Add to ORKGLIGO is exploring cryogenics as a technique of last resort to reduce the thermal noise of mirrors and suspensions in gravitational wave interferometric detectors. Some of the cryogenic, or cryogenic-related, R&D done at LIGO is reported here. Some ideas being considered to make cryogenics possible may be useful even for room temperature detectors
The detection of gravitational waves from compact binary mergers by LIGO has opened the era of gravi...
The Caltech-MIT joint LIGO project is operating three long-baseline interferometers (one of 2 km and...
The Caltech-MIT joint LIGO project is operating three long-baseline interferometers (one of 2 km and...
LIGO is exploring cryogenics as a technique of last resort to reduce the thermal noise of mirrors an...
This chapter discusses how mirrors at cryogenic temperature can be used to improve the sensitivity o...
This chapter discusses how mirrors at cryogenic temperature can be used to improve the sensitivity o...
The success of a precision experiment is often associated to the use of low temperature techniques. ...
The LIGO (Laser Interferometer Gravitational-Wave Observatory) project is designed to open a new fie...
A laser interferometer gravitational wave observatory (LIGO) is being developed with sensitivities w...
Gravitational waves were first predicted by Albert Einstein's Theory of general relativity, publishe...
Construction activities at the LIGO Observatories near Hanford, Washington and Livingston, Louisiana...
Future generations of gravitational wave interferometers are likely to be operated at cryogenic temp...
The detection of gravitational waves from compact binary mergers by LIGO has opened the era of gravi...
The detection of gravitational waves from compact binary mergers by LIGO has opened the era of gravi...
A remarkable design of LCGT was established by experimental efforts to detect gravi-tational waves i...
The detection of gravitational waves from compact binary mergers by LIGO has opened the era of gravi...
The Caltech-MIT joint LIGO project is operating three long-baseline interferometers (one of 2 km and...
The Caltech-MIT joint LIGO project is operating three long-baseline interferometers (one of 2 km and...
LIGO is exploring cryogenics as a technique of last resort to reduce the thermal noise of mirrors an...
This chapter discusses how mirrors at cryogenic temperature can be used to improve the sensitivity o...
This chapter discusses how mirrors at cryogenic temperature can be used to improve the sensitivity o...
The success of a precision experiment is often associated to the use of low temperature techniques. ...
The LIGO (Laser Interferometer Gravitational-Wave Observatory) project is designed to open a new fie...
A laser interferometer gravitational wave observatory (LIGO) is being developed with sensitivities w...
Gravitational waves were first predicted by Albert Einstein's Theory of general relativity, publishe...
Construction activities at the LIGO Observatories near Hanford, Washington and Livingston, Louisiana...
Future generations of gravitational wave interferometers are likely to be operated at cryogenic temp...
The detection of gravitational waves from compact binary mergers by LIGO has opened the era of gravi...
The detection of gravitational waves from compact binary mergers by LIGO has opened the era of gravi...
A remarkable design of LCGT was established by experimental efforts to detect gravi-tational waves i...
The detection of gravitational waves from compact binary mergers by LIGO has opened the era of gravi...
The Caltech-MIT joint LIGO project is operating three long-baseline interferometers (one of 2 km and...
The Caltech-MIT joint LIGO project is operating three long-baseline interferometers (one of 2 km and...