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dc.contributor.authorBenczik, Sen_US
dc.contributor.authorChang, LNen_US
dc.contributor.authorMinic, Den_US
dc.contributor.authorOkamura, Nen_US
dc.contributor.authorRayyan, Sen_US
dc.contributor.authorTakeuchi, Ten_US
dc.date.accessioned2016-10-18T23:38:45Z
dc.date.available2016-10-18T23:38:45Z
dc.identifier.urihttp://hdl.handle.net/10919/73244
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_US
dc.relation.urihttp://arxiv.org/abs/hep-th/0209119v1en_US
dc.rightsIn Copyright (InC)
dc.rightsThis Item is protected by copyright and/or related rights. You are free to use this Item in any way that is permitted by the copyright and related rights legislation that applies to your use. For other uses you need to obtain permission from the rights-holder(s).
dc.rights.urihttp://rightsstatements.org/vocab/InC/1.0/
dc.subjecthep-then_US
dc.subjecthep-then_US
dc.subjectastro-phen_US
dc.titleClassical Implications of the Minimal Length Uncertainty Relationen_US
dc.typeReport
dc.description.notes12 pages, REVTEX4, 1 eps figureen_US
pubs.organisational-group/Virginia Tech
pubs.organisational-group/Virginia Tech/All T&R Faculty
pubs.organisational-group/Virginia Tech/Science
pubs.organisational-group/Virginia Tech/Science/COS T&R Faculty
pubs.organisational-group/Virginia Tech/Science/Physics


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