Coherence length of cosmic background radiation enlarges the attenuation length of the ultra-high energy proton

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

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8 pages, 2 figures,study about the second coherence length has been added

Scientific paper

It is pointed out that an agreement of the one particle energy spectrum of the cosmic background radiation (CMBR) with Plank distribution of 2.725 [K] does not give a strong constraint on the coherence length of CMBR if the mean free path of CMBR is very long. The coherence length in this situation is estimated as a few times of $k_BT$. Due to this finite coherence length, the attenuation length of ultra-high energy cosmic rays (UHECR) is reduced in the $\Delta $ resonance region,i.e., around $10^{20}$ [eV]. The small attenuation length makes the suppression of the flux of cosmic rays in this energy region less prominent than the naive estimation

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