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Gravitational Waves [Sources]


This chapter is based on omega tau 223 – Relativität und Gravitationswellen.


Advances in bonding for the construction of mirror suspensions of future generation gravitational wave detectorsMariëlle van VeggelPresentationPDF
Beam QualityRP PhotonicsArticleWebsite
CoherenceWikipediaArticle Website
Coherence LengthRP PhotonicsArticleWebsite
CryopumpWikipediaArticle Website
Damping ratioWikipediaArticle Website
Design of the Advanced LIGO recycling cavitiesOSAArain/MuellerPaperPDF
Detection of gravitational wavesJu/Blair/ZhaoPaperPDF
Distortion in the thermal noise spectrum and quality factor of nanomechanical devices due to finite frequency resolution with applications to the atomic force microscopeSader/Sanelli/Hughes/Monty/BieskePaperPDF
"Documentation of damping capacity of metallic, ceramic and metal-matrix composite materials "Zhang et al.PaperPDF
Einstein's gravitational waves found at lastNatureCastelvecchi/WitzeArticle Website
Electromagnetic ModeWikipediaArticle Website
First Observation gravitational wavesWikipediaArticle Website
Fluctuation-Dissipation TheoremWikipediaArticle Website
GE170817WikipediaArticle Website
"GEO 600 triple pendulum suspension system: Seismic isolation and control"Plissi et al.PaperPDF
GEO-HF und gequetschtes LichtGEO 600Article Website
GEO600 High-TechGEO 600Article Website
Gravitational Wave Detection Heralds New EraSky and TelescopeRobert NaeyeArticleWebsite
Gravitational waves frequencyStackexchangeForum PostWebsite
Higher-order ModesRP PhotonicsArticleWebsite
Intensity and Website
Kamioka Gravitational Wave DetectorWikipediaArticle Website
LaserWikipediaArticle Website
LIGO TechnologyLIGOArticle Website
LIGO's InterferometerLIGOArticle Website
LISAWikipediaArticle Website
LISA MissionLISAHomepageWebsite
Mechanical Quality Factor of Sapphire MembranesKane ScipioniPaperPDF
Michelson InterferometerWikipediaArticle Website
MicrotremorWikipediaArticle Website
Normal DistributionWikipediaArticle Website
Notes on thermal noise, with a bibliographyEric BlackPaperPDF
Observations and Modeling of Seismic NoiseJon PetersonPaperPDF
P-ValueWikipediaArticle Website
Power recycling for an interferometric gravitational wave detectorMasaki AndoPaperPDF
Quadruple suspension design for Advanced LIGORobertson et al.PaperPDF
Quality Factor / Q Factor; formulas and equationselectronics notesArticle Website
Quality Factor of a Single Pendulum for Use in Gravitational Wave InterferometryLauren WielgusPaperPDF
Quantum NoiseWikipediaArticle Website
"Quantum Noise in Gravitational Wave Detectors "Nergis MavalvalaPresentationPDF
Quasi-monolithic SuspensionsU Glasgow Institute for Gravitational ResearchArticle Website
Resonator ModesRP PhotonicsArticleWebsite
Seismic NoiseWikipediaArticle Website
SidebandWikipediaArticle Website
Squeezed states of light and their applications in laser interferometersRoman SchnabelPaperPDF
Stabilized high-power laser system for the gravitational wave detector advanced LIGOOSAKwee et al. PaperPDF
Standard DeviationWikipediaArticle Website
Study of the noise of micromechanical oscillators under quality factor enhancement via driving force controlJavier TamayoaPaperPDF
The GEO 600 laser systemZawischa et al. PaperPDF
"The modecleaner system and suspension aspects of GEO 600"Gossler et al.PaperPDF
The Vacuum System of GEO 600GEO 600Article Website
Thermal NoiseUTorontoArticlePDF
Time-Delay InterferometryTinto/DhurandharPaperPDF
Transverse ModeWikipediaArticle Website
Tuned Mass DamperWikipediaArticle Website
Turbomolecular PumpWikipediaArticle Website
Ultra-high VacuumWikipediaArticle Website
Ultra-High VacuumLIGOArticle Website
Vibration IsolationLIGOArticle Website
Virgo interferometerWikipediaArticle Website
What is the dark fringe in the Michelson interferometer? How would you explain it?QuoraForum PostWebsite

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