Cosmic-ray propagation and interactions in the Galaxy

Abstract

We survey the theory and experimental tests for the propagation of cosmic rays in the Galaxy up to energies of 10^15 eV. A guide to the previous reviews and essential literature is given, followed by an exposition of basic principles. The basic ideas of cosmic-ray propagation are described, and the physical origin of its processes are explained. The various techniques for computing the observational consequences of the theory are described and contrasted. These include analytical and numerical techniques. We present the comparison of models with data including direct and indirect - especially gamma-ray - observations, and indicate what we can learn about cosmic-ray propagation. Some particular important topics including electrons and antiparticles are chosen for discussion.

39 pages, 29 figures; Solicited by the Annual Review of Nuclear and Particle Science (v.57), manuscript submitted Jan 2007

References in corpus (8)

• Revised equipartition & minimum energy formula for magnetic field strength estimates from radio synchrotron observations
• Parameterization of Gamma, e^+/- and Neutrino Spectra Produced by p-p Interaction in Astronomical Environment
• Gamma-ray continuum emission from the inner Galactic region as observed with INTEGRAL/SPI
• Cosmic ray production in supernova remnants including reacceleration: the secondary to primary ratio
• Observations of the Li, Be, and B isotopes and constraints on cosmic-ray propagation
• Is the dark matter interpretation of the EGRET gamma excess compatible with antiproton measurements?
• Enhanced Cosmic Ray Flux and Ionization for Star Formation in Molecular Clouds Interacting with Supernova Remnants
• Thermal and non-thermal components of the interstellar medium at sub-kiloparsec scales in galaxies

Cited by in corpus (680)

• Fermi Large Area Telescope Second Source Catalog
• Fermi Large Area Telescope First Source Catalog
• Giant Gamma-ray Bubbles from Fermi-LAT: AGN Activity or Bipolar Galactic Wind?
• PAMELA Measurements of Cosmic-ray Proton and Helium Spectra
• Fermi-LAT Observations of the Diffuse Gamma-Ray Emission: Implications for Cosmic Rays and the Interstellar Medium
• Theoretical Challenges in Galaxy Formation
• A New Model of the Galactic Magnetic Field
• WIMP dark matter candidates and searches - current status and future prospects
• Direct detection of a break in the teraelectronvolt cosmic-ray spectrum of electrons and positrons
• Acceleration of petaelectronvolt protons in the Galactic Centre
• The Characterization of the Gamma-Ray Signal from the Central Milky Way: A Compelling Case for Annihilating Dark Matter
• Background model systematics for the Fermi GeV excess
• Development of the Model of Galactic Interstellar Emission for Standard Point-Source Analysis of Fermi Large Area Telescope Data
• The Fermi Galactic Center GeV Excess and Implications for Dark Matter
• GeV Observations of Star-forming Galaxies with \textit{Fermi} LAT
• Fermi LAT observations of cosmic-ray electrons from 7 GeV to 1 TeV
• TeV Gamma Rays from Geminga and the Origin of the GeV Positron Excess
• The 2HWC HAWC Observatory Gamma Ray Catalog
• Cosmic-Ray Nuclei, Antiprotons and Gamma-rays in the Galaxy: a New Diffusion Model
• Observations of Milky Way Dwarf Spheroidal galaxies with the Fermi-LAT detector and constraints on Dark Matter models
• The 511 keV emission from positron annihilation in the Galaxy
• Teraelectronvolt Astronomy
• The Fermi Haze: A Gamma-Ray Counterpart to the Microwave Haze
• Planck 2015 results. X. Diffuse component separation: Foreground maps
• Measurement of the cosmic-ray proton spectrum from 40 GeV to 100 TeV with the DAMPE satellite
• Global cosmic-ray related luminosity and energy budget of the Milky Way
• GALPROP WebRun: an internet-based service for calculating galactic cosmic ray propagation and associated photon emissions
• On possible interpretations of the high energy electron-positron spectrum measured by the Fermi Large Area Telescope
• Novel dark matter constraints from antiprotons in the light of AMS-02
• New limits on dark matter annihilation from AMS cosmic ray positron data
• Inverse Compton Origin of the Hard X-Ray and Soft Gamma-Ray Emission from the Galactic Ridge
• Possible dark matter annihilation signal in the AMS-02 antiproton data
• Measurements of cosmic-ray secondary nuclei at high energies with the first flight of the CREAM balloon-borne experiment
• Fermi observations of Cassiopeia and Cepheus: diffuse gamma-ray emission in the outer Galaxy
• Launching cosmic-ray-driven outflows from the magnetized interstellar medium
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Galactic Foreground Emission
• The Fermi Bubbles. I. Possible Evidence for Recent AGN Jet Activity in the Galaxy
• The origin of Galactic cosmic rays: challenges to the standard paradigm
• Pulsars versus Dark Matter Interpretation of ATIC/PAMELA
• GeV-Scale Thermal WIMPs: Not Even Slightly Dead
• The interstellar cosmic-ray electron spectrum from synchrotron radiation and direct measurements
• But What About... Cosmic Rays, Magnetic Fields, Conduction, & Viscosity in Galaxy Formation
• Dark Matter Candidates: A Ten-Point Test
• CRDB: a database of charged cosmic rays
• Spectrum of Galactic Cosmic Rays Accelerated in Supernova Remnants
• Production and evolution of Li, Be and B isotopes in the Galaxy
• DarkSUSY 6 : An Advanced Tool to Compute Dark Matter Properties Numerically
• The Large Scale Cosmic-Ray Anisotropy as Observed with Milagro
• Galactic electrons and positrons at the Earth:new estimate of the primary and secondary fluxes
• Fermi Large Area Telescope Measurements of the Diffuse Gamma-Ray Emission at Intermediate Galactic Latitudes
• Bayesian analysis of cosmic-ray propagation: evidence against homogeneous diffusion
• Galactic synchrotron emission with cosmic ray propagation models
• A Measurement of the Spatial Distribution of Diffuse TeV Gamma Ray Emission from the Galactic Plane with Milagro
• Dark Matter and Pulsar Origins of the Rising Cosmic Ray Positron Fraction in Light of New Data From AMS
• Implications of High-Resolution Simulations on Indirect Dark Matter Searches
• High-energy antiprotons from old supernova remnants
• Pre-launch estimates for GLAST sensitivity to Dark Matter annihilation signals
• Cosmic ray feedback in the FIRE simulations: constraining cosmic ray propagation with GeV gamma ray emission
• Limits on Dark Matter Annihilation Signals from the Fermi LAT 4-year Measurement of the Isotropic Gamma-Ray Background
• The exceptionally powerful TeV gamma-ray emitters in the Large Magellanic Cloud
• Solution of heliospheric propagation: unveiling the local interstellar spectra of cosmic ray species
• Cooler and smoother -- the impact of cosmic rays on the phase structure of galactic outflows
