Newton's Equation on the kappa space-time and the Kepler problem
arXiv:1003.4603 · doi:10.1142/S021773231003416X
Abstract
We study the modification of Newton's second law, upto first order in the deformation parameter , in the -space-time. We derive the deformed Hamiltonian, expressed in terms of the commutative phase space variables, describing the particle moving in a central potential in the -space-time. Using this, we find the modified equations of motion and show that there is an additional force along the radial direction. Using Pioneer anomaly data, we set a bond as well as fix the sign of . We also analyse the violation of equivalence principle predicted by the modified Newton's equation, valid up to first order in and use this also to set an upper bound on .
8 pages, Minor changes in subsection III A made for clarity, to appear in Mod. Phys. Lett. A
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