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In relativity theory, proper acceleration is the physical acceleration (i.e., measurable acceleration as by an accelerometer) experienced by an object. It is thus acceleration relative to a free-fall, or inertial, observer who is momentarily at rest relative to the object being measured. Gravitation therefore does not cause proper acceleration, because…
Applications, Classical applications & Viewed from a flat spacetime slice
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| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| Proper acceleration | is a | physical acceleration | 0.90 | text |
| Proper acceleration | is a | rate of change of proper velocity with respect to coordinate time.In an inertial frame in which the object is momentarily at rest | 0.90 | text |
| Proper acceleration | is a | acceleration felt by the occupants | 0.90 | text |
| Proper acceleration | has application | At | 0.60 | section |
| Proper acceleration | has application | Newtonian | 0.60 | section |
| Proper acceleration | has application | As | 0.60 | section |
| Proper acceleration | has application | Newton's | 0.60 | section |
| Proper acceleration | has application | If | 0.60 | section |
| Proper acceleration | has application | For | 0.60 | section |
| Proper acceleration | has application | Thus | 0.60 | section |
| Proper acceleration | related to Acceleration in (1+1)D | In | 0.60 | section |
| Proper acceleration | related to Acceleration in (1+1)D | Lorentz | 0.60 | section |
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