• Implications of CoGeNT and DAMA for Light WIMP Dark Matter
• A Precision Search for WIMPs with Charged Cosmic Rays
• Magnetohydrodynamic Simulations of Disk Galaxy Formation: the Magnetization of The Cold and Warm Medium
• The Fermi Bubbles: Supersonic AGN Jets with Anisotropic Cosmic Ray Diffusion
• On cosmic ray acceleration in supernova remnants and the FERMI/PAMELA data
• Galactic cosmic rays after the AMS-02 observations
• Inverse Compton constraints on the Dark Matter e+e- excesses
• Model-Independent Indirect Detection Constraints on Hidden Sector Dark Matter
• Dark Matter Searches with Astroparticle Data
• Evolution of the cosmic ray anisotropy above 10^{14} eV
• Impact of Cosmic Ray Transport on Galactic Winds
• A Markov Chain Monte Carlo technique to sample transport and source parameters of Galactic cosmic rays: II. Results for the diffusion model combining B/C and radioactive nuclei
• High Energy Positrons From Annihilating Dark Matter
• Extended Very-High-Energy Gamma-Ray Emission Surrounding PSR J0622 + 3749 Observed by LHAASO-KM2A
• A non-ideal MHD Gadget: Simulating massive galaxy clusters
• PICARD: A novel code for the Galactic Cosmic Ray propagation problem
• Global galactic dynamo driven by cosmic-rays and exploding magnetized stars
• Modelling the Galactic Magnetic Field on the Plane in 2D
• Cosmic rays can drive strong outflows from gas-rich high-redshift disk galaxies
• Reverse Direct Detection: Cosmic Ray Scattering With Light Dark Matter
• Five-Year Wilkinson Microwave Anisotropy Probe (WMAP) Observations: Bayesian Estimation of CMB Polarization Maps
• Absorption of Very High Energy Gamma Rays in the Milky Way
• Propagation of cosmic rays in the AMS-02 era
• INTEGRAL SPI All-Sky View in Soft Gamma Rays: Study of Point Source and Galactic Diffuse Emissions
• Unified interpretation of cosmic-ray nuclei and antiproton recent measurements
• Magnetohydrodynamic-Particle-in-Cell Method for Coupling Cosmic Rays with a Thermal Plasma: Application to Non-relativistic Shocks
• High-Energy Gamma Rays from the Milky Way: Three-Dimensional Spatial Models for the Cosmic-Ray and Radiation Field Densities in the Interstellar Medium
• Multi-wavelength signals of dark matter annihilations at the Galactic center
• The Galactic Center GeV Excess from a Series of Leptonic Cosmic-Ray Outbursts
• Connecting Far-Infrared and Radio Morphologies of Disk Galaxies: Cosmic-Ray Electron Diffusion After Star Formation Episodes
• Scrutinizing the evidence for dark matter in cosmic-ray antiprotons
• Current status and desired accuracy of the isotopic production cross sections relevant to astrophysics of cosmic rays I. Li, Be, B, C, N
• A Hitch-hiker's Guide to Stochastic Differential Equations: Solution Methods for Energetic Particle Transport in Space Physics and Astrophysics
• Nonthermal particles and photons in starburst regions and superbubbles
• SILCC VI -- Multi-phase ISM structure, stellar clustering, and outflows with supernovae, stellar winds, ionising radiation and cosmic rays
• Spectra of Cosmic Ray Protons and Helium Produced in Supernova Remnants
• Constraints on the Cosmic-Ray Density Gradient beyond the Solar Circle from Fermi gamma-ray Observations of the Third Galactic Quadrant
• The Implications of a High Cosmic-Ray Ionization Rate in Diffuse Interstellar Clouds
• A revised catalogue of EGRET gamma-ray sources
• Signatures of a two million year old supernova in the spectra of cosmic ray protons, antiprotons and positrons
• Indirect Searches for Decaying Dark Matter
• Inference of the Local Interstellar Spectra of Cosmic Ray Nuclei Z<=28 with the GalProp-HelMod Framework
• Testing Physical Models for Cosmic Ray Transport Coefficients on Galactic Scales: Self-Confinement and Extrinsic Turbulence at GeV Energies
• The nature of the low-frequency emission of M51: First observations of a nearby galaxy with LOFAR
• Non-linear diffusion of cosmic rays escaping from supernova remnants - I. The effect of neutrals
• Bayesian analysis of spatial-dependent cosmic-ray propagation: astrophysical background of antiprotons and positrons
• Planck 2015 results. XXV. Diffuse low-frequency Galactic foregrounds
• Beyond the myth of the supernova-remnant origin of cosmic rays
• Imprints of Cosmic Rays in Multifrequency Observations of the Interstellar Emission
• Pulsar wind nebulae with bow shocks: non-thermal radiation and cosmic ray leptons
• Cosmic Ray Electrons, Positrons and the Synchrotron emission of the Galaxy: consistent analysis and implications
• Components of the Extragalactic Gamma Ray Background
• Diffuse emission measurement with INTEGRAL/SPI as indirect probe of cosmic-ray electrons and positrons
• Gamma rays from molecular clouds illuminated by accumulated diffusive protons from supernova remnant W28
• Cosmic-ray protons, nuclei, electrons, and antiparticles under a two-halo scenario of diffusive propagation
• $e^{\pm }$ Excesses in the Cosmic Ray Spectrum and Possible Interpretations
• Detection of spectral hardenings in cosmic-ray boron-to-carbon and boron-to-oxygen flux ratios with DAMPE
• High Energy Positrons and the WMAP Haze from Exciting Dark Matter
• Quantitative study of the AMS-02 electron/positron spectra: implications for the pulsar and dark matter properties
• Time-resolved hadronic particle acceleration in the recurrent Nova RS Ophiuchi
• New very local interstellar spectra for electrons, positrons, protons and light cosmic ray nuclei
• Magnetic Fields in the Milky Way
• Polarised radio filaments outside the Galactic plane
• Constraints on dark matter annihilation from AMS-02 results
• Molecular Clouds as a Probe of Cosmic-Ray Acceleration in a Supernova Remnant
• A common solution to the cosmic ray anisotropy and gradient problems
• Ultra-High-Energy Cosmic Rays: The Intersection of the Cosmic and Energy Frontiers
• Detection of the Small Magellanic Cloud in gamma-rays with Fermi/LAT
• The dependence of cosmic ray driven galactic winds on halo mass
• Constraints on Decaying Dark Matter from the Isotropic Gamma-Ray Background
• Statistics of gamma-ray point sources below the Fermi detection limit
• Anisotropic CR diffusion and gamma-ray production close to supernova remnants, with an application to W28
• An Ultrahigh-energy $\gamma$-ray Bubble Powered by a Super PeVatron
• Spectral analysis and interpretation of the γ-ray emission from the Starburst galaxy NGC 253
• Systematic Investigation of Solar Modulation of Galactic Protons for Solar Cycle 23 using a Monte Carlo Approach with Particle Drift Effects and Latitudinal Dependence
• Is the PAMELA Positron Excess Winos?
• The Fermi Bubbles. II. The Potential Roles of Viscosity and Cosmic Ray Diffusion in Jet Models
• What Does The PAMELA Antiproton Spectrum Tell Us About Dark Matter?
