Derivation of muon spectrum at high energies from the recent JACEE primary cosmic-ray spectrum using Fermilab data on meson production

1992 ◽  
Vol 15 (4) ◽  
pp. 401-407 ◽  
Author(s):  
Pratibha Pal ◽  
D. P. Bhattacharyya
2012 ◽  
Vol 349 ◽  
pp. 011001
Author(s):  
Giorgio Giardina ◽  
Fabio Bossi ◽  
Paolo Levi Sandri ◽  
Paolo Pedroni ◽  
Hartmut Schmieden

2001 ◽  
Vol 64 (2) ◽  
pp. 266-274 ◽  
Author(s):  
L. V. Volkova ◽  
G. T. Zatsepin

2015 ◽  
Vol 2 ◽  
pp. 39-44 ◽  
Author(s):  
P. L. Biermann ◽  
L. I. Caramete ◽  
A. Meli ◽  
B. N. Nath ◽  
E.-S. Seo ◽  
...  

Abstract. A model is introduced, in which the irregularity spectrum of the Galactic magnetic field beyond the dissipation length scale is first a Kolmogorov spectrum k-5/3 at small scales λ = 2 π/k with k the wave-number, then a saturation spectrum k-1, and finally a shock-dominated spectrum k-2 mostly in the halo/wind outside the Cosmic Ray disk. In an isotropic approximation such a model is consistent with the Interstellar Medium (ISM) data. With this model we discuss the Galactic Cosmic Ray (GCR) spectrum, as well as the extragalactic Ultra High Energy Cosmic Rays (UHECRs), their chemical abundances and anisotropies. UHECRs may include a proton component from many radio galaxies integrated over vast distances, visible already below 3 EeV.


2014 ◽  
Vol 41 (11) ◽  
pp. 115003 ◽  
Author(s):  
A Kendi Kohara ◽  
Erasmo Ferreira ◽  
Takeshi Kodama
Keyword(s):  

1972 ◽  
Vol 29 (7) ◽  
pp. 445-448 ◽  
Author(s):  
Einar Juliusson ◽  
Peter Meyer ◽  
Dietrich Müller
Keyword(s):  

1963 ◽  
Vol 28 (2) ◽  
pp. 444-445 ◽  
Author(s):  
C. F. Gauld ◽  
C. B. A. McCusker ◽  
L. S. Peak
Keyword(s):  

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