| Revista: | Brazilian journal of physics |
| Base de datos: | PERIÓDICA |
| Número de sistema: | 000379556 |
| ISSN: | 0103-9733 |
| Autores: | Letessier Selvon, Antoine1 |
| Instituciones: | 1Universite Pierre et Marie Curie, Laboratoire de Physique Nucleaire et des Hautes Energies, ´, París. Francia |
| Año: | 2014 |
| Periodo: | Oct |
| Volumen: | 44 |
| Número: | 5 |
| Paginación: | 560-570 |
| País: | Brasil |
| Idioma: | Inglés |
| Tipo de documento: | Conferencia o discurso |
| Enfoque: | Analítico, descriptivo |
| Resumen en inglés | The Pierre Auger Observatory is the world’s largest cosmic ray observatory. Our current exposure reaches nearly 40,000 km2sr and provides us with an unprecedented quality data set. The performance and stability of the detectors and their enhancements are described. Data analyses have led to a number of major breakthroughs. Among these, we discuss the energy spectrum and the searches for large-scale anisotropies. We present analyses of our Xmax data and show how it can be interpreted in terms of mass composition. We also describe some new analyses that extract mass-sensitive parameters from the 100 % duty cycle surface detector (SD) data. A coherent interpretation of all these recent results opens new directions. The consequences regarding the cosmic ray composition and the properties of ultrahigh-energy cosmic ray (UHECR) sources are briefly discussed |
| Disciplinas: | Física y astronomía |
| Palabras clave: | Astronomía, Observatorios astronómicos, Rayos cósmicos de ultra-alta energía, Espectro de energía |
| Keyword: | Physics and astronomy, Astronomy, Astronomical observatories, Ultrahigh-energy cosmic rays, Energy spectrum |
| Texto completo: | Texto completo (Ver PDF) |
