Apparent Hubble acceleration from large-scale electroweak domain structure

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dc.creatorAnderberg, Tommy
dc.date2005-11-22
dc.date2008-11-26
dc.date.accessioned2026-07-07T11:34:01Z
dc.date.available2026-07-07T11:34:01Z
dc.descriptionThe observed luminosity deficit of Type Ia supernovae (SNe Ia) at high redshift z can be explained by partial conversion to weak vector bosons of photons crossing large-scale electroweak domain boundaries, making Hubble acceleration only apparent and eliminating the need for a cosmological constant > 0.
dc.description15 pages, 7 figures. Adopted conventions of arxiv:0804.2284, simplified computation of luminosity distributions, added footnotes
dc.identifierhttps://arxiv.org/abs/astro-ph/0511647
dc.identifierhttp://arxiv.org/abs/astro-ph/0511647
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/198099
dc.subjectAstrophysics
dc.subjectHigh Energy Physics - Phenomenology
dc.titleApparent Hubble acceleration from large-scale electroweak domain structure
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