Graduate Why Can't We Detect Cosmic Rays Beyond the GZK Limit?

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Cosmic rays with energies exceeding approximately 10^20 eV cannot be detected due to the Greisen-Zatsepin-Kuz'min (GZK) limit, which suggests that such high-energy protons interact with the cosmic microwave background (CMB) and lose energy. The discussion highlights confusion regarding the interaction of protons with the CMB and the implications of neutrino interactions in creating high-energy hadrons. It is clarified that high-energy particles do indeed interact with the CMB, contradicting the notion that they do not. The complexities of cosmic ray detection and the associated paradoxes are acknowledged, emphasizing the challenges in understanding these extreme-energy cosmic phenomena. Overall, the inability to detect cosmic rays beyond the GZK limit is linked to their interactions with the CMB.
Zuzana
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Hello,
I would like to ask, why there cannot be detected cosmic rays with energies higher than ~ 10^20 eV, i.e. beyond the GZK limit?

Thanks a lot in advance for the answer.
 
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What have you found out? For example, did you look on Wikipedia? What was hard to understand?
 
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I do not understand why proton with energy > 50 EeV cannot interact with CMB, because there is a cosmic ray paradox and one of possible explanations is that neutrino and antineutrino interacts and create hadrons with extreme energies, is there for these extreme-energy CRs interaction with CMB or not?
 
That may be the longest sentence I have read in a while. I have a hard time parsing it, but you seem to have the sign of the limit backwards. High energy particles do interact with the CMB.
 
This is an alert about a claim regarding the standard model, that got a burst of attention in the past two weeks. The original paper came out last year: "The electroweak η_W meson" by Gia Dvali, Archil Kobakhidze, Otari Sakhelashvili (2024) The recent follow-up and other responses are "η_W-meson from topological properties of the electroweak vacuum" by Dvali et al "Hiding in Plain Sight, the electroweak η_W" by Giacomo Cacciapaglia, Francesco Sannino, Jessica Turner "Astrophysical...

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