• Cosmic ray driven dynamo in galactic disks. A parameter study
• Propagation of Cosmic Rays in Heliosphere: the HelMod Model
• New calculation of antiproton production by cosmic ray protons and nuclei
• Particle Transport in Young Pulsar Wind Nebulae
• Physical Processes in Star Formation
• Positron transport in the interstellar medium
• AMS-02 Antiprotons Reloaded
• Origin of Small-Scale Anisotropies in Galactic Cosmic Rays
• Positron flux and gamma-ray emission from Geminga pulsar and pulsar wind nebula
• Radio haloes in nearby galaxies modelled with 1D cosmic-ray transport using SPINNAKER
• Cosmic Rays from Leptophilic Dark Matter Decay via Kinetic Mixing
• IMAGINE: A comprehensive view of the interstellar medium, Galactic magnetic fields and cosmic rays
• Nuclear-Astrophysics Lessons from INTEGRAL
• Circum-Galactic Gas and the Isotropic Gamma Ray Background
• Dark matter and pulsar signals for Fermi LAT, PAMELA, ATIC, HESS and WMAP data
• Propagation of galactic cosmic rays in the presence of self-generated turbulence
• Measurements of Cosmic-Ray Hydrogen and Helium Isotopes with the PAMELA experiment
• AMS-02 positron excess: new bounds on dark matter models and hint for primary electron spectrum hardening
• Cosmic ray feedback from supernovae in dwarf galaxies
• Multi-scale Radio-IR Correlations in M31 and M33: The Role of Magnetic Fields and Star Formation
• Dark Matter Sees The Light
• Nuclear astrophysics: the unfinished quest for the origin of the elements
• Understanding the spectral hardenings and radial distribution of Galactic cosmic rays and Fermi diffuse gamma-rays with spatially-dependent propagation
• New constraints on modelling the random magnetic field of the MW
• The Fermi Bubbles: Gamma-ray, Microwave, and Polarization Signatures of Leptonic AGN Jets
• Diffuse gamma-ray emission in the vicinity of young star cluster Westerlund 2
• The Three-Dimensional Spatial Distribution of Interstellar Gas in the Milky Way: Implications for Cosmic Rays and High-Energy Gamma-Ray Emissions
• Ultrahigh-energy Cosmic-ray Nuclei from Black Hole Jets: Recycling Galactic Cosmic Rays through Shear Acceleration
• Implications of the AMS-02 positron fraction in cosmic rays
• Galactic cosmic-ray propagation in the light of AMS-02: I. Analysis of protons, helium, and antiprotons
• Deciphering the local Interstellar spectra of secondary nuclei with GALPROP/HelMod framework and a hint for primary lithium in cosmic rays
• Neutron monitors and muon detectors for solar modulation studies: 2. $\varphi$ time series
• Constraining the properties of the magnetic turbulence in the Geminga region using HAWC $\gamma$-ray data
• Gamma-rays from molecular clouds illuminated by accumulated diffusive protons. II: interacting supernova remnants
• Reconciling cosmic ray diffusion with Galactic magnetic field models
• Constraining models of the large scale Galactic magnetic field with WMAP5 polarization data and extragalactic Rotation Measure sources
• Gamma-ray halos around pulsars as the key to understanding cosmic ray transport in the Galaxy
• Constraining Galactic cosmic-ray parameters with Z<=2 nuclei
• Parameterizing the interstellar dust temperature
• Gauged $U(1{)}_{L_{\mu }-L_{\tau }}$ model in light of muon $g-2$ anomaly, neutrino mass and dark matter phenomenology
• Global diffusion of cosmic rays
• Probing Cosmic Rays in Nearby Giant Molecular Clouds with the Fermi Large Area Telescope
• Ultrahard spectra of PeV neutrinos from supernovae in compact star clusters
• Cosmic-Ray Propagation in Light of Recent Observation of Geminga
• Isotopic Composition of Light Nuclei in Cosmic Rays: Results from AMS-01
• Theoretical uncertainties in extracting cosmic-ray diffusion parameters: the boron-to-carbon ratio
• Observing a column-dependent zeta in dense interstellar sources: the case of the Horsehead Nebula
• Extracting limits on Dark Matter annihilation from gamma-ray observations towards dwarf spheroidal galaxies
• Anisotropic diffusion of galactic cosmic ray protons and their steady-state azimuthal distribution
• Production and attenuation of cosmic-ray boosted dark matter
• The suppression of direct collapse black hole formation by soft X-ray irradiation
• Connecting Synchrotron, Cosmic Rays, and Magnetic Fields in the Plane of the Galaxy
• On the Energy Spectra of GeV/TeV Cosmic Ray Leptons
• Cosmic-ray Antinuclei as Messengers of New Physics: Status and Outlook for the New Decade
• Penetration of cosmic rays into dense molecular clouds: role of diffuse envelope
• A Markov Chain Monte Carlo for Galactic Cosmic Ray physics: I. Method and results for the Leaky Box Model
• How cosmic-ray electron propagation affects radio-far-infrared correlations in M31 and M33
• The Star-Forming Galaxy Contribution to the Cosmic MeV and GeV Gamma-Ray Background
• Deciphering Contributions to the Extragalactic Gamma-Ray Background from 2 GeV to 2 TeV
• The origin of the spectral intensities of cosmic-ray positrons
• A signature of anisotropic cosmic-ray transport in the gamma-ray sky
• The cosmic-ray and gas content of the Cygnus region as measured in gamma rays by the Fermi Large Area Telescope
• Advective and diffusive cosmic ray transport in galactic haloes
• Acceleration and transport of relativistic electrons in the jets of the microquasar SS 433
• Synchrotron Spectral Curvature from 22 MHz to 23 GHz
• Diffuse Hard X-ray Emission in Starburst Galaxies as Synchrotron from Very High Energy Electrons
• Cosmic Ray Models
• USINE: semi-analytical models for Galactic cosmic-ray propagation
• Deciphering the local Interstellar spectra of primary cosmic ray species with HelMod
• Radio data and synchrotron emission in consistent cosmic ray models
• Hint for a TeV neutrino emission from the Galactic Ridge with ANTARES
• Numerical propagation of high energy cosmic rays in the Galaxy I: technical issues
• Secondary antiprotons as a Galactic Dark Matter probe
• HelMod in the works: from direct observations to the local interstellar spectrum of cosmic-ray electrons
• First Predicted Cosmic Ray Spectra, Primary-to-Secondary Ratios, and Ionization Rates from MHD Galaxy Formation Simulations
• Acceleration and Escape Processes of High-energy Particles in Turbulence inside Hot Accretion Flows
• WIMP searches with gamma rays in the Fermi era: challenges, methods and results
• Measuring the tensor to scalar ratio from CMB B-modes in presence of foregrounds
• Unified model for the gamma-ray emission of supernova remnants
• SILCC VII -- Gas kinematics and multiphase outflows of the simulated ISM at high gas surface densities
• Standard Self-Confinement and Extrinsic Turbulence Models for Cosmic Ray Transport are Fundamentally Incompatible with Observations
• Solar and nuclear physics uncertainties in cosmic-ray propagation
• New local interstellar spectra for protons, Helium and Carbon derived from PAMELA and Voyager 1 observations
• Detecting Gamma-Ray Anisotropies from Decaying Dark Matter: Prospects for Fermi LAT
• Excesses of Cosmic Ray Spectra from A Single Nearby Source
• An implicit scheme for solving the anisotropic diffusion of heat and cosmic rays in the RAMSES code
• Photodissociation Region Diagnostics Across Galactic Environments
• Implications of current nuclear cross sections on secondary cosmic rays with the upcoming DRAGON2 code
• Deriving the cosmic ray spectrum from gamma-ray observations
• Particle acceleration by supernova shocks and spallogenic nucleosynthesis of light elements
• Cosmic ray signatures of a 2-3 Myr old local supernova
• CHANG-ES VI: Probing Supernova Energy Deposition in Spiral Galaxies Through Multi-Wavelength Relationships
• The Connection Between the Positron Fraction Anomaly and the Spectral Features in Galactic Cosmic-Ray Hadrons
• Are Starburst Galaxies Proton Calorimeters?
• Implications of Lithium to Oxygen AMS-02 spectra on our understanding of cosmic-ray diffusion
• Cosmic rays and non-thermal emission in simulated galaxies. II. $\gamma$-ray maps, spectra and the far infrared-$\gamma$-ray relation
• The impact of Galactic synchrotron emission on CMB anisotropy measurements. I. Angular power spectrum analysis of total intensity all-sky surveys
• CHAMP Cosmic Rays
• Ab initio Simulations of a Supernova Driven Galactic Dynamo in an Isolated Disk Galaxy
• CosRayMC: a global fitting method in studying the properties of the new sources of cosmic e${}^{\pm }$ excesses
• Test particle simulations of cosmic rays
• Low energy cosmic rays
• The Astrochemical Impact of Cosmic Rays in Protoclusters I: Molecular Cloud Chemistry
• ATIC, PAMELA, HESS, Fermi and nearby Dark Matter subhalos
• Cosmic rays in galactic and extragalactic magnetic fields
• Does the Geminga, Monogem and PSR J0622+3749 $\gamma$-ray halos imply slow diffusion around pulsars?
