We show that recently multi-messenger astronomy has provided compelling evidence that the bulk of high energy cosmic rays (CRs) are produced by highly relativistic narrow jets of plasmoids launched in core collapse of stripped-envelope massive stars to neutron stars and stellar mass black holes. Such events produce also a visible GRB if the jet happens to point in our direction. This has been long advocated by the cannon ball (CB) model of high energy CRs and GRBs, but the evidence has been provided only recently by what were widely believed to be unrelated discoveries. They include the very recent discovery of a knee around TeV in the energy spectrum of high energy CR electrons, the peak photon energy in the “brightest of all time” GRB221009A, and the failure of IceCube to detect high energy neutrinos from GRBs, including GRB221009A. They were all predicted by the cannonball (CB) model of high energy CRs and GRBs long before they were discovered in observations, despite a negligible probability to occur by chance.
Dar, A., Kozlovsky, B.Z., Nussinov, S. and Ramaty, R. (1992) ApJ, 363, 118. https://doi.org/10.1086/171138
[11]
Dar, A. (1998) ApJ, 500, L93. https://doi.org/10.1086/311401
[12]
Dar, A. and Plaga, R. (1999) Astronomy and Astrophysics, 349, 259-266.
[13]
Dar, A. and De Rújula, A. (2008) Physics Reports, 466, 179-241. https://doi.org/10.1016/j.physrep.2008.05.004
[14]
Dado, S. and Dar, A. (2015) ApJ, 812, 38.
[15]
De Rújula, A. (2019) Physics Letters B, 790, 444-452. https://doi.org/10.1016/j.physletb.2019.01.059
[16]
Shaviv, N.J. and Dar, A. (1995) ApJ, 447, 863. https://doi.org/10.1086/175923
[17]
Dado, S., Dar, A. and De Rujula, A. (2022) Universe, 8, Article No. 350. https://doi.org/10.3390/universe8070350
[18]
Zhang, P.-P., Guo, Y.-Q., Qiao, B.-Q. and Liu, W. (2112) Constraining the Position of the Knee in the Galactic Cosmic Ray Spectrum with Ultra-High-Energy Diffuse γ-Rays.
[19]
Kerszberg, D. (2017) Contributions of the High Energy Stereoscopic System (H.E.S.S.) to the 35th International Cosmic Ray Conference (ICRC), Busan, Korea 2017.
[20]
Aharonian, F., et al. (2008) PRL, 101, Article ID: 261104.
Chang, J., et al. (2017) Astroparticle Physics, 95, 6-24.
[24]
Adriani, O., et al. (2018) PRL, 120, Article ID: 261102.
[25]
Frederiks, D., Svinkin, D., Lysenko, A.L., Molkov, S., et al. (2023) The Astrophysical Journal Letters, 949, L7. https://doi.org/10.3847/2041-8213/acd1eb
[26]
Amati, L. (2006) Monthly Notices of the Royal Astronomical Society, 372, 233-245. https://doi.org/10.1111/j.1365-2966.2006.10840.x
