Classical Implications of the Minimal Length Uncertainty Relation

Simple item page
dc.creatorBenczik, Sandor
dc.creatorChang, Lay Nam
dc.creatorMinic, Djordje
dc.creatorOkamura, Naotoshi
dc.creatorRayyan, Saifuddin
dc.creatorTakeuchi, Tatsu
dc.date2002-09-14
dc.date.accessioned2026-07-07T04:14:08Z
dc.date.available2026-07-07T04:14:08Z
dc.descriptionWe study the phenomenological implications of the classical limit of the "stringy" commutation relations [x_i,p_j]=i hbar[(1+beta p^2) delta_{ij} + beta' p_i p_j]. In particular, we investigate the "deformation" of Kepler's third law and apply our result to the rotation curves of gas and stars in spiral galaxies.
dc.description12 pages, REVTEX4, 1 eps figure
dc.identifierhttps://arxiv.org/abs/hep-th/0209119
dc.identifierhttp://arxiv.org/abs/hep-th/0209119
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/51508
dc.subjectHigh Energy Physics - Theory
dc.subjectAstrophysics
dc.titleClassical Implications of the Minimal Length Uncertainty Relation
dc.typetext

Files

Collections

arXiv