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Kinetic Simulations of Radiative Magnetic Reconnection in the Coronae of Accreting Black Holes

Kinetic Simulations of Radiative Magnetic Reconnection in the Coronae of Accreting Black Holes

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2278322390

Kinetic Simulations of Radiative Magnetic Reconnection in the Coronae of Accreting Black Holes

About this item

Full title

Kinetic Simulations of Radiative Magnetic Reconnection in the Coronae of Accreting Black Holes

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2020-07

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

We perform two- and three-dimensional particle-in-cell simulations of reconnection in magnetically-dominated pair plasmas subject to strong Compton cooling. Reconnection under such conditions operates in accretion disk coronae around black holes, which produce hard X-rays through Comptonization. Our simulations show that most of the plasma in the r...

Alternative Titles

Full title

Kinetic Simulations of Radiative Magnetic Reconnection in the Coronae of Accreting Black Holes

Authors, Artists and Contributors

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_2278322390

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_2278322390

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.1908.08138

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