A multi-frame FLRW model for cosmic fluids produces an alternative Hubble parameter consistent with DESI DR2 BAO and CC data up to z<2.33 while providing sufficient time for high-redshift SMBH formation.
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An Alternative Hubble parameter: Explaining DESI data and High redshift Supermassive Black Hole
A multi-frame FLRW model for cosmic fluids produces an alternative Hubble parameter consistent with DESI DR2 BAO and CC data up to z<2.33 while providing sufficient time for high-redshift SMBH formation.