Gravitational Waves from Perturbed Black Holes and Relativistic Stars
โ Scribed by Rezzolla L.
- Book ID
- 127397394
- Publisher
- SISSA
- Year
- 2002
- Tongue
- English
- Weight
- 356 KB
- Edition
- lectures
- Category
- Library
No coin nor oath required. For personal study only.
โฆ Synopsis
These lectures aim at providing an introduction to the properties of gravitational waves and in particular to those gravitational waves that are expected as a consequence of perturbations of black holes and neutron stars. Imprinted in the gravitational ra- radiation emitted by these objects is, in fact, a wealth of physical information. In the case of black holes, a detailed knowledge of the gravitational radiation emitted as a response to perturbations will reveal us important details about their mass and spin, but also about the fundamental properties of the event horizon. In the case of neutron stars, on the other hand, this information can provide a detailed map of their internal structure and tell us about the equation of state of matter at very high density, thus filling-in a gap in energies and densities that cannot be investigated by experiments in terrestrial laboratories.
๐ SIMILAR VOLUMES
A comprehensive summary of progress made during the past decade on the theory of black holes and relativistic stars, this collection includes discussion of structure and oscillations of relativistic stars, the use of gravitational radiation detectors, observational evidence for black holes, cosmic c