In this video presentation I describe the history of the development of the standard big bang cosmology and how it is understood in terms of its philosophical underpinnings. The Cosmological Principle is explained as the major and essential assumption upon which it all depends. Due to this it has been required to invent unknown stuff, expansion of space, Dark Energy, Dark Matter, CMB radiation as afterglow of Big Bang, and Inflation. None of these are experimental observed in the lab. Yet all of these are needed else the standard ΛCDM model utterly fails. Though we hear for the first time those speaking of discarding the standard model, they have built themselves a modern-day tower of Babel, an edifice of a structure that must be supported at all costs, especially since in 2011 the Nobel Prize was awarded for the accelerating universe driven by the unknown stuff of science fiction—Dark Energy.
The big bang model, used to describe the observations made in the universe, according to its advocates, now precisely has determined the history of the Universe. See left graphic. Yet to do so it is filled with unproveable fudge factors. That may sound like an exaggerated claim but it seems to be the state of cosmology today. (This article was edited and updated from my article ‘Cosmology is not even astrophysics,’ originally published 3 December 2008, creation.com.)
This situation has come about because of the unverifiable starting assumptions are inherently wrong! Some brave physicists have had the temerity to challenge the ruling paradigm—the standard big bang ΛCDM inflation cosmology.1 One of those is Prof. Richard Lieu, astrophysicist, of the Department of Physics, University of Alabama, who wrote:2
‘Cosmology is not even astrophysics: all the principal assumptions in this field are unverified (or unverifiable) in the laboratory … .’ [emphasis added]
A theorist has an idea about the mixing (coupling) of dark matter axions with normal matter through an S/N/S junction. Firstly, the axion is a theorized particle in the WIMPcategory but this expected particle with a mass of 1 μeV is in the WISP (Weakly Interacting Slim Particle) category. The latter is what I have been searching for in a lab experiment—a 53 μeV mass paraphoton—for four years.1 In all these type of experimental searches, these types of putative particles cannot be directly observed but only by their expected effects on normal matter and radiation sectors. So a theorist calculates the magnitude of the mixing parameter (nowadays < 10-8, or much lower) and they run experiments to put an upper limit on it. So if you get a signal—instead of just noise—the signal is from real normal type radiation, thus you have to exclude all possible spurious signals, and usually the detection expected is extremely small so it becomes extremely problematic to definitively say—even if you had an unknown signal—that you have made a detection.