Tanja Hinderer

Constraining neutron-star tidal Love numbers with gravitational-wave detectors

Ground-based gravitational wave detectors may be able to constrain the nuclear equation of state using the early, low frequency portion of the signal of detected neutron star--neutron star inspirals. In this early adiabatic regime, the influence of a neutron stars internal structure on the phase of the waveform depends only on a single parameter

Tidal deformability of neutron stars with realistic equations of state and their gravitational wave signatures in binary inspiral

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Effective-one-body model for black-hole binaries with generic mass ratios and spins

of the star related to its tidal Love number, namely, the ratio of the induced quadrupole moment to the perturbing tidal gravitational field. We analyze the information obtainable from gravitational wave frequencies smaller than a cutoff frequency of 400 Hz, where corrections to the internal-structure signal are less than 10%. For an inspiral of two nonspinning

Tidal Love numbers of neutron stars

1.4{M}_{\ensuremath{\bigodot}}

Cross section, final spin and zoom-whirl behavior in high-energy black hole collisions

neutron stars at a distance of 50 Megaparsecs, LIGO II detectors will be able to constrain

Spin effects on gravitational waves from inspiraling compact binaries at second post-Newtonian order

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Semianalytical estimates of scattering thresholds and gravitational radiation in ultrarelativistic black hole encounters

to

Dynamical Tides in General Relativity: Effective Action and Effective-One-Body Hamiltonian

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Periastron advance in spinning black hole binaries: comparing effective-one-body and Numerical Relativity

with 90% confidence. Fully relativistic stellar models show that the corresponding constraint on radius

Distinguishing Boson Stars from Black Holes and Neutron Stars from Tidal Interactions in Inspiraling Binary Systems

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