Numerical ray-tracing of Vaidya black holes reveals a dynamical redshift ring that emerges, contracts inward, and brightens during accretion, alongside evolving shadows and lensing rings.
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2 Pith papers cite this work. Polarity classification is still indexing.
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gr-qc 2years
2026 2representative citing papers
Simulated polarization images of non-topological soliton Bardeen boson stars show that magnetic field geometry and scalar parameters produce distinct Q-U loop fragmentation absent in black hole spacetimes.
citing papers explorer
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Gravitational lensing and observational features of a dynamic black hole
Numerical ray-tracing of Vaidya black holes reveals a dynamical redshift ring that emerges, contracts inward, and brightens during accretion, alongside evolving shadows and lensing rings.
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Polarization images of non-topological soliton Bardeen boson stars
Simulated polarization images of non-topological soliton Bardeen boson stars show that magnetic field geometry and scalar parameters produce distinct Q-U loop fragmentation absent in black hole spacetimes.