Classical Implications of the Minimal Length Uncertainty Relation

dc.contributor.authorBenczik, S. Z.en
dc.contributor.authorChang, Lay Namen
dc.contributor.authorMinic, Djordjeen
dc.contributor.authorOkamura, Naotoshien
dc.contributor.authorRayyan, S.en
dc.contributor.authorTakeuchi, Tatsuen
dc.contributor.departmentInstitute for Particle, Nuclear and Astronomical Sciences (IPNAS)en
dc.date.accessioned2016-10-18T23:38:45Zen
dc.date.available2016-10-18T23:38:45Zen
dc.date.issued2002-09-12en
dc.description.abstractWe 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.en
dc.description.notes12 pages, REVTEX4, 1 eps figureen
dc.identifier.urihttp://hdl.handle.net/10919/73244en
dc.relation.urihttp://arxiv.org/abs/hep-th/0209119v1en
dc.rightsIn Copyrighten
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/en
dc.subjecthep-then
dc.subjectastro-phen
dc.titleClassical Implications of the Minimal Length Uncertainty Relationen
dc.typeReporten
pubs.organisational-group/Virginia Techen
pubs.organisational-group/Virginia Tech/All T&R Facultyen
pubs.organisational-group/Virginia Tech/Scienceen
pubs.organisational-group/Virginia Tech/Science/COS T&R Facultyen
pubs.organisational-group/Virginia Tech/Science/Physicsen

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