astro.wikisort.org - InstitutionAllegro was a ground-based, cryogenic resonant Weber bar, gravitational-wave detector[1] run by Warren Johnson, et al. at Louisiana State University in Baton Rouge, Louisiana. The detector was commissioned in the early 1990s, and was decommissioned in 2008.
Allegro gravitational-wave detectorLocation(s) | Louisiana |
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Organization | Louisiana State University  |
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Telescope style | gravitational-wave observatory  |
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Mechanical design
The resonant bar in Allegro is 2300 kg of aluminum, 3 meters in length. Suspended in a cryogenic vacuum tank at 4.2 Kelvin, the bar's natural resonant frequency (the lowest longitudinal mode) is near 904 Hz.
The strain on the bar is measured by coupling a second, much lighter, suspended mass to the main heavier mass as a mechanical transformer at the same resonant frequency. Therefore, small motions of the primary mass generate much larger motions in the smaller mass. The differential displacement of the two masses is recorded using an inductive transducer and amplifier (a SQUID).[2]
Collaboration with LIGO
Due its close proximity to the LIGO Livingston Detector (one in the array of three, large-scale, laser interferometric detectors), Allegro has partnered with the LIGO Scientific collaboration to produce several results during the fourth science run of LIGO.[3]
References
Gravitational-wave astronomy |
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Detectors | Resonant mass antennas | Active | |
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Past |
- EXPLORER (IGEC)
- ALLEGRO (IGEC)
- NIOBE (IGEC)
- Stanford gravitational wave detector
- ALTAIR
- GEOGRAV
- AGATA
- Weber bar
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Proposed | |
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Past proposals | |
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Ground-based Interferometers | Active | |
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Past | |
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Planned | |
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Proposed | |
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Past proposals | |
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Space-based interferometers | |
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Pulsar timing arrays | |
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Data analysis |
- Einstein@Home
- PyCBC
- Zooniverse: Gravity Spy
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Observations | Events |
- List of observations
- First observation (GW150914)
- GW151012
- GW151226
- GW170104
- GW170608
- GW170729
- GW170809
- GW170814
- GW170817 (first neutron star merger)
- GW170818
- GW170823
- GW190412
- GW190521 (first-ever possible light from bh-bh merger)
- GW190814 (first-ever "mass gap" collision)
- GW200105 (first black hole - neutron star merger)
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Methods |
- Direct detection
- Laser interferometers
- Resonant mass detectors
- Proposed: Atom interferometers
- Indirect detection
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Theory |
- General relativity
- Tests of general relativity
- Metric theories
- Graviton
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Effects / properties | |
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Types / sources |
- Stochastic
- Binary inspiral
- Supermassive black holes
- Stellar black holes
- Neutron stars
- EMRI
- Continuous
- Burst
- Hypothesis
- Colliding cosmic string and other unknown sources
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На других языках
- [en] Allegro gravitational-wave detector
[ru] ALLEGRO
ALLEGRO — наземный криогенный резонансный детектор гравитационных волн[1]. Работал под управлением Варрена Джонсона и других учёных из Университета штата Луизиана в Батон-Руж, Луизиана с начала 90-х по 2008 год.
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