000453253 001__ 453253
000453253 005__ 20250716151853.0
000453253 0247_ $$2doi$$a10.1103/PhysRevLett.124.225001
000453253 0247_ $$2INSPIRETeX$$aKuhn:2019ysm
000453253 0247_ $$2inspire$$ainspire:1766645
000453253 0247_ $$2ISSN$$a0031-9007
000453253 0247_ $$2ISSN$$a1079-7114
000453253 0247_ $$2ISSN$$a1092-0145
000453253 0247_ $$2arXiv$$aarXiv:1911.09707
000453253 0247_ $$2datacite_doi$$a10.3204/PUBDB-2020-05089
000453253 0247_ $$2altmetric$$aaltmetric:71126546
000453253 0247_ $$2pmid$$apmid:32567918
000453253 0247_ $$2WOS$$aWOS:000537197200006
000453253 0247_ $$2openalex$$aopenalex:W3033278648
000453253 037__ $$aPUBDB-2020-05089
000453253 041__ $$aEnglish
000453253 082__ $$a530
000453253 088__ $$2arXiv$$aarXiv:1911.09707
000453253 1001_ $$0P:(DE-H253)PIP1026953$$aKühn, Steffen$$b0$$eCorresponding author
000453253 245__ $$aHigh Resolution Photoexcitation Measurements Exacerbate the Long-Standing Fe XVII Oscillator Strength Problem
000453253 260__ $$aCollege Park, Md.$$bAPS$$c2020
000453253 3367_ $$2DRIVER$$aarticle
000453253 3367_ $$2DataCite$$aOutput Types/Journal article
000453253 3367_ $$0PUB:(DE-HGF)16$$2PUB:(DE-HGF)$$aJournal Article$$bjournal$$mjournal$$s1609926704_16909
000453253 3367_ $$2BibTeX$$aARTICLE
000453253 3367_ $$2ORCID$$aJOURNAL_ARTICLE
000453253 3367_ $$00$$2EndNote$$aJournal Article
000453253 500__ $$aPhys. Rev. Lett. 124, 225001 (2020). Main text (6 pages, 3 figures), Supplmentary Material (8 pages, 4 figure), Published in Physical Review Letters
000453253 520__ $$aFor more than 40 years, most astrophysical observations and laboratory studies of two key soft x-ray diagnostic $2p$−$3d$ transitions, $3C$ and $3D$, in Fe XVII ions found oscillator strength ratios $f(3C)$/$f(3D)$ disagreeing with theory, but uncertainties had precluded definitive statements on this much studied conundrum. Here, we resonantly excite these lines using synchrotron radiation at PETRA III, and reach, at a millionfold lower photon intensities, a 10 times higher spectral resolution, and 3 times smaller uncertainty than earlier work. Our final result of $f(3C)$/$f(3D)$=3.09(8)(6) supports many of the earlier clean astrophysical and laboratory observations, while departing by five sigmas from our own newest large-scale ab initio calculations, and excluding all proposed explanations, including those invoking nonlinear effects and population transfers.
000453253 536__ $$0G:(DE-HGF)POF3-6G3$$a6G3 - PETRA III (POF3-622)$$cPOF3-622$$fPOF III$$x0
000453253 536__ $$0G:(DE-H253)I-20180534$$aFS-Proposal: I-20180534 (I-20180534)$$cI-20180534$$x1
000453253 588__ $$aDataset connected to CrossRef
000453253 650_7 $$2autogen$$aPlasma and Beam Physics
000453253 693__ $$0EXP:(DE-H253)P-P04-20150101$$1EXP:(DE-H253)PETRAIII-20150101$$6EXP:(DE-H253)P-P04-20150101$$aPETRA III$$fPETRA Beamline P04$$x0
000453253 7001_ $$0P:(DE-H253)PIP1030583$$aShah, Chintan$$b1$$eCorresponding author
000453253 7001_ $$00000-0002-2937-8037$$aLópez-Urrutia, José R. Crespo$$b2
000453253 7001_ $$0P:(DE-H253)PIP1086531$$aFujii, Keisuke$$b3
000453253 7001_ $$0P:(DE-H253)PIP1014894$$aSteinbrügge, René$$b4
000453253 7001_ $$0P:(DE-H253)PIP1086625$$aStierhof, Jakob$$b5
000453253 7001_ $$0P:(DE-H253)PIP1086553$$aTogawa, Moto$$b6
000453253 7001_ $$0P:(DE-HGF)0$$aHarman, Zoltán$$b7
000453253 7001_ $$00000-0003-0814-3287$$aOreshkina, Natalia S.$$b8
000453253 7001_ $$00000-0002-3724-3730$$aCheung, Charles$$b9
000453253 7001_ $$00000-0002-7751-6553$$aKozlov, Mikhail G.$$b10
000453253 7001_ $$00000-0003-0417-2726$$aPorsev, Sergey G.$$b11
000453253 7001_ $$0P:(DE-HGF)0$$aSafronova, Marianna S.$$b12
000453253 7001_ $$00000-0002-7366-1091$$aBerengut, Julian C.$$b13
000453253 7001_ $$0P:(DE-H253)PIP1080493$$aRosner, Michael$$b14
000453253 7001_ $$0P:(DE-H253)PIP1086635$$aBissinger, Matthias$$b15
000453253 7001_ $$0P:(DE-H253)PIP1086623$$aBallhausen, Ralf$$b16
000453253 7001_ $$0P:(DE-H253)PIP1015139$$aHell, Natalie$$b17
000453253 7001_ $$0P:(DE-HGF)0$$aPark, SungNam$$b18
000453253 7001_ $$00000-0001-7014-4120$$aChung, Moses$$b19
000453253 7001_ $$0P:(DE-H253)PIP1083334$$aHoesch, Moritz$$b20
000453253 7001_ $$0P:(DE-H253)PIP1010720$$aSeltmann, Jörn$$b21
