Special Theory of Relativity in Curved Space Time

dc.creatorModgil, Moninder Singh
dc.date2004-12-12
dc.date.accessioned2026-07-07T05:53:40Z
dc.date.available2026-07-07T05:53:40Z
dc.descriptionSpace-time measurements, of gedanken experiments of special relativity need modification in curved spaces-times. It is found that in a space-time with metric $g$, the special relativistic factor $γ$, has to be replaced by $γ_g=1/\sqrt{g_{μν} V^μV^ν}$, where $V_μ=(1,v,0,0)$, is the 4-velocity, and $v$ the relative velocity between the two frames Examples are given for Schwarzschild metric, Friedmann-Robertson-Walker metric, and the Gödel metric. Among the novelties are paradoxical tachyonic states, with $γ_g$ becoming imaginary, for velocities less than that of light, due to space-time curvature. Relativistic mass becomes a function of space-time curvature, $m=\sqrt{g_{μν}P^μP^ν}$, where $P_μ=(E,p)$ is the 4-momentum, signaling a new form of Mach's principle, in which a global object - namely the metric tensor, is effecting interia.
dc.description13 pages
dc.identifierhttps://arxiv.org/abs/physics/0412068
dc.identifierhttp://arxiv.org/abs/physics/0412068
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/86725
dc.subjectGeneral Physics
dc.titleSpecial Theory of Relativity in Curved Space Time
dc.typetext

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