Special relativity (1905) governs physics without gravity and predicts time dilation, length contraction, and the relativity of simultaneity using Lorentz transformations.
Einstein’s theory of relativity consists of two interrelated theories: special relativity (proposed in 1905) and general relativity (published in 1915). Special relativity applies to all physical phenomena in the absence of gravity and is based on two postulates that replace classical mechanics’ assumptions with Lorentz transformations. It leads to effects such as relativity of simultaneity, time dilation, length contraction, a finite maximum speed (the speed of light), and mass–energy equivalence (E = mc2). General relativity extends these ideas to gravitation and explains the law of gravitation as a feature of spacetime itself. It begins with the equivalence principle, treating accelerated motion and free-fall in a gravitational field as physically identical, which implies that free fall is inertial motion. Einstein then formulated gravity using curved spacetime and the Einstein field equations, linking spacetime curvature to mass, energy, and momentum. The theory predicts phenomena including gravitational time dilation, orbital precession, light deflection, frame-dragging, and cosmic expansion, and it has been repeatedly confirmed by experiments and observations. Both theories are “principle-theories” grounded in experimentally verified regularities, making testable predictions. Special relativity was validated through key experiments such as Michelson–Morley, Kennedy–Thorndike, and Ives–Stilwell, while general relativity has been confirmed by classic tests like Mercury’s perihelion precession, deflection of light by the Sun, and gravitational redshift. Relativity also became essential for practical technologies (e.g., GPS) and for explaining major astrophysical discoveries such as neutron stars, black holes, and gravitational waves.
Special relativity (1905) governs physics without gravity and predicts time dilation, length contraction, and the relativity of simultaneity using Lorentz transformations.
General relativity (1915) explains gravity via curved spacetime using the Einstein field equations, predicting effects like gravitational time dilation, light deflection, and frame-dragging.
Relativity’s predictions are experimentally testable: special relativity was validated by Michelson–Morley, Kennedy–Thorndike, and Ives–Stilwell, while general relativity is supported by classic tests such as Mercury’s perihelion precession and gravitational redshift.
Relativity transformed 20th-century physics and astronomy and is required for precision engineering and navigation systems such as GPS.
A theory describing the structure of spacetime in the absence of gravity, based on Lorentz transformations and predicting effects like time dilation and length contraction.
A theory of gravitation in which spacetime is curved, with the Einstein field equations relating curvature to mass, energy, and momentum.
The principle that accelerated motion and being at rest in a gravitational field are physically identical, implying that free fall is inertial motion.
The mathematical transformations that replace Galilean transformations in special relativity and preserve the speed of light across inertial frames.
The equations of general relativity that determine how spacetime curvature (via a metric tensor) is produced by mass, energy, and momentum.
The idea that whether two events are simultaneous depends on the observer’s relative motion.
The prediction that clocks run slower in stronger gravitational fields (deeper gravitational wells).
A general relativity effect where rotating masses influence the motion of spacetime itself, effectively dragging nearby spacetime around them.
The special relativity relation stating that mass and energy are interchangeable forms of the same physical quantity.
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