A Crucial Dipole Test of the Expansion Center Universe

Details A Crucial Dipole Test of the Expansion Center Universe A Crucial Dipole Test of the Expansion Center Universe

2011-05-18

arxiv.org/abs/1105.3697v3

Astronomy and Astrophysics

Astrophysics

Cosmology and Extragalactic Astrophysics

19 pages in TeX, 3 figures - New revised version of the contribution presented at the 55th Annual Meeting of the Italian Astro

Scientific paper

The expansion center Universe (ECU) gives a dipole anisotropy to the Hubble law, at any Hubble depth D. After a long series of successful dipole tests on the nearby Universe, using historic data sets of about half a century, and that carried out on 53 SCP SNe Ia ranging around the average redshift =0.5 (ECM paper VI: SAIt2004 in Milan), here is a crucial multiple dipole test at z bins centred on the mean =1.0, or Hubble depth D=c/H0, and based on data from SCP Union compilation (SCPU: Kowalski et al. 2008) and SCP Union2 (SCPU2: Amanullah et al. 2010), including those obtained within "The new wedge-shaped Hubble diagram of 398 SCP supernovae..." (ECM paper IX: SAIt2010 in Naples). 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. This means a maximum cz range of about 50000 km/s at the central redshift z0=1. Here is included the Appendix - November 2011 - "Introduction to the Hubble Magnitude and a new relativistic q0". A further check and deepening of the topic is given in the parallel paper XI "Dipole analysis of 249 High-z SCP Union supernovae according to the expansion center model" and its Addendum Note - October 2011 -.

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