Propagation of cosmic-ray nucleons in the Galaxy

Abstract

We describe a method for the numerical computation of the propagation of primary and secondary nucleons, primary electrons, and secondary positrons and electrons. Fragmentation and energy losses are computed using realistic distributions for the interstellar gas and radiation fields, and diffusive reacceleration is also incorporated. The models are adjusted to agree with the observed cosmic-ray B/C and 10Be/9Be ratios. Models with diffusion and convection do not account well for the observed energy dependence of B/C, while models with reacceleration reproduce this easily. The height of the halo propagation region is determined, using recent 10Be/9Be measurements, as >4 kpc for diffusion/convection models and 4-12 kpc for reacceleration models. For convection models we set an upper limit on the velocity gradient of dV/dz < 7 km/s/kpc. The radial distribution of cosmic-ray sources required is broader than current estimates of the SNR distribution for all halo sizes. Full details of the numerical method used to solve the cosmic-ray propagation equation are given.

15 pages including 23 ps-figures and 3 tables, latex2e, uses emulateapj.sty (ver. of 11 May 1998, enclosed), apjfonts.sty, timesfonts.sty. To be published in ApJ 1998, v.509 (December 10 issue). More details can be found at http://www.gamma.mpe-garching.mpg.de/~aws/aws.html Some references are corrected

References in corpus (3)

• Production and propagation of cosmic-ray positrons and electrons
• The Energy Spectra and Relative Abundances of Electrons and Positrons in the Galactic Cosmic Radiation
• Modelling cosmic rays and gamma rays in the Galaxy

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• Neutralino Dark Matter from Indirect Detection Revisited
• Stochasticity of Cosmic Rays from Supernova Remnants and the Ionization Rates in Molecular Clouds
• Excess of EGRET Galactic Gamma Ray Data interpreted as Dark Matter Annihilation
• A dark matter model that reconciles tensions between the cosmic-ray $e^{\pm }$ excess and the gamma-ray and CMB constraints
• Revisit cosmic ray propagation by using ${}^1$H, ${}^2$H, ${}^3$He and ${}^4$He
• AMS-02 Positron Excess and Indirect Detection of Three-body Decaying Dark Matter
• Systematic study of the uncertainties in fitting the cosmic positron data by AMS-02
• Strong magnetic fields and cosmic rays in very young galaxies
• The Propagation of Cosmic Rays from the Galactic Wind Termination Shock: Back to the Galaxy?
• Entering the Era of Dark Matter Astronomy? Near to Long-Term Forecasts in X-Ray and Gamma-Ray Bands
• Recovering the observed B/C ratio in a dynamic spiral-armed cosmic ray model
• Anisotropic cosmic-ray diffusion in isotropic Kolmogorov turbulence
• Astrophysical Uncertainties in the Cosmic Ray Electron and Positron Spectrum From Annihilating Dark Matter
• CRT: A numerical tool for propagating ultra-high energy cosmic rays through Galactic magnetic field models
• Deciphering Residual Emissions: Time-Dependent Models for the Non-Thermal Interstellar Radiation from the Milky Way
• Pevatron at the Galactic Center: Multi-Wavelength Signatures from Millisecond Pulsars
• Limits on the Dark Matter from AMS-02 antiproton and positron fraction data
• Antiproton Limits on Decaying Gravitino Dark Matter
• On the origin of galactic cosmic rays
• Diffuse Galactic Gamma Rays at intermediate and high latitudes. I. Constraints on the ISM properties
• Indirect Detection of Dirac Right-Handed Neutrino Dark Matter
• What is the Cosmic-Ray luminosity of our Galaxy?
