English

From time to timescape - Einstein's unfinished revolution

General Relativity and Quantum Cosmology 2010-04-21 v1 Cosmology and Nongalactic Astrophysics

Abstract

I argue that Einstein overlooked an important aspect of the relativity of time in never quite realizing his quest to embody Mach's principle in his theory of gravity. As a step towards that goal, I broaden the Strong Equivalence Principle to a new principle of physics, the Cosmological Equivalence Principle, to account for the role of the evolving average regional density of the universe in the synchronisation of clocks and the relative calibration of inertial frames. In a universe dominated by voids of the size observed in large-scale structure surveys, the density contrasts of expanding regions are strong enough that a relative deceleration of the background between voids and the environment of galaxies, typically of order 10^{-10} m/s^2, must be accounted for. As a result one finds a universe whose present age varies by billions of years according to the position of the observer: a timescape. This model universe is observationally viable: it passes three critical independent tests, and makes additional predictions. Dark energy is revealed as a mis-identification of gravitational energy gradients and the resulting variance in clock rates. Understanding the biggest mystery in cosmology therefore involves a paradigm shift, but in an unexpected direction: the conceptual understanding of time and energy in Einstein's own theory is incomplete.

Keywords

Cite

@article{arxiv.0912.4563,
  title  = {From time to timescape - Einstein's unfinished revolution},
  author = {David L. Wiltshire},
  journal= {arXiv preprint arXiv:0912.4563},
  year   = {2010}
}

Comments

13 pages, 3 figures; A runner-up in the 2008 FQXi Essay Contest on the Nature of Time; Int. J. Mod. Phys. D 18, in press

R2 v1 2026-06-21T14:27:36.456Z