1998/12/31 by Frederick W. Kantor
Physics and Astronomy · #astro-ph
published as Frederick W. Kantor, International Journal of Theoretical Physics, Vol. 38, No. 3, pp. 993-996, 1999. · 4 pages; LaTeX2e; in press, International Journal of Theoretical Physics
arxiv created 1999/02/23 · arxiv updated 2009/12/01
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.