Non-Keplerian Charged Accretion Disk Orbiting a Black Hole Pulsar
Recent studies have focused on how spinning black holes (BHs) within a binary system containing a strongly magnetized neutron star, then immersed in external magnetic fields, can acquire charge through mechanisms like the Wald process and how this charge could power pulsar-like electromagnetic radia...
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| Autors principals: | , |
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| Format: | Artigo |
| Idioma: | Inglês |
| Publicat: |
MDPI AG
2025-02-01
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| Col·lecció: | Universe |
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| Accés en línia: | https://www.mdpi.com/2218-1997/11/2/45 |
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