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Journal ArticleDOI

Solutions of Two Problems in the Theory of Gravitational Radiation

Subrahmanyan Chandrasekhar
- 16 Mar 1970 - 
- Vol. 24, Iss: 11, pp 611-615
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TLDR
In this paper, the authors considered the evolution of an elongated rotating configuration by gravitational radiation and the possibility of a secular instability being induced by it, in the context of the classical homogeneous figures of Maclaurin and Jacobi.
Abstract
The evolution of an elongated rotating configuration by gravitational radiation and the possibility of a secular instability being induced by it are considered in the context of the classical homogeneous figures of Maclaurin and Jacobi. The triaxial Jacobian ellipsoid evolves in the direction of increasing angular velocity and approaches (exponentially) the point of bifurcation where it ceases to radiate. Further, radiation reaction does not make the Maclaurin spheroid secularly unstable past the point of bifurcation.

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Journal ArticleDOI

Quasi-normal modes of stars and Black holes

TL;DR: The successes, as well as the limits, of perturbation theory are presented, and its role in the emerging era of numerical relativity and supercomputers is discussed.
Journal ArticleDOI

Testing general relativity with present and future astrophysical observations

Emanuele Berti, +64 more
TL;DR: In this article, a catalog of modified theories of gravity for which strong-field predictions have been computed and contrasted to Einstein's theory is presented, and the current understanding of the structure and dynamics of compact objects in these theories is summarized.
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Gravitational wave experiments and early universe cosmology

TL;DR: In this paper, a pedagogical derivation of the various relations that characterize the response of a detector to a stochastic background is given, and the sensitivities of the large interferometers under constructions (LIGO, VIRGO, GEO600, TAMA300, AIGO) or planned (Avdanced LIGO and presently operating resonant bars).
Journal ArticleDOI

Quasinormal modes: the characteristic `sound' of black holes and neutron stars

TL;DR: In this paper, the authors summarize how quasinormal modes are defined and computed, see why they have been regarded as closely analogous to normal modes, and discover why they are actually quite different.
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