Snowmass 2021 LoI: Determination of cosmic ray properties in the local interstellar medium with all-sky anisotropy observations
arXiv:2009.04883
Abstract
Propagation of Galactic cosmic rays (CR) in the interstellar medium (ISM) is among the unsolved problems in particle astrophysics. Interpretation of CR spectrum and composition measurements and their possible link to dark matter crucially relies on our understanding of CR propagation in the Galaxy. Several air shower experiments have measured a significant anisotropy of CRs in the TeV to PeV energy range. These observations hint to a complicated overlap of more than one cause: from the distribution of the CR sources in the Milky Way to the nature of such sources, from the turbulence properties of interstellar plasmas to the inhomogeneous nature of the interstellar medium. Coherent magnetic structures such as the heliosphere greatly influence the CR arrival direction distribution. It is necessary to account for and remove the heliosphere's distortion effects if we want to determine the pristine CR arrival direction distribution in the local interstellar medium (LISM), the environment surrounding the solar system up to the distance of particle mean free path. The recent availability of accurate all-sky maps of CR arrival direction distribution and the latest advancements in heliospheric modeling, make it possible to infer the CR pitch angle distribution in the LISM using a Liouville mapping technique. With the interstellar CR distribution, we can study the global characteristics of CR diffusion, tap into the properties of interstellar plasma turbulence, test the recent and local CR source hypothesis, and whether clumps of dark matter have a role in the observed CR observations. The study can lead to developments aiming to a better understanding of the heliosphere, particularly the boundary region with the ISM, and additional constraints on the LISM properties.
arXiv comment7 pages, Letter of Interest for Snowmass 2021
References in corpus (26)
- Propagation of cosmic-ray nucleons in the Galaxy
- Observation of a Large-scale Anisotropy in the Arrival Directions of Cosmic Rays above eV
- Anisotropy and Corotation of Galactic Cosmic Rays
- Discovery of Localized Regions of Excess 10-TeV Cosmic Rays
- Observation of the Anisotropy of 10 TeV Primary Cosmic Ray Nuclei Flux with the Super-Kamiokande-I Detector
- High-energy antiprotons from old supernova remnants
- Measurement of the Anisotropy of Cosmic Ray Arrival Directions with IceCube
- Observation of Anisotropy in the Arrival Directions of Galactic Cosmic Rays at Multiple Angular Scales with IceCube
- Anisotropy in Cosmic-Ray Arrival Directions in the Southern Hemisphere with Six Years of Data from the IceCube Detector
- Three-dimensional Features of the Outer Heliosphere Due to Coupling between the Interstellar and Heliospheric Magnetic Field. V. The Bow Wave, Heliospheric Boundary Layer, Instabilities, and Magnetic Reconnection
- Deciphering the Dipole Anisotropy of Galactic Cosmic Rays
- Magnetic reconnection as the cause of cosmic ray excess from the heliospheric tail
- Solution to the cosmic ray anisotropy problem
- Neutrino Mass and Dark Matter in light of recent AMS-02 results
- The puzzling MILAGRO hot spots
- Solar cycle dependence of the diurnal anisotropy of 0.6 TeV cosmic ray intensity observed with the Matsushiro underground muon detector
- Antiprotons from dark matter annihilation through light mediators and a possible excess in AMS-02 data
- The Southern Wide-Field Gamma-Ray Observatory (SWGO): A Next-Generation Ground-Based Survey Instrument for VHE Gamma-Ray Astronomy
- Modeling the Solar Wind at the Ulysses, Voyager, and New Horizons Spacecraft
- On the spectrum of stable secondary nuclei in cosmic rays
- On the Observation of the Cosmic Ray Anisotropy below 10 eV
- TeV Cosmic-Ray Anisotropy from the Magnetic Field at the Heliospheric Boundary
- The problem of small angular scale structure in the cosmic ray anisotropy data
- Search for anisotropies in cosmic-ray positrons detected by the PAMELA experiment
- Cosmic Rays and Stochastic Magnetic Reconnection in the Heliotail
- Experimental biases on the heliospheric contribution to the observed TeV cosmic ray anisotropy