Geodesics, Mass and the Uncertainty Principle in a Warped de Sitter Space-time
Jose A. Magpantay

TL;DR
This paper solves geodesic equations in a warped de Sitter space-time, revealing how extra dimensions influence particle mass and the uncertainty principle, with implications for forces constraining particles on the brane.
Contribution
It provides explicit solutions to geodesic equations in a Randall-Sundrum warped de Sitter space and analyzes the resulting time-dependent effects on particle mass and quantum uncertainty.
Findings
Particle moves in the bulk, not restricted to the 3-brane.
Time-dependent mass and uncertainty principle emerge from extra-dimensional effects.
Classical corrections can be removed, but quantum corrections restore the effects.
Abstract
We present the explicit solution to the geodesic equations in a warped de Sitter space-time proposed by Randall-Sundrum. We find that a test particle moves in the bulk and is not restricted on a 3-brane (to be taken as our universe). On the 3-brane, the test particle moves with uniform velocity, giving the appearance that it is not subject to a force. But computing the particle's energy using the energy-momentum tensor yields a time-dependent energy that suggests a time-dependent mass. Thus, the extra force, which is the effect of the warped extra dimension on the particle's motion on the 3-brane, does not change the velocity but the mass of the particle. The particle's motion in the bulk also results in a time-dependent modification of the Heisenberg uncertainty principle as viewed on the 3-brane. These two results show that the classical physics along the extra dimension results in…
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Noncommutative and Quantum Gravity Theories · Cosmology and Gravitation Theories
