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Time Delay of Light in the Gravitational lensing of Supermassive Black Holes in Dark Matter Halos

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arxiv 2403.05682 v3 pith:ADP7HQTD submitted 2024-03-08 gr-qc astro-ph.GA

classification gr-qcastro-ph.GA
keywords darkmattergravitationalhalolensingblacklightdelay
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The dark matter halo has non-negligible effects on the gravitational lensing of supermassive black hole in the galaxy center. Our work presents a study on the time-delay of light in gravitational lensing of black holes enclosed by dark matter halos. To provide a precise description on the distribution of dark matter in galaxies, we choose several famous phenomenological dark matter halo models in astrophysics, including the NFW, Beta, Burkert and Moore models, to carry out the present study. Through numerically calculating the time-delay of light in gravitational lensing, a comparative analysis of the dark matter effects within different halo models has been performed. Assuming typical length scales associated with the galactic gravitational lensing, numerical results indicate that the NFW, Beta, Burkert and Moore dark matter halos can significantly enhance the time delay of light in gravitational lenisng of central supermassive black holes. The enhancing effect becomes more pronounced with a small dark matter halo scale and an increasing dark matter halo mass. Keywords: Black Hole; Gravitational Lensing; Time Delay; Dark Matter Halo

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Eccentricity-Modulated Phase Degeneracy and Distinguishability between Dark Matter and Accretion Disk Environmental Effects in EMRIs

    gr-qc 2026-07 conditional novelty 5.5 of 10

    DM dephasing in EMRIs is nearly eccentricity-independent while disk dephasing is strongly suppressed by e0, so residual SNR and distinguishability time favor slightly eccentric orbits for LISA separation of the two effects.

  2. Black hole in the Dekel-Zhao dark matter profile

    gr-qc 2025-01 reject novelty 4.0 of 10

    A new black hole solution in a Dekel-Zhao dark matter halo is derived, with shadow size and deflection angle depending on halo density and scale radius.

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