The causal structure of black holes, including horizons and interiors, can be encoded in wind-Finsler metrics whose shifted indicatrices track null geodesics.
Finsler, ¨Uber Kurven und Fl¨ achen in allgemeinen R¨ aumen, G¨ ottingen University Dissertation (1918)
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Wind-Finslerian structure of black holes
The causal structure of black holes, including horizons and interiors, can be encoded in wind-Finsler metrics whose shifted indicatrices track null geodesics.