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| | '''Relativity''' refers to two theories in [[physics]], and to a principle which led to the first theory. Special relativity (SR) is a theory which describes the laws of motion for non-accelerating bodies traveling at a significant fraction of the speed of light. At speeds approaching zero, special relativity is identical to Newton's Laws of Motion. Special relativity was developed by [[Hendrik Lorentz]], [[Henri Poincaré]] and [[Albert Einstein]]. | | '''Relativity''' refers to two theories in [[physics]], and to a principle which led to the first theory. Special relativity (SR) is a theory which describes the laws of motion for non-accelerating bodies traveling at a significant fraction of the speed of light. At speeds approaching zero, special relativity is identical to Newton's Laws of Motion. Special relativity was developed by [[Hendrik Lorentz]], [[Henri Poincaré]] and [[Albert Einstein]]. |
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| − | General Relativity (GR) is a theory which explains the laws of motion as viewed from accelerating reference frames and includes a geometric explanation for gravity. This theory was developed by [[Albert Einstein]] as an extension of the postulates of Special Relativity. A dramatic but later discredited claim by Sir [[Arthur Eddington]] of experimental proof of General Relativity in 1919 made Einstein a household name. | + | General Relativity (GR) is a theory which explains the laws of motion as viewed from accelerating reference frames and includes a geometric explanation for gravity. This theory was developed by [[David Hilbert]] and [[Albert Einstein]] as an extension of the postulates of Special Relativity.<ref>"[T]he German mathematician David Hilbert submitted an article containing the correct field equations for general relativity five days before Einstein."[http://nobelprize.org/educational_games/physics/relativity/history-1.html Nobel Prize historical account]</ref> A dramatic but later discredited claim by Sir [[Arthur Eddington]] of experimental proof of General Relativity in 1919 made Einstein a household name. |
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| | == Special Relativity == | | == Special Relativity == |
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| | Special relativity is the limiting case of general relativity where all gravitational fields are weak. | | Special relativity is the limiting case of general relativity where all gravitational fields are weak. |
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| − | ===Time dilation===
| + | ==Time dilation== |
| | [[Image:Light cone.png|right|thumb|Light-cone diagram]] | | [[Image:Light cone.png|right|thumb|Light-cone diagram]] |
| | One important consequence of SR's postulates is that an observer in one reference frame will observe a clock in another frame to be "ticking" more slowly than in the observer's own frame. This can be proven mathematically using basic geometry. | | One important consequence of SR's postulates is that an observer in one reference frame will observe a clock in another frame to be "ticking" more slowly than in the observer's own frame. This can be proven mathematically using basic geometry. |
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| | :<math>c</math> is the speed of light (3x10<sup>8</sup> ms<sup>-1</sup>). | | :<math>c</math> is the speed of light (3x10<sup>8</sup> ms<sup>-1</sup>). |
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| − | ===Mass increase===
| + | ==Mass increase== |
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| | We also see that as a body moves with increasing velocity its [[mass]] also increases. | | We also see that as a body moves with increasing velocity its [[mass]] also increases. |
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| | Since speed is relative, it follows that two observers in different inertial reference frames may disagree on the mass and kinetic energy of a body. Since all inertial reference frames are treated on an equal footing, it follows that mass and energy are interchangeable. | | Since speed is relative, it follows that two observers in different inertial reference frames may disagree on the mass and kinetic energy of a body. Since all inertial reference frames are treated on an equal footing, it follows that mass and energy are interchangeable. |
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