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  1. General relativity formula123:
    • The simplest equation for general relativity is R = GE, where R is the curvature of spacetime, G is the gravitational constant, and E is the energy-momentum tensor.
    • The formula for special relativity is γ = 1 / √(1 - v2 / c2), where γ is the relativistic factor, v is the velocity of an object, and c is the speed of light.
    • The formula for the equivalence of mass and energy is E = mc2, where E is the energy, m is the mass, and c is the speed of light.
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    The General Theory of Relativity can actually be described using a very simple equation: R = GE (although Einstein 's own formulation of his field equations are much more complex).
    www.physicsoftheuniverse.com/topics_relativity_ge…
    Formula for Relativity: According to the theory of relativity, the formula is: γ = 1 1−(v c√)2 Where γ is gamma a unitless quantity, and it is popular as a relativistic factor.
    www.toppr.com/guides/physics-formulas/relativity-f…
    In the famous relativity equation, E = mc2, the speed of light (c) serves as a constant of proportionality, linking the formerly disparate concepts of mass (m) and energy (E).
    www.britannica.com/science/E-mc2-equation
  2. People also ask
    Yet despite its success over more than 100 years, almost no one understands what the one equation that governs general relativity is actually about. Here, in plain English, is what it truly means. Einstein’s original equation relates spacetime curvature to the stress-energy of a system (top).
    General relativity, also known as the general theory of relativity and Einstein's theory of gravity, is the geometric theory of gravitation published by Albert Einstein in 1915 and is the current description of gravitation in modern physics.
    Statement of the obvious: Solving these equations turns out to be hard. Statement of the awesome: These equations can be broken down into simpler equations by those with a lot of skill. Some of these simpler equations are appropriate to the level of this book, which means you can learn how to do some general relativity.
    Originally, Einstein formulated general relativity with only the first and last terms in the equations, that is, with the Einstein tensor on one side and the stress-energy tensor (multiplied by the Einstein gravitational constant) on the other side.
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    General relativity, also known as the general theory of relativity and Einstein's theory of gravity, is the geometric theory of gravitation published by Albert Einstein in 1915 and is the current description of gravitation in modern physics. General relativity generalizes special relativity and refines Newton's law of universal … See more

    Henri Poincaré's 1905 theory of the dynamics of the electron was a relativistic theory which he applied to all forces, including gravity. … See more

    Advanced concepts image

    General relativity has a number of physical consequences. Some follow directly from the theory's axioms, whereas others have become clear only … See more

    Gravitational lensing
    The deflection of light by gravity is responsible for a new class of astronomical … See more

    From classical mechanics to general relativity image
    Consequences of Einstein's theory image

    General relativity can be understood by examining its similarities with and departures from classical physics. The first step is the realization that classical mechanics and … See more

    The derivation outlined in the previous section contains all the information needed to define general relativity, describe its key properties, and address a question of crucial importance in … See more

    Neo-Lorentzian Interpretation
    Examples of physicists who support neo-Lorentzian explanations of general relativity are Franco Selleri and Antony Valentini See more

    Asymptotic symmetries
    The spacetime symmetry group for special relativity is the Poincaré group, which is a ten-dimensional group of three Lorentz boosts, three rotations, and four spacetime translations. It is logical to ask what symmetries if any … See more

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  4. WebGravity feels strongest where spacetime is most curved, and it vanishes where spacetime is flat. This is the core of Einstein's theory of general relativity, which is often summed up in words as follows: "matter …

  5. WebGeneral relativity is Einstein's theory of gravity, in which gravitational forces are presented as a consequence of the curvature of spacetime. In general relativity, objects moving under gravitational attraction are …

  6. Einstein Field Equations: A Step-By-Step Derivation (Two Methods)