Zobrazeno 1 - 6
of 6
pro vyhledávání: '"Rita C. dos Anjos"'
Publikováno v:
Galaxies, Vol 10, Iss 4, p 83 (2022)
The investigation about cosmic-ray sources through the study of the arrival direction of the particles is completely dependent on primary mass compositions. This is due to heavier particles having an average larger deflection during propagation in ga
Externí odkaz:
https://doaj.org/article/a964482300a944778611b6b298e9ba84
Publikováno v:
Galaxies, Vol 10, Iss 4, p 84 (2022)
The source, origin, and acceleration mechanisms of ultra-high-energy cosmic rays (UHECR) (E>1020 eV, beyond the GZK limit) remain uncertain and unclear. The main explanations are associated with particular mechanisms, such as the Fermi mechanism, in
Externí odkaz:
https://doaj.org/article/54dc4b48349e4800ba2c069387b7a9cf
Autor:
Jaziel G. Coelho, Rita. C. Dos Anjos
Publikováno v:
Galaxies, Vol 11, Iss 2, p 48 (2023)
The era of multi-messenger astronomy has recently be inaugurated with pioneering experiments, theoretical interpretation, and models [...]
Externí odkaz:
https://doaj.org/article/6623b0e709f94ca09842314b2700d9a8
Autor:
Rita C. dos Anjos, Rodrigo Sasse
Publikováno v:
Proceedings of 37th International Cosmic Ray Conference — PoS(ICRC2021).
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::b87c1abbf5cc88edae8f0d7b2e94c604
https://doi.org/10.22323/1.395.0461
https://doi.org/10.22323/1.395.0461
Autor:
Rita C. dos Anjos, Fernando Catalani
Publikováno v:
Repositório Institucional da USP (Biblioteca Digital da Produção Intelectual)
Universidade de São Paulo (USP)
instacron:USP
Universidade de São Paulo (USP)
instacron:USP
After the discovery of Fermi Bubbles and the excess of gamma-ray emission, the Galactic Centre has received increasing attention with the aim to understand its role in the origin and acceleration of primary cosmic rays (CRs). Based on a diffusion/re-
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::d3d0342e1ca5aa5a208f0cf2cda124b7
http://arxiv.org/abs/2006.02584
http://arxiv.org/abs/2006.02584
Autor:
Lawrence Wiencke, Roberto J. Moncada, Luis A. Anchordoqui, T. Paul, Angela V. Olinto, John Krizmanic, Diego F. Torres, F. Sarazin, Timothy A. D. Paglione, Rita C. dos Anjos, Jorge F. Soriano
The sources of ultrahigh-energy cosmic rays (UHECRs) have been difficult to catch. It was recently pointed out that while sources of UHECR protons exhibit anisotropy patterns that become denser and compressed with rising energy, nucleus-emitting-sour
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_dedup___::b1740071f9e3c98cce7ae445cbd6ff0b
http://arxiv.org/abs/1810.04251
http://arxiv.org/abs/1810.04251