Peculiar motion of Solar system from the Hubble diagram of supernovae Ia and its implications for cosmology
Ashok K. Singal

TL;DR
This paper introduces a new method using Type Ia Supernovae to measure the solar system's peculiar motion, revealing a velocity significantly larger than the CMBR estimate, with implications for cosmic isotropy.
Contribution
A novel technique based on the supernova Hubble diagram to determine solar peculiar velocity, showing larger values than traditional CMBR-based measurements.
Findings
Measured solar peculiar velocity as 1600 km/s, larger than CMBR estimate.
Found the velocity direction consistent within 2σ of the CMBR dipole.
Suggested potential evidence for anisotropy in the universe.
Abstract
Peculiar motion of the solar system, determined from the dipole anisotropy in the Cosmic Microwave Background Radiation (CMBR), has given a velocity km s along RA, Dec. Subsequent peculiar motion determinations from the number counts, sky brightness or redshift dipoles observed in large samples of distant radio galaxies and quasars yielded peculiar velocities two to ten times larger than CMBR, though in all cases the directions matched with the CMBR dipole. Here we introduce a novel technique for determining the peculiar motion from the magnitude-redshift () Hubble diagram of Type Ia Supernovae (SN Ia), one of the best standard candles available. We find a peculiar velocity km s, larger than the CMBR value roughly by a factor of four, along RA, Dec,…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Solar and Space Plasma Dynamics · Stellar, planetary, and galactic studies
