Our Peculiar Motion Inferred from Number Counts of Mid Infra Red AGNs and the Discordance Seen with the Cosmological Principle
arXiv:2102.12084 · doi:10.3390/universe7040107
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 the same irrespective of the data or the technique employed to estimate it. Therefore, such discordant dipole amplitudes, might mean that the explanation for these dipoles, including that of the CMBR, might in fact be something else. But, the observed fact that the direction in all cases, is the same, though obtained from completely independent surveys using different instruments and techniques, by different sets of people employing different computing routines, might nonetheless indicate that these dipoles are not merely due to some systematics, otherwise why would they all be pointing along the same direction. It might instead suggest a preferred direction in the Universe, implying a genuine anisotropy, which would violate the Cosmological Principle, the core of the modern cosmology.
arXiv comment18 pages, 10 figures, 3 tables, accepted in Universe
References in corpus (33)
- The Wide-field Infrared Survey Explorer (WISE): Mission Description and Initial On-orbit Performance
- Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Data Processing, Sky Maps, and Basic Results
- Planck 2018 results. I. Overview and the cosmological legacy of Planck
- The GMRT 150 MHz All-sky Radio Survey: First Alternative Data Release TGSS ADR1
- Initial Performance of the NEOWISE Reactivation Mission
- Indications of a spatial variation of the fine structure constant
- A measurement of large-scale peculiar velocities of clusters of galaxies: results and cosmological implications
- A Test of the Cosmological Principle with Quasars
- Spatial variation in the fine-structure constant -- new results from VLT/UVES
- The Dipole Observed in the COBE DMR Four-Year Data
- A new measurement of the bulk flow of X-ray luminous clusters of galaxies
- Cosmic radio dipole from NVSS and WENSS
- Identification of 1.4 Million AGNs in the Mid-Infrared using WISE Data
- Large peculiar motion of the solar system from the dipole anisotropy in sky brightness due to distant radio sources
- High redshift radio galaxies and divergence from the CMB dipole
- Probing the Cosmological Principle in the counts of radio galaxies at different frequencies
- Is there Correlation between Fine Structure and Dark Energy Cosmic Dipoles?
- Dipole anisotropy in sky brightness and source count distribution in radio NVSS data
- A measurement of large-scale peculiar velocities of clusters of galaxies: technical details
- CMB Maximum Temperature Asymmetry Axis: Alignment with Other Cosmic Asymmetries
- Detecting the Cosmic Dipole Anisotropy in Large-Scale Radio Surveys
- Is there further evidence for spatial variation of fundamental constants?
- Probing the Dark Flow signal in WMAP 9 yr and PLANCK cosmic microwave background maps
- Is the CMB asymmetry due to the kinematic dipole?
- A large disparity in cosmic reference frames determined from the sky distributions of radio sources and the microwave background radiation
- Directional dependence of CMB parity asymmetry
- Clusters of galaxies and variation of the fine structure constant
- Constraining spatial variations of the fine structure constant using clusters of galaxies and Planck data
- Peculiar motion of the solar system derived from a dipole anisotropy in the redshift distribution of distant quasars
- Preferred axis of CMB parity asymmetry in the masked maps
- A model for CMB anisotropies on large angular scales
- CMB dipole revisited
- A reanalysis of quasar absorption spectra results suggesting a spatial gradient in values of the fine-structure constant