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  2. Hoyle–Narlikar theory of gravity - Wikipedia

    en.wikipedia.org/wiki/Hoyle–Narlikar_theory_of...

    Unlike the standard cosmological model, the quasi steady state hypothesis implies the universe is eternal.According to Narlikar, multiple mini bangs would occur at the center of quasars, with various creation fields (or C-field) continuously generating matter out of empty space due to local concentration of negative energy that would also prevent violation of conservation laws, in order to ...

  3. Scalar–tensor–vector gravity - Wikipedia

    en.wikipedia.org/wiki/Scalar–tensor–vector...

    Observations show that in "undisturbed" galaxy clusters the reconstructed mass from gravitational lensing is located where matter is distributed, and a separation of matter from gravitation only seems to appear after a collision or interaction has taken place. According to Ethan Siegel: "Adding dark matter makes this work, but non-local gravity ...

  4. List of equations in gravitation - Wikipedia

    en.wikipedia.org/wiki/List_of_equations_in...

    A common misconception occurs between centre of mass and centre of gravity.They are defined in similar ways but are not exactly the same quantity. Centre of mass is the mathematical description of placing all the mass in the region considered to one position, centre of gravity is a real physical quantity, the point of a body where the gravitational force acts.

  5. Scalar theories of gravitation - Wikipedia

    en.wikipedia.org/wiki/Scalar_theories_of_gravitation

    The Watt–Misner theory (1999) is a recent example of a scalar theory of gravitation. It is not intended as a viable theory of gravitation (since, as Watt and Misner point out, it is not consistent with observation), but as a toy theory which can be useful in testing numerical relativity schemes. It also has pedagogical value. [10]

  6. Equations for a falling body - Wikipedia

    en.wikipedia.org/wiki/Equations_for_a_falling_body

    A set of equations describing the trajectories of objects subject to a constant gravitational force under normal Earth-bound conditions.Assuming constant acceleration g due to Earth's gravity, Newton's law of universal gravitation simplifies to F = mg, where F is the force exerted on a mass m by the Earth's gravitational field of strength g.

  7. Brans–Dicke theory - Wikipedia

    en.wikipedia.org/wiki/Brans–Dicke_theory

    Both Brans–Dicke theory and general relativity are examples of a class of relativistic classical field theories of gravitation, called metric theories.In these theories, spacetime is equipped with a metric tensor, , and the gravitational field is represented (in whole or in part) by the Riemann curvature tensor, which is determined by the metric tensor.

  8. Einstein–Cartan theory - Wikipedia

    en.wikipedia.org/wiki/Einstein–Cartan_theory

    (April 2024) (Learn how and when to remove this message Classical theory of gravitation In theoretical physics , the Einstein–Cartan theory , also known as the Einstein–Cartan–Sciama–Kibble theory , is a classical theory of gravitation , one of several alternatives to general relativity . [ 1 ]

  9. Nonsymmetric gravitational theory - Wikipedia

    en.wikipedia.org/wiki/Nonsymmetric_gravitational...

    In theoretical physics, the nonsymmetric gravitational theory [1] (NGT) of John Moffat is a classical theory of gravitation that tries to explain the observation of the flat rotation curves of galaxies. In general relativity, the gravitational field is characterized by a symmetric rank-2 tensor, the metric tensor.