• Intermediate mass and heavy Galactic cosmic-ray nuclei: the case of new AMS-02 measurements
• PAMELA/Fermi-LAT electron cosmic ray spectrum at $\sim$100 GeV: implication for dark matter annihilation signal in accordance with the 130 GeV $\gamma$-ray line
• Experimental constraints on the astrophysical interpretation of the cosmic ray Galactic-extragalactic transition region
• Galactic-Centre Gamma Rays in CMSSM Dark Matter Scenarios
• Cosmic Ray Positrons from Annihilations into a New, Heavy Lepton
• Cosmic Rays and Magnetic Fields in the Core and Halo of the Starburst M82: Implications for Galactic Wind Physics
• Recent Result of the AMS-02 Experiment and Decaying Gravitino Dark Matter in Gauge Mediation
• Cosmic ray $e^{+}{e}^{-}$ spectrum excess and peak feature observed by the DAMPE experiment from dark matter
• Signatures of Cosmic Ray Heating in 21-cm Observables
• Diffuse Galactic gamma-rays: constraining cosmic-ray origin and propagation
• Anti-Deuterons and Anti-Helium Nuclei from Annihilating Dark Matter
• The impact of propagation uncertainties on the potential Dark Matter contribution to the Fermi LAT mid-latitude gamma-ray data
• A Latitude-Dependent Analysis of the Leptonic Hypothesis for the Fermi Bubbles
• Theoretical interpretation of Pass 8 Fermi-LAT $e^{+}+e^{-}$ data
• Creation of X-ray cavities in galaxy clusters with cosmic rays
• Origin of Ultrahigh Energy Galactic Cosmic Rays: The Isotropy Problem
• Sensitivity of the GAPS Experiment to Low-energy Cosmic-ray Antiprotons
• Antimatter cosmic rays from dark matter annihilation: First results from an N-body experiment
• Implications of the latest XENON100 and cosmic ray antiproton data for isospin violating dark matter
• Reevaluation of the cosmic antideuteron flux from cosmic-ray interactions and from exotic sources
• The connection between warm carbon chain chemistry and interstellar irradiation of star-forming cores
• Cosmic-ray propagation around the Sun: investigating the influence of the solar magnetic field on the cosmic-ray Sun shadow
• Recent results in nuclear astrophysics
• The coherent magnetic field of the Milky Way halo, Local Bubble and Fan Region
• Radiative Seesaw Model and DAMPE Excess from Leptophilic Gauge Symmetry
• Constraining Dark Matter Properties with Gamma-Rays from the Galactic Center with Fermi-LAT
• Remnants of Galactic subhalos and their impact on indirect dark matter searches
• Building up the spectrum of cosmic-rays in star-forming regions
• Gamma-ray emission from globular clusters
• A possible Universal Origin of Hadronic Cosmic Rays from Ultrarelativistic Ejecta of Bipolar Supernovae
• Universal profiles for radio searches of dark matter in dwarf galaxies
• Electrons and Positrons in Cosmic Rays
• Utilizing cosmic-ray positron and electron observations to probe the averaged properties of Milky Way pulsars
• Searching for Dark Matter Annihilation in the Smith High-Velocity Cloud
• Collider Bounds on Indirect Dark Matter Searches: The $WW$ Final State
• Charge Asymmetric Cosmic Rays as a probe of Flavor Violating Asymmetric Dark Matter
• Synchrotron X-ray diagnostics of cutoff shape of nonthermal electron spectrum at young supernova remnants
• Mass of Decaying Wino from AMS-02 2014
• Decaying Dark Atom constituents and cosmic positron excess
• Transport of Protostellar Cosmic Rays in Turbulent Dense Cores
• Robust inference of the Galactic centre gamma-ray excess spatial properties
• A Phantom Menace: On the Morphology of the Galactic Center Excess
• Outflow and Emission Model of Pulsar Wind Nebulae with the Back-reaction of Particle Diffusion
• Multimessenger search for electrophilic feebly interacting particles from supernovae
• Prospects of detecting dark matter through cosmic-ray antihelium with the antiproton constraints
