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SageMath notebooks associated to the Black Hole Lectures (https://luth.obspm.fr/~luthier/gourgoulhon/bh16)
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Effective potential for timelike geodesic motion in Schwarzschild spactime
This Jupyter/SageMath worksheet is relative to the lectures Geometry and physics of black holes.
Click here to download the worksheet file (ipynb format). To run it, you must start SageMath with the Jupyter notebook, with the command sage -n jupyter
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Effective potential
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Circular orbits
Circular orbits are obtained by imposing and , which imply :
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l=0: r1=0, r2=0
l=2: r1=-2*sqrt(-2) + 2, r2=2*sqrt(-2) + 2
l=3.00000000000000: r1=4.50000000000000 - 2.59807621135332*I, r2=4.50000000000000 + 2.59807621135332*I
l=2*sqrt(3): r1=6, r2=6
l=3.80000000000000: r1=4.25210512315547, r2=10.1878948768445
l=4.20000000000000: r1=3.83277632344408, r2=13.8072236765559
l=4.60000000000000: r1=3.61893686280608, r2=17.5410631371939
l=5.00000000000000: r1=3.48612181134003, r2=21.5138781886600
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Coordinate on a circular orbit of angular momentum :
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Non-circular orbits
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