Anagram & Information om | Engelska ordet LIGO


LIGO

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Exempel på hur man kan använda LIGO i en mening

  • 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.
  • Livingston hosts one of the two LIGO gravitational wave detector sites, the other one being located in Hanford, Washington.
  • In 2017, Weiss was awarded the Nobel Prize in Physics, along with Kip Thorne and Barry Barish, "for decisive contributions to the LIGO detector and the observation of gravitational waves".
  • LIGO, the Laser Interferometer Gravitational-Wave Observatory, is a large-scale physics experiment and observatory to detect cosmic gravitational waves and to develop gravitational-wave observations as an astronomical tool.
  • The Einstein@Home project was originally created to perform all-sky searches for previously unknown continuous gravitational-wave (CW) sources using data from the Laser Interferometer Gravitational-Wave Observatory (LIGO) detector instruments in Washington and Louisiana, USA.
  • He is portrayed as a brilliant theoretical physicist and cosmologist, who researches supersymmetry, string theory, 11-dimensional supergravity theory, doubly special relativity, black holes, Ly-alpha emitters, the cosmic microwave background, and gravitational waves, using LIGO to check predictions on quantum corrections.
  • This includes neutrino detections by observatories such as IceCube or Super-Kamiokande, gravitational wave events from the LIGO, Virgo and KAGRA interferometers, and gamma-ray bursts observed by Fermi, Swift or INTEGRAL.
  • For example, the waves given off by the cataclysmic final merger of GW150914 reached Earth after travelling over a billion light-years, as a ripple in spacetime that changed the length of a 4 km LIGO arm by a thousandth of the width of a proton, proportionally equivalent to changing the distance to the nearest star outside the Solar System by one hair's width.
  • There are several ground-based laser interferometers which span several miles/kilometers, including: the two Laser Interferometer Gravitational-Wave Observatory (LIGO) detectors in WA and LA, USA; Virgo, at the European Gravitational Observatory in Italy; GEO600 in Germany, and the Kamioka Gravitational Wave Detector (KAGRA) in Japan.
  • 2016 Ronald Drever, Kip Thorne, Rainer Weiss, and the entire Laser Interferometer Gravitational-Wave Observatory (LIGO) discovery team.
  • The Gravitational Wave Group at the School of Physics (part of the Indian Initiative in Gravitational-wave Observations (IndIGO) comprising scientists from nine institutions working under the LIGO) Scientific Collaboration (LSC), IISER TVM also contributed to historic discovery of gravitational waves.
  • The Holometer will consist of two 39 m arm-length power-recycled Michelson interferometers, similar to the LIGO instruments.
  • Barish became the principal investigator of the Laser Interferometer Gravitational-wave Observatory (LIGO) in 1994 and director in 1997.
  • Matt Walker's new sleep book, a LIGO Nobel Prize and Janna Levin's book on it, the downside of grass-fed beef, and cargo cults.
  • An engineering run to assess the sensitivity of LIGO, Virgo, and KAGRA began in April, with the Hanford detector's first operations beginning on April 29, and the Livingston and Virgo detectors' first operations beginning on May 5.
  • In addition to its filming of the secret internal confirmation months of the gravitational wave detection and LIGO's continuing breakthrough science, the Advanced LIGO Documentary Project filmed LIGO's Nobel Prize week in Stockholm; three important post-detection lectures by Thorne, Barish and LIGO astrophysicist Alessandra Buonanno.
  • Gladney has served on the National Science Foundation-Department of Energy High Energy Physics Advisory Panel (HEPAP), the director's Review Board of the Lawrence Berkeley National Laboratory (LBNL), the Experimental Physics Advisory Committee for the Stanford Linear Accelerator Center (SLAC), and the Program Advisory Committee for the Laser Interferometer Gravitational-Wave Observatory (LIGO) at Caltech.
  • Norna Robertson (FRSE, FInstP, FRAS, FAPS) is a lead scientist at LIGO at California Institute of Technology, and professor of experimental physics at the University of Glasgow.


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