Radiative plasma simulations of black hole accretion flow coronae in the hard and soft states
Radiative plasma simulations of black hole accretion flow coronae in the hard and soft states
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Ithaca: Cornell University Library, arXiv.org
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English
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Ithaca: Cornell University Library, arXiv.org
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Stellar-mass black holes in x-ray binary systems are powered by mass transfer from a companion star. The accreted gas forms an accretion disk around the black hole and emits x-ray radiation in two distinct modes: hard and soft state. The origin of the states is unknown. We perform radiative plasma simulations of the electron-positron-photon corona...
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Full title
Radiative plasma simulations of black hole accretion flow coronae in the hard and soft states
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TN_cdi_proquest_journals_3093676521
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https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_3093676521
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E-ISSN
2331-8422
DOI
10.48550/arxiv.2408.08161
