Sub-percent constraints on cosmological temperature evolution

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Sub-percent constraints on cosmological temperature evolution

The redshift dependence of the cosmic microwave background temperature is one of the key cosmological observables. In the standard cosmological model one has T (z) = T0(1 + z), where T0 is the present-day temperature. Deviations from this behavior would imply the presence of new physics. Here we dis...

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Bibliographic Details
Main Authors:	Avgoustidis, A., Genova-Santos, R.T ., Luzzi, G., Martins, C.J.A.P.
Format:	Article
Published:	American Physical Society 2016
Online Access:	https://eprints.nottingham.ac.uk/34957/

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