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  2. Modified Newtonian dynamics - Wikipedia

    en.wikipedia.org/wiki/Modified_Newtonian_dynamics

    For instance, if the gravitational acceleration equals a 0 at a distance from a mass, at ten times that distance, Newtonian gravity predicts a hundredfold decline in gravity whereas MOND predicts only a tenfold reduction. By fitting Milgrom's law to rotation curve data, Begeman et al. found a 0 ≈ 1.2 × 1010 m/s 2 to be optimal. [23]

  3. Parameterized post-Newtonian formalism - Wikipedia

    en.wikipedia.org/wiki/Parameterized_post...

    In physics, precisely in the study of the theory of general relativity and many alternatives to it, the post-Newtonian formalism is a calculational tool that expresses Einstein's (nonlinear) equations of gravity in terms of the lowest-order deviations from Newton's law of universal gravitation.

  4. Entropic gravity - Wikipedia

    en.wikipedia.org/wiki/Entropic_gravity

    Entropic gravity provides an underlying framework to explain Modified Newtonian Dynamics, or MOND, which holds that at a gravitational acceleration threshold of approximately 1.2 × 1010 m/s 2, gravitational strength begins to vary inversely linearly with distance from a mass rather than the normal inverse-square law of the distance.

  5. Brans–Dicke theory - Wikipedia

    en.wikipedia.org/wiki/Brans–Dicke_theory

    In physics, the Brans–Dicke theory of gravitation (sometimes called the Jordan–Brans–Dicke theory) is a competitor to Einstein's general theory of relativity.It is an example of a scalar–tensor theory, a gravitational theory in which the gravitational interaction is mediated by a scalar field as well as the tensor field of general relativity.

  6. Causal dynamical triangulation - Wikipedia

    en.wikipedia.org/wiki/Causal_dynamical_triangulation

    Causal dynamical triangulation (CDT), theorized by Renate Loll, Jan Ambjørn and Jerzy Jurkiewicz, is an approach to quantum gravity that, like loop quantum gravity, is background independent. This means that it does not assume any pre-existing arena (dimensional space) but, rather, attempts to show how the spacetime fabric itself evolves.

  7. Scalar–tensor theory - Wikipedia

    en.wikipedia.org/wiki/Scalar–tensor_theory

    Thus, Newtonian gravity is called a scalar theory. The gravitational force is dependent of the distance r of the massive objects to each other (more exactly, their centre of mass). Mass is a parameter and space and time are unchangeable. Einstein's theory of gravity, the General Relativity (GR) is of another nature.

  8. Loop quantum cosmology - Wikipedia

    en.wikipedia.org/wiki/Loop_quantum_cosmology

    An important feature of loop quantum cosmology is the effective space-time description of the underlying quantum evolution. [10] The effective dynamics approach has been extensively used in loop quantum cosmology to describe physics at the Planck scale and the very early universe.

  9. History of gravitational theory - Wikipedia

    en.wikipedia.org/.../History_of_gravitational_theory

    The whole landscape of physics was changed with the discovery of Lorentz transformations, and this led to attempts to reconcile it with gravity. At the same time, experimental physicists started testing the foundations of gravity and relativity— Lorentz invariance , the gravitational deflection of light , the Eötvös experiment .

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