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On the Galactic Center Being the Main Source of Galactic Cosmic Rays as Evidenced by Recent Cosmic Ray and Gamma Ray Observations

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arxiv 1101.5192 v4 pith:MQXSRRE3 submitted 2011-01-27 astro-ph.HE hep-ph

classification astro-ph.HEhep-ph
keywords cosmicgalacticgcrsgammarayscenterpairproduce
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abstract

We revisit the idea that the Galactic center (GC) is the dominant source of Galactic cosmic rays (GCRs), based on a series of new observational evidence. A unified model is proposed to explain the new phenomena of GCRs and $\gamma$-rays simultaneously. The GCRs are thought to be accelerated during past activities of the GC. The pair production process of GCRs in the strong radiation field due to the GC activity is responsible for the knee structure of the cosmic ray spectra. A f raction of $e^+e^-$ produced by pair production interactions, can be reaccelerated in the induced bipolar jets and be transported into the halo, leaving the Fermi $\gamma$-ray bubbles and WMAP microwave haze as the remnant signal. Finally, the CRs diffuse in the bulge could further interact with the interstellar medium to produce low energy $e^+e^-$. After cooling down, these positrons may annihilate to produce the 511 keV line emission as discovered by INTEGRAL.

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Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Correlation of high energy neutrinos and gamma rays on the direction of Fermi Bubbles

    astro-ph.HE 2019-08 conditional novelty 3.0 of 10

    A lepto-hadronic fit to Fermi-LAT and IceCube data finds no single model connects the selected neutrino events to the Northern Fermi Bubble, while the Southern Bubble remains unexcluded.

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