Relativity and Cosmology

   

Kinematic Interpretation of 580 Supernovae Type 1a Redshifts: a Cosmic Scale Link to Mond Acceleration?

Authors: Berry C. Ives

We present an empirical analysis of redshift of 580 supernovae type 1a using special relativistic Doppler to derive velocity of recession. A theory of cosmological scale is developed in which scale history is parabolic in relation to observed distance and time. The parabolic relationship suggests that the present lies on the accelerated contraction side of the scale history. The first-order coefficient of the scale equation matches very precisely the post-Planck value of the Hubble parameter, H0. The second-order coefficient of the parabolic scale history is taken as an acceleration parameter, I0. H0 is thus merely the slope of the parabola at the present time, and it can be eliminated by shifting the abscissa so that t = 0 aligns with the vertex. In this way, the scale history is entirely dependent on the acceleration parameter, I0. A methodology is used to infer physical radial distance from scale. The resulting acceleration rate precisely matches modified Newtonian dynamics (MOND) universal acceleration a0 and thus appears to provide a general cosmological link to that phenomenon, implying a universe under accelerated contraction.

Comments: 24 Pages. In the full text of the article, the abstract is also presented in French.

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[v1] 2018-08-31 21:00:31

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