.HEPRD49 citations
Compact star properties from an extended linear sigma model
János Takátsy🇭🇺 · Péter Kovács🇭🇺 · Zsolt Szép🇭🇺 · György Wolf🇭🇺
Jul 15, 20191907.05841↳ hep-phUniverse6 citations
Affiliations
own affiliationscollaboratorsvia INSPIRE
Shows only papers in the locally ingested corpus, matched through the INSPIRE author identity. This may not match the author's full publication record.