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Device used to measure gravitational waves
A gravitational-wave detector (used in a gravitational-wave observatory) is any device designed to measure tiny distortions of spacetime called gravitational
Gravitational-wave observatory
Gravitational-wave_observatory
Gravitational wave observatory site
Interferometer Gravitational-Wave Observatory (LIGO) is a large-scale physics experiment and observatory designed to detect cosmic gravitational waves. Prior
LIGO
Japanese underground gravitational wave detector
hdl:11572/371989. "KAGRA gravitational-wave observatory completes construction". "Status of KAGRA Large-scale Cryogenic Gravitational Wave Telescope" (PDF).
Kamioka Gravitational Wave Detector
Kamioka_Gravitational_Wave_Detector
Proposed gravitational wave observatory
Gravitational wave Observatory (or DECIGO) is a proposed Japanese space-based gravitational wave observatory. The laser interferometric gravitational
Deci-hertz Interferometer Gravitational wave Observatory
Deci-hertz_Interferometer_Gravitational_wave_Observatory
Branch of astronomy using gravitational waves
by passing waves. Observatories like LIGO (Laser Interferometer Gravitational-wave Observatory), Virgo and KAGRA (Kamioka Gravitational Wave Detector)
Gravitational-wave_astronomy
Gravitational wave observatory unit, india
advanced experimental facilities for a multi-institutional observatory project in gravitational-wave astronomy to be located near Aundha Nagnath, Hingoli District
Indian Initiative in Gravitational-wave Observations
Indian_Initiative_in_Gravitational-wave_Observations
Astronomy organization
The North American Nanohertz Observatory for Gravitational Waves (NANOGrav) Physics Frontier Center is a consortium of astronomers who share a common
North American Nanohertz Observatory for Gravitational Waves
North_American_Nanohertz_Observatory_for_Gravitational_Waves
European space mission to measure gravitational waves
the first dedicated space-based gravitational-wave observatory. It aims to measure gravitational waves directly by using laser interferometry. The LISA
Laser Interferometer Space Antenna
Laser_Interferometer_Space_Antenna
Proposed ground-based gravitational wave observatory
Cosmic Explorer (CE) is a proposed next-generation ground-based gravitational wave observatory. It will consist of two L-shaped interferometers, similar to
Cosmic Explorer (gravitational wave observatory)
Cosmic_Explorer_(gravitational_wave_observatory)
Consortium managing the Virgo interferometric antenna in Pisa, Italy
The European Gravitational Observatory (EGO) is a consortium established to manage the Virgo interferometer and its related infrastructure, as well as
European Gravitational Observatory
European_Gravitational_Observatory
Aspect of relativity in physics
since 2015, directly through dedicated observatories. Gravitational waves transport energy as gravitational radiation, a form of radiant energy similar
Gravitational_wave
Random background of gravitational waves permeating the Universe
The gravitational wave background (also GWB and stochastic background) is a random background of gravitational waves permeating the Universe, which is
Gravitational_wave_background
Research facility in Western Australia
The Australian International Gravitational Observatory (AIGO) is a research facility located near Gingin, north of Perth in Western Australia. It is part
AIGO
2015 detection made by LIGO interferometers
portal Gravitational-wave astronomy – Branch of astronomy using gravitational waves Gravitational-wave observatory – Device used to measure gravitational waves
First observation of gravitational waves
First_observation_of_gravitational_waves
Chinese space program
satellite-based gravitational-wave observatory. It is scheduled for launch in 2033 to study ripples in spacetime caused by gravitational waves. The program
Taiji_program
Topics referred to by the same term
or Ligo may refer to: LIGO, gravitational wave observatory site LIGO Scientific Collaboration gravitational wave observatory scientific collaboration LIGO
Ligo
Proposed space-borne gravitational-wave observatory
Project (Chinese: 天琴计划) is a proposed space-borne gravitational-wave observatory (gravitational-wave detector) consisting of three spacecraft in Earth
TianQin
American experimental physicist (born 1974)