• Limits on Sub-GeV Dark Matter from the PROSPECT Reactor Antineutrino Experiment
• p, He, and C to Fe cosmic-ray primary fluxes in diffusion models: Source and transport signatures on fluxes and ratios
• A Fixed-Target Programme at the LHC: Physics Case and Projected Performances for Heavy-Ion, Hadron, Spin and Astroparticle Studies
• Indication of nearby source signatures of cosmic rays from energy spectra and anisotropies
• Radiation-MagnetoHydrodynamics simulations of cosmic ray feedback in disc galaxies
• Acceleration of cosmic rays and gamma-ray emission from supernova remnants in the Galaxy
• Gamma rays as probes of cosmic-ray propagation and interactions in galaxies
• Fermi-LAT Observations of High- and Intermediate-Velocity Clouds: Tracing Cosmic Rays in the Halo of the Milky Way
• Determination of the Cosmic Antideuteron Flux in a Monte Carlo approach
• Spectral Intensities of Antiprotons and the lifetime of Cosmic Rays in the Galaxy
• Fermi-LAT Observations of Gamma-Ray Emission Towards the Outer Halo of M31
• The Spatially Uniform Spectrum of the Fermi Bubbles: the Leptonic AGN Jet Scenario
• Relative distribution of cosmic rays and magnetic fields
• Evidence of Fermi bubbles around M31
• CHANG-ES XIII: Transport processes and the magnetic fields of NGC 4666 - indication of a reversing disk magnetic field
• Revisiting Spatial-Dependent Propagation Model with Latest Observations of Cosmic Ray Nuclei
• Cosmic-ray propagation in the bi-stable interstellar medium. I. Conditions for cosmic-ray trapping
• What can we really learn from positron flux 'anomalies'?
• Spiral Arms as Cosmic Ray Source Distributions
• The Positron Puzzle
• Cosmic rays and non-thermal emission in simulated galaxies. I. Electron and proton spectra compared to Voyager-1 data
• New constraints on the primordial black hole number density from Galactic gamma-ray astronomy
• Propagation in 3D spiral-arm cosmic-ray source distribution models and secondary particle production using PICARD
• Cosmic-Ray Transport in Simulations of Star-forming Galactic Disks
• Direct constraints on diffusion models from cosmic-ray positron data: Excluding the Minimal model for dark matter searches
• The theory of cosmic-ray scattering on pre-existing MHD modes meets data
• Secondary Cosmic Ray Nuclei from Supernova Remnants and Constraints to the Propagation Parameters
• Probing magnetic turbulence by synchrotron polarimetry: statistics and structure of magnetic fields from Stokes correlators
• General Analysis of Antideuteron Searches for Dark Matter
• Search for Cosmic-ray Boosted Sub-GeV Dark Matter using Recoil Protons at Super-Kamiokande
• On prospects for dark matter indirect detection in the Constrained MSSM
• Filamentary Diffusion of Cosmic Rays on Small Scales
• Investigating the dark matter signal in the cosmic ray antiproton flux with the machine learning method
• Robust cosmic-ray constraints on $p$-wave annihilating MeV dark matter
• Millicharged Cosmic Rays and Low Recoil Detectors
• Possible Evidence for the Stochastic Acceleration of Secondary Antiprotons by Supernova Remnants
• CHANG-ES XVI: An in-depth view of the cosmic-ray transport in the edge-on spiral galaxies NGC 891 and NGC 4565
• Simulations of cosmic ray propagation
• Cosmic-Ray Transport in Varying Galactic Environments
• The isotropic radio background revisited
• Les Houches Lectures on Indirect Detection of Dark Matter
• The Fermi Gamma-Ray Haze from Dark Matter Annihilations and Anisotropic Diffusion
• GeV-TeV Cosmic Ray Leptons in the Solar System from the Bow Shock Wind Nebula of the Nearest Millisecond Pulsar J0437-4715
• Production of secondary particles and nuclei in cosmic rays collisions with the interstellar gas using the FLUKA code
• Updated Constraints on Primordial Black Hole Evaporation
• Anisotropic Cosmic Ray Diffusion and its Implications for Gamma-Ray Astronomy
• Planck intermediate results. XLII. Large-scale Galactic magnetic fields
• Global simulations of the magnetic field evolution under the influence of the cosmic-ray-driven dynamo
• Tracing the sources of cosmic rays with molecular ions
• Propagation of H and He cosmic ray isotopes in the Galaxy: astrophysical and nuclear uncertainties
• Fermi-LAT observations of the Sagittarius B complex
• Do Cosmic Rays Heat the Early Intergalactic Medium?
• Constraining Supersymmetric Dark Matter With Synchrotron Measurements
• A local fading accelerator and the origin of TeV cosmic ray electrons
• Pinpointing Cosmic Ray Propagation With The AMS-02 Experiment
• A cosmic-ray precursor model for a Balmer-dominated shock in Tycho's supernova remnant
• Properties of the Magneto-ionic Medium in the Halo of M51 revealed by Wide-band Polarimetry
• LikeDM: likelihood calculator of dark matter detection
• A possible approach to three-dimensional cosmic-ray propagation in the Galaxy IV. Electrons and electron-induced gamma-rays
• Implications on cosmic ray injection and propagation parameters from Voyager/ACE/AMS-02 nucleus data
• Parameterization of the Angular Distribution of Gamma Rays Produced by p-p Interaction in Astronomical Environment
• Probing Cosmic-Ray Accelerated Light Dark Matter with IceCube
• Calibrating the relation of low-frequency radio continuum to star formation rate at 1 kpc scale with LOFAR
• Implementation of CR Energy SPectrum (CRESP) algorithm in PIERNIK MHD code. I. Spectrally resolved propagation of CR electrons on Eulerian grids
• New minimal, median, and maximal propagation models for dark matter searches with Galactic cosmic rays
• Characterizing Cosmic-Ray Propagation in Massive Star-Forming Regions: The Case of 30 Doradus and the Large Magellanic Cloud
• A Multi-Wavelength Analysis of Annihilating Dark Matter as the Origin of the Gamma-Ray Emission from M31
• A new nearby pulsar wind nebula overlapping the RX J0852.0-4622 supernova remnant
• The gamma-ray / infrared luminosity correlation of star-forming galaxies
• H.E.S.S. and Suzaku observations of the Vela X pulsar wind nebula
• On the origin of matter in the Universe
• Cosmic Ray Acceleration by a Versatile Family of Galactic Wind Termination Shocks
• The Elemental Composition of High-Energy Cosmic Rays: Measurements with TRACER
• Anisotropies of different mass compositions of cosmic rays
• On the progressive hardening of the cosmic-ray proton spectrum in the inner Galaxy
• Secondary cosmic-ray nucleus spectra disfavor particle transport in the Galaxy without reacceleration
• Primordial magnetic field generation via primordial black hole disks
• The radio continuum perspective on cosmic-ray transport in external galaxies
• Source detection using a 3D sparse representation: application to the Fermi gamma-ray space telescope
• New Constraints from PAMELA anti-proton data on Annihilating and Decaying Dark Matter
• Cosmic ray spectrum of protons plus helium nuclei between 6 TeV and 158 TeV from HAWC data
• Eight-channel reconfigurable microring filters with tunable frequency, extinction ratio and bandwidth
• Foreground Analysis Using Cross-Correlations of External Templates on the 7-year WMAP data
• Cosmic-ray antiproton constraints on light singlino-like dark matter candidates
• Measurement of the cosmic ray antiproton/proton flux ratio at TeV energies with the ARGO-YBJ detector
• Turbulent diffusion of streaming cosmic rays in compressible, partially ionised plasma
• Hard and bright gamma-ray emission at the base of the Fermi bubbles
• CHANG-ES XXVI: Insights into cosmic-ray transport from radio halos in edge-on galaxies
• Examination of uncertainties in nuclear data for cosmic ray physics with the AMS experiment
• A systematic study on the cosmic ray antiproton flux
• Photon, Neutrino and Charged Particle Spectra from R-violating Gravitino Decays
• Measurement of the low-energy antideuteron inelastic cross section
• On the small scale turbulent dynamo in the intracluster medium: A comparison to dynamo theory
• Where are Milky Way's Hadronic PeVatrons?
