A Dirac Sea of Quantized Superluminal States in the Kerr-Newman Disk

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dc.creatorBock, Robert D.
dc.date2008-06-10
dc.date2008-06-16
dc.date.accessioned2026-07-07T09:44:27Z
dc.date.available2026-07-07T09:44:27Z
dc.descriptionWe model the continuous material component of the Kerr-Newman disk as a discrete distribution of superluminal particles undergoing quantized orbital rotation with velocity $v/c = a/r$. By matching the discrete distribution in the continuous limit with the Kerr disk densities, we derive the quantized energy and momentum states of the superluminal orbits. We conclude that the Kerr-Newman disk may be modeled as a Dirac sea of these superluminal states and we identify possible excited states of the disk.
dc.identifierhttps://arxiv.org/abs/0806.1674
dc.identifierhttp://arxiv.org/abs/0806.1674
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/162878
dc.subjectGeneral Relativity and Quantum Cosmology
dc.subjectHigh Energy Physics - Theory
dc.titleA Dirac Sea of Quantized Superluminal States in the Kerr-Newman Disk
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