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Explaining cosmic ray antimatter with secondaries from old supernova remnants


Detection of a gamma-ray halo around Geminga with the Fermi-LAT and implications for the positron flux


Leptophilic-portal dark matter in the light of AMS-02 positron excess



Test of the superdiffusion model in the interstellar medium around the Geminga pulsar



Emission of cosmic rays from Pulsar wind nebulae



Consistent explanation for the cosmic-ray positron excess in p-wave Sommerfeld-enhanced dark matter annihilation



Cosmic-Ray Positrons Strongly Constrain Leptophilic Dark Matter



Explaining cosmic ray antimatter with secondaries from old supernova remnants



An excess of excesses examined via dark matter radio emissions from galaxies



Reanalyze the pulsar scenario to explain the cosmic positron excess considering the recent developments



Origin of Cosmic Ray Electrons and Positrons



Overview of Direct Measurements of Cosmic Rays



Detection of a γ -ray halo around Geminga with the Fermi-LAT data and implications for the positron flux



Method of positron detection using the Earth magnetic field in orbital experiment



Indirect effects of dark matter



Spectrum of Electrons Accelerated in Supernova Remnants.



Dark matter decaying into millicharged particles as a solution to AMS-02 positron excess



P 2 0 1 9 ) 0 9 9 A multicomponent dark matter scenario and the experimental evidence supporting it



Positron flux and γ-ray emission from Geminga pulsar and pulsar wind nebula



Gauged $U(1)_{L_\mu-L_\tau}$ Scotogenic Model in light of $R_{K^{(*)}}$ Anomaly and AMS-02 Positron Excess



Multicomponent Dark Matter in the Light of CALET and DAMPE



Positron Excess from Cosmic Ray Interactions in Galactic Molecular Clouds



Origin of Cosmic Ray Electrons and Positrons



Detection of a gamma-ray halo around Geminga with the Fermi-LAT and implications for the positron flux


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