Relatore
Descrizione
According to Thomas Kuhn (1962), the recognition of the Expansion Center of the Universe has to be considered as a new scientific PARADIGM for a revolution in Cosmology (Lorenzi 2009, p.5). Indeed, the discovery by Bahcall & Soneira (1982) of a Huge Void of Rich Clusters didn’t recognize its Center 𝑽𝑪(𝜶 ≈ 𝟗𝒉, 𝜹 ≈ +𝟑𝟎°) as the Cosmic Expansion Cente, but the Expansion Center Model (ECM: Lorenzi 1999ab) has proven it (compare also Dirac's LNH results: 1937-1938)! Now we present a series of 23 DIPOLES of the Expansion Center Hubble ratio of the Universe (Lorenzi 1991, 1999b, 2004ab, 2012b) at the mean redshifts 〈z〉≪0.1,〈z〉≅0.5,〈z〉=1.00.
Figures 1-2-3 show the first five 𝒓̇/𝒓 Hubble Ratio DIPOLES of ECU1 (Lorenzi–Ferrari–Masani 1991), while in Fig.5 the two DIPOLES of Fig. 4 have a minimum of the 𝒔 standard deviation of the least square fitting at 𝑹 ≈ 𝟐𝟔𝟎 𝑴𝒑𝒄. The listed Figures 1-2-3-4-5-6-7 of ECM paper II (Lorenzi 1999b) represent seven DIPOLES of the 𝒓̇/𝒓 Hubble ratio versus − 𝐜𝐨𝐬 𝜸 of the nearby Universe, with the result H_0≅(70±3) H.u.. In 4x2 Figures at 〈𝒛〉 ≈ 𝟎.𝟓 of SCP SNe Ia (Lorenzi 2004ab) and in the 3 Figures 1-2-3 (Lorenzi 2012b: ECM paper XV or ECU20), at 〈𝒛〉 = 𝟏.𝟎𝟎 of SCP SNe Ia, we have a series of DIPOLES, or NORMAL COSMIC DIPOLES CD accoding to the eq. cz/D=H_0 〖- a〗^ cosγ. The final result at 〈z〉=1.00 is an angular coefficient 〈a^ 〉=(5.47±0.25) H.u. as an average of 33 values of a^*.
| Sessione | Cosmologia |
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