• Radio spectra and sizes of ALMA-identified submillimetre galaxies: evidence of age-related spectral curvature and cosmic ray diffusion?
• Testing the Dark Matter Interpretation of the PAMELA Excess through Measurements of the Galactic Diffuse Emission
• Deciphering the Origin of the GeV--TeV Gamma-ray Emission from SS 433
• Galactic cosmic-ray model in the light of AMS-02 nuclei data
• The `excess' of primary cosmic ray electrons
• Modelling the cosmic ray electron propagation in M 51
• Supernova explosions of massive stars and cosmic rays
• 3-D Model of Broadband Emission from Supernova Remnants Undergoing Non-linear Diffusive Shock Acceleration
• Ultra-High Energy Probes of Classicalization
• Giant cosmic ray halos around M31 and the Milky Way
• Observational signatures of cosmic ray interactions in molecular clouds
• Grammage of cosmic rays in the proximity of supernova remnants embedded in a partially ionized medium
• Galactic annihilation emission from nucleosynthesis positrons
• Supernovae in compact star clusters as sources of high-energy cosmic rays and neutrinos
• Anisotropic diffusion cannot explain TeV halo observations
• Testing the universality of cosmic-ray nuclei from protons to oxygen with AMS-02
• Cosmic antihelium-3 nuclei sensitivity of the GAPS experiment
• Interpretations of the cosmic ray secondary-to-primary ratios measured by DAMPE
• Milky Way as a Neutrino Desert Revealed by IceCube Galactic Plane Observation
• Probing the Cosmic Ray density in the inner Galaxy
• Dark Matter Search in Space: Combined Analysis of Cosmic Ray Antiproton-to-Proton Flux Ratio and Positron Flux Measured by AMS-02
• A Genetic Algorithm for Astroparticle Physics Studies
• SKA-Phase 1 sensitivity for synchrotron radio emission from multi-TeV Dark Matter candidates
• The Morphology of the Galactic Dark Matter Synchrotron Emission with Self-Consistent Cosmic Ray Diffusion Models
• Constraining the regular Galactic Magnetic Field with the 5-year WMAP polarization measurements at 22 GHz
• Galactic magnetic fields and the large-scale anisotropy at MILAGRO
• A simple determination of the halo size $L$ from ${}^{10}$Be/${}^9$Be data
• Deciphering the radio-star formation correlation on kpc-scales I. Adaptive kernel smoothing experiments
• Azimuthal asymmetry in cosmic-ray boosted dark matter flux
• Spectral index of synchrotron emission: insights from the diffuse and magnetised interstellar medium
• Impact on the tensor-to-scalar ratio of incorrect Galactic foreground modelling
• Super-Knee Cosmic Rays from Galactic Neutron Star Merger Remnants
• Walk on the Low Side: LOFAR explores the low-frequency radio emission of GASP jellyfish galaxies
• Fermi Gamma-ray Haze via Dark Matter and Millisecond Pulsars
• Spectral softening in core-collapse supernova remnant expanding inside wind-blown bubble
• Panglossian Prospects for Detecting Neutralino Dark Matter in Light of Natural Priors
• 3D global simulations of a cosmic-ray-driven dynamo in dwarf galaxies
• Starburst and post-starburst high-redshift protogalaxies: The feedback impact of high energy cosmic rays
• Evidence for Cosmic-Ray Escape in the Small Magellanic Cloud using Fermi Gamma-rays
• Towards First-principle Characterization of Cosmic-ray Transport Coefficients from Multi-scale Kinetic Simulations
• Cosmic Ray production of Beryllium and Boron at high redshift
• AMS-02 Positron Excess and Indirect Detection of Three-body Decaying Dark Matter
• 3D magneto-hydrodynamic models of non-thermal photon emission in the binary system ${\gamma }^2$ Velorum
• Stochasticity of Cosmic Rays from Supernova Remnants and the Ionization Rates in Molecular Clouds
• Revisit cosmic ray propagation by using ${}^1$H, ${}^2$H, ${}^3$He and ${}^4$He
• The Propagation of Cosmic Rays from the Galactic Wind Termination Shock: Back to the Galaxy?
• The magnetized galactic wind and synchrotron halo of the starburst dwarf galaxy IC10
• Possible Breaking of the FIR-Radio Correlation in Tidally Interacting Galaxies
• Recovering the observed B/C ratio in a dynamic spiral-armed cosmic ray model
• Deciphering Residual Emissions: Time-Dependent Models for the Non-Thermal Interstellar Radiation from the Milky Way
• Astrophysical Uncertainties in the Cosmic Ray Electron and Positron Spectrum From Annihilating Dark Matter
• Interstellar gamma-ray emission from cosmic rays in star-forming galaxies
• Antiproton Limits on Decaying Gravitino Dark Matter
• A local interstellar spectrum for galactic electrons
• Limits on the Dark Matter from AMS-02 antiproton and positron fraction data
• Diffuse Galactic Gamma Rays at intermediate and high latitudes. I. Constraints on the ISM properties
• Systematic effects in the extraction of the 'WMAP haze'
• Cosmic Rays and Magnetic Fields in the Core and Halo of the Starburst M82: Implications for Galactic Wind Physics
• Cosmic ray electron anisotropies as a tool to discriminate between exotic and astrophysical sources
• Cosmic ray $e^{+}{e}^{-}$ spectrum excess and peak feature observed by the DAMPE experiment from dark matter
• IceCube Constraints on Fast-Spinning Pulsars as High-Energy Neutrino Sources
• The Earth-like Galactic cosmic ray intensity in the habitable zone of the M dwarf GJ 436
• Exploring A Cosmic-Ray Origin of the Multi-wavelength Emission in M31
• Constraining the halo size from possible density profiles of hydrogen gas of Milky Way Galaxy
• Constraining dark matter annihilation with cosmic ray antiprotons using neural networks
• Pulsar interpretation of the lepton spectra measured by AMS-02
• Reevaluation of the cosmic antideuteron flux from cosmic-ray interactions and from exotic sources
• The impact of propagation uncertainties on the potential Dark Matter contribution to the Fermi LAT mid-latitude gamma-ray data
• Sensitivity of the GAPS Experiment to Low-energy Cosmic-ray Antiprotons
• StellarICS: Inverse Compton Emission from the Quiet Sun and Stars from keV to TeV
• Novel interpretation of the latest AMS-02 cosmic-ray electron spectrum
• Recent results in nuclear astrophysics
• Cherenkov Telescope Array sensitivity to the putative millisecond pulsar population responsible for the Galactic center excess
• A novel prediction for secondary positrons and electrons in the Galaxy
• The Electron Injection Spectrum Determined by Anomalous Excesses in Cosmic Ray, Gamma Ray, and Microwave Signals
• Gamma-ray signatures of annihilation to charged leptons in dark matter substructure
• Cosmic-ray antiprotons in the AMS-02 era: A sensitive probe of dark matter
• Mirror diffusion of cosmic rays in highly compressible turbulence near supernova remnants
• Universal profiles for radio searches of dark matter in dwarf galaxies
• Correction Method for the Readout Saturation of the DAMPE Calorimeter
• Prospects of detecting dark matter through cosmic-ray antihelium with the antiproton constraints
• Supernova remnants in the very-high-energy gamma-ray domain: the role of the Cherenkov telescope array
• Characterising the signatures of star-forming galaxies in the extra-galactic $\gamma$-ray background
• Multi-wavelength Searches for Particle Dark Matter
• Imprints of magnetic power and helicity spectra on radio polarimetry statistics
• The First Stars: formation under cosmic ray feedback
• Astrophysical Implications of a Visible Dark Matter Sector from a Custodially Warped-GUT
