ELECTRON/POSITRON EXCESSES IN THE COSMIC RAY SPECTRUM AND POSSIBLE INTERPRETATIONS

DOI10.1142/S0218271810018268zbMath1205.85034arXiv1008.4646OpenAlexW3122160430MaRDI QIDQ3070382

Jin Chang, Bing Zhang, Yizhong Fan

Publication date: 3 February 2011

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1008.4646

zbMATH Keywords

pulsardark matterparticlesupernova remnants\(e^{\pm }\) excess

Mathematics Subject Classification ID

Electromagnetic theory (general) (78A25) Equations of motion in general relativity and gravitational theory (83C10) Radiative transfer in astronomy and astrophysics (85A25) Astrophysical cosmology (85A40)

Related Items (1)

Gravitational Bhabha scattering

Cites Work

• Common gauge origin of discrete symmetries in observable sector and hidden sector
• Electroweak and dark matter constraints on a \(Z^{\prime}\) in models with a hidden valley
• Diffuse gamma ray constraints on annihilating or decaying dark matter after Fermi
• White dwarf axions, PAMELA data, and flipped-\(SU(5)\)
• Model-independent implications of the \(e^{\pm }\), \(\bar{p}\) cosmic ray spectra on properties of Dark Matter
• Inverse compton constraints on the dark matter \(e^{\pm }\) excesses
• UNDERSTANDING THE VERY-HIGH-ENERGY EMISSION FROM MICROQUASARS
• Über die Beugung und Bremsung der Elektronen

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