Physical Interpretation of Coordinates for the Schwarzschild Metric
Tarun Biswas

TL;DR
This paper explores various coordinate systems for the Schwarzschild metric, aiming to find physically meaningful interpretations and discussing how different coordinates relate to the presence of black holes and the nature of the horizon.
Contribution
It analyzes well-known and lesser-known coordinate systems to understand their physical significance and how they relate to the black hole interior and horizon.
Findings
Coordinate systems differ in their origin placement and physical interpretation.
Some coordinates exclude the black hole interior, potentially offering more physically acceptable models.
Mathematical signature distinctions help differentiate time and space coordinates across horizons.
Abstract
Since its first introduction, the Schwarzschild metric has been written in various coordinate systems. This has been done primarily to understand the nature of the coordinate singularity at the event horizon. However, very often, the mathematics of a coordinate system does not provide a clear physical interpretation. In Schwarzschild's original work, the origin of the radial coordinate was at the event horizon. Hence, there was no black hole. The generally accepted current definition of the radial coordinate has an origin beyond the horizon. This necessitates the discussion of black holes. Here, some well-known and some not-so-well-known coordinate systems will be visited in search of a physical interpretation. It will be noted that they all agree at large radial distances. However, the location of the origin of the radial coordinate can be different for different systems. Some…
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Taxonomy
TopicsGeophysics and Gravity Measurements · Relativity and Gravitational Theory · Geophysics and Sensor Technology
