Classical Implications of the Minimal Length Uncertainty Relation
dc.contributor.author | Benczik, S. Z. | en |
dc.contributor.author | Chang, Lay Nam | en |
dc.contributor.author | Minic, Djordje | en |
dc.contributor.author | Okamura, Naotoshi | en |
dc.contributor.author | Rayyan, S. | en |
dc.contributor.author | Takeuchi, Tatsu | en |
dc.contributor.department | Institute for Particle, Nuclear and Astronomical Sciences (IPNAS) | en |
dc.date.accessioned | 2016-10-18T23:38:45Z | en |
dc.date.available | 2016-10-18T23:38:45Z | en |
dc.date.issued | 2002-09-12 | en |
dc.description.abstract | We 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.notes | 12 pages, REVTEX4, 1 eps figure | en |
dc.identifier.uri | http://hdl.handle.net/10919/73244 | en |
dc.relation.uri | http://arxiv.org/abs/hep-th/0209119v1 | en |
dc.rights | In Copyright | en |
dc.rights.uri | http://rightsstatements.org/vocab/InC/1.0/ | en |
dc.subject | hep-th | en |
dc.subject | astro-ph | en |
dc.title | Classical Implications of the Minimal Length Uncertainty Relation | en |
dc.type | Report | en |
pubs.organisational-group | /Virginia Tech | en |
pubs.organisational-group | /Virginia Tech/All T&R Faculty | en |
pubs.organisational-group | /Virginia Tech/Science | en |
pubs.organisational-group | /Virginia Tech/Science/COS T&R Faculty | en |
pubs.organisational-group | /Virginia Tech/Science/Physics | en |