Quasi-normal modes of stars and black holes
KD Kokkotas, BG Schmidt - Living Reviews in Relativity, 1999 - Springer
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 …
astrophysics for the last few decades. They are of particular importance today, because of …
Rotating stars in relativity
N Stergioulas - Living Reviews in Relativity, 2003 - Springer
Rotating relativistic stars have been studied extensively in recent years, both theoretically
and observationally, because of the information they might yield about the equation of state …
and observationally, because of the information they might yield about the equation of state …
Effective potential for even-parity Regge-Wheeler gravitational perturbation equations
FJ Zerilli - Physical Review Letters, 1970 - APS
Effective Potential for Even-Parity Regge-Wheeler Gravitational Perturbation Equations Page 1
VOLUME 24, NUMBER 13 PHYSICAL REVIEW I ETTERS $0 MARcH 1970 EFFECTIVE …
VOLUME 24, NUMBER 13 PHYSICAL REVIEW I ETTERS $0 MARcH 1970 EFFECTIVE …
Gravitational field of a particle falling in a Schwarzschild geometry analyzed in tensor harmonics
FJ Zerilli - Physical Review D, 1970 - APS
We are concerned with the pulse of gravitational radiation given off when a star falls into a"
black hole" near the center of our galaxy. We look at the problem of a small particle falling in …
black hole" near the center of our galaxy. We look at the problem of a small particle falling in …
General relativistic collapse to black holes and gravitational waves from black holes
T Nakamura, K Oohara, Y Kojima - Progress of Theoretical …, 1987 - academic.oup.com
One of the important problems in general relativity is to clarify the dynamical nature of space-
times. In this article two aspects of dynamical space-times are treated. In Part I general …
times. In this article two aspects of dynamical space-times are treated. In Part I general …
Rotating stars in relativity
V Paschalidis, N Stergioulas - Living Reviews in Relativity, 2017 - Springer
Rotating relativistic stars have been studied extensively in recent years, both theoretically
and observationally, because of the information they might yield about the equation of state …
and observationally, because of the information they might yield about the equation of state …
The gravitational-wave signature of core-collapse supernovae
CD Ott - Classical and Quantum Gravity, 2009 - iopscience.iop.org
We review the ensemble of anticipated gravitational-wave (GW) emission processes in
stellar core collapse and postbounce core-collapse supernova evolution. We discuss recent …
stellar core collapse and postbounce core-collapse supernova evolution. We discuss recent …
Perturbation analysis for gravitational and electromagnetic radiation in a Reissner-Nordström geometry
FJ Zerilli - Physical Review D, 1974 - APS
We consider the gravitational and electromagnetic fields produced by a charged (or
uncharged) test particle moving in a Reissner-Nordström geometry as perturbations on the …
uncharged) test particle moving in a Reissner-Nordström geometry as perturbations on the …
The quadrupole oscillations of neutron stars
L Lindblom, SL Detweiler - … Series (ISSN 0067-0049), vol. 53 …, 1983 - adsabs.harvard.edu
The influence of the equation of state of matter (in the nuclear density regime) on the
dynamical behavior of neutron stars is investigated. The properties of the quadrupole (f …
dynamical behavior of neutron stars is investigated. The properties of the quadrupole (f …
[PDF][PDF] A new class of g-modes in neutron stars
A Reisenegger, P Goldreich - Astrophysical Journal, 1992 - authors.library.caltech.edu
Because a neutron star is born hot, its internal composition is close to chemical equilibrium.
In the fluid core, this implies that the ratio of the number densities of charged particles …
In the fluid core, this implies that the ratio of the number densities of charged particles …