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EPJC-2021-vacaru-1.jpg
We construct nonassociative quasi-stationary solutions describing deformations of Schwarzschild black holes, BHs, to ellipsoid configurations, which can be black ellipsoids, BEs, and/or BHs with ellipsoidal accretion disks. Such solutions are defined…
Output Formats

atom, dcmes-xml, json, omeka-xml, rss2