dc.identifier.uri |
http://dx.doi.org/10.15488/1858 |
|
dc.identifier.uri |
http://www.repo.uni-hannover.de/handle/123456789/1883 |
|
dc.contributor.author |
Mavalvala, Nergis
|
|
dc.contributor.author |
McClelland, David E.
|
|
dc.contributor.author |
Mueller, Guido
|
|
dc.contributor.author |
Reitze, D.H.
|
|
dc.contributor.author |
Schnabel, Roman
|
|
dc.contributor.author |
Willke, Benno
|
|
dc.date.accessioned |
2017-09-07T13:27:58Z |
|
dc.date.available |
2017-09-07T13:27:58Z |
|
dc.date.issued |
2011 |
|
dc.identifier.citation |
Mavalvala, N.; McClelland, D.E.; Mueller, G.; Reitze, D.H.; Schnabel, R.; Willke, B.: Lasers and optics: Looking towards third generation gravitational wave detectors. In: General Relativity and Gravitation 43 (2011), Nr. 2, S. 569-592. DOI: https://doi.org/10.1007/s10714-010-1023-3 |
|
dc.description.abstract |
Third generation terrestrial interferometric gravitational wave detectors will likely require significant advances in laser and optical technologies to reduce two of the main limiting noise sources: thermal noise due to mirror coatings and quantum noise arising from a combination of shot noise and radiation pressure noise. Increases in laser power and possible changes of the operational wavelength require new high power laser sources and new electro-optic modulators and Faraday isolators. Squeezed light can be used to further reduce the quantum noise while nano-structured optical components can be used to reduce or eliminate mirror coating thermal noise as well as to implement all-reflective interferometer configurations to avoid thermal effects in mirror substrates. This paper is intended to give an overview on the current state-of-the-art and future trends in these areas of ongoing research and development. |
eng |
dc.description.sponsorship |
NSF/PHY0555453 |
|
dc.description.sponsorship |
NSF/PHY0757968 |
|
dc.description.sponsorship |
NSF/PHY0653582 |
|
dc.description.sponsorship |
DFG/SFB/407 |
|
dc.description.sponsorship |
DFG/SFB/TR7 |
|
dc.description.sponsorship |
DFG/EXC/QUEST |
|
dc.language.iso |
eng |
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dc.publisher |
Heidelberg : Springer Verlag |
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dc.relation.ispartofseries |
General Relativity and Gravitation 43 (2011), Nr. 2 |
|
dc.rights |
CC BY-NC 4.0 Unported |
|
dc.rights.uri |
https://creativecommons.org/licenses/by-nc/4.0/ |
|
dc.subject |
Gravitational wave detection |
eng |
dc.subject |
Laser interferometry |
eng |
dc.subject |
Gravitationswelle |
ger |
dc.subject.ddc |
530 | Physik
|
ger |
dc.title |
Lasers and optics: Looking towards third generation gravitational wave detectors |
|
dc.type |
Article |
|
dc.type |
Text |
|
dc.relation.issn |
00017701 |
|
dc.relation.doi |
https://doi.org/10.1007/s10714-010-1023-3 |
|
dc.bibliographicCitation.issue |
2 |
|
dc.bibliographicCitation.volume |
43 |
|
dc.bibliographicCitation.firstPage |
569 |
|
dc.bibliographicCitation.lastPage |
592 |
|
dc.description.version |
publishedVersion |
|
tib.accessRights |
frei zug�nglich |
|