• Outflow and Emission Model of Pulsar Wind Nebulae with the Back-reaction of Particle Diffusion
• Chemical Composition of Galactic Cosmic Rays with Space Experiments
• Fermi-LAT gamma-ray study of the interstellar medium and cosmic rays in the Chamaeleon Molecular-Cloud Complex: A look at the dark gas as optically thick HI
• Cosmic ray propagation and interactions in the Galaxy
• Implications of a possible TeV break in the cosmic-ray electron and positron flux
• Upper Limits on Very-High-Energy Gamma-ray Emission from Core-Collapse Supernovae Observed with H.E.S.S
• Implications on Spatial Models of Interstellar Gamma-Ray Inverse-Compton Emission from Synchrotron Emission Studies in Radio and Microwaves
• Ultrahigh-energy diffuse gamma-ray emission from cosmic-ray interactions with medium surrounding acceleration sources
• On the knee of Galactic cosmic rays in light of sub-TeV spectral hardenings
• Modeling of GeV-TeV gamma-ray emission of Cygnus Cocoon
• A general study of decaying scalar dark matter: existing limits and projected radio signals at the SKA
• Wavelet-Based Techniques for the Gamma-Ray Sky
• Spectra of Cosmic Ray Sodium and Aluminum and Unexpected Aluminum Excess
• Predictions of a Natural SUSY Dark Matter Model for Direct and Indirect Detection Experiments
• Inverse Compton emission from millisecond pulsars in the Galactic bulge
• Heating of the Warm Ionized Medium by Low-Energy Cosmic Rays
• Relic density and PAMELA events in a heavy wino dark matter model with Sommerfeld effect
• The impact of a young radio galaxy: clues from the cosmic-ray electron population
• Cosmic ray propagation time scales: lessons from radioactive nuclei and positron data
• Turbulent Reacceleration of Streaming Cosmic Rays
• Abundance ratios of OH/CO and HCO+/CO as probes of the cosmic ray ionization rate in diffuse clouds
• Cosmic Ray Interstellar Propagation Tool using Itô Calculus (criptic): software for simultaneous calculation of cosmic ray transport and observational signatures
• A radiative transfer model for the spiral galaxy M33
• Bayesian analysis of the hardening in AMS-02 nuclei spectra
• Electron and positron spectra in the three dimensional spatial-dependent propagation model
• Prospects for a survey of the Galactic plane with the Cherenkov Telescope Array
• Testing the Dark Matter Annihilation Model for the WMAP Haze
• The angular momentum structure of cosmic ray driven galactic outflows triggered by stream accretion
• Understanding the phase reversals of Galactic cosmic ray anisotropies
• Contribution of the Galactic center to the local cosmic-ray flux
• Muonphilic Dark Matter explanation of gamma-ray galactic center excess: a comprehensive analysis
• Steepening of Cosmic Ray Spectra in Shocks with Varying Magnetic Field Direction
• Correlation of the radio continuum, infrared, and CO molecular emissions in NGC 3627
• Foreground Bias From Parametric Models of Far-IR Dust Emission
• Two Numerical Methods for the 3D Anisotropic Propagation of Galactic Cosmic Rays
• Warped diffusive radio halo around the quiescent spiral edge-on galaxy NGC 4565
• The Effect of Cosmic Rays on the Observational Properties of the CGM
• A self-consistent model of cosmic-ray fluxes and positron excess: Roles of nearby pulsars and a sub-dominant source population
• Cosmic Ray Anomalies from the MSSM?
• Determining the Spectrum of Cosmic Rays in Interstellar Space from the Diffuse Galactic Gamma-Ray Emissivity
• The B/C and sub-Iron/Iron Cosmic ray ratios - further evidence in favor of the spiral arm diffusion model
• A High-Resolution Radio Continuum Study Of The Dwarf Irregular Galaxy IC 10
• Ultrahigh-energy Gamma Rays and Gravitational Waves from Primordial Exotic Stellar Bubbles
• Positron Excess from Cosmic Ray Interactions in Galactic Molecular Clouds
• Unexpected cyclic behavior in cosmic ray protons observed by PAMELA at 1 AU
• Can the Production Cross-Section Uncertainties Explain the Cosmic Fluorine Anomaly?
• New Constraints on Cosmic Particle Populations at the Galactic Center using X-ray Observations of the Molecular Cloud Sagittarius B2
• Nuclear de-excitation lines as a probe of low-energy cosmic rays
• Diffusion of cosmic-ray electrons in M 51 observed with LOFAR at 54 MHz
• Analysis of branon dark matter and extra-dimensional models with AMS-02
• On the surface brightness radial profile of the extended $\gamma$-ray sources
• Hadronic Interactions of Energetic Charged Particles in Protogalactic Outflow Environments and Implications for the Early Evolution of Galaxies
• Fermi Bubbles and Bubble-like emission from the Galactic Plane
• MiXDM: Cosmic Ray Signals from Multiple States of Dark Matter
• The consequence of a new ISRF model of the Milky Way on predictions for diffuse gamma-ray emission
• Monte Carlo Study of Electron and Positron Cosmic-Ray Propagation with the CALET Spectrum
• Recent extensions to GALPROP
• Confronting recent AMS-02 positron fraction and Fermi-LAT Extragalactic Gamma-Ray Background measurements with gravitino dark matter
• A spatially resolved study of hard X-ray emission in Kepler's SNR: indications of different regimes of particle acceleration
• Spectrum and fraction of cosmic ray positrons: results of the anomalous diffusion approach
• Quantifying the Interstellar Medium and Cosmic Rays in the MBM 53, 54, and 55 Molecular Clouds and the Pegasus Loop using Fermi-LAT Gamma-ray Observations
• Anomalous Galactic Cosmic Rays in the Framework of AMS-02
• TeV cosmic-ray proton and helium spectra in the myriad model II
• On discrepancy between ATIC and Fermi data
• On the PeV knee of cosmic rays spectrum and TeV cutoff of electron spectrum
• On The {\it Fermi} -Lat Surplus of the Diffuse Galactic Gamma-Ray Emission
• Type II Seesaw with scalar dark matter in light of AMS-02, DAMPE and Fermi-LAT
• Universal properties of primary and secondary cosmic ray energy spectra
• The phase structure of cosmic ray driven outflows in stream fed disc galaxies
• Model independent interpretation of recent CR lepton data after AMS-02
• Emission from hadronic and leptonic processes in galactic jet-driven bubbles
• G279.0+1.1: a new extended source of high-energy gamma rays
• Galactic Magnetic Turbulence from Radio data
• Search for the Gamma-ray Emission from M33 with Fermi LAT
• Extracting the size of the cosmic electron-positron anomaly
• Testing afterglow models of FRB 200428 with early post-burst observations of SGR 1935+2154
• LeXInt: Package for Exponential Integrators employing Leja interpolation
• Fireball anti-nucleosynthesis
• $e^{+}$ and $\bar{p}$ production in $pp$ collisions and the cosmic-ray $e^{+}/\bar{p}$ flux ratio
• High-energy cosmic rays from compact galactic star clusters: particle fluxes and anisotropy
• Evidence of fresh cosmic ray in galactic plane based on DAMPE measurement of B/C and B/O ratios
• Galaxies at a Cosmic-Ray Eddington Limit
• Secondary Production as the Origin for the Cosmic Ray Positron Excess
• On Dark Matter Explanations of the Gamma-Ray Excesses from the Galactic Center and M31
• Cosmic-ray transport and gamma-ray emission in M31
• Connecting direct and indirect detection with a dark spike in the cosmic-ray electron spectrum
• Implications of a Possible Spectral Structure of Cosmic-ray Protons Unveiled by the DAMPE
