Cosmological Redshift. An Information Mechanics Perspective
arXiv:astro-ph/9812444
Abstract
A photon's observed wavelength tells an astronomical detector about the amount of position information obtained by observing that photon. This amount of position information may depend on time in a way which, to first order over distances small compared to the size of the universe, might account for the cosmological redshift.
4 pages; LaTeX2e; in press, International Journal of Theoretical Physics