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Magnetic Reconnection and Hot Spot Formation in Black Hole Accretion Disks

4 Pith papers cite this work. Polarity classification is still indexing.

4 Pith papers citing it

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years

2026 3 2025 1

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UNVERDICTED 4

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representative citing papers

Photon spheres in dynamical space-times

gr-qc · 2026-06-01 · unverdicted · novelty 7.0

A covariant framework is developed for photon surfaces in dynamical spherical spacetimes, recovering static limits and applied to collapse and accretion/evaporation models.

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Showing 4 of 4 citing papers.

  • Photon spheres in dynamical space-times gr-qc · 2026-06-01 · unverdicted · none · ref 51

    A covariant framework is developed for photon surfaces in dynamical spherical spacetimes, recovering static limits and applied to collapse and accretion/evaporation models.

  • Relative Magnification Factor of Point Sources on Accretion Disks gr-qc · 2026-04-10 · unverdicted · none · ref 49

    Corotating point sources on accretion disks near black holes distort the relative magnification factor distribution, modulating caustics and encoding accretion flow kinematics via time-delayed images.

  • Testing solitonic boson star interpretations of Sagittarius A* with near-infrared flare astrometry astro-ph.HE · 2026-04-23 · unverdicted · none · ref 42

    Fitting GRAVITY flare astrometry to solitonic boson star models requires masses larger than 4.3 million solar masses, with more diffuse models yielding values closer to the standard black hole mass and thus placing stringent but incomplete constraints on such interpretations of Sgr A*.

  • Energy extraction from a rotating black hole via magnetic reconnection: Bumblebee gravity gr-qc · 2025-10-27 · unverdicted · none · ref 5

    In a Kerr-Sen-like spacetime from Bumblebee gravity, increasing the Lorentz symmetry breaking rate and Bumblebee charge enlarges the allowed region for energy extraction via magnetic reconnection and moves it closer to the horizon, with peak efficiency when cosmic censorship is marginally violated.