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  1. In this series, we build together the theory of general relativity. This seventh video focuses on the Einstein equation, the key ingredient of the theory whi...

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  2. Converting Matter into Energy. The remarkable equivalence between matter and energy is given in one of the most famous equations: E = mc2 E = m c 2. In this equation, E stands for energy, m stands for mass, and c, the constant that relates the two, is the speed of light (3 × 10 8 meters per second). Note that mass is a measure of the quantity ...

  3. Aimed at both physics students and non-science majors, this unique book explains Einstein’s Special Theory of Relativity pictorially, using diagrams rather than equations. The diagrams guide the reader, step-by-step, from the basics of relativity to advanced topics including the addition of velocities, Lorentz contraction, time dilation, twin ...

  4. t. e. General relativity is a theory of gravitation developed by Albert Einstein between 1907 and 1915. The theory of general relativity says that the observed gravitational effect between masses results from their warping of spacetime . By the beginning of the 20th century, Newton's law of universal gravitation had been accepted for more than ...

  5. Malcolm A.H. MacCallum (2013), Scholarpedia, 8 (12):8584. Exact Solutions of Einstein's Equations. Einstein's General Relativity is the leading theory of space-time and gravity: it is highly nonlinear. Exact solutions of Einstein's equations thus model gravitating systems and enable exploration of the mathematics and physics of the theory.

  6. The. general theory of relativity. Albert Einstein's general theory of relativity, phrased in terms of warps and curves in space and time, provides our most refined description of the gravitational force. This video is an episode in Brian Greene's Daily Equation series. Consider a society of two-dimensional beings living on a surface that is ...

  7. Jun 9, 2021 · Proposed in 1916, Einstein’s general theory of relativity explained that gravity was a special force that existed because of the curvature of space-time itself. Space-time, according to this theory, is not flat. Thus, orbiting bodies travel in geodesics—the shortest distance between two points. This is the nearest thing to a straight line.

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