Relativity and Cosmology

    

Weak Interaction as the Origin of the Hubble Tension

Authors: Sylwester Kornowski

Here we show that the Hubble tension, i.e. the two different values of the Hubble constant for the early Universe (about 68)and near Universe (about 74), is the result of a step change in the value of the density parameter for the part of baryonic matter that due to the weak force interacts with dark matter.

Comments: 4 Pages.

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Submission history

[v1] 2020-08-30 08:50:00
[v2] 2020-09-17 13:50:22

Unique-IP document downloads: 204 times

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