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dc.contributor.authorROBERTS, B. M.
hal.structure.identifierSystèmes de Référence Temps Espace [SYRTE]
dc.contributor.authorDELVA, P.
dc.contributor.authorAL-MASOUDI, A.
hal.structure.identifierLaboratoire de Physique des Lasers [LPL]
dc.contributor.authorAMY-KLEIN, A.
hal.structure.identifierSystèmes de Référence Temps Espace [SYRTE]
dc.contributor.authorBAERENTSEN, C.
dc.contributor.authorBAYNHAM, C. F. A.
dc.contributor.authorBENKLER, E.
hal.structure.identifierSystèmes de Référence Temps Espace [SYRTE]
dc.contributor.authorBILICKI, S.
hal.structure.identifierSystèmes de Référence Temps Espace [SYRTE]
dc.contributor.authorBIZE, S.
dc.contributor.authorBOWDEN, W.
hal.structure.identifierSystèmes de Référence Temps Espace [SYRTE]
dc.contributor.authorCALVERT, J.
hal.structure.identifierSystèmes de Référence Temps Espace [SYRTE]
dc.contributor.authorCAMBIER, V.
hal.structure.identifierLaboratoire Photonique, Numérique et Nanosciences [LP2N]
dc.contributor.authorCANTIN, E.
dc.contributor.authorCURTIS, E. A.
dc.contributor.authorDÖRSCHER, S.
dc.contributor.authorFRANK, F.
dc.contributor.authorGILL, P.
dc.contributor.authorGODUN, R. M.
dc.contributor.authorGROSCHE, G.
dc.contributor.authorGUO, C.
hal.structure.identifierSystèmes de Référence Temps Espace [SYRTE]
dc.contributor.authorHEES, A.
dc.contributor.authorHILL, I. R.
dc.contributor.authorHOBSON, R.
dc.contributor.authorHUNTEMANN, N.
dc.contributor.authorKRONJÄGER, J.
dc.contributor.authorKOKE, S.
dc.contributor.authorKUHL, A.
dc.contributor.authorLANGE, R.
dc.contributor.authorLEGERO, T.
dc.contributor.authorLIPPHARDT, B.
dc.contributor.authorLISDAT, C.
hal.structure.identifierSystèmes de Référence Temps Espace [SYRTE]
dc.contributor.authorLODEWYCK, J.
dc.contributor.authorLOPEZ, O.
dc.contributor.authorMARGOLIS, H. S.
hal.structure.identifierSystèmes de Référence Temps Espace [SYRTE]
dc.contributor.authorÁLVAREZ-MARTÍNEZ, Hector
hal.structure.identifierSystèmes de Référence Temps Espace [SYRTE]
dc.contributor.authorMEYNADIER, F.
dc.contributor.authorOZIMEK, F.
hal.structure.identifierPhysikalisch-Technische Bundesanstalt [Braunschweig] [PTB]
dc.contributor.authorPEIK, E.
dc.contributor.authorPOTTIE, P. -E.
dc.contributor.authorQUINTIN, N.
dc.contributor.authorSANNER, C.
hal.structure.identifierSystèmes de Référence Temps Espace [SYRTE]
dc.contributor.authorDE SARLO, L.
dc.contributor.authorSCHIOPPO, M.
dc.contributor.authorSCHWARZ, R.
hal.structure.identifierInstituto de Plasmas e Fusão Nuclear [Lisboa] [IPFN]
dc.contributor.authorSILVA, A.
dc.contributor.authorSTERR, U.
dc.contributor.authorTAMM, Chr.
dc.contributor.authorTARGAT, R. Le
hal.structure.identifierSystèmes de Référence Temps Espace [SYRTE]
dc.contributor.authorTUCKEY, P.
hal.structure.identifierSystèmes de Référence Temps Espace [SYRTE]
dc.contributor.authorVALLET, Guy
dc.contributor.authorWATERHOLTER, T.
dc.contributor.authorXU, D.
hal.structure.identifierSystèmes de Référence Temps Espace [SYRTE]
dc.contributor.authorWOLF, P.
dc.date.accessioned2023-05-12T10:43:10Z
dc.date.available2023-05-12T10:43:10Z
dc.identifier.urihttps://oskar-bordeaux.fr/handle/20.500.12278/181668
dc.description.abstractEnWe search for transient variations of the fine structure constant using data from a European network of fiber-linked optical atomic clocks. By searching for coherent variations in the recorded clock frequency comparisons across the network, we significantly improve the constraints on transient variations of the fine structure constant. For example, we constrain the variation in alpha to <5*10^-17 for transients of duration 10^3 s. This analysis also presents a possibility to search for dark matter, the mysterious substance hypothesised to explain galaxy dynamics and other astrophysical phenomena that is thought to dominate the matter density of the universe. At the current sensitivity level, we find no evidence for dark matter in the form of topological defects (or, more generally, any macroscopic objects), and we thus place constraints on certain potential couplings between the dark matter and standard model particles, substantially improving upon the existing constraints, particularly for large (>~10^4 km) objects.
dc.language.isoen
dc.title.enSearch for transient variations of the fine structure constant and dark matter using fiber-linked optical atomic clocks
dc.typeDocument de travail - Pré-publication
dc.subject.halPhysique [physics]/Relativité Générale et Cosmologie Quantique [gr-qc]
dc.identifier.arxiv1907.02661
bordeaux.hal.laboratoriesLaboratoire Photonique, Numérique et Nanosciences (LP2N) - UMR 5298*
bordeaux.institutionUniversité de Bordeaux
bordeaux.institutionCNRS
hal.identifierhal-02410377
hal.version1
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-02410377v1
bordeaux.COinSctx_ver=Z39.88-2004&amp;rft_val_fmt=info:ofi/fmt:kev:mtx:journal&amp;rft.au=ROBERTS,%20B.%20M.&amp;DELVA,%20P.&amp;AL-MASOUDI,%20A.&amp;AMY-KLEIN,%20A.&amp;BAERENTSEN,%20C.&amp;rft.genre=preprint


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