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The matter-wave laser interferometer gravitation antenna (MIGA): New perspectives for fundamental physics and geosciences

hal.structure.identifierlp2n-02,lp2n-11
hal.structure.identifierSystèmes de Référence Temps Espace [SYRTE]
dc.contributor.authorCANUEL, B.
hal.structure.identifierSystèmes de Référence Temps Espace [SYRTE]
dc.contributor.authorAMAND, L.
hal.structure.identifierlp2n-02,lp2n-11
dc.contributor.authorBERTOLDI, A.
hal.structure.identifierAstrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux [ARTEMIS]
dc.contributor.authorCHAIBI, W.
hal.structure.identifierSystèmes de Référence Temps Espace [SYRTE]
dc.contributor.authorGEIGER, R.
hal.structure.identifierlp2n-02,lp2n-11
dc.contributor.authorGILLOT, J.
hal.structure.identifierSystèmes de Référence Temps Espace [SYRTE]
dc.contributor.authorLANDRAGIN, A.
hal.structure.identifierAstrophysique Relativiste Théories Expériences Métrologie Instrumentation Signaux [ARTEMIS]
dc.contributor.authorMERZOUGUI, M.
hal.structure.identifierlp2n-02,lp2n-11
dc.contributor.authorRIOU, I.
hal.structure.identifierlp2n-02,lp2n-11
dc.contributor.authorSCHMID, S. P.
hal.structure.identifierlp2n-02,lp2n-11
dc.contributor.authorBOUYER, P.
hal.structure.identifierEnvironnement Méditerranéen et Modélisation des Agro-Hydrosystèmes [EMMAH]
dc.contributor.authorDANQUIGNY, Charles
dc.date.accessioned2023-05-12T11:00:59Z
dc.date.available2023-05-12T11:00:59Z
dc.date.issued2014-12
dc.date.conference2014-05-05
dc.identifier.urihttps://oskar-bordeaux.fr/handle/20.500.12278/182040
dc.description.abstractEnWe are building a hybrid detector of new concept that couples laser and matter-wave interferometry to study sub Hertz variations of the strain tensor of space-time and gravitation. Using a set of atomic interferometers simultaneously manipulated by the resonant optical field of a 200 m cavity, the MIGA instrument will allow the monitoring of the evolution of the gravitational field at unprecedented sensitivity, which will be exploited both for geophysical studies and for Gravitational Waves (GWs) detection. This new infrastructure will be embedded into the LSBB underground laboratory, ideally located away from major anthropogenic disturbances and benefitting from very low background noise.
dc.language.isoen
dc.source.titleE3S Web of Conferences
dc.title.enThe matter-wave laser interferometer gravitation antenna (MIGA): New perspectives for fundamental physics and geosciences
dc.typeCommunication dans un congrès avec actes
dc.identifier.doi10.1051/e3sconf/20140401004
dc.subject.halPhysique [physics]/Physique [physics]/Optique [physics.optics]
bordeaux.page01004
bordeaux.volume4
bordeaux.hal.laboratoriesLaboratoire Photonique, Numérique et Nanosciences (LP2N) - UMR 5298*
bordeaux.institutionUniversité de Bordeaux
bordeaux.institutionCNRS
bordeaux.countryFR
bordeaux.title.proceedingi-DUST 2014 – Inter-Disciplinary Underground Science & Technology
bordeaux.conference.cityApt
bordeaux.peerReviewednon
hal.identifierhal-01142050
hal.version1
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-01142050v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.btitle=E3S%20Web%20of%20Conferences&rft.date=2014-12&rft.volume=4&rft.spage=01004&rft.epage=01004&rft.au=CANUEL,%20B.&AMAND,%20L.&BERTOLDI,%20A.&CHAIBI,%20W.&GEIGER,%20R.&rft.genre=proceeding


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