• Confronting the DAMPE Excess with the Scotogenic Type-II Seesaw Model
• Prospects for detection of a Galactic diffuse neutrino flux
• 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
• On the contribution of nearby sources to the observed cosmic-ray nuclei
• Pulsars as the Source of the WMAP Haze
• Chemical Composition of Galactic Cosmic Rays with Space Experiments
• Testing universality of cosmic-ray acceleration with proton/helium data from AMS and Voyager-1
• Hybrid model of GeV-TeV gamma ray emission from Galactic Center
• Implications of a possible TeV break in the cosmic-ray electron and positron flux
• hammurabi X: Simulating Galactic Synchrotron Emission with Random Magnetic Fields
• Observational constraints on the maximum energies of accelerated particles in supernova remnants: low maximum energies and a large variety
• Constraining the Milky Way Dark Matter Density Profile with Gamma-Rays with Fermi-LAT
• Bayesian analysis of the hardening in AMS-02 nuclei spectra
• Explaining TeV Cosmic-Ray Anisotropies with Non-Diffusive Cosmic-Ray Propagation
• On the Contribution of "Fresh" Cosmic Rays to the Excesses of Secondary Particles
• The diffuse neutrino flux from the inner Galaxy: constraints from very high energy gamma-ray observations
• Turbulent Reacceleration of Streaming Cosmic Rays
• Robust constraints on feebly interacting particles using XMM-Newton
• Multi-Phase Magnetic Fields in the Galaxy NGC 3627
• Cosmic Ray Interstellar Propagation Tool using Itô Calculus (criptic): software for simultaneous calculation of cosmic ray transport and observational signatures
• Galactic diffuse gamma rays --- recalculation based on the new measurements of cosmic electron spectrum
• Gamma-ray emitting supernova remnants as the origin of Galactic cosmic rays?
• Cosmic rays and molecular clouds
• Robustness of the Galactic Center Excess Morphology Against Masking
• Contribution of the Galactic center to the local cosmic-ray flux
• Dark matter implications of the WMAP-Planck Haze
• Possible bump structure of cosmic ray electrons unveiled by AMS-02 data and its common origin along with the nuclei and positron
• Systematic Effects in Extracting a "Gamma-Ray Haze" from Spatial Templates
• The Steady-State Multi-TeV Diffuse Gamma-Ray Emission Predicted with GALPROP and Prospects for the Cherenkov Telescope Array
• Selected Topics in Cosmic Ray Physics
• Diffuse Gamma Rays: Galactic and Extragalactic Diffuse Emission
• Galaxy clusters in high definition: a dark matter search
• Cosmic Ray Anomalies from the MSSM?
• Overcoming Gamma Ray Constraints with Annihilating Dark Matter in Milky Way Subhalos
• Gamma-rays From Warm WIMP Dark Matter Annihilation
• Dark Matter in X-rays: Revised XMM-Newton Limits and New Constraints from eROSITA
• Spatial and Spectral Modeling of the Gamma-ray Distribution in the Large Magellanic Cloud
• Constraining primordial black holes as dark matter using AMS-02 data
• A self-consistent model of cosmic-ray fluxes and positron excess: Roles of nearby pulsars and a sub-dominant source population
• Neutral iron line in the supernova remnant IC 443 and implications for MeV cosmic rays
• Two Numerical Methods for the 3D Anisotropic Propagation of Galactic Cosmic Rays
• The B/C and sub-Iron/Iron Cosmic ray ratios - further evidence in favor of the spiral arm diffusion model
• B/C ratio and the PAMELA positron excess
• Hints of a Charge Asymmetry in the Electron and Positron Cosmic-Ray Excesses
• Pinpointing the knee of cosmic rays with diffuse PeV gamma-rays and neutrinos
• The Galactic positron flux and dark matter substructures
• The puzzling origin of the 6Li plateau
• Cosmic Sum Rules
• Can the Production Cross-Section Uncertainties Explain the Cosmic Fluorine Anomaly?
