SIMBAD references

2015ApJ...806..184D - Astrophys. J., 806, 184 (2015/June-3)

Neutrino constraints to the diffuse gamma-ray emission from accretion shocks.

DOBARDZIC A. and PRODANOVIC T.

Abstract (from CDS):

Accretion of gas during the large-scale structure formation has been thought to give rise to shocks that can accelerate cosmic rays. This process then results in an isotropic extragalactic gamma-ray emission contributing to the extragalactic gamma-ray background (EGRB) observed by Fermi-LAT. Unfortunately, this emission has been difficult to constrain and thus presents an uncertain foreground to any attempts to extract a potential dark matter signal. Recently, IceCube has detected high-energy isotropic neutrino flux that could be of an extragalactic origin. In general, neutrinos can be linked to gamma rays since cosmic-ray interactions produce neutral and charged pions where neutral pions decay into gamma rays, while charged pions decay to give neutrinos. By assuming that isotropic high-energy IceCube neutrinos are entirely produced by cosmic rays accelerated in accretion shocks during the process of structure formation, we obtain the strongest constraint to the gamma-ray emission from large-scale structure formation (strong) shocks and find that they can make at best ∼20% of the EGRB, corresponding to neutrino flux with spectral index αν= 2, or ∼10% for spectral index αν= 2.46. Since typical objects where cosmic rays are accelerated in accretion shocks are galaxy clusters, observed high-energy neutrino fluxes can then be used to determine the gamma-ray emission of a dominant cluster type and constrain acceleration efficiency, and thus probe the process of large-scale structure formation.

Abstract Copyright:

Journal keyword(s): cosmic rays - diffuse radiation - gamma rays: diffuse background - gamma rays: galaxies: clusters - large-scale structure of universe - neutrinos

Simbad objects: 2

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2019.12.13-13:50:16

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