Ultra-high-energy cosmic ray acceleration by magnetic reconnection in newborn pulsars
We investigate the possibility that the ultra-high energy cosmic ray (UHECR)events observed above the GZK limit are mostly protons accelerated in reconnectionsites just above the magnetosphere of newborn millisecond pulsars that areoriginated by accretion induced collapse (AIC).
I tiakina i:
| I whakaputaina i: | Revista Mexicana de Astronomía y Astrofísica |
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| Ngā kaituhi matua: | , |
| Hōputu: | Artigo |
| Reo: | Inglês |
| I whakaputaina: |
Universidad Nacional Autónoma de México
2000
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| Ngā marau: | |
| Urunga tuihono: | https://www.redalyc.org/articulo.oa?id=57100923 |
| Ngā Tūtohu: |
Kāore He Tūtohu, Me noho koe te mea tuatahi ki te tūtohu i tēnei pūkete!
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