Hubble Diagram Test of 280 Supernovae Redshift Data

Laszlo A Marosi

doi:10.4236/jmp.2014.51005

Abstract

We compare the Hubble diagram calculated from the observed redshift (RS)/magnitude (μ) data of 280 Supernovae in the RS range of z = 0.0104 to 8.1 with Hubble diagrams inferred on the basis of the exponential tired light and the Lambda Cold Dark Matter (ΛCDM) cosmological model. We show that the experimentally measured Hubble diagram follows clearly the exponential photon flight time (tS)/RS relation, whilst the data calculated on the basis of the ΛCDM model exhibit poor agreement with the observed data.

Highlights

IntroductionLaViolette [2] and more recently, López-Corredoira [3], Crawford [4], and Marosi [5,6,7] have shown that the static or slowly expanding universe models fit the observational data better than the data calculated on the basis of the presently prevailing ΛCDM model
The basic assumption of the Lambda Cold Dark Matter (ΛCDM) cosmological model is that the universe is expanding, according to the Hubble’s law [1], at a velocity of v = zc = H0DC, where z is the redshift (RS), c is the velocity of light, H0 is the Hubble constant, and DC is the co-moving radial distance that can be derived from the observable z/μ data by (1)
LaViolette [2] and more recently, López-Corredoira [3], Crawford [4], and Marosi [5,6,7] have shown that the static or slowly expanding universe models fit the observational data better than the data calculated on the basis of the presently prevailing ΛCDM model

Summary

Introduction

LaViolette [2] and more recently, López-Corredoira [3], Crawford [4], and Marosi [5,6,7] have shown that the static or slowly expanding universe models fit the observational data better than the data calculated on the basis of the presently prevailing ΛCDM model. Such results, are usually refuted with the argument that the static universe contradicts many other cosmological observations, for example, the time dilation test and the cosmic microwave background (CMB) temperature versus RS test [8]. MAROSI relation; an effect that is perceptible only slightly in the z < 1 region

Data Collection and Processing

Results

Conclusions