• Simplified dark matter models in the light of AMS-02 antiproton data
• Fickian and non-Fickian diffusion of cosmic rays
• GALPROP cosmic-ray propagation code: recent results and updates
• Revisiting simplified dark matter models in terms of AMS-02 and Fermi-LAT
• Interpretation of the cosmic ray positron and electron excesses with an annihilating-decaying dark matter scenario
• Cosmic ray backgrounds for dark matter indirect detection
• Solar modulation of AMS-02 daily proton and Helium fluxes with modified force field approximation models
• Imprints of PeV cosmic-ray sources on the diffuse gamma-ray emission
• Inverse Problem of Cosmic-Ray Electron/Positron from Dark Matter
• Secondary cosmic-ray nuclei in the Galactic halo model with nonlinear Landau damping
• A tale of cosmic rays narrated in gamma rays by Fermi
• Cosmic Rays in the Milky Way and Beyond
• Detectors for high-energy messengers from the Universe
• Consistent explanation for the cosmic-ray positron excess in $p$-wave Breit-Wigner enhanced dark matter annihilation
• A gamma-ray study of galactic PeVatron candidates LHAASO J1825-1326 and LHAASO J1839-0545
• Current status and new perspectives on cosmic ray deuterons
• Obtaining the diffusion coefficient for cosmic ray propagation in the Galactic Centre Ridge through time-dependent simulations of their gamma-ray emission
• The XMM-Newton X-ray Spectra of the Most X-ray Luminous Radio-quiet ROSAT Bright Survey-QSOs: A Reference Sample for the Interpretation of High-redshift QSO Spectra
• The impact of cosmic ray heating on the cooling of the low-metallicity interstellar medium
• Pulsar Wind Nebulae
• The Origin of the Very-High-Energy Diffuse $\gamma$-Ray Emission: The Case for Galactic Source Cocoons
• CHANG-ES XXXIV: Magnetic Field Structure in Edge-On Galaxies Characterising large-scale magnetic fields in galactic halos
• Current status and desired accuracy of the isotopic production cross-sections relevant to astrophysics of cosmic rays II. Fluorine to Silicon (and updated LiBeB)
• On the Integrability of the Geodesic Flow on a Friedmann-Robertson-Walker Spacetime
• Constraining annihilating dark matter by x-ray data
• Cosmic Ray Accelerators in the Large Magellanic Cloud
• A New Perspective on the Diffuse Gamma-Ray Emission Excess
• A 3D Diffusive and Advective Model of Electron Transport Applied to the Pulsar Wind Nebula HESS J1825-137
• Injection spectra of different species of cosmic rays from AMS-02, ACE-CRIS and Voyager-1
• Modeling the Galactic center gamma-ray emission with more realistic cosmic-ray dynamics
• Searches for Particle Dark Matter: An Introduction
• Explanation of nearby SNRs for primary electron excess and proton spectral bump
• Synchrotron Emission From Young And Nearby Pulsars
• Revealing a new region of gamma-ray emission in the vicinity of HESS J1825-137
• Gamma-Ray Emission from Supernova Remnants and Surrounding Molecular Clouds
• Runaway O-star Bow Shocks as Particle Accelerators? The Case of AE Aur revisited
• Cosmic Ray e^+/(e^- + e^+) and pbar/p Ratios Explained by an Injection Model Based on Gamma-ray Observations
• Modeling Hadronic Gamma-ray Emissions from Solar Flares and Prospects for Detecting Non-thermal Signatures from Protostars
• Galactic Centre as an efficient source of cosmic rays
• The dynamical impact of cosmic rays in the Rhea magnetohydrodynamics simulations
• Gas and Cosmic-Ray Properties in the MBM 53, 54, and 55 Molecular Clouds and the Pegasus Loop as Revealed by HI Line Profiles, Dust, and Gamma-Ray Data
• Measurement and analysis of nuclear $\gamma$-ray production cross sections in proton interactions with Mg, Si and Fe nuclei abundant in astrophysical sites over the incident energy range $E=30-66$ MeV
• Time variability of TeV cosmic ray sky map
• AMS-02 antiprotons and dark matter: Trimmed hints and robust bounds
• Cosmic ray acceleration and non-thermal emission from fast luminous optical transient sources
• Magnetic field evolution in dwarf and Magellanic-type galaxies
• Cosmic ray knee and new physics at the TeV scale
• Regions of suppressed diffusion around supernova remnants?
• Muon anomalous magnetic moment and positron excess at AMS-02 in a gauged horizontal symmetric model
• Astronomy with ultra high-energy particles
• Sharpening up Galactic all-sky maps with complementary data - A machine learning approach
• Lower limits on the nucleosynthezis of ${}^{44}$Ti and ${}^{60}$Fe in the dynamic spiral-arms model
• Probing the astrophysical origin of high-energy cosmic-ray electrons with Monte Carlo simulation
• Detection of diffuse gamma-ray emission towards a massive star forming region hosting Wolf-Rayet stars
• Exploring magnetised galactic outflows in starburst dwarf galaxies NGC 3125 and IC 4662
• Enhanced cosmic-ray antihelium production from dark matter annihilation through light mediators
• An interacting molecular cloud scenario for production of gamma-rays and neutrinos from MAGIC J1835-069, and MAGIC J1837-073
• Potential of Constraining Propagation Parameters of Galactic Cosmic Rays with the High Energy cosmic-Radiation Detection facility onboard China's Space Station
• Transport parameters from AMS-02 F/Si data and fluorine source abundance
• Constraining cosmic-ray acceleration in the magnetospheric gaps of Sgr A*
• Inelastic Scattering of Dark Matter with Heavy Cosmic Rays
• Particle Acceleration in Cosmic Sites - Astrophysics Issues in our Understanding of Cosmic Rays
• The HelMod Model in the Works for Inner and Outer Heliosphere: from AMS to Voyager Probes Observations
• High-energy emissions from neutron star mergers
• Exploring the MeV Sky with a Combined Coded Mask and Compton Telescope: The Galactic Explorer with a Coded Aperture Mask Compton Telescope (GECCO)
• Cosmic Ray Electron and Positron Excesses from a Fourth Generation Heavy Majorana Neutrino
• HESS J1745$-$290 spectrum explained by a transition in the diffusion regime of PeV cosmic rays in the Sgr A* accretion flow
• Evidence for GeV Cosmic Rays from White Dwarfs in the Local Cosmic Ray Spectra and in the Gamma-ray Emissivity of the Inner Galaxy
• The impact of cosmic ray feedback during the epoch of reionisation
• Reanalysis of the Systematic Uncertainties in Cosmic-Ray Antiproton Flux
• Deep Learning Models of the Discrete Component of the Galactic Interstellar Gamma-Ray Emission
• Hillas meets Eddington: The case for blazars as ultra-high-energy neutrino sources
• Study of the Cosmic Rays and Interstellar Medium in Local HI Clouds using Fermi-LAT Gamma-Ray Observations
• X-ray Binaries: a potential dominant contributor to the cosmic ray spectral knee structure
• Forecasting of the time-dependent fluxes of antiprotons in the AMS-02 era
• Contribution of dark matter annihilation to gamma-ray burst afterglows near massive galaxy centers
• Cosmic Ray transport in mixed magnetic fields and their role on the observed anisotropies
• AMS-02 fits Dark Matter
• Cosmic-ray electrons and the magnetic field of the North Polar Spur
• Radio-FIR correlation- A probe into cosmic ray propagation in the nearby galaxy IC 342
• AMS-02 in Space: Physics Results
• The Morphology of the Anomalous Microwave Emission in the Planck 2015 data release
• Reexamine the dark matter scenario accounting for the positron excess in a new cosmic ray propagation model
