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File:Equatorial null geodesics from ∞ around an extreme Kerr black hole (top view).png

Equatorial_null_geodesics_from_∞_around_an_extreme_Kerr_black_hole_(top_view).png ‎(400 × 400 pixels, file size: 56 KB, MIME type: image/png)

Captions

Captions

Top view of an equatorial trajectory of a photon coming from infinity around an extreme Kerr black hole (ā = 1)

Summary

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Description
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/c²
English: 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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Date/TimeThumbnailDimensionsUserComment
current22:00, 19 May 2024Thumbnail for version as of 22:00, 19 May 2024400 × 400 (56 KB)Cornelius Fyla (talk | contribs)Uploaded own work with UploadWizard

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