A mechanism to explain Galaxy alignment over a range of scales
Prabhakar Tiwari (Beijing Observ.), Pankaj Jain (Indian Inst. Tech.,, Kanpur)

TL;DR
This paper proposes that correlations in the intergalactic magnetic field can explain galaxy and polarization alignments across scales from Gpc to Mpc, challenging standard cosmological assumptions.
Contribution
It introduces a magnetic field correlation model that accounts for galaxy and radio source alignments over multiple scales, extending previous explanations.
Findings
The model explains the FIRST radio source alignment with a spectral index of -2.62.
It partially accounts for galaxy alignments within clusters.
Large-scale magnetic correlations can unify explanations across different scales.
Abstract
The observed large-scale alignment of polarization angles and galaxy axis have been challenging the fundamental assumption of homogeneity and isotropy in standard cosmology since more than two decades. The intergalactic magnetic field, and its correlations in real space, potentially seems as a viable candidate for explaining this phenomenon. It has been shown earlier that the large-scale intergalactic magnetic field correlations can explain the alignment signal of quasars over Gpc scale, interestingly they can also explain the radio polarization alignment observed in JVAS/CLASS data over 100 Mpc. Motivated with recent observations of galaxy axis alignment over several tens of Mpc, and Mpc scale, i.e., the cluster scale, we further explore the correlations of background magnetic field to explain these relatively small scale alignment observations. In particular, we explore two recently…
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