Large peculiar motion of the solar system from the dipole anisotropy in sky brightness due to distant radio sources
Ashok K. Singal

TL;DR
This study measures the solar system's peculiar velocity using sky brightness anisotropy from distant radio sources, finding a magnitude significantly larger than the CMBR-based value, which could challenge the cosmological principle.
Contribution
It provides a novel measurement of the solar system's velocity from radio source anisotropy, revealing a magnitude larger than the CMBR estimate, suggesting potential anisotropy in the Universe.
Findings
Velocity magnitude ~1600 km/s, larger than CMBR estimate
Direction of velocity aligns with CMBR results
Potential implications for cosmological isotropy
Abstract
According to the cosmological principle, the Universe should appear isotropic, without any preferred directions, to an observer whom we may consider to be fixed in the co-moving co-ordinate system of the expanding Universe. Such an observer is stationary with respect to the average distribution of the matter in the Universe and the sky brightness at any frequency should appear uniform in all directions to such an observer. However a peculiar motion of such an observer, due to a combined effect of Doppler boosting and aberration, will introduce a dipole anisotropy in the observed sky brightness; in reverse an observed dipole anisotropy in the sky brightness could be used to infer the peculiar velocity of the observer with respect to the average Universe. We determine the peculiar velocity of the solar system relative to the frame of distant radio sources, by studying the anisotropy in…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
