Correlation of supernova redshifts with temperature fluctuations of the Cosmic Microwave Background

TL;DR

This study finds a statistically significant correlation between supernova redshifts and temperature fluctuations in the CMB, suggesting potential cosmological effects like the integrated Sachs-Wolfe effect.

Contribution

It presents the first evidence of a correlation between supernova redshifts and WMAP temperature fluctuations, highlighting a new observational link.

Findings

Significant correlation for z=0.5-1.0 with +29.9 microK deviation

Moderate correlation for z=0.0-0.4 with +8.6 microK deviation

Results support the integrated Sachs-Wolfe effect at lower redshifts

Abstract

Redshifts of a supernova (SN) and gamma-ray burst (GRB) samples are compared with the pixel temperatures of the Wilkinson Microwave Anisotropy Probe (WMAP) seven-years data, the pixels locations corresponding to the SN and GRB sky coordinates. We have found a statistically significant correlation of the SN redshifts with the WMAP data, the average temperature deviation being +29.9 +-4.4 microK for the redshifts z ranging from 0.5 to 1.0 and +8.6 +-1.3 microK for z within the range (0.0,0.4). The latter value accords with the theoretical estimates for the distortion of the cosmic microwave background due to the integrated Sachs-Wolfe effect, whereas the larger anomaly for higher redshifts should be studied in more detail in the future.