Tired light models invoke a gradual energy loss by photons as they travel through the cosmos to produce the redshift-distance law. This has three main problems:
In 2001 Goldhaber and the Supernova Cosmology Project published results of a time dilation analysis of 60 supernovae. A plot of their width factor w versus the redshift z is shown below.
If the redshift were due to a tired light effect, the width of a supernova light curve would be independent of the redshift, as shown by the red horizontal line. If the redshift is due to an expanding Universe, the width factor should be w = (1+z) as shown by the blue line. The best fit to the data is the black line, and it is clearly consistent with the blue line and rules out the tired light model. My best fit line is
w = 0.985*(1+z)(1.045 +/- 0.089)using a least sum of absolute errors robust estimator to find the fit and the half-sample bootstrap to estimate the errors. This data excludes the tired light model by more than 11 standard deviations.
Blondin et al. (2008) also studied distant supernovae, but used spectra to judge the age of the supernovae. They found an aging rate that varied like
1/(1+z)(0.97 +/- 0.10),compatible with the expected 1/(1+z) for expanding Universes, but 9.7 standard deviations away from the constant aging rate expected in the tired light model.
The expanding balloon analogy for cosmological models can be used to
show this. The figure below shows the analogy at
two different times.

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© 1996-2008 Edward L. Wright. Last modified 24 Apr 2008