Escape of cosmic rays from the Galaxy and effects on the circumgalactic medium

Abstract

The escape of cosmic rays from the Galaxy is expected to shape their spectrum inside the Galaxy. Yet, this phenomenon is very poorly understood and, in the absence of a physical description, it is usually modelled as free escape from a given boundary, typically located at a few kpc distance from the Galactic disc. We show that the assumption of free escape leads to the conclusion that the cosmic ray current propagating in the circumgalactic medium is responsible for a non resonant cosmic ray induced instability that in turn leads to the generation of a magnetic field of strength $\sim 2\times 10^{-8}$ Gauss on a scale $\sim 10$ kpc around our Galaxy. The self-generated diffusion produces large gradients in the particle pressure that induce a displacement of the intergalactic medium with velocity $\sim 10-100$ km/s. Cosmic rays are then carried away by advection. If the overdensity of the intergalactic gas in a region of size $\sim 10$ kpc around our Galaxy is $\gtrsim 100$ with respect to the cosmological baryon density ${\Omega }_b{\rho }_{cr}$, then the flux of high energy neutrinos as due to pion production becomes comparable with the flux of astrophysical neutrinos recently measured by IceCube.

arXiv commentAccepted for publication in Phys. Rev. Letters

References in corpus (12)

• Evidence for High-Energy Extraterrestrial Neutrinos at the IceCube Detector
• The Interstellar Environment of our Galaxy
• The spectrum of isotropic diffuse gamma-ray emission between 100 MeV and 820 GeV
• A combined maximum-likelihood analysis of the high-energy astrophysical neutrino flux measured with IceCube
• Non-linear Study of Bell's Cosmic Ray Current-driven Instability
• A Galactic Halo Origin of the Neutrinos Detected by IceCube
• Origin of the Cosmic Ray Galactic Halo Driven by Advected Turbulence and Self-Generated Waves
• On the cosmic ray spectrum from type II Supernovae expanding in their red giant presupernova wind
• Environments for Magnetic Field Amplification by Cosmic Rays
• From cosmic ray source to the Galactic pool
• High energy cosmic ray self-confinement close to extragalactic sources
• Environmental limits on the non-resonant cosmic-ray current-driven instability

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• LHAASO sensitivity for diffuse gamma-ray signals from the Galaxy
• Deciphering Residual Emissions: Time-Dependent Models for the Non-Thermal Interstellar Radiation from the Milky Way
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• High-energy neutrinos from cosmic ray interactions in the Local Bubble
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• Mapping large-scale diffuse gamma-ray emission in 10-100 TeV band with Cherenkov telescopes
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