Classical Implications of the Minimal Length Uncertainty Relation

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.

12 pages, REVTEX4, 1 eps figure

References in corpus (1)

• The Effect of the Minimal Length Uncertainty Relation on the Density of States and the Cosmological Constant Problem

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