• On the Galactic Center Being the Main Source of Galactic Cosmic Rays as Evidenced by Recent Cosmic Ray and Gamma Ray Observations
• Plasmon-enhanced Direct Detection Method for Boosted sub-MeV Dark Matter
• Propagation model for cosmic ray species in the Galaxy
• Cosmic Ray Positrons from Cosmic Strings
• 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
• The Andromeda Gamma-Ray Excess: Background Systematics of the Millisecond Pulsars and Dark Matter Interpretations
• The consequence of a new ISRF model of the Milky Way on predictions for diffuse gamma-ray emission
• Anomalous Galactic Cosmic Rays in the Framework of AMS-02
• PAMELA through a Magnetic Lens
• A radiation transfer model for the Milky Way. II The global properties and large scale structure
• A stochastic simulation of the propagation of Galactic cosmic rays reflecting the discreteness of cosmic ray sources. Age and path length distribution
• TeV cosmic-ray proton and helium spectra in the myriad model II
• The diffuse GeV-TeV $\gamma$-ray emission of the Cygnus region
• Pamela, FGST and Sub-Tev Dark Matter
• Small-Scale Magnetic Fields are Critical to Shaping Solar Gamma-Ray Emission
• Constraining $U(1{)}_{L_{\mu }-L_{\tau }}$ charged dark matter model for muon $g-2$ anomaly with AMS-02 electron and positron data
• Revisiting GeV-scale annihilating dark matter with the AMS-02 positron fraction
• Non-linear acceleration at supernova remnant shocks and the hardening in the cosmic ray spectrum
• Impact of transport modelling on the ${}^{60}$Fe abundance inside Galactic cosmic ray sources
• High-energy gamma-ray emission from SNR G57.2+0.8 hosting SGR J1935+2154
• Cosmic Ray Excesses from Multi-component Dark Matter Decays
• The Important Role of Cosmic-Ray Re-Acceleration
• Extracting the size of the cosmic electron-positron anomaly
• Cosmic-ray transport and gamma-ray emission in M31
• Cosmic-ray propagation under consideration of a spatially resolved source distribution
• Neutrino emission of Fermi supernova remnants
• Constraining the Charge-, Time- and Rigidity-Dependence of Cosmic-Ray Solar Modulation with AMS-02 Observations during Solar Cycle 24
• In-flight positron annihilation as a probe of feebly interacting particles
• Interpretation of the cosmic ray positron and electron excesses with an annihilating-decaying dark matter scenario
• GALPROP cosmic-ray propagation code: recent results and updates
• Dark Matter with multi-annihilation channels and AMS-02 positron excess and antiproton
• Revisiting simplified dark matter models in terms of AMS-02 and Fermi-LAT
• Spallation dominated propagation of Heavy Cosmic Rays and the Local Interstellar Medium (LISM)
• Cosmic e^\pm, \bar p, γand neutrino rays in leptocentric dark matter models
• A hard spectrum diffuse gamma-ray component associated with HII gas in the Galactic plane
• Propagation of secondary antiprotons and cosmic rays in the Galaxy
• 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
• On Dark Matter Explanations of the Gamma-Ray Excesses from the Galactic Center and M31
• New constraints on cosmic ray-boosted dark matter from the LUX-ZEPLIN experiment
• Gamma-ray Production in the Extended Halo of the Galaxy and Possible Implications for the Origin of Galactic Cosmic Rays
• Modulation of cosmic ray anti-protons in the heliosphere: simulations for a solar cycle
• Search for Features in the Cosmic-Ray Electron and Positron spectrum measured by the Fermi Large Area Telescope
• Hybrid origins of the cosmic-ray nuclei spectral hardening at a few hundred GV
• Cosmic Rays during BBN as Origin of Lithium Problem
• Imprints of PeV cosmic-ray sources on the diffuse gamma-ray emission
• Solar modulation of AMS-02 daily proton and Helium fluxes with modified force field approximation models
