[At the outset, I want to express my sincere gratitude and heartfelt congratulations to this community for this unmatched openness in welcoming unconventional ideas. I completely understand that most such ideas would be flawed, however, absolute restriction of such ideas as done the mainstream academia is detrimental to science and is borne out of an inflated sense of self-worth, in my humble opinion.]
I went through the velocity-distance data for Type Ia supernovae. I have tried to come up with an alternative model which potentially resolves some observational peculiarities.
The idea at its fundamental level is this: The velocity-distance data for Type Ia Supernovae have been traditionally plotted to pass through origin. This models an accelerating Universe as conventionally concluded. However, when we allow for an intercept in the velocity-distance plot, in other words when we allow for an extra-Hubble-Lemaitre (eHL) velocity, we, interestingly, potentially resolve the following three long-persisting intrigues:
1. 'Crisis in Cosmology': Allowing for an eHL velocity also allows us to model the rate of expansion as measured by the Planck collaboration (67.4 km/s) thus removing the existing 'tension' between values of the Hubble-Lemaitre constant. The rest of the velocity vector, that remains unaccounted for by the Hubble-Lemaitre velocity (67.4 \times Distance), is the eHL velocity.
2. Counter-intuitive accelerating expansion of the Universe: It turns out, amazingly, that allowing for eHL velocities in the model turns the observational data for accelerating expansion into one for decelerating expansion. How this happens is illustrated in detail in the section titled 'Decelerating Universe?' in the complete article: https://vixra.org/pdf/2003.0196v1.pdf
3. Direct observational evidence for reheating and inflation: Allowing for eHL velocities also permits it to be a potential direct remnant of explosive particle creation during reheating and inflation. Such a direct observational evidence was long sought by the Astronomy community.
I do not claim to have given sufficient evidence for the correctness of my model over others. Far from it. However, given that this model potentially resolves some longstanding peculiarities in theory and observations, I humbly believe that the Astronomy community would not be disadvantaged in going through this model.