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arxiv: astro-ph/0612735 · v1 · submitted 2006-12-26 · 🌌 astro-ph

Rotating Braneworld Black Holes

classification 🌌 astro-ph
keywords blackholesbraneworldchargerotatingtidalappearanceappears
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We present a Kerr-Newman type stationary and axisymmetric solution that describes rotating black holes with a tidal charge in the Randall-Sundrum braneworld. The tidal charge appears as an imprint of nonlocal gravitational effects from the bulk space. We also discuss the physical properties of these black holes and their possible astrophysical appearance.

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  1. Investigating the interplay of the braneworld gravity and the plasma environment on the black hole shadow

    gr-qc 2025-12 unverdicted novelty 4.0

    Negative tidal charge enlarges the shadow of rotating braneworld black holes while inhomogeneous plasma shrinks it and homogeneous plasma enlarges it; EHT data limits q to roughly -1.15 to 0.45 for M87* in the low-den...