Michael Smith
Michael Smith received his Ph.D. from Colorado State University and then studied biophysics and computerized data handling at Johns Hopkins University, Maryland. He has been publishing on the topic of the proper interpretation of supernovae type Ia (SNe Ia) observations since 2006. Several of his articles deal with dark energy, dark matter, and Hubble\'s constant determinations. Lately, he has been investigating the basis for the current Hubble tension as stemming from improper handling of the SNe Ia data and differing interpretations of the Friedmann (FLRW) model. He has also published new fundamental relations over the relations between matter, energy, spacetime, and gravity. He has published more than fifty articles in peer-reviewed journals, edited two books on cosmology, and produced six short videos for public education.