High-energy neutrino astronomy: the cosmic ray connection

Abstract

This is a review of neutrino astronomy anchored to the observational fact that Nature accelerates protons and photons to energies in excess of 10 20 and 10 13 eV, respectively.Although the discovery of cosmic rays dates back close to a century, we do not know how and where they are accelerated. There is evidence that the highest energy cosmic rays are extra-galactic -they cannot be contained by our galaxy's magnetic field anyway because their gyroradius far exceeds its dimension. Elementary elementary-particle physics dictates a universal upper limit on their energy of 5 × 10 19 eV, the so-called Greisen-Kuzmin-Zatsepin cutoff; however, particles in excess of this energy have been observed by all experiments, adding one more puzzle to the cosmic ray mystery. Mystery is fertile ground for progress: we will review the facts as well as the speculations about the sources.There is a realistic hope that the oldest problem in astronomy will be resolved soon by ambitious experimentation: air shower arrays of 10 4 km 2 area, arrays of air Cerenkov detectors and, the subject of this review, kilometer-scale neutrino observatories.We will review why cosmic accelerators are also expected to be cosmic beam dumps producing associated high-energy photon and neutrino beams. We will work in detail through an example of a cosmic beam dump, gamma ray bursts. These are expected to produce neutrinos from MeV to EeV energy by a variety of mechanisms. We will also discuss active galaxies and GUT-scale remnants, two other classes of sources speculated to be associated with the highest energy cosmic rays. Gamma ray bursts and active galaxies are also the sources of the highest energy gamma rays, with emission observed up to 20 TeV, possibly higher. The important conclusion is that, independently of the specific blueprint of the source, it takes a kilometer-scale neutrino observatory to detect the neutrino beam associated with the highest energy cosmic rays and gamma rays. We also briefly review the ongoing efforts to commission such instrumentation. Contents

High-energy cosmic rays: Puzzles, models, and giga-ton neutrino telescopes

“…For a more general, yet concise, discussion of high energy neutrino telescopes and their science goals see chapters 2 and 3 of [30]. For more detailed review see [31].…”

IceCube and ANTARES

“…From observation with photons such shock waves are known to exist in various objects in our own Galaxy as well as up to cosmological distances. Various models for neutrino production exist [28][29][30]. Promising neutrino point source candidates in our own Galaxy are Supernovae Remnants and Micro Quasars whereas the vicinity of the super-massive black holes in Active Galactic Nuclei and Gamma Ray Bursts are prominent extragalactic candidates.…”

A Search for Ultra-High Energy Neutrinos and Cosmic-Rays with ANITA-2

“…[111] for a review). When considering the diffuse neutrino flux, no expectation is placed on the energy spectrum which is being constrained and the resulting flux limits are model-independent.…”