Analytic calculations of the spectra of ultra-high energy cosmic ray nuclei. I. The case of CMB radiation

Astronomy and Astrophysics – Astrophysics

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The paper is the first part of a two papers series, it is composed by 36 pages, 4 appendixes and 22 eps figures

Scientific paper

We present a systematic study of different methods for analytic calculations of diffuse spectra of ultra-high energy cosmic rays nuclei. Nuclei propagating in the intergalactic space are photo-disintegrated and decrease their Lorentz factor due to the interaction with Cosmic Microwave Background (CMB) and Extragalactic Background Light (EBL). We calculate the evolution trajectories in the backward time, that describe how atomic mass number $A$ and the Lorentz factor $\Gamma$ change with redshift $z$. Three methods of spectra calculations are investigated and compared: {\it (i)} trajectory method, {\it(ii)} kinetic equation combined with trajectory calculations and {\it (iii)} coupled kinetic equations. We believe that these three methods exhaust at least the principal possibilities for any analytic solution of the problem. An important element of the calculations for all methods is the systematic use of Lorentz factor instead of energy. We consider here the interaction of nuclei only with CMB, this case is particularly suitable for understanding of the physical results. In paper (II) of this series the EBL will be also included. Estimating the uncertainties of all methods discussed above, we conclude that the method of coupled kinetic equations gives the most reliable results.

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