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19952026
most citedQuasi-Normal Modes of Stars and Black Holes

2.1k citations · 15.5k across the 182 of their papers we have counts for

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Showing 1999Show all

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gr-qc1999★ 2.1k cited

Quasi-Normal Modes of Stars and Black Holes

Kostas D. Kokkotas, Bernd G. Schmidt

Perturbations of stars and black holes have been one of the main topics of relativistic astrophysics for the last few decades. They are of particular importance today, because of t…

gr-qc1999★ 118 cited

Nonlinear hydrodynamical evolution of rotating relativistic stars: Numerical methods and code tests

Jose A. Font, Nikolaos Stergioulas, Kostas D. Kokkotas

We present numerical hydrodynamical evolutions of rapidly rotating relativistic stars, using an axisymmetric, nonlinear relativistic hydrodynamics code. We use four different high-…

gr-qc1999★ 13 cited

Construction of Astrophysical Initial Data for Perturbations of Relativistic Stars

Nils Andersson, Kostas D. Kokkotas, Pablo Laguna +2

We develop a framework for constructing initial data sets for perturbations about spherically symmetric matter distributions. This framework facilitates setting initial data repres…

gr-qc1999★ 19 cited

The close-limit approximation to Neutron Star Collisions

G. D. Allen, N. Andersson, K. D. Kokkotas +3

We develop a close-limit approximation to the head-on collision of two neutron stars similar to that used to treat the merger of black hole binaries . This approximation can serve…

gr-qc1999★ 48 cited

On the r-mode spectrum of relativistic stars

H. R. Beyer, K. D. Kokkotas

We present a mathematically rigorous proof that the r-mode spectrum of relativistic stars to the rotational lowest order has a continuous part. A rigorous definition of this spectr…

gr-qc1999★ 212 cited

The inverse problem for pulsating neutron stars: A ``fingerprint analysis'' for the supranuclear equation of state

K. D. Kokkotas, T. A. Apostolatos, N. Andersson

We study the problem of detecting, and infering astrophysical information from, gravitational waves from a pulsating neutron star. We show that the fluid f and p-modes, as well as…