Cosmological Redshift. An Information Mechanics Perspective

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dc.creatorKantor, Frederick W.
dc.date1998-12-24
dc.date1999-02-23
dc.date.accessioned2026-07-07T02:29:49Z
dc.date.available2026-07-07T02:29:49Z
dc.descriptionA 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.
dc.description4 pages; LaTeX2e; in press, International Journal of Theoretical Physics
dc.identifierhttps://arxiv.org/abs/astro-ph/9812444
dc.identifierhttp://arxiv.org/abs/astro-ph/9812444
dc.identifierFrederick W. Kantor, International Journal of Theoretical Physics, Vol. 38, No. 3, pp. 993-996, 1999.
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/13621
dc.subjectAstrophysics
dc.titleCosmological Redshift. An Information Mechanics Perspective
dc.typetext

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