eFTC-171201
No Black Hole Mergers Sources for LIGO/Virgo Gravitational Waves and Accreting Super Quasar J1342+0928 |
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Author: Y. Leblanc (eFieldTheory.COM) Email: AbstractA direct consequence of the Strong Principle of Equivalence (SPOE) is the complete elimination of all finite mass (and rotating) astrophysical black holes (BHs) from General Relativity (GR). In fact, good agreement with astrophysical data has been reported by interpreting Galactic Black Hole Candidates (GBHC) as well as Active Galactic Nuclei (AGN) as quasi-black holes (ECOs/MECOs) with an intrinsic magnetic moment, a property not shared with true black holes. Consequently, the positive signals at the LIGO/Virgo gravitational waves detectors as well as the recently observed primitive and supermassive J1342+0928 Quasar should not be interpreted as originating from black holes mergers. Instead, the LIGO/Virgo gravitational waves sources are very likely GBHC binaries while the supermassive J1342+0928 Quasar may originate from ancient AGNs mergers, i.e. both identified as merger systems of ECOs/MECOs, not black holes. Furthermore, the J1342+0928 Quasar redshift at z=7.54 cannot describe a Kerr black hole since true black holes have infinite redshift. Calculations involving true black hole mergers may provide nevertheless a reasonable fit to astrophysical data as an approximation to ECOs/MECOs merger systems, for times short compared to Hubble time. Copyright © 2017 Yvan Leblanc. All rights reserved
PACS: 4.60.+n, 11.17.+y, 97.60.Lf Cite as: Leblanc, Y., "No Black Hole Mergers Sources for LIGO/Virgo Gravitational Waves and Accreting Super Quasar J1342+0928", manuscript no. eFTC-171201 (2017). http://www.efieldtheory.com/abs/?eFTC-171201; doi:10.13140/RG.2.2.10292.96647. |
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