Curved Spacetime Dirac Equation Revisited

dc.contributor.authorNyambuya, G. G.
dc.date.accessioned2026-04-07T12:48:46Z
dc.date.issued2025
dc.description.abstractWe revisit the Curved Spacetime (CST) Dirac equation that we presented earlier and our motive for this is to proffer a new alternative and elegant derivation of this equation. Having done this, we re-examine the resulting energy-momentum dispersion relation. It is seen that this energy-momentum dispersion relation is capable of describing massive braydons, luxons and tachyons. It is seen that how a particle turnouts to either be a braydon (k= 0), luxon (k=− 1) or a tachyon (k=+ 1) depends on the curvature (k= 0,±1) associated with the particle in question. The derived refractive index, nr, of a non-vacuo material medium predicts time-delays in the arrival times of cosmological photons of different frequencies emanating simultaneously from the same region of space as is the case with time-delays observed in radio photons emanating from GRB events. In its functional form, the derived formula for, nr, qualitatively fits the time-delays observed in GRBs and allows for the determination of the photon mass.
dc.identifier.citationNyambuya, G.G., (2025). Curved Spacetime Dirac Equation Revisited. Springer Nature
dc.identifier.urihttp://ir.nust.ac.zw:4000/handle/123456789/43
dc.language.isoen
dc.publisherSpringer Nature
dc.subjectcurvature
dc.subjectDirac equation
dc.subjecttime delay: gamma-ray bursts
dc.subjectmassive photon
dc.subjectspacetime
dc.titleCurved Spacetime Dirac Equation Revisited
dc.typeArticle

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