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A model of light from ancient blue emissions
Anabol Labs.
Hacettepe University, Ankara.
Luleå University of Technology, Department of Engineering Sciences and Mathematics, Material Science.
2006 (English)In: International journal of theoretical physics, ISSN 0020-7748, E-ISSN 1572-9575, Vol. 45, no 5, p. 908-923Article in journal (Refereed) Published
Abstract [en]

A model is presented to explain the luminar distances and associated red-shifts from ancient supernovae. Light frequencies of supernovae type Ia (SNe Ia) vary smoothly with time, decreasing from singularity to present and intergalactic luminar distances are described as linear combinations of Hubble expansion and smaller components from the time-dependent decrease of emission frequencies. When tested with current cosmic matter densities, SNe Ia distances, red-shifts and the Hubble constant the errors between this model and the vacuum energy model favor this new model, though our model suffers from mathematics about zero. An expression between energy and frequency, derived from the model, reducing to the Planck equation for short observation intervals is also discovered and estimated to within 10% using current SNe Ia data. We also propose a relationship for the deceleration of frequency over time, solve at infinity and discover frequency and time will eventually become uncoupled.

Place, publisher, year, edition, pages
2006. Vol. 45, no 5, p. 908-923
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Fysik
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URN: urn:nbn:se:ltu:diva-3245DOI: 10.1007/s10773-006-9083-6ISI: 000238832600007Scopus ID: 2-s2.0-33745746659Local ID: 10cc0d10-f1be-11db-bb1b-000ea68e967bOAI: oai:DiVA.org:ltu-3245DiVA, id: diva2:976101
Note
Validerad; 2006; 20070423 (ysko)Available from: 2016-09-29 Created: 2016-09-29 Last updated: 2018-07-10Bibliographically approved

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Paul, Jan

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