enow.com Web Search

Search results

  1. Results from the WOW.Com Content Network
  2. Graviton - Wikipedia

    en.wikipedia.org/wiki/Graviton

    Alternatively, if gravitons are massive at all, the analysis of gravitational waves yielded a new upper bound on the mass of gravitons. The graviton's Compton wavelength is at least 1.6 × 10 16 m , or about 1.6 light-years , corresponding to a graviton mass of no more than 7.7 × 10 −23 eV / c 2 . [ 18 ]

  3. LIGO - Wikipedia

    en.wikipedia.org/wiki/LIGO

    The Laser Interferometer Gravitational-Wave Observatory (LIGO) is a large-scale physics experiment and observatory designed to detect cosmic gravitational waves and to develop gravitational-wave observations as an astronomical tool. [1]

  4. GW170104 - Wikipedia

    en.wikipedia.org/wiki/GW170104

    GW170104 was a gravitational wave signal detected by the LIGO observatory on 4 January 2017. On 1 June 2017, the LIGO and Virgo collaborations announced that they had reliably verified the signal, making it the third such signal announced, after GW150914 and GW151226, and fourth overall.

  5. First observation of gravitational waves - Wikipedia

    en.wikipedia.org/wiki/First_observation_of...

    Although no neutrinos were detected, the lack of such observations provided a limit on neutrino emission from this type of gravitational wave event. [69] Observations by the Swift Gamma-Ray Burst Mission of nearby galaxies in the region of the detection, two days after the event, did not detect any new X-ray, optical or ultraviolet sources. [70]

  6. Gravitational-wave observatory - Wikipedia

    en.wikipedia.org/wiki/Gravitational-wave_observatory

    A more sensitive detector uses laser interferometry to measure gravitational-wave induced motion between separated 'free' masses. [7] This allows the masses to be separated by large distances (increasing the signal size); a further advantage is that it is sensitive to a wide range of frequencies (not just those near a resonance as is the case ...

  7. Mario Schenberg (Gravitational Wave Detector) - Wikipedia

    en.wikipedia.org/wiki/Mario_Schenberg...

    The Mario Schenberg (Gravitational Wave Detector, or Brazilian Graviton Project [1] or Graviton) is a spherical, resonant-mass, gravitational wave detector formerly run by the Physics Institute of the University of São Paulo, named after Mário Schenberg.

  8. Talk:Graviton - Wikipedia

    en.wikipedia.org/wiki/Talk:Graviton

    Thanks for the addition. Now I am thinking would even the Jupiter size detector (if it didn't collapse to a black hole) be able to detect single gravitons, as the source above states that Bell like inequalities need to be violated (or something similar) before you can prove quantization and not just classical fields producing "clicks".

  9. Ultrasonic transducer - Wikipedia

    en.wikipedia.org/wiki/Ultrasonic_transducer

    Ultrasonic sensors can detect the movement of targets and measure the distance to them in many automated factories and process plants. Sensors can have an on or off digital output for detecting the movement of objects, or an analog output proportional to distance. They can sense the edge of the material as part of a web guiding system.