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Magnetorotational collapse of supermassive stars: Black hole formation, gravitational waves, and jets
We perform magnetohydrodynamic simulations in full general relativity of uniformly rotating stars that are marginally unstable to collapse. These simulations model the direct collapse of supermassive stars (SMSs) to seed black holes that can grow to become the supermassive black holes at the centers...
Enregistré dans:
| Publié dans: | Phys Rev D |
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| Auteurs principaux: | , , , |
| Format: | Artigo |
| Langue: | Inglês |
| Publié: |
2017
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| Sujets: | |
| Accès en ligne: | https://ncbi.nlm.nih.gov/pmc/articles/PMC6053688/ https://ncbi.nlm.nih.gov/pubmed/30038964 https://ncbi.nlm.nih.govhttp://dx.doi.org/10.1103/PhysRevD.96.043006 |
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