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dc.contributor.authorAGUILERA, D.
dc.contributor.authorAHLERS, H.
hal.structure.identifierlp2n-02,lp2n-11
dc.contributor.authorBATTELIER, Baptiste
dc.contributor.authorBAWAMIA, A.
hal.structure.identifierlp2n-02,lp2n-11
dc.contributor.authorBERTOLDI, Andrea
dc.contributor.authorBONDARESCU, R.
dc.contributor.authorBONGS, K.
hal.structure.identifierlp2n-02,lp2n-11
dc.contributor.authorBOUYER, Philippe
dc.contributor.authorBRAXMAIER, C.
hal.structure.identifierAgence Spatiale Européenne = European Space Agency [ESA]
dc.contributor.authorCACCIAPUOTI, L.
dc.contributor.authorCHALONER, C.
dc.contributor.authorCHWALLA, M.
dc.contributor.authorERTMER, W.
hal.structure.identifierMax-Planck-Institut für Sonnensystemforschung = Max Planck Institute for Solar System Research [MPS]
dc.contributor.authorFRANZ, M.
dc.contributor.authorGAALOUL, N.
dc.contributor.authorGEHLER, M.
dc.contributor.authorGERARDI, D.
dc.contributor.authorGESA, L.
dc.contributor.authorGÜRLEBECK, N.
dc.contributor.authorHARTWIG, J.
dc.contributor.authorHAUTH, M.
dc.contributor.authorHELLMIG, O.
dc.contributor.authorHERR, W.
dc.contributor.authorHERRMANN, S.
dc.contributor.authorHESKE, A.
dc.contributor.authorHINTON, A.
dc.contributor.authorIRELAND, P.
dc.contributor.authorJETZER, P.
dc.contributor.authorJOHANN, U.
dc.contributor.authorKRUTZIK, M.
dc.contributor.authorKUBELKA, A.
dc.contributor.authorLÄMMERZAHL, C.
hal.structure.identifierSystèmes de Référence Temps Espace [SYRTE]
dc.contributor.authorLANDRAGIN, A.
dc.contributor.authorLLORO, I.
hal.structure.identifierCentre National d'Études Spatiales [Toulouse] [CNES]
dc.contributor.authorMASSONNET, D.
dc.contributor.authorMATEOS, I.
dc.contributor.authorMILKE, A.
dc.contributor.authorNOFRARIAS, M.
dc.contributor.authorOSWALD, M.
dc.contributor.authorPETERS, A.
dc.contributor.authorPOSSO-TRUJILLO, K.
dc.contributor.authorRASEL, E.
dc.contributor.authorROCCO, E.
dc.contributor.authorROURA, A.
dc.contributor.authorRUDOLPH, J.
dc.contributor.authorSCHLEICH, W.
hal.structure.identifierChemnitz University of Technology / Technische Universität Chemnitz
dc.contributor.authorSCHUBERT, C.
dc.contributor.authorSCHULDT, T.
dc.contributor.authorSEIDEL, S.
dc.contributor.authorSENGSTOCK, K.
dc.contributor.authorSOPUERTA, C. F.
hal.structure.identifierDipartimento di Fisica e Astronomia [Firenze]
dc.contributor.authorSORRENTINO, F.
dc.contributor.authorSUMMERS, D.
hal.structure.identifierDipartimento di Fisica e Astronomia [Firenze]
dc.contributor.authorTINO, G. M.
dc.contributor.authorTRENKEL, C.
dc.contributor.authorUZUNOGLU, N.
dc.contributor.authorVON KLITZING, W.
dc.contributor.authorWALSER, R.
dc.contributor.authorWENDRICH, T.
dc.contributor.authorWENZLAWSKI, A.
dc.contributor.authorWESSELS, P.
dc.contributor.authorWICHT, A.
dc.contributor.authorWILLE, E.
dc.contributor.authorWILLIAMS, M.
dc.contributor.authorWINDPASSINGER, P.
hal.structure.identifierLaboratoire Aimé Cotton [LAC]
dc.contributor.authorZAHZAM, N.
dc.date.accessioned2023-05-12T10:20:30Z
dc.date.available2023-05-12T10:20:30Z
dc.date.created2013-12-20
dc.date.issued2014
dc.identifier.issn0264-9381
dc.identifier.urihttps://oskar-bordeaux.fr/handle/20.500.12278/181076
dc.description.abstractEnThe theory of general relativity describes macroscopic phenomena driven by the influence of gravity while quantum mechanics brilliantly accounts for microscopic effects. Despite their tremendous individual success, a complete unification of fundamental interactions is missing and remains one of the most challenging and important quests in modern theoretical physics. The STE-QUEST satellite mission, proposed as a medium-size mission within the Cosmic Vision program of the European Space Agency (ESA), aims for testing general relativity with high precision in two experiments by performing a measurement of the gravitational redshift of the Sun and the Moon by comparing terrestrial clocks, and by performing a test of the Universality of Free Fall of matter waves in the gravitational field of Earth comparing the trajectory of two Bose-Einstein condensates of Rb85 and Rb87. The two ultracold atom clouds are monitored very precisely thanks to techniques of atom interferometry. This allows to reach down to an uncertainty in the Eötvös parameter of at least 2x10E-15. In this paper, we report about the results of the phase A mission study of the atom interferometer instrument covering the description of the main payload elements, the atomic source concept, and the systematic error sources.
dc.language.isoen
dc.publisherIOP Publishing
dc.title.enSTE-QUEST - Test of the Universality of Free Fall Using Cold Atom Interferometry
dc.typeArticle de revue
dc.identifier.doi10.1088/0264-9381/31/11/115010
dc.subject.halPhysique [physics]/Relativité Générale et Cosmologie Quantique [gr-qc]
dc.subject.halPhysique [physics]/Physique [physics]/Physique Atomique [physics.atom-ph]
dc.subject.halPhysique [physics]/Physique [physics]/Physique de l'espace [physics.space-ph]
dc.subject.halPhysique [physics]/Physique Quantique [quant-ph]
dc.identifier.arxiv1312.5980
bordeaux.journalClassical and Quantum Gravity
bordeaux.page115010
bordeaux.volume31
bordeaux.hal.laboratoriesLaboratoire Photonique, Numérique et Nanosciences (LP2N) - UMR 5298*
bordeaux.institutionUniversité de Bordeaux
bordeaux.institutionCNRS
bordeaux.peerReviewedoui
hal.identifierhal-00943329
hal.version1
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00943329v1
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