File:Null geodesics from ∞ around an extreme Kerr black hole.gif
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Null_geodesics_from_∞_around_an_extreme_Kerr_black_hole.gif (400 × 400 pixels, file size: 85 KB, MIME type: image/gif, looped, 645 frames, 21 s)
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Captions
Captions
Animation of the trajectory of a photon arriving from infinity and almost captured by an extreme Kerr black hole (ā = 1)
Summary
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| Description |
Français : Avec G constante gravitationnelle, M masse du trou noir, c vitesse de la lumière dans le vide, rs = 2GM/c² et m = GM/c², les constantes de la trajectoire sont :
cLz/mE = -6 avec Lz composante du moment cinétique du photon sur l'axe de rotation du trou noir et E énergie du photon, c²Q/(m²E²) = -13 + 16 racine(2) avec Q constante de Carter.English: With G gravitational constant, M mass of the black hole, c speed of light in vacuum, rs = 2GM/c² and m = GM/c², the trajectory constants are:
cLz/mE = -6 with Lz component of the photon's angular momentum on the black hole's axis of rotation and E photon energy, c²Q/(m²E²) = -13 + 16 sqrt (2), with Q Carter constant. |
| Date | |
| Source | Own work |
| Author | Cornelius Fyla |
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 21:29, 19 May 2024 | | 400 × 400 (85 KB) | Cornelius Fyla (talk | contribs) | Uploaded own work with UploadWizard |
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