• WIMP constraints from black hole low-mass X-ray binaries
• Simulation of Cosmic Ray propagation in the Galactic Centre Ridge in Accordance with Observed VHE gamma-ray Emission
• Cosmic-ray deuteron excess from a primary component
• The dark connection between the EGRET excess of diffuse Galactic gamma rays, the Canis Major dwarf, the Monoceros ring, the INTEGRAL 511 keV annihilation line, the gas flaring and the Galactic rotation curve
• Probing solar modulation of AMS-02 time-dependent D, ${}^3$He and ${}^4$He fluxes with modified force field approximation
• Cosmic rays: interstellar gamma-ray and radio emission
• Evidence for protostellar jets as a population of hadronic gamma-ray sources
• PeV particle acceleration and non-thermal emission in the `minimalist' model of the extended jets in W50/SS433
• Sources and Radiations of the Fermi Bubbles
• Nuclear de-excitation line emissions from giant molecular clouds
• Bayesian approach to equipartition estimation of magnetic field strength
• Improved Modeling of the Discrete Component of the Galactic Interstellar Gamma-ray Emission and Implications for the Fermi-LAT Galactic Center Excess
• The GALPROP Cosmic-ray Propagation and Non-thermal Emissions Framework: Release v57
• Fundamental physics in space with the Fermi Gamma-ray Space Telescope
• The contribution of nearby supernova remnants on the cosmic ray flux at Earth
• Consistent explanation for the cosmic-ray positron excess in p-wave Sommerfeld-enhanced dark matter annihilation
• Probing maximum energy of cosmic rays in SNR through gamma rays and neutrinos from the molecular clouds around SNR W28
• Electron-Capture Isotopes could Constrain Cosmic-Ray Propagation Models
• Cosmic ray propagation in the interstellar magnetic fields
• Analysis of the Positron Fraction and the Spectrum of the Electronic Component in Cosmic Rays
• Direct Simulations of Particle Acceleration in Fluctuating Electromagnetic Field across a Shock
• Nonthermal processes and particle acceleration in supernova remnants
• Modelling the Gamma-Ray Morphology of HESS J1804-216 from Two Supernova Remnants in a Hadronic Scenario
• A GeV-TeV particle component and the barrier of cosmic-ray sea in the Central Molecular Zone
• The effects of drift and winds on the propagation of Galactic cosmic rays
• Thermal damping of Weak Magnetosonic Turbulence in the Interstellar Medium
• On the hadronic origin of the very high energy $\gamma$-ray emission surrounding the young massive stellar cluster Westerlund 1
• Diffusive Origin of the Cosmic-Ray Spectral Hardening
• CHILLING: Continuum Halos in LVHIS Local Irregular Nearby Galaxies - Radio continuum spectral behavior of dwarf galaxies
• Cosmic positron excess: is the dark matter solution a good bet?
• Uncovering neutrinos from cosmic ray factories: the Multi Point Source method
• Tight correlation of star formation with [Ci] and CO lines across cosmic time
• SILCC -- IX. The multi-phase interstellar medium at low metallicity
• MHD Models of Gamma-ray Emission in WR 11
• Synthetic Turbulence via an Instanton Gas Approximation
• The high energy window of probing dark matter with cosmic-ray antideuterium and antihelium
• A New Approach to Searching for Dark Matter Signals in Fermi-LAT Gamma Rays
• Tracing the propagation of cosmic rays in the Milky Way halo with Fermi-LAT observations of high- and intermediate-velocity clouds
• The cosmic $e^{\pm }$ anomaly
• Possible evidence for extended X-ray emission surrounding PSR B0656+14 with eROSITA
• Interactions of Cosmic Rays in the Atmosphere: Growth Curves Revisited
• Cosmic Radioactivity and Galactic Chemical Evolution
• Fermi bubble simulations: black hole feedback in the Milky Way
• Cosmic rays from multiwavelength observations of the Galactic diffuse emission
• Searching for Neutrinos from WIMP Annihilations in the Galactic Stellar Disk
• Limits on Dark Matter Annihilation from the Shape of Radio Emission in M31
• Explaining AMS-02 positron excess and muon anomalous magnetic moment in dark left-right gauge model
• Measurement of the antiproton/proton ratio in the few-TeV energy range with ARGO-YBJ
• Multi-wavelength emission from leptonic processes in ageing galaxy bubbles
• Absorption spectra of electrified hydrogen molecules
• Comparing different closure relations for cosmic ray hydrodynamics
• Effect of cosmic rays and ionizing radiation on observational ultraviolet plasma diagnostics in the circumgalactic medium
• Rethinking Habitability using Biogenic Precursors: Formaldehyde in Millimeter Molecular Clouds of the Inner Galaxy
• Non-thermal emission in the central starburst region of M82
• Shocking Signals of Dark Matter Annihilation
• Particle Reacceleration by Turbulence and Radio Constraints on Multi-Messenger High-Energy Emission from the Coma Cluster
• Impact of Fermi-LAT and AMS-02 results on cosmic-ray astrophysics
• Constraining the cosmic ray propagation halo thickness using Fermi-LAT observations of high-latitude clouds
• On the stochastic nature of Galactic cosmic-ray sources
• Cosmic-Ray Induced Diffuse Emissions from the Milky Way and Local Group Galaxies
• Spectrally resolved cosmic rays: II -- Momentum-dependent cosmic ray diffusion drives powerful galactic winds
• Method for testing diffusive shock acceleration and diffusion propagation of 1-100 TeV cosmic electrons with multiwavelength observations of the Geminga halo and pulsar wind nebula
• The Discrepancy in Modelling of Galactic Cosmic Ray Primaries and Secondaries
• Antinuclei from Primordial Black Holes
• Measuring the smearing of the Galactic 511 keV signal: positron propagation or supernova kicks?
• Deciphering the Electron Spectral Hardening in AMS-02
• Study of Galactic interactions and propagation properties of ultrahigh energy cosmic rays using the precision spectrum from the Pierre Auger Observatory
• Antiproton Flux in Cosmic Ray Propagation Models with Anisotropic Diffusion
• On the contribution of the bow shock pulsar wind nebula PSR J0437-4715 to the observed fluxes of GeV-TeV positrons and antiprotons
• UHECR primary identification using the lateral profile of muons in EAS
• Research on electron and positron spectrum in the high-energy region based on the gluon condensation model
• The cosmic-ray puzzle and the census of the interstellar medium: the Fermi LAT view of Cassiopeia, Cepheus and the Perseus arm
• Young Massive Star Clusters as TeV Emitters: Constraints from H.E.S.S. and LHAASO
• MEDUSA I. Tracing magnetic field structures in tidal arms of the dwarf-dwarf merger NGC 1487
• Cosmic-ray electron propagation in NGC 3044 from radio continuum observations
• Experimental Efforts on Very High-Energy Cosmic Rays and their Interactions - Conference Summary
• Joint constraint on the propagation origin of the cosmic-ray spectral knee from energy spectrum and anisotropy observations
• The influence of the 3D Galactic gas structure on cosmic-ray transport and $\gamma$-ray emission
• Revisiting electron-capture decay for Galactic cosmic-ray data
• Spectra of He isotopes and the ${}^3$He/${}^4$He ratio
• Deciphering the spectral bumps of Galactic cosmic rays through gamma-ray observations of nearby molecular clouds
• Testing astroparticle physics with the Fermi Large Area Telescope
• Past activity of Sgr A* is unlikely to affect the local cosmic-ray spectrum up to the TeV regime