Kernel: SageMath 8.0
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Spacetime: black hole extension
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4-dimensional differentiable manifold M
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We introduce the new coordinate such that . The metric thus takes the following form:
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No coordinate singularity appears for in the metric and inverse metric. It allows to cross both the outer and inner horizons, if they exist.
Radial null vectors
Outgoing null vector
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Ingoing null vector
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Check that is a null vector
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Check that is a null vector
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Normalization
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Induced metric
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Expansion of a congruence of null geodesics
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Levi-Civita connection nabla_g associated with the Lorentzian metric g on the 4-dimensional differentiable manifold M
Check that the covariant derivative does not act on the metric:
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Scalar field on the 4-dimensional differentiable manifold M
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The zeros of , hence of , correspond to the presence of horizons. The region with , where the expansion of outgoing null rays becomes negative, is a (future) trapped region.
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Scalar field on the 4-dimensional differentiable manifold M
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The expansion of ingoing radial null rays is strictly negative, which is expected in the presence of a .
Ricci's scalar
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Kretschmann's scalar
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Tensor field Riem(g) of type (1,3) on the 4-dimensional differentiable manifold M
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