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
Gespeichert in:
| Hauptverfasser: | , , |
|---|---|
| Dokumenttyp: | Article (Journal) |
| Sprache: | Englisch |
| Veröffentlicht: |
[February 2019]
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| In: |
Monthly notices of the Royal Astronomical Society
Year: 2018, Jahrgang: 482, Heft: 4, Pages: 4290-4302 |
| ISSN: | 1365-2966 |
| DOI: | 10.1093/mnras/sty2981 |
| Online-Zugang: | 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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| Verfasserangaben: | Steffen Hahn, Ralf Hofmann and Daniel Kramer |
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| 246 | 3 | 3 | |a SU(2) cmb and the cosmological model |
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| 520 | |a 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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