physics of gravitational wave detection and is among the scientists responsible for the U.S.-based Laser Interferometer Gravitational-wave Observatory (LIGO)
Rana_X._Adhikari
Location used for observing terrestrial or celestial events
Lamont–Doherty Earth Observatory EarthScope GEOSCOPE Observatory World-Wide Standardized Seismograph Network Example gravitational wave observatories include: LIGO
Observatory
Quantum astrophysicist (born 1968)
known for her work on the detection of gravitational waves in the Laser Interferometer Gravitational-Wave Observatory (LIGO) project, and for the exploration
Nergis_Mavalvala
Method of detecting gravitational waves
Explorer: A Next-Generation Ground-Based Gravitational-Wave Observatory "Astrophysical Sources of Gravitational Waves – Virgo". www.virgo-gw.eu. Retrieved
Ground-based interferometric gravitational-wave search
Ground-based_interferometric_gravitational-wave_search
Proposed gravitational wave detector
Einstein Telescope (ET), is a planned third-generation ground-based gravitational wave (GW) detector, currently under study by some institutions in the European
Einstein_Telescope
2015 European Space Agency spacecraft
needed for the Laser Interferometer Space Antenna (LISA), an ESA gravitational wave observatory planned to be launched in 2035. Formerly, the mission was known
LISA_Pathfinder
Gravitational-wave astronomy technique
nanohertz gravitational waves, marking a new era in nanoHertz gravitational research. Rini, Matteo (June 2023). "Researchers Capture Gravitational-Wave Background
Pulsar_timing_array
Relativistic effect due to rotation
light wave depends on the strength of the gravitational potential along its path". This is called the Shapiro delay. However, since the gravitational field
Sagnac_effect
Topics referred to by the same term
another name of barium borate Big Bang Observer, planned space gravitational wave observatory IATA code for Berbera Airport "BBO (Bad Bitches Only)", a song
BBO
Quantum states light can be in
the gravitational-wave observatories LIGO and Virgo employ squeezed laser light, which has significantly increased the rate of observed gravitational-wave
Squeezed_states_of_light
Device used in gravitational wave observatories
A Weber bar is a type of resonant mass gravitational wave detector designed to detect gravitational waves, devised and constructed by physicist Joseph
Weber_bar
Topics referred to by the same term
ngo, a file extension for an NG Linker Object (NGML) file New Gravitational-wave Observatory, a European Space Agency project Chūbu Centrair International
NGO_(disambiguation)
Detector for gravitational waves in Japan
Interferometer Observatory) is a prototype detector for gravitational waves. It is testing cryogenic mirror technologies for the Kamioka Gravitational Wave Detector
CLIO
Gravitational-wave detector in Italy
two Laser Interferometer Gravitational-Wave Observatories (LIGO) in the United States and the Japanese Kamioka Gravitational Wave Detector (KAGRA), because
Virgo_interferometer
2019 studio album by William Basinski
album, Basinski collaborated with LIGO (Laser Interferometer Gravitational-Wave Observatory) to record the sounds of two black holes merging 1.3 billion
On_Time_Out_of_Time
Speculative feature of the early universe
earthbound Laser Interferometer Gravitational-Wave Observatory (LIGO) and especially the space-based gravitational wave detector Laser Interferometer Space
Cosmic_string
of the perihelion of Mercury, the bending of light in gravitational fields, and the gravitational redshift. The precession of Mercury was already known;
Tests_of_general_relativity
American physicist
physicist known for her work on gravitational physics, especially gravitational waves, gravitons, and gravitational singularities. Alongside Berger's
Beverly_Berger
Gravitational wave detector
gravitational wave detector located at the Mitaka campus of the National Astronomical Observatory of Japan. It is a project of the gravitational wave
TAMA_300
Radio telescope observatory in New South Wales, Australia
(IPTA), which also includes the North American Nanohertz Observatory for Gravitational Waves (NANOGrav) and the European Pulsar Timing Array (EPTA). Fast
Parkes_Observatory
The Gravitational Wave International Committee (or GWIC) is a panel of gravitational wave detection Laboratory or Observatory directors that promotes
Gravitational Wave International Committee
Gravitational_Wave_International_Committee
Study involving matter and electromagnetic radiation
