Detection of virial shocks in stacked Fermi-LAT clusters

TL;DR

This study detects a gamma-ray signal from virial shocks in galaxy clusters by stacking Fermi-LAT data, confirming the shock paradigm and its role in cosmic background emissions.

Contribution

It presents the first detection of a virial gamma-ray ring in galaxy clusters, validating the shock acceleration model and calibrating its parameters.

Findings

Detection of a bright gamma-ray ring at the expected shock position

Confirmation of relativistic electron acceleration in virial shocks

Implication that shocks contribute significantly to extragalactic backgrounds

Abstract

In the hierarchical paradigm of structure formation, galaxy clusters are the largest objects ever to virialize. They are thought to grow by accreting mass through large scale, strong virial shocks. Such a collisionless shock is expected to accelerate relativistic electrons, thus generating a spectrally flat leptonic virial ring. However attempts to detect virial rings have all failed, leaving the shock paradigm unconfirmed. Here we identify a virial $\gamma$-ray signal by stacking Fermi-LAT data for 112 clusters, enhancing the ring sensitivity by rescaling clusters to their virial radii and utilizing the anticipated spectrum. In addition to a central unresolved, hard signal (detected at the nominal $5.8\sigma$ confidence level), probably dominated by active galactic nuclei, we identify ($5.9\sigma$) a bright, spectrally flat $\gamma$-ray ring at the expected shock position. It corresponds to $\sim 0.6\%$ (with an uncertainty factor $\sim2$) thermal energy deposition in relativistic electrons over a Hubble time. This result validates the shock paradigm, calibrates its parameters, and indicates that the cumulative emission from such shocks significantly contributes to the diffuse extragalactic $\gamma$-ray and radio backgrounds.