Bulk Flow Motion Detection in the Local Universe with Pantheon+ Type Ia Supernovae
Maria Lopes,
Armando Bernui,
Camila Franco
et al.
Abstract:The bulk flow in the Local Universe is a collective phenomenon due to the peculiar motions of matter structures, which, instead of moving in random directions, appears to follow an approximate dipole velocity flow. We apply a directional analysis to investigate, through the Hubble-Lemaître diagram, the angular dependence of the Hubble constant H
0 of a sample of Type Ia supernovae from the Pantheon+ catalog in the Local Universe (0.015 ≤ z ≤ 0.06). We perform a directional analysis that revea… Show more
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