spectral signature in the context of the Laser Interferometer Gravitational-Wave Observatory (LIGO). Spectroscopy is a branch of science concerned with the
Spectroscopy
Collapsed core of a massive star
the gravitationally collapsed core of a massive supergiant star. It results from the supernova explosion of a massive star—combined with gravitational collapse—that
Neutron_star
Physics Institute in Potsdam and Hanover
experimental gravitational physics, quantum gravity, multi-messenger astronomy and cosmology. The institute has a strong research focus on gravitational-wave astronomy:
Max Planck Institute for Gravitational Physics
Max_Planck_Institute_for_Gravitational_Physics
Radio telescope array
for gravitational waves. The project is managed by the California Institute of Technology (Caltech) as part of their Owens Valley Radio Observatory, with
Deep_Synoptic_Array
helped the LIGO (Laser Interferometer Gravitational-Wave Observatory) succeed at detecting gravitational waves. The company also provides power supplies
Kepco_Power
Optical and UV Research (CASTOR) Deci-hertz Interferometer Gravitational wave Observatory (DECIGO) EChO Fast Infrared Exoplanet Spectroscopy Survey Explorer
List of proposed space telescopes
List_of_proposed_space_telescopes
Gravitational-wave detector
Allegro was a ground-based, cryogenic resonant Weber bar, gravitational-wave detector run by Warren Johnson, et al. at Louisiana State University in Baton
Allegro gravitational-wave detector
Allegro_gravitational-wave_detector
Common configuration for optical interferometry
the Laser Interferometer Gravitational-Wave Observatory. This was the first experimental validation of gravitational waves, predicted by Albert Einstein's
Michelson_interferometer
Compact astronomical body
information about what caused the gravitational waves. Since gravitational waves are very weak, gravitational-wave observatories such as LIGO must have arms
Black_hole
Sun's gravitational field. 1969 – William B. Bonnor introduces the Bonnor beam. 1969 – Joseph Weber reports observation of gravitational waves a claim
Timeline of gravitational physics and relativity
Timeline_of_gravitational_physics_and_relativity
Gravitational wave detector
Mario Schenberg (Gravitational Wave Detector, or Brazilian Graviton Project or Graviton) is a spherical, resonant-mass, gravitational wave detector formerly
Mario Schenberg (Gravitational Wave Detector)
Mario_Schenberg_(Gravitational_Wave_Detector)
contains a list of observed and candidate gravitational wave events. Direct observation of gravitational waves, which commenced with the detection of an
List of gravitational wave observations
List_of_gravitational_wave_observations
Private university in Pasadena, California
W. M. Keck Observatory at the Mauna Kea Observatory, the Laser Interferometer Gravitational-Wave Observatory at Livingston, Louisiana and Richland, Washington
California Institute of Technology
California_Institute_of_Technology
the first direct detection of gravitational waves. He is a founding member of the Indian Initiative in Gravitational-wave Observations (IndIGO) consortium
Tarun_Souradeep
Software infrastructure for building distributed control systems
2019-09-04 at the Wayback Machine CosyLab GLResearch idt Mobiis Nusano, Inc Observatory Sciences Osprey Distributed Control Systems Varian Medical Systems Pyramid
EPICS
American laser physicist (born 1961)
served as the scientific spokesman of the Laser Interferometer Gravitational-Wave Observatory (LIGO) experiment in 2007-2011. In August 2011, he took a leave
David_Reitze
NASA project
Observer, a follow-up mission to LISA and Inflation Probe, also a gravitational-wave observatory Black-Hole Imager (MAXIM): an X-ray observation of infalling
Beyond_Einstein_program
Indian astrophysicist
LIGO." – 2016 Gravitational-wave astronomy Gravitational-wave observatory "Vadodara man behind simulation of Einstein's gravitational waves | Vadodara News
Karan_Jani
Gravitational-wave signal detected in 2017
GW170817 was a gravitational wave (GW) observed by the LIGO and Virgo detectors on 17 August 2017, originating within the shell elliptical galaxy NGC 4993
GW170817
Type of stellar collision
type of standard candle. In April 2019, the LIGO and Virgo gravitational wave observatories announced the detection of GW190425, a candidate event that
Neutron_star_merger
Five-radio telescope collaboration to track stellar remnants' gravitational waves
