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  2. LIGO - Wikipedia

    en.wikipedia.org/wiki/LIGO

    Their existence was indirectly confirmed when observations of the binary pulsar PSR 1913+16 in 1974 showed an orbital decay which matched Einstein's predictions of energy loss by gravitational radiation. The Nobel Prize in Physics 1993 was awarded to Hulse and Taylor for this discovery. [60] Direct detection of gravitational waves had long been ...

  3. Gravitational wave - Wikipedia

    en.wikipedia.org/wiki/Gravitational_wave

    Gravitational waves transport energy as gravitational radiation, a form of radiant energy similar to electromagnetic radiation. [7] Newton's law of universal gravitation , part of classical mechanics , does not provide for their existence, instead asserting that gravity has instantaneous effect everywhere.

  4. Radiation pressure - Wikipedia

    en.wikipedia.org/wiki/Radiation_pressure

    Direct applications of the radiation pressure force in these fields are, for example, laser cooling (the subject of the 1997 Nobel Prize in Physics), [5] quantum control of macroscopic objects and atoms (2012 Nobel Prize in Physics), [6] interferometry (2017 Nobel Prize in Physics) [7] and optical tweezers (2018 Nobel Prize in Physics). [8]

  5. Light pollution - Wikipedia

    en.wikipedia.org/wiki/Light_pollution

    Light pollution is the presence of any unwanted, inappropriate, or excessive artificial lighting. [1] [2] In a descriptive sense, the term light pollution refers to the effects of any poorly implemented lighting sources, during the day or night. Light pollution can be understood not only as a phenomenon resulting from a specific source or kind ...

  6. Ground-based interferometric gravitational-wave search

    en.wikipedia.org/wiki/Ground-based_interfero...

    Supernova explosions—the gravitational collapse of massive stars at the end of their lives—emit gravitational radiation that may be seen by current interferometers. [23] A multi-messenger detection (electromagnetic and gravitational radiation, and neutrinos ) would help to better understand the supernova process and the formation of black ...

  7. Gravitational microlensing - Wikipedia

    en.wikipedia.org/wiki/Gravitational_microlensing

    A typical microlensing light curve is shown below: Typical light curve of gravitational microlensing event (OGLE-2005-BLG-006) with its model fitted (red) A typical microlensing event like this one has a very simple shape, and only one physical parameter can be extracted: the time scale, which is related to the lens mass, distance, and velocity.

  8. pp-wave spacetime - Wikipedia

    en.wikipedia.org/wiki/Pp-wave_spacetime

    The gravitational field of a beam of light is modelled, in general relativity, by a certain axi-symmetric pp-wave. An example of pp-wave given when gravity is in presence of matter is the gravitational field surrounding a neutral Weyl fermion: the system consists in a gravitational field that is a pp-wave, no electrodynamic radiation, and a ...

  9. Gravitational redshift - Wikipedia

    en.wikipedia.org/wiki/Gravitational_redshift

    [5] [8] A gravitational redshift can also equivalently be interpreted as gravitational time dilation at the source of the radiation: [8] [2] if two oscillators (attached to transmitters producing electromagnetic radiation) are operating at different gravitational potentials, the oscillator at the higher gravitational potential (farther from the ...