• Morphological Tests of the Pulsar and Dark Matter Interpretations of the WMAP Haze
• The Making of Catalogues of Very-High-Energy γ-ray Sources
• Dark matter annihilation and non-thermal Sunyaev-Zel'dovich effect: I. galaxy cluster
• Diffuse flux of galactic neutrinos and gamma rays
• Diffuse $\gamma$-rays and $\bar{p}$ flux from dark matter annihilation -- a model for consistent results with EGRET and cosmic ray data
• The Contribution of Millisecond Pulsars to the Galactic Cosmic-Ray Lepton Spectrum
• Indirect dark matter searches: towards a consistent top-bottom approach for studying the gamma-ray signals and associated backgrounds
• The diffuse Galactic gamma-rays from dark matter annihilation
• Observing Signals of Spectral Features in the Cosmic-Ray Positrons and Electrons from Milky Way Pulsars
• When Dark Matter interacts with Cosmic Rays or Interstellar Matter: A Morphological Study
• Searches for Particle Dark Matter: An Introduction
• Calibrating Column Density Tracers with Gamma-ray Observations of the $\rho$ Ophiuchi Molecular Cloud
• Cosmic Rays in the Milky Way and Beyond
• Injection spectra of different species of cosmic rays from AMS-02, ACE-CRIS and Voyager-1
• Testing the dark matter origin of the WMAP-Planck Haze with radio observations of Spiral Galaxies
• Prospects of future MeV telescopes in probing weak-scale Dark Matter
• A new Determination of the Extragalactic Background of Diffuse Gamma Rays taking into account Dark Matter Annihilation
• Multi messenger astronomy and CTA: TeV cosmic rays and electrons
• A gamma-ray study of galactic PeVatron candidates LHAASO J1825-1326 and LHAASO J1839-0545
• Current status and desired accuracy of the isotopic production cross-sections relevant to astrophysics of cosmic rays II. Fluorine to Silicon (and updated LiBeB)
• Consistency test of the AMS-02 antiproton excess with direct detection data based on the effective field theory approach
• Consistent explanation for the cosmic-ray positron excess in $p$-wave Breit-Wigner enhanced dark matter annihilation
• Explanation of nearby SNRs for primary electron excess and proton spectral bump
• 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
• High energy emission from the nebula around the Black Widow binary system containing millisecond pulsar B1957+20
• Direct and indirect constraints on isospin-violating dark matter
• Probing local cosmic rays using Fermi-LAT observation of a mid-latitude region in the third Galactic quadrant
• The AMS-02 cosmic ray deuteron flux is consistent with a secondary origin
• Positron annihilation as a cosmic-ray probe
• Coulomb Bubbles: Over-stable Driving of Magnetoacoustic Waves Due to the Rapid and Anisotropic Diffusion of Energy
• Heavy Nuclei Enrichment of the Galactic Cosmic Rays at High Energy: Astrophysical Interpretation
• The population of Galactic supernova remnants in the TeV range
• Diffuse gamma-ray emission around the Rosette Nebula
• From 10 Kelvin to 10 TeraKelvin: Insights on the Interaction Between Cosmic Rays and Gas in Starbursts
• Galactic Centre as an efficient source of cosmic rays
• Circular Polarization of Pulsar Wind Nebulae and the Cosmic-Ray Positron Excess
• Decaying Fermionic Dark Matter Search with CALET
• AMS-02 antiprotons and dark matter: Trimmed hints and robust bounds
• High Latitude, Translucent Molecular Clouds as Probes of Local Cosmic Rays
• Probing the astrophysical origin of high-energy cosmic-ray electrons with Monte Carlo simulation
• Spectra of cosmic ray electrons and diffuse gamma rays with the constraints of AMS-02 and HESS data
• Galactic Propagation of Cosmic Rays from Individual Supernova Remnants
• On the origin of the diffuse gamma-ray background radiation
• Origin Of The Cosmic Ray Positrons Observed Near Earth- Meson Decay Or Dark Matter Decay?
