Electromagnetic Induced Gravitational Perturbations

Simple item page
dc.creatorAdamo, T. M.
dc.creatorNewman, E. T.
dc.date2008-07-23
dc.date.accessioned2026-07-07T12:38:43Z
dc.date.available2026-07-07T12:38:43Z
dc.descriptionWe study the physical consequences of two diffferent but closely related perturbation schemes applied to the Einstein-Maxwell equations. In one case the starting space-time is flat while in the other case it is Schwarzschild. In both cases the perturbation is due to a combined electric and magnetic dipole field. We can see, within the Einstein-Maxwell equations a variety of physical consequences. They range from induced gravitational energy-momentum loss, to a well defined spin angular momentum with its loss and a center-of-mass with its equations of motion.
dc.description17
dc.identifierhttps://arxiv.org/abs/0807.3671
dc.identifierhttp://arxiv.org/abs/0807.3671
dc.identifierClass.Quant.Grav.26:015004,2009
dc.identifierdoi:10.1088/0264-9381/26/1/015004
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/218854
dc.subjectGeneral Relativity and Quantum Cosmology
dc.titleElectromagnetic Induced Gravitational Perturbations
dc.typetext

Files

Collections

arXiv