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¿Supernova - origen remanente de los rayos cósmicos?
Yousaf M Butt1, Diego F Torres, Gustavo E Romero
1Harvard-Smithsonian Center for Astrophysics, Cambridge, Massachusetts 02138, USA. ybutt@cfa.harvard.edu
Nature
|August 2, 2002
Resumen
La aceleración de los núcleos de rayos cósmicos galácticos en los restos de supernovas sigue sin ser confirmada. Una nueva investigación desafía las afirmaciones de evidencia definitiva, lo que sugiere que el origen de estas partículas de alta energía sigue siendo incierto.
Área de la Ciencia:
- La astrofísica es la astrofísica.
- Física de las partículas Física de las partículas
Sus antecedentes:
- Los remanentes de supernovas (SNR) son aceleradores hipotéticos de núcleos de rayos cósmicos galácticos a altas energías (hasta 300 TeV / núcleo).
- La confirmación observacional directa de este mecanismo de aceleración se ha buscado desde 1953.
- Las afirmaciones recientes sugirieron que los rayos gamma del rango TeV de SNR RX J1713.7-3946 proporcionan evidencia definitiva.
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