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arxiv: 0807.3671 · v1 · submitted 2008-07-23 · 🌀 gr-qc

Electromagnetic Induced Gravitational Perturbations

classification 🌀 gr-qc
keywords equationscaseconsequenceseinstein-maxwellgravitationalinducedlossperturbation
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We 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.

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