Slowly rotating black hole spacetimes in Einstein-Bel-Robinson gravity are constructed to leading order in spin and coupling, and their geodesics, shadows, ISCOs, and massive scalar superradiance are computed, yielding a weak astrophysical constraint on the coupling.
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Slowly rotating black hole solution to Einstein-Bel-Robinson gravity
Slowly rotating black hole spacetimes in Einstein-Bel-Robinson gravity are constructed to leading order in spin and coupling, and their geodesics, shadows, ISCOs, and massive scalar superradiance are computed, yielding a weak astrophysical constraint on the coupling.