Schwarzschild black holes and propagation of electromagnetic and gravitational waves

Simple item page
dc.creatorKarkowski, Janusz
dc.creatorMalec, Edward
dc.creatorSwierczynski, Zdobyslaw
dc.date2002-04-29
dc.date.accessioned2026-07-07T03:26:49Z
dc.date.available2026-07-07T03:26:49Z
dc.descriptionDisturbing of a spacetime geometry may result in the appearance of an oscillating and damped radiation - the so-called quasinormal modes. Their periods of oscillations and damping coefficients carry unique information about the mass and the angular momentum, that would allow one to identify the source of the gravitational field. In this talk we present recent bounds on the diffused energy, applicable to the Schwarzschild spacetime, that give also rough estimates of the energy of excited quasinormal modes.
dc.description3 figures eps
dc.identifierhttps://arxiv.org/abs/gr-qc/0204086
dc.identifierhttp://arxiv.org/abs/gr-qc/0204086
dc.identifierActa Phys.Polon. B32 (2001) 3593-3603
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/34197
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleSchwarzschild black holes and propagation of electromagnetic and gravitational waves
dc.typetext

Files

Collections

arXiv