Passage of Time in a Planck Scale Rooted Local Inertial Structure

TL;DR

This paper proposes a refined local inertial structure at the Planck scale, replacing Minkowski spacetime with a higher-dimensional pseudo-Euclidean framework, leading to bounded energies and durations, and predicts measurable deviations from special relativity.

Contribution

It introduces a 4+2n dimensional pseudo-Euclidean structure to address the problem of time in quantum gravity, redefining invariants and predicting testable deviations from special relativity.

Findings

Energies and lengths are bounded by Planck scale values.

Deviations from special relativity are suppressed quadratically by the Planck energy.

Proposes an experiment with gamma-ray pulsars to detect these deviations.

Abstract

It is argued that the `problem of time' in quantum gravity necessitates a refinement of the local inertial structure of the world, demanding a replacement of the usual Minkowski line element by a 4+2n dimensional pseudo-Euclidean line element, with the extra 2n being the number of internal phase space dimensions of the observed system. In the refined structure, the inverse of the Planck time takes over the role of observer-independent conversion factor usually played by the speed of light, which now emerges as an invariant but derivative quantity. In the relativistic theory based on the refined structure, energies and momenta turn out to be invariantly bounded from above, and lengths and durations similarly bounded from below, by their respective Planck scale values. Along the external timelike world-lines, the theory naturally captures the `flow of time' as a genuinely structural attribute of the world. The theory also predicts expected deviations--suppressed quadratically by the Planck energy--from the dispersion relations for free fields in the vacuum. The deviations from the special relativistic Doppler shifts predicted by the theory are also suppressed quadratically by the Planck energy. Nonetheless, in order to estimate the precision required to distinguish the theory from special relativity, an experiment with a binary pulsar emitting TeV range gamma-rays is considered in the context of the predicted deviations from the second-order shifts.