• Enhanced cosmic-ray antihelium production from dark matter annihilation through light mediators
• Analytical view of diffusive and convective cosmic ray transport in elliptical galaxies
• Lower limits on the nucleosynthezis of ${}^{44}$Ti and ${}^{60}$Fe in the dynamic spiral-arms model
• Exploring sub-GeV Dark Matter Physics with Cosmic Ray and Future Telescopes
• An updated view and perspectives on high-energy gamma-ray emission from SGR J1935+2154 and its environment
• Snowmass 2021 LoI: Determination of cosmic ray properties in the local interstellar medium with all-sky anisotropy observations
• Transport parameters from AMS-02 F/Si data and fluorine source abundance
• A radio-frequency WIMP search with the MeerKAT Galaxy Cluster Legacy Survey
• Strong Constraints on Dark Photon and Scalar Dark Matter Decay from INTEGRAL and AMS-02 data
• Potential of Constraining Propagation Parameters of Galactic Cosmic Rays with the High Energy cosmic-Radiation Detection facility onboard China's Space Station
• Antiprotons below 200 MeV in the interstellar medium: perspectives for observing exotic matter signatures
• Cosmic Ray Electron and Positron Excesses from a Fourth Generation Heavy Majorana Neutrino
• On the use of X-ray and gamma-ray telescopes for identifying the origin of electrons and positrons observed by ATIC, Fermi, and PAMELA
• Inelastic Scattering of Dark Matter with Heavy Cosmic Rays
• Reanalysis of the Systematic Uncertainties in Cosmic-Ray Antiproton Flux
• AMS-02 fits Dark Matter
• Rotation measure and synchrotron emission signatures in simulations of magnetized galactic discs
• Study of the Cosmic Rays and Interstellar Medium in Local HI Clouds using Fermi-LAT Gamma-Ray Observations
• The HelMod Model in the Works for Inner and Outer Heliosphere: from AMS to Voyager Probes Observations
• Deep Learning Models of the Discrete Component of the Galactic Interstellar Gamma-Ray Emission
• Testing the consistency of proapgation between light and heavy cosmic ray nuclei
• Galactic Traversability: A New Concept for Extragalactic SETI
• On the Origin of Cosmic Rays
• Monochromatic Gamma Rays from Dark Matter Annihilation to Leptons
• Positron Annihilations at the Galactic Center: Generating More Questions Than Answers
• Improved Modeling of the Discrete Component of the Galactic Interstellar Gamma-ray Emission and Implications for the Fermi-LAT Galactic Center Excess
• Between the cosmic-ray `knee' and the `ankle': Contribution from star clusters
• Cosmic ray propagation in the interstellar magnetic fields
• Possible counterpart signal of the Fermi bubbles at the cosmic-ray positrons
• Monte Carlo Study of Cosmic-Ray Propagation in the Galaxy and Diffuse Gamma-Ray Production
• Electron-Capture Isotopes could Constrain Cosmic-Ray Propagation Models
• Cosmic-ray deuteron excess from a primary component
• Indirect Dark Matter Signals
• Consistent explanation for the cosmic-ray positron excess in p-wave Sommerfeld-enhanced dark matter annihilation
• Looking for a charge asymmetry in cosmic rays
• Cosmic rays: interstellar gamma-ray and radio emission
• Revisiting the effect of nearby supernova remnants on local cosmic rays
• Primordial black holes in Randall-Sundrum: Cosmological signatures
• Observations of the Fermi bubbles and the Galactic center excess with the DArk Matter Particle Explorer
• 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
• Uncertainties of the antiproton flux from Dark Matter annihilation in comparison to the EGRET excess of diffuse gamma rays
• SZ effects from annihilating dark matter in the Milky Way: smooth halo, subhalos and intermediate-mass-black-holes
• 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
• $\overline{\text{D}}$arkRayNet: Emulation of cosmic-ray antideuteron fluxes from dark matter
• Dark matter signals and cosmic ray anomalies in an extended seesaw model
• Composite asymmetric dark matter with a dark photon portal: Multimessenger tests
• Production of antimatter in the galaxy
• Implications of the first AMS-02 antiproton data for dark matter
• Radio-Frequency Searches for Dark Matter in Dwarf Galaxies
• Cosmic positron excess: is the dark matter solution a good bet?
