principle of equivalence
Học thuậtThân thiện
Definition
Noun: 1. (Physics) A foundational concept in the theory of general relativity stating that the effects of gravity are locally indistinguishable from the effects of acceleration. An observer in a closed laboratory cannot determine through any experiment whether the laboratory is at rest in a gravitational field or is accelerating in the absence of gravity.
Usage Examples
- Noun:
- Einstein's principle of equivalence was a crucial step in the development of his theory of general relativity.
- The principle of equivalence implies that inertial mass and gravitational mass are identical.
Advanced Usage
- "Strong equivalence principle": A more stringent version that extends the principle to all laws of nature, including those governing gravitational interactions themselves.
- The strong equivalence principle is a key feature of Einstein's theory and is tested by observing the motion of compact objects.
- "Weak equivalence principle": The foundational form, often tested by experiments demonstrating that all objects fall with the same acceleration in a gravitational field, independent of their mass or composition.
- Experiments with torsion balances provide precise tests of the weak equivalence principle.
Variants and Related Words
- Equivalence principle (noun): A common shortened form of "principle of equivalence."
- General relativity (noun): The theory of gravitation whose foundation is the principle of equivalence.
Synonyms
- Equivalence postulate (noun): A less common synonym emphasizing its axiomatic role in the theory.
Related Phrases
- Local Lorentz invariance: A related concept stating that in small enough regions of spacetime, the laws of special relativity hold.
- The principle of equivalence is closely connected to the idea of local Lorentz invariance.
Noun
- (physics) the principle that an observer has no way of distinguishing whether his laboratory is in a uniform gravitational field or is in an accelerated frame of reference