Planckian Scatterings of Massive Particles and Gravitational Shock Waves

dc.creatorHAYASHI, Koichi
dc.creatorSAMURA, Toshiharu
dc.date1994-05-03
dc.date.accessioned2026-07-07T04:20:11Z
dc.date.available2026-07-07T04:20:11Z
dc.descriptionThe scattering process of two particles at Planck energies or beyond is calculated using the gravitational shock wave metric for a massive black hole. Then, the scattering between a heavy mass particle and a small mass one is deal with. The cross section contains an extra new term of $σ\propto G^3$ as the correction term of the leading term derived by 't Hooft. The ultrarelativistic limit of the Lorentz boosted Reissner--Norstrom black hole is also calculated.
dc.description10 Pages, KOBE--FHD--93--05, LaTeX
dc.identifierhttps://arxiv.org/abs/hep-th/9405013
dc.identifierhttp://arxiv.org/abs/hep-th/9405013
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/53862
dc.subjectHigh Energy Physics - Theory
dc.titlePlanckian Scatterings of Massive Particles and Gravitational Shock Waves
dc.typetext

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