Our Peculiar Motion Inferred from Number Counts of Mid Infra Red AGNs and the Discordance Seen with the Cosmological Principle
Ashok K. Singal

TL;DR
This study finds that the peculiar velocity inferred from mid-infrared AGN counts is significantly larger than the CMBR-based value, suggesting possible anisotropy in the universe that challenges the Cosmological Principle.
Contribution
It provides a new measurement of our peculiar motion using a large AGN sample, revealing a discrepancy with the CMBR result and indicating potential universe anisotropy.
Findings
Peculiar velocity from AGNs is over four times the CMBR value.
The direction of the velocity aligns with the CMBR dipole within uncertainties.
Results suggest possible violation of the Cosmological Principle.
Abstract
The dipole anisotropy in the Cosmic Microwave Background Radiation (CMBR) has given a peculiar velocity vector 370 km s along . However, some other dipoles, for instance, from the number counts, sky brightness or redshift distributions in large samples of distant Active Galactic Nuclei (AGNs), have yielded values of the peculiar velocity many times larger than that from the CMBR, though surprisingly, in all cases the directions agreed with the CMBR dipole. Here we determine our peculiar motion from a sample of ~0.28 million AGNs, selected from the Mid Infra Red Active Galactic Nuclei (MIRAGN) sample comprising more than a million sources. From this, we find a peculiar velocity, which is more than four times the CMBR value, although the direction seems to be within of the CMBR dipole. A genuine value of the solar peculiar velocity should be…
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