A gravity antenna based on quantum technologies: MIGA
hal.structure.identifier | Laboratoire Photonique, Numérique et Nanosciences [LP2N] | |
dc.contributor.author | CANUEL, B. | |
hal.structure.identifier | Laboratoire Photonique, Numérique et Nanosciences [LP2N] | |
dc.contributor.author | ZOU, X. | |
hal.structure.identifier | Laboratoire Photonique, Numérique et Nanosciences [LP2N] | |
dc.contributor.author | SABULSKY, D.O. | |
hal.structure.identifier | Laboratoire Photonique, Numérique et Nanosciences [LP2N] | |
dc.contributor.author | JUNCA, J. | |
hal.structure.identifier | Laboratoire Photonique, Numérique et Nanosciences [LP2N] | |
dc.contributor.author | BERTOLDI, A. | |
hal.structure.identifier | Systèmes de Référence Temps Espace [SYRTE] | |
dc.contributor.author | BEAUFILS, Q. | |
hal.structure.identifier | Systèmes de Référence Temps Espace [SYRTE] | |
dc.contributor.author | GEIGER, R. | |
hal.structure.identifier | Systèmes de Référence Temps Espace [SYRTE] | |
dc.contributor.author | LANDRAGIN, A. | |
dc.contributor.author | PREVEDELLI, M. | |
hal.structure.identifier | Laboratoire Souterrain à Bas Bruit [LSBB] | |
dc.contributor.author | GAFFET, S. | |
hal.structure.identifier | Laboratoire Souterrain à Bas Bruit [LSBB] | |
dc.contributor.author | BOYER, D. | |
hal.structure.identifier | Laboratoire Souterrain à Bas Bruit [LSBB] | |
dc.contributor.author | ROCHE, I. Lázaro | |
hal.structure.identifier | Laboratoire Photonique, Numérique et Nanosciences [LP2N] | |
dc.contributor.author | BOUYER, P. | |
dc.date.accessioned | 2023-05-12T10:32:47Z | |
dc.date.available | 2023-05-12T10:32:47Z | |
dc.date.conference | 2022-01-30 | |
dc.identifier.uri | https://oskar-bordeaux.fr/handle/20.500.12278/181446 | |
dc.description.abstractEn | We report the realization of a large scale gravity antenna based on matter-wave interferometry, the MIGA project. This experiment consists in an array of cold Rb sources correlated by a 150 m long optical cavity. MIGA is in construction at the LSBB underground laboratory, a site that benefits from a low background noise and is an ideal premise to carry out precision gravity measurements. The MIGA facility will be a demonstrator for a new generation of GW detector based on atom interferometry that could open the infrasound window for the observation of GWs. We describe here the status of the instrument construction, focusing on the infrastructure works at LSBB and the realization of the vacuum vessel of the antenna. | |
dc.language.iso | en | |
dc.title.en | A gravity antenna based on quantum technologies: MIGA | |
dc.type | Communication dans un congrès avec actes | |
dc.subject.hal | Physique [physics]/Physique [physics]/Physique Générale [physics.gen-ph] | |
dc.subject.hal | Physique [physics]/Relativité Générale et Cosmologie Quantique [gr-qc] | |
dc.subject.hal | Physique [physics]/Physique [physics]/Instrumentations et Détecteurs [physics.ins-det] | |
dc.identifier.arxiv | 2204.12137 | |
bordeaux.hal.laboratories | Laboratoire Photonique, Numérique et Nanosciences (LP2N) - UMR 5298 | * |
bordeaux.institution | Université de Bordeaux | |
bordeaux.institution | CNRS | |
bordeaux.country | IT | |
bordeaux.title.proceeding | 56th Rencontres de Moriond on Gravitation | |
bordeaux.conference.city | La Thuile | |
bordeaux.peerReviewed | non | |
hal.identifier | hal-03667511 | |
hal.version | 1 | |
hal.origin.link | https://hal.archives-ouvertes.fr//hal-03667511v1 | |
bordeaux.COinS | ctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.au=CANUEL,%20B.&ZOU,%20X.&SABULSKY,%20D.O.&JUNCA,%20J.&BERTOLDI,%20A.&rft.genre=proceeding |
Files in this item
Files | Size | Format | View |
---|---|---|---|
There are no files associated with this item. |