A gravitational wave detector operating beyond the quantum shot-noise limit: Squeezed light in application

Schnabel, Roman; LIGO Scientific Collaboration

dc.identifier.uri	http://dx.doi.org/10.15488/1009
dc.identifier.uri	http://www.repo.uni-hannover.de/handle/123456789/1033
dc.contributor.author	Schnabel, Roman
dc.contributor.author	LIGO Scientific Collaboration
dc.date.accessioned	2016-12-22T11:58:58Z
dc.date.available	2016-12-22T11:58:58Z
dc.date.issued	2013
dc.identifier.citation	Schnabel, R.: A gravitational wave detector operating beyond the quantum shot-noise limit: Squeezed light in application. In: EPJ Web of Conferences 57 (2013), 2002. DOI: https://doi.org/10.1051/epjconf/20135702002
dc.description.abstract	This contribution reviews our recent progress on the generation of squeezed light [1], and also the recent squeezed-light enhancement of the gravitational wave detector GEO 600 [2]. GEO 600 is currently the only GW observatory operated by the LIGO Scientific Collaboration in its search for gravitational waves. With the help of squeezed states of light it now operates with its best ever sensitivity, which not only proves the qualification of squeezed light as a key technology for future gravitational wave astronomy but also the usefulness of quantum entanglement.	eng
dc.language.iso	eng
dc.publisher	Les Ulis : EDP Sciences
dc.relation.ispartofseries	EPJ Web of Conferences 57 (2013)
dc.rights	CC BY 2.0 Unported
dc.rights.uri	https://creativecommons.org/licenses/by/2.0/
dc.subject.classification	Konferenzschrift	ger
dc.subject.ddc	620 \| Ingenieurwissenschaften und Maschinenbau	ger
dc.subject.ddc	530 \| Physik	ger
dc.title	A gravitational wave detector operating beyond the quantum shot-noise limit: Squeezed light in application	eng
dc.type	Article
dc.type	Text
dc.relation.issn	21016275
dc.relation.doi	https://doi.org/10.1051/epjconf/20135702002
dc.bibliographicCitation.volume	57
dc.bibliographicCitation.lastPage	2002
dc.description.version	publishedVersion
tib.accessRights	frei zug�nglich