measuring gravitational waves, the International Pulsar Timing Array, which also includes the North American Nanohertz Observatory for Gravitational Waves (NANOGrav)
European_Pulsar_Timing_Array
American physicist
the Laser Interferometer Gravitational-Wave Observatory (LIGO) project when the first direct detection of gravitational waves was made in September 2015
Stanley_E._Whitcomb
Europe-US-Canada-India-Australian radio astronomy and cosmology collaboration
Pulsar Timing Array (EPTA), the North American Nanohertz Observatory for Gravitational Waves (NANOGrav), the Parkes Pulsar Timing Array (PPTA) in Australia
International Pulsar Timing Array
International_Pulsar_Timing_Array
Speed of electromagnetic waves
speed c as do massless particles and field perturbations, such as gravitational waves. The speed of light in vacuum is the same for all observers, no matter
Speed_of_light
Attraction of masses and energy
physics, gravity (from Latin gravitas 'weight'), also known as gravitation or a gravitational interaction, is a fundamental interaction, which may be described
Gravity
Subfield of astronomy
A few gravitational wave observatories have been constructed, but gravitational waves are extremely difficult to detect. Neutrino observatories have also
Astrophysics
Change in wavelength of light
the relative motions of radiation sources, gravitational redshift as radiation escapes from gravitational potentials, and cosmological redshifts caused
Redshift
Native American physicist
Siksika Nation (Blackfoot) / Laser Interferometer Gravitational-Wave Observatory (LIGO) / Gravitational-Wave Astronomy | Winds of Change". woc.aises.org. Retrieved
Corey_Gray
Signal with equal energy per octave
are ground-based detectors, the initial Laser Interferometer Gravitational-Wave Observatory (LIGO) and its advanced configuration (aLIGO). The characteristic
Pink_noise
cosmic rays or gravitational waves. Thus, new types of observatories have been developed. Interferometers are at the core of gravitational wave detectors.
List of astronomical observatories
List_of_astronomical_observatories
American scientist (1936–2024)
including overseeing the creation of the Laser Interferometer Gravitational-Wave Observatory (LIGO) during his tenure as chair of Caltech's Division of Physics
Edward_C._Stone
Software used in gravitational-wave astronomy
gravitational waveform generation, among other tasks common in gravitational-wave data analysis. The software is developed by the gravitational-wave community
PyCBC
Topics referred to by the same term
Taiji Program in Space, a proposed Chinese satellite-based gravitational-wave observatory Taiji dolphin drive hunt, an annual dolphin hunt in Taiji, Wakayama
Taiji
Gravitational wave detector in Germany
capable of detecting gravitational waves in the frequency range 50 Hz to 1.5 kHz, and is part of a worldwide network of gravitational wave detectors. This
GEO600
Alteration of orbits of celestial bodies through gravity
objects can emit gravitational waves, which have been detected by observatories such as the Laser Interferometer Gravitational-Wave Observatory (LIGO). Analyses
Gravitational_scattering
radiated away as gravitational waves. The Laser Interferometer Gravitational-Wave Observatory (LIGO) detected the gravitational waves by using two mirrors
History_of_black_hole_physics
Book by Marcia Bartusiak
the gravitational waves predicted by Einstein's theory of general relativity. She tells the story of LIGO's two gravitational-wave observatories in Louisiana
Einstein's Unfinished Symphony
Einstein's_Unfinished_Symphony
American physicist
D. in 2015. Her dissertation, Gravitational-wave science with the Laser Interferometer Gravitational-Wave Observatory, was jointly supervised by Jolien
Madeline_Wade
American astrophysicist and aerospace engineer
the Laser Interferometer Gravitational-Wave Observatory (LIGO) collaboration as part of an attempt to detect gravitational waves from the Crab Pulsar. She
Erin_Macdonald
Gravitational-wave event
merger detected by LIGO on January 14, 2025. It generated the clearest gravitational wave signal received to date, with a signal-to-noise ratio (SNR) of about
GW250114
Indian astronomer
Proposal for an Interferometric Gravitation-Wave Observatory (PDF) (Report). Indian Initiative in Gravitational wave Observations – via LIGO Document
Sanjeev_Dhurandhar
Underground physics laboratory in Japan
