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SU(2)cmb and the cosmological model: angular power spectra

ABSTRACT. Driven by the CMB temperature-redshift (T-z) relation as demanded by deconfining SU(2) Yang-Mills thermodynamics, an according cosmological model is

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Bibliographic Details
Main Authors: Hahn, Steffen (Author) , Hofmann, Ralf (Author) , Kramer, Daniel (Author)
Format: Article (Journal)
Language:English
Published: [February 2019]
In: Monthly notices of the Royal Astronomical Society
Year: 2018, Volume: 482, Issue: 4, Pages: 4290-4302
ISSN:1365-2966
DOI:10.1093/mnras/sty2981
Online Access:Verlag, Volltext: https://doi.org/10.1093/mnras/sty2981
Verlag, Volltext: https://academic.oup.com/mnras/article/482/4/4290/5159500
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Author Notes:Steffen Hahn, Ralf Hofmann and Daniel Kramer
Description
Summary:ABSTRACT. Driven by the CMB temperature-redshift (T-z) relation as demanded by deconfining SU(2) Yang-Mills thermodynamics, an according cosmological model is
Item Description:cmb ist im Titel tiefgestellt
Published: 03 November 2018
Gesehen am 18.06.2019
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/sty2981

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