Electromagnetic perturbations of non-vacuum locally rotationally symmetric class II spacetimes

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dc.creatorBurston, Raymond
dc.creatorLun, Anthony
dc.date2006-10-12
dc.date.accessioned2026-07-07T07:27:59Z
dc.date.available2026-07-07T07:27:59Z
dc.descriptionWe present a method that yields three decoupled covariant equations for three complex scalars, which completely govern electromagnetic perturbations of non-vacuum, locally rotationally symmetric class II spacetimes. One of these equations is equivalent to the previously established generalized Regge-Wheeler equation for electromagnetic fields. The remaining two equations are a direct generalization of the Bardeen-Press equations. The approach undertaken makes use of the well established 3+1 (and 2+1+1) formalism, and therefore, it is an ideal setting for specifying interpretable energy-momentum on an initial spacelike three-slice as the perturbation sources to the resultant electromagnetic radiation.
dc.description15 pages, submitted to Classical and Quantum Gravity
dc.identifierhttps://arxiv.org/abs/gr-qc/0610062
dc.identifierhttp://arxiv.org/abs/gr-qc/0610062
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/117574
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleElectromagnetic perturbations of non-vacuum locally rotationally symmetric class II spacetimes
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