pronunciation: [kamioka ɯtɕɯː soɾʲɯꜜːɕi keŋkʲɯː ɕiꜜsetsɯ]) is a neutrino and gravitational waves laboratory located ~1 km (2700 mwe) underground in the Mozumi mine
Kamioka_Observatory
Category of disciplines and sub-disciplines in Physics
Gravitational-Wave Observatory, is a large-scale physics experiment and observatory to detect cosmic gravitational waves and to develop gravitational-wave
Experimental_physics
Volunteer computing project
that searches for signals from spinning neutron stars in data from gravitational-wave detectors, from large radio telescopes, and from a gamma-ray telescope
Einstein@Home
Effective mass of a binary system
system as a result of energy loss from emitting gravitational waves. Because the gravitational wave frequency is determined by orbital frequency, the
Chirp_mass
Measurement method using interference of waves
Interferometer Gravitational-Wave Observatory (LIGO) uses two 4-km Michelson–Fabry–Pérot interferometers for the detection of gravitational waves. In this application
Interferometry
Star cluster in the center of a galaxy
mass-ratio inspirals (EMRIs) detectable by future space-based gravitational wave observatories such as LISA. Nuclear star clusters are found in most galaxies
Nuclear_star_cluster
American theoretical cosmologist
history of the Laser Interferometer Gravitational-Wave Observatory and the 2015 discovery of gravitational waves. In a review of the book published in
Janna_Levin
First black hole event observed jointly by LIGO and Virgo observatories, 2017-08-14
GW170814 was a gravitational wave signal from two merging black holes, detected by the LIGO and Virgo observatories on 14 August 2017. On 27 September
GW170814
Laser interferometer at Fermilab
2014 Backreaction, Holographic Noise Weiss; et al. (2017). "MHz gravitational wave constraints with decameter Michelson interferometers". Phys. Rev.
Fermilab_Holometer
Hypothetical black hole formed soon after the Big Bang
can emit gravitational waves that interact with regular matter. Finally, the discovery of PBHs could explain some of the observed gravitational lensing
Primordial_black_hole
Type of quantum state
"First Long-Term Application of Squeezed States of Light in a Gravitational-Wave Observatory". Phys. Rev. Lett. 110 (18) 181101. arXiv:1302.2188. Bibcode:2013PhRvL
Squeezed_coherent_state
Array of robotic optical telescopes
The Gravitational-wave Optical Transient Observer (GOTO) is an array of robotic optical telescopes optimized for the discovery of optical counterparts
GOTO_(telescope_array)
American physicist, writer, and Nobel Laureate (born 1940)
relevance to LIGO (Laser Interferometer Gravitational Wave Observatory), a multi-institution gravitational wave experiment for which Thorne has been a
Kip_Thorne
Branch of physics that studies mathematical models of the universe
scenario. Gravitational waves are ripples in the curvature of spacetime that propagate as waves at the speed of light, generated in certain gravitational interactions
Physical_cosmology
International physics organization
physics institutes and research groups dedicated to the search for gravitational waves. It complements the LIGO Laboratory, an organization based at the
LIGO_Scientific_Collaboration
Type of wave in geophysics
A Kelvin wave is a wave in the ocean, a large lake or the atmosphere that balances the Earth's Coriolis force against a topographic boundary such as a
Kelvin_wave
Italian astrophysicist
the founding Director of the Institute for Gravitational Wave Astronomy. His research spans gravitational-wave astronomy across the frequency spectrum,
Alberto_Vecchio
American physicist
Interferometer Gravitational-Wave Observatory (LIGO) collaboration and played a significant role in two discoveries: the first detection of gravitational waves in
Daniel_Holz
Italian physicist
LISA, the Laser Interferometer Space Antenna, is the future gravitational wave-observatory in space, led by ESA. Stefano Vitale has served on many different
Stefano_Vitale
Award
Kip Thorne, Rainer Weiss, and the entire Laser Interferometer Gravitational-Wave Observatory (LIGO) discovery team. 2017 Sandra M. Faber 2018 Nazzareno Mandolesi
Gruber_Prize_in_Cosmology
Indian astrophysicist (born 1950)
Thirty Meter Telescope (TMT), and the Laser Interferometer Gravitational-Wave Observatory LIGO). He also conceived and executed the INFONET project under
Ajit_Kembhavi
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