Classical Implications of the Minimal Length Uncertainty Relation

Details Classical Implications of the Minimal Length Uncertainty Relation Classical Implications of the Minimal Length Uncertainty Relation

2002-09-14

arxiv.org/abs/hep-th/0209119v1

Physics

High Energy Physics

High Energy Physics - Theory

12 pages, REVTEX4, 1 eps figure

Scientific paper

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.

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