• On the morphology of $\gamma -$ray emission induced by $e^{\pm }$ from annihilating self-interacting dark matter
• Multicomponent Dark Matter in the Light of CALET and DAMPE
• Spatial dependence of the break in the energy spectrum of cosmic rays in the new anisotropic diffusion approach
• Imprint of a 2 Myr old source on the cosmic ray anisotropy
• The search for Milky Way halo substructure WIMP annihilations using the GLAST LAT
• Efficient charged particle propagation methods
• An Interpretation of the Cosmic Ray $e^{+}+e^{-}$ Spectrum from 10 GeV to 3 TeV Measured by CALET on the ISS
• Cosmic Radioactivity and Galactic Chemical Evolution
• A New Approach to Searching for Dark Matter Signals in Fermi-LAT Gamma Rays
• Limits on Dark Matter Annihilation from the Shape of Radio Emission in M31
• Thermal damping of Weak Magnetosonic Turbulence in the Interstellar Medium
• The high energy window of probing dark matter with cosmic-ray antideuterium and antihelium
• Models of diffusion of galactic Cosmic Rays from Super-bubbles
• The influence of the 3D Galactic gas structure on cosmic-ray transport and $\gamma$-ray emission
• Measurement of High Energy Gamma Rays from 200 MeV to 1 TeV with the Alpha Magnetic Spectrometer on the International Space Station
• Precision measurement of the cosmic-ray electron and positron fluxes as a function of time and energy with the Alpha Magnetic Spectrometer on the International Space Station
• Research on electron and positron spectrum in the high-energy region based on the gluon condensation model
• The Use Case of a New ISRF on Diffuse Gamma-ray Emission Models
• Testing astroparticle physics with the Fermi Large Area Telescope
• Combined analyses of the antiproton production from cosmic-ray interactions and its possible dark matter origin
• On the stochastic nature of Galactic cosmic-ray sources
• The low cosmic-ray density in Polaris Flare
• The cosmic-ray puzzle and the census of the interstellar medium: the Fermi LAT view of Cassiopeia, Cepheus and the Perseus arm
• Galactic Electron-Positron Annihilation Emission from X-Ray Binaries with Transient and Persistent Jets
• The Discrepancy in Modelling of Galactic Cosmic Ray Primaries and Secondaries
• Diffusion of Cosmic Antiprotons Generated throughout the Dark Matter Halo -- A Semi-Analytical Solution for a Linear Galactic Wind Model
• Analyzing Cosmic Ray Spectral Features: A Numerical Investigation
• TeV-PeV Gamma-ray and Neutrino Emission in the Galactic Plane
• Measurement of Cosmic-Ray Density in the Spiral Arms toward Galactic Anticenter
• Reconstructing Dark Matter Properties via Gamma-Rays with Fermi-LAT
• The Cosmic-ray Knee as a Local Signature of Nearby PeVatrons
• Galactic neutrino background from cosmic ray interaction with the ISM content
• Anisotropic diffusion modeling of cosmic-ray lepton propagation
• Particle Astrophysics with High and Ultrahigh Energy Neutrinos
• Unveiling extended gamma-ray emission around HESS J1813-178
• A Search for Z=-1 Dark Matter Annihilation Products in Cosmic Rays with AMS-01
• Physics and astrophysics with gamma-ray telescopes
• Perspective of Galactic dark matter subhalo detection on Fermi from the EGRET observation
• Consequences of the common origin of the knee and ankle in Cosmic Ray Physics
• A possible explanation of the knee of cosmic light component spectrum from 100 TeV to 3 PeV