Indications for a high-rigidity break in the cosmic-ray diffusion coefficient (2017)
Source: Physical Review Letters. Unidade: IFSC
Subjects: FÍSICA DE ALTA ENERGIA, ENERGIA, RAIOS CÓSMICOS, ASTROFÍSICA
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GÉNOLINI, Yoann et al. Indications for a high-rigidity break in the cosmic-ray diffusion coefficient. Physical Review Letters, v. 119, n. 24, p. 241101-1-241101-6, 2017Tradução . . Disponível em: https://doi.org/10.1103/PhysRevLett.119.241101. Acesso em: 14 set. 2024.APA
Génolini, Y., Serpico, P. D., Boudaud, M., Caroff, S., Poulin, V., Derome, L., et al. (2017). Indications for a high-rigidity break in the cosmic-ray diffusion coefficient. Physical Review Letters, 119( 24), 241101-1-241101-6. doi:10.1103/PhysRevLett.119.241101NLM
Génolini Y, Serpico PD, Boudaud M, Caroff S, Poulin V, Derome L, Lavalle J, Maurin D, Poireau V, Rosier S, Salati P, Vecchi M. Indications for a high-rigidity break in the cosmic-ray diffusion coefficient [Internet]. Physical Review Letters. 2017 ; 119( 24): 241101-1-241101-6.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevLett.119.241101Vancouver
Génolini Y, Serpico PD, Boudaud M, Caroff S, Poulin V, Derome L, Lavalle J, Maurin D, Poireau V, Rosier S, Salati P, Vecchi M. Indications for a high-rigidity break in the cosmic-ray diffusion coefficient [Internet]. Physical Review Letters. 2017 ; 119( 24): 241101-1-241101-6.[citado 2024 set. 14 ] Available from: https://doi.org/10.1103/PhysRevLett.119.241101