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In relativity, proper time along a timelike world line is defined as the time as measured by a clock following that line. The proper time interval between two events on a world line is the change in proper time, which is independent of coordinates, and is a Lorentz scalar. The interval is the quantity of interest, since proper time itself is fixed only…
Mathematical formalism, Examples in general relativity & Overview
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time proper displaystyle tau coordinate relativity interval clock observer earth events sqrt coordinates dt 10 line frac two world inertial
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Proper time | is a | pseudo-Riemannian arc length of world lines in four-dimensional spacetime | 0.90 | text |
| Proper time | related to Example 1: The twin paradox | For | 0.60 | section |
| Proper time | related to Example 1: The twin paradox | A-coordinates | 0.60 | section |
| Proper time | related to Example 1: The twin paradox | This | 0.60 | section |
| Proper time | related to Example 1: The twin paradox | A-coordinate | 0.60 | section |
| Proper time | related to Example 1: The twin paradox | The | 0.60 | section |
| Proper time | related to Example 1: The twin paradox | Delta | 0.60 | section |
| Proper time | related to Example 1: The twin paradox | So | 0.60 | section |
| Proper time | related to Example 2: The rotating disk | An | 0.60 | section |
| Proper time | related to Example 2: The rotating disk | For | 0.60 | section |
| Proper time | related to Example 2: The rotating disk | Let | 0.60 | section |
| Proper time | related to Example 2: The rotating disk | The | 0.60 | section |
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