File:Equatorial null geodesics from ∞ around an extreme Kerr black hole.png
Equatorial_null_geodesics_from_∞_around_an_extreme_Kerr_black_hole.png (400 × 400 pixels, file size: 55 KB, MIME type: image/png)
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Summary
editDescriptionEquatorial null geodesics from ∞ around an extreme Kerr black hole.png |
Français : Effet Lense-Thirring : le photon est entraîné dans le sens du rotation du trou noir avant de rentrer dans l'ergosphère externe.
Le photon rejoint ensuite l'anneau de singularité nue de rayon cartésien = a. Constantes de la trajectoire : cL/E = 6,772 GM/c² avec c vitesse de la lumière dans le vide, L norme du moment cinétique du photon, E énergie du photon, Q constante de Carter = 0. G constante gravitationnelle, M masse du trou noir, a = GM/c² et rs = 2GM/c²English: Lense-Thirring effect: the photon is dragged in the direction of the black hole's spin before entering the outer ergosphere.
The photon then joins the naked singularity ring of Cartesian radius = a. Trajectory constants: cL/E = 6.772 GM/c² with c speed of light in vacuum, L norm of the photon's angular momentum, E photon energy, Q Carter constant = 0. G gravitational constant, M black hole mass, a = GM/c² and rs = 2GM/c² |
Date | |
Source | Own work |
Author | Cornelius Fyla |
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current | 21:53, 19 May 2024 | 400 × 400 (55 KB) | Cornelius Fyla (talk | contribs) | Uploaded own work with UploadWizard |
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File change date and time | 19:50, 14 April 2024 |
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