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  2. Diffraction - Wikipedia

    en.wikipedia.org/wiki/Diffraction

    Diffraction from a large three-dimensional periodic structure such as many thousands of atoms in a crystal is called Bragg diffraction. It is similar to what occurs when waves are scattered from a diffraction grating. Bragg diffraction is a consequence of interference between waves reflecting from many different crystal planes.

  3. Two-body problem in general relativity - Wikipedia

    en.wikipedia.org/wiki/Two-body_problem_in...

    The third term is attractive and dominates at small r values, giving a critical inner radius r inner at which a particle is drawn inexorably inwards to r = 0; this inner radius is a function of the particle's angular momentum per unit mass or, equivalently, the a length-scale defined above.

  4. General relativity - Wikipedia

    en.wikipedia.org/wiki/General_relativity

    The deflection of light by gravity is responsible for a new class of astronomical phenomena. If a massive object is situated between the astronomer and a distant target object with appropriate mass and relative distances, the astronomer will see multiple distorted images of the target. Such effects are known as gravitational lensing. [109]

  5. Introduction to general relativity - Wikipedia

    en.wikipedia.org/wiki/Introduction_to_general...

    Objects are falling to the floor because the room is resting on the surface of the Earth and the objects are being pulled down by gravity. Objects are falling to the floor because the room is aboard a rocket in space, which is accelerating at 9.81 m/s 2, the standard gravity on Earth, and is far from any source of gravity. The objects are being ...

  6. Gravitational lens - Wikipedia

    en.wikipedia.org/wiki/Gravitational_lens

    One of Eddington's photographs of the 1919 solar eclipse experiment, presented in his 1920 paper announcing its success. Henry Cavendish in 1784 (in an unpublished manuscript) and Johann Georg von Soldner in 1801 (published in 1804) had pointed out that Newtonian gravity predicts that starlight will bend around a massive object [15] as had already been supposed by Isaac Newton in 1704 in his ...

  7. Gravitational microlensing - Wikipedia

    en.wikipedia.org/wiki/Gravitational_microlensing

    If the lensing object is a star with a planet orbiting it, this is an extreme example of a binary lens event. If the source crosses a caustic, the deviations from a standard event can be large even for low mass planets. These deviations allow us to infer the existence and determine the mass and separation of the planet around the lens.

  8. Equivalence principle - Wikipedia

    en.wikipedia.org/wiki/Equivalence_principle

    In other words, passive gravitational mass must be proportional to inertial mass for objects, independent of their material composition if the weak equivalence principle is obeyed. The dimensionless Eötvös -parameter or Eötvös ratio η ( A , B ) {\displaystyle \eta (A,B)} is the difference of the ratios of gravitational and inertial masses ...

  9. Babinet's principle - Wikipedia

    en.wikipedia.org/wiki/Babinet's_principle

    For instance, the size of red blood cells can be found by comparing their diffraction pattern with an array of small holes. One consequence of Babinet's principle is the extinction paradox, which states that in the diffraction limit, the radiation removed from the beam due to a particle is equal to twice the particle's cross section times the flux.

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