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Two-zone Diffusion of Electrons and Positrons from Geminga Explains the Positron Anomaly

The Astrophysical journal, 2018-08, Vol.863 (1), p.30

2018

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Propagation of cosmic rays in the AMS-02 era

Physical review. D, 2017-04, Vol.95 (8), Article 083007

2017

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Possible origin of the slow-diffusion region around Geminga

Monthly notices of the Royal Astronomical Society, 2019-09, Vol.488 (3), p.4074-4080

2019

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Reanalysis of the Pulsar Scenario to Explain the Cosmic Positron Excess Considering the Recent Developments

The Astrophysical journal, 2019-10, Vol.884 (2), p.124

2019

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Hybrid ViT-CNN Network for Fine-Grained Image Classification

IEEE signal processing letters, 2024, Vol.31, p.1109-1113

2024

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DAMPE Proton Spectrum Indicates a Slow-diffusion Zone in the nearby ISM

The Astrophysical journal, 2020-11, Vol.903 (1), p.69

2020

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Nearby SNR: A Possible Common Origin of Multi-messenger Anomalies in the Spectra, Ratios, and Anisotropy of Cosmic Rays

The Astrophysical journal, 2023-10, Vol.956 (2), p.75

2023

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Klein–Nishina Effect and the Cosmic Ray Electron Spectrum

Chinese physics letters, 2021-03, Vol.38 (3), p.39801-131

2021

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Transformers Meet Small Datasets

IEEE access, 2022, Vol.10, p.1-1

2022

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Slow Diffusion is Necessary to Explain the γ-Ray Pulsar Halos

The Astrophysical journal, 2022-09, Vol.936 (2), p.183

2022

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Exploring fermionic dark matter via Higgs boson precision measurements at the Circular Electron Positron Collider

Physical review. D, 2018-03, Vol.97 (5), Article 055004

2018

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Soft scattering evaporation of dark matter subhalos by inner galactic gases

The European physical journal. C, Particles and fields, 2023-09, Vol.83 (9), p.808-10, Article 808

2023

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Perspective on the Cosmic-ray Electron Spectrum above TeV

The Astrophysical journal, 2017-02, Vol.836 (2), p.172

2017

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Geminga SNR: Possible Candidate of the Local Cosmic-Ray Factory

The Astrophysical journal, 2022-02, Vol.926 (1), p.41

2022

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A dark matter model that reconciles tensions between the cosmic-ray e± excess and the gamma-ray and CMB constraints

Physics letters. B, 2017-10, Vol.773, p.448-454

2017

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Adaptive ε-Constraint Multi-Objective Evolutionary Algorithm Based on Decomposition and Differential Evolution

IEEE access, 2021, Vol.9, p.17596-17609

2021

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Nearby source interpretation of differences among light and medium composition spectra in cosmic rays

Frontiers of physics, 2021-04, Vol.16 (2), p.24501, Article 24501

2021

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基于RCNN-LSTM的脑电情感识别研究

自动化学报, 2022-03, Vol.48 (3), p.917-925

2022

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The 750 GeV diphoton excess at the LHC and dark matter constraints

Nuclear physics. B, 2016-08, Vol.909 (C), p.43-64

2016

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Constraining the interaction strength between dark matter and visible matter: II. Scalar, vector and spin-3/2 dark matter

Nuclear physics. B, 2012-07, Vol.860 (1), p.115-151

2012

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Parameters in a class of leptophilic dark matter models from PAMELA, ATIC and FERMI

Physics letters. B, 2009-07, Vol.678 (2), p.168-173

2009

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Fermi Large Area Telescope Detection of Gamma-Ray Emission from the Direction of Supernova iPTF14hls

Astrophysical journal. Letters, 2018-02, Vol.854 (2), p.L18

2018

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Interpretations of the cosmic ray secondary-to-primary ratios measured by DAMPE

Frontiers of physics, 2023-08, Vol.18 (4), p.44301, Article 44301

2023

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Value of Intraplaque Neovascularization on Contrast-Enhanced Ultrasonography in Predicting Ischemic Stroke Recurrence in Patients With Carotid Atherosclerotic Plaque

Korean journal of radiology, 2023-04, Vol.24 (4), p.338-348

2023

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Constraining the interaction strength between dark matter and visible matter: I. Fermionic dark matter

Nuclear physics. B, 2012-01, Vol.854 (2), p.350-374

2012

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Two-zone Diffusion of Electrons and Positrons from Geminga Explains the Positron Anomaly

Propagation of cosmic rays in the AMS-02 era

Possible origin of the slow-diffusion region around Geminga

Reanalysis of the Pulsar Scenario to Explain the Cosmic Positron Excess Considering the Recent Developments

Hybrid ViT-CNN Network for Fine-Grained Image Classification

DAMPE Proton Spectrum Indicates a Slow-diffusion Zone in the nearby ISM

Nearby SNR: A Possible Common Origin of Multi-messenger Anomalies in the Spectra, Ratios, and Anisotropy of Cosmic Rays

Klein–Nishina Effect and the Cosmic Ray Electron Spectrum

Transformers Meet Small Datasets

Slow Diffusion is Necessary to Explain the γ-Ray Pulsar Halos

Exploring fermionic dark matter via Higgs boson precision measurements at the Circular Electron Positron Collider

Soft scattering evaporation of dark matter subhalos by inner galactic gases

Perspective on the Cosmic-ray Electron Spectrum above TeV

Geminga SNR: Possible Candidate of the Local Cosmic-Ray Factory

A dark matter model that reconciles tensions between the cosmic-ray e± excess and the gamma-ray and CMB constraints

Adaptive ε-Constraint Multi-Objective Evolutionary Algorithm Based on Decomposition and Differential Evolution

Nearby source interpretation of differences among light and medium composition spectra in cosmic rays

基于RCNN-LSTM的脑电情感识别研究

The 750 GeV diphoton excess at the LHC and dark matter constraints

Constraining the interaction strength between dark matter and visible matter: II. Scalar, vector and spin-3/2 dark matter

Parameters in a class of leptophilic dark matter models from PAMELA, ATIC and FERMI

Fermi Large Area Telescope Detection of Gamma-Ray Emission from the Direction of Supernova iPTF14hls

Interpretations of the cosmic ray secondary-to-primary ratios measured by DAMPE

Value of Intraplaque Neovascularization on Contrast-Enhanced Ultrasonography in Predicting Ischemic Stroke Recurrence in Patients With Carotid Atherosclerotic Plaque

Constraining the interaction strength between dark matter and visible matter: I. Fermionic dark matter

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