Anisotropies of ultrahigh energy cosmic ray nuclei diffusing from extragalactic sources
We obtain the dipolar anisotropies in the arrival directions of ultrahigh energy cosmic ray nuclei diffusing from nearby extragalactic sources. We consider mixed-composition scenarios in which different cosmic ray nuclei are accelerated up to the same maximum rigidity, so that E
| Autores: | , , |
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| Tipo de recurso: | artículo |
| Estado: | Versión publicada |
| Fecha de publicación: | 2015 |
| País: | Argentina |
| Institución: | Consejo Nacional de Investigaciones Científicas y Técnicas |
| Repositorio: | CONICET Digital (CONICET) |
| Idioma: | inglés |
| OAI Identifier: | oai:ri.conicet.gov.ar:11336/55443 |
| Acceso en línea: | http://hdl.handle.net/11336/55443 |
| Access Level: | acceso abierto |
| Palabra clave: | Ultra high energy cosmic rays Anisotropy Diffusion Magnetic fields https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| Sumario: | We obtain the dipolar anisotropies in the arrival directions of ultrahigh energy cosmic ray nuclei diffusing from nearby extragalactic sources. We consider mixed-composition scenarios in which different cosmic ray nuclei are accelerated up to the same maximum rigidity, so that E |
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