A crucial dipole test of the expansion center Universe - based on high-z SCP Union & Union2 supernovae
Luciano Lorenzi

TL;DR
This paper presents a crucial multiple dipole test confirming the expansion center universe model using high-redshift supernova data, and introduces a new computation of the relativistic deceleration parameter q0 consistent with the model.
Contribution
It provides a model-independent dipole anisotropy test at z=1 and a novel calculation of q0 that supports the expansion center universe hypothesis.
Findings
Confirmed dipole anisotropy at z=1 consistent with ECM
Maximum cz range of about 50000 km/s at z=1
Computed q0=+2 consistent with ECM predictions
Abstract
The expansion center Universe (ECU) gives a dipole anisotropy to the Hubble ratio, at any Hubble depth D. After a long series of successful dipole tests, here is a crucial multiple dipole test at z bins centred on the mean <z>=z0=1, or Hubble depth D=c/H0, and based on data from SCP Union & Union2 compilation. Table 5abc lists data of two main samples, with 48 SCPU SNe Ia and 58 SCPU2 SNe Ia respectively. The confirmed dipole anisotropy, shown by 6 primary sample tests and by another 27 from 9 encapsulated z bins with DL=D(1+z) assumed and the Hubble Magnitude definition, gives a model independent result, in full accordance with the expansion center model (ECM). That means a maximum cz range of about 50000 km/s at the central redshift z0=1. As a complement to the dipole tests, here is a new computation of the relativistic deceleration parameter q0, based on the extrapolated total M…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Stellar, planetary, and galactic studies · Astronomy and Astrophysical Research
