Challenges in thermal noise for 3rd generation of gravitational wave detectors
DOI10.1007/S10714-010-1066-5zbMath1208.83038OpenAlexW2088952348WikidataQ60278798 ScholiaQ60278798MaRDI QIDQ630009
Fulvio Ricci, Michele Punturo, Jean-Yves Vinet, Ronny Nawrodt, Sheila Rowan, James Hough
Publication date: 10 March 2011
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://www.openaccessrepository.it/record/21664
Applications of statistics to physics (62P35) Classical and relativistic thermodynamics (80A10) Observational and experimental questions in relativity and gravitational theory (83B05) Gravitational waves (83C35) Statistical astronomy (85A35)
Cites Work
- Mechanical thermal noise in coupled oscillators.
- Thermal noise reduction in interferometric gravitational wave antennas: using high order TEM modes
- Ground-based gravitational-wave detection: now and future
- Finite element modelling of the mechanical loss of silica suspension fibres for advanced gravitational wave detectors
- Excess mechanical loss associated with dielectric mirror coatings on test masses in interferometric gravitational wave detectors
- Thermal noise in interferometric gravitational wave detectors due to dielectric optical coatings
- Ground-based interferometric gravitational-wave detectors in the LISA epoch
- Mechanical loss in tantala/silica dielectric mirror coatings
- Suspensions thermal noise in the LIGO gravitational wave detector
- Mirror thermal noise in flat-beam cavities for advanced gravitational wave interferometers
- Very high quality factor measured in annealed fused silica
- Investigation of mechanical dissipation in CO 2 laser-drawn fused silica fibres and welds
- The dependence of test-mass thermal noises on beam shape in gravitational-wave interferometers
- Fundamentals of Interferometric Gravitational Wave Detectors
- Irreversibility and Generalized Noise
- On a Theorem of Irreversible Thermodynamics
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