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arXiv · 1008.4769

Limits on the Time Variation of the Fermi Constant G_F Based on Type Ia Supernova Observations

Alejandro Ferrero·Brett Altschul
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Abstract

The light curve of a type Ia supernova decays at a rate set by the beta-decay lifetimes of the Ni-56 and Co-56 produced in the explosion. This makes such a light curve sensitive to the value of the Fermi constant G_F at the time of the supernova. Using data from the CfA Supernova Archive, we measure the dependence of the light curve decay rate on redshift and place a bound on the time variation of G_F of |(dG_F/dt)/G_F| < 10^(-9) / y.

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Alejandro Ferrero, Brett Altschul. 2011-02-07. Limits on the Time Variation of the Fermi Constant G_F Based on Type Ia Supernova Observations. https://doi.org/10.1103/physrevd.82.123002

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