Slowly rotating wormholes in Rényi, mixed, and Moradpour holographic dark energy produce distinct photon orbits and shadow morphologies, with Rényi models yielding smaller asymmetric shadows.
Carter, Commun
2 Pith papers cite this work. Polarity classification is still indexing.
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gr-qc 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Increasing the mass of a perturbing scalar field around Einstein-Maxwell-dilaton black holes strongly suppresses damping in several quasinormal branches, producing quasi-resonant long-lived oscillations.
citing papers explorer
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Holographic dark energy as a source for slowly rotating wormholes: Implications for null geodesics and shadows
Slowly rotating wormholes in Rényi, mixed, and Moradpour holographic dark energy produce distinct photon orbits and shadow morphologies, with Rényi models yielding smaller asymmetric shadows.
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Quasi-resonances in the vicinity of Einstein-Maxwell-dilaton black hole
Increasing the mass of a perturbing scalar field around Einstein-Maxwell-dilaton black holes strongly suppresses damping in several quasinormal branches, producing quasi-resonant long-lived oscillations.