000453253 7001_ $$00000-0002-6441-0864$$aSurzhykov, Andrey S.$$b22
000453253 7001_ $$00000-0002-2328-8444$$aYerokhin, Vladimir A.$$b23
000453253 7001_ $$0P:(DE-HGF)0$$aWilms, Jörn$$b24
000453253 7001_ $$00000-0002-6374-1119$$aPorter, F. Scott$$b25
000453253 7001_ $$0P:(DE-H253)PIP1026382$$aStöhlker, Thomas$$b26
000453253 7001_ $$0P:(DE-H253)PIP1024013$$aKeitel, Christoph H.$$b27
000453253 7001_ $$0P:(DE-H253)PIP1010834$$aPfeifer, Thomas$$b28
000453253 7001_ $$0P:(DE-H253)PIP1015227$$aBrown, Gregory V.$$b29
000453253 7001_ $$0P:(DE-H253)PIP1015150$$aLeutenegger, Maurice A.$$b30
000453253 7001_ $$0P:(DE-H253)PIP1015029$$aBernitt, Sven$$b31
000453253 773__ $$0PERI:(DE-600)1472655-5$$a10.1103/PhysRevLett.124.225001$$gVol. 124, no. 22, p. 225001$$n22$$p225001 (1-7)$$tPhysical review letters$$v124$$x1079-7114$$y2020
000453253 7870_ $$0PUBDB-2019-05599$$aKühn, Steffen et.al.$$d2019$$iIsParent$$rarXiv:1911.09707$$tHigh-resolution Photo-excitation Measurements Exacerbate the Long-standing Fe XVII Emission Problem
000453253 8564_ $$uhttps://bib-pubdb1.desy.de/record/453253/files/PhysRevLett.124.225001.pdf$$yOpenAccess
000453253 8564_ $$uhttps://bib-pubdb1.desy.de/record/453253/files/PhysRevLett.124.225001.gif?subformat=icon$$xicon$$yOpenAccess
000453253 8564_ $$uhttps://bib-pubdb1.desy.de/record/453253/files/PhysRevLett.124.225001.jpg?subformat=icon-1440$$xicon-1440$$yOpenAccess
000453253 8564_ $$uhttps://bib-pubdb1.desy.de/record/453253/files/PhysRevLett.124.225001.jpg?subformat=icon-180$$xicon-180$$yOpenAccess
000453253 8564_ $$uhttps://bib-pubdb1.desy.de/record/453253/files/PhysRevLett.124.225001.jpg?subformat=icon-640$$xicon-640$$yOpenAccess
000453253 8564_ $$uhttps://bib-pubdb1.desy.de/record/453253/files/PhysRevLett.124.225001.pdf?subformat=pdfa$$xpdfa$$yOpenAccess
000453253 909CO $$ooai:bib-pubdb1.desy.de:453253$$pdnbdelivery$$pdriver$$pVDB$$popen_access$$popenaire
000453253 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1026953$$aExternal Institute$$b0$$kExtern
000453253 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1030583$$aExternal Institute$$b1$$kExtern
000453253 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1086531$$aExternal Institute$$b3$$kExtern
000453253 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1014894$$aDeutsches Elektronen-Synchrotron$$b4$$kDESY
000453253 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1014894$$aExternal Institute$$b4$$kExtern
000453253 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1086625$$aExternal Institute$$b5$$kExtern
000453253 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1086553$$aExternal Institute$$b6$$kExtern
000453253 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1080493$$aExternal Institute$$b14$$kExtern
000453253 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1086635$$aExternal Institute$$b15$$kExtern
000453253 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1086623$$aExternal Institute$$b16$$kExtern
000453253 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1015139$$aExternal Institute$$b17$$kExtern
000453253 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1083334$$aDeutsches Elektronen-Synchrotron$$b20$$kDESY
000453253 9101_ $$0I:(DE-588b)2008985-5$$6P:(DE-H253)PIP1010720$$aDeutsches Elektronen-Synchrotron$$b21$$kDESY
000453253 9101_ $$0I:(DE-588)1043621512$$6P:(DE-H253)PIP1010720$$aEuropean XFEL$$b21$$kXFEL.EU
000453253 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1026382$$aExternal Institute$$b26$$kExtern
000453253 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1024013$$aExternal Institute$$b27$$kExtern
000453253 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1010834$$aExternal Institute$$b28$$kExtern
000453253 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1015227$$aExternal Institute$$b29$$kExtern
000453253 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1015150$$aExternal Institute$$b30$$kExtern
000453253 9101_ $$0I:(DE-HGF)0$$6P:(DE-H253)PIP1015029$$aExternal Institute$$b31$$kExtern
000453253 9131_ $$0G:(DE-HGF)POF3-621$$1G:(DE-HGF)POF3-620$$2G:(DE-HGF)POF3-600$$3G:(DE-HGF)POF3$$4G:(DE-HGF)POF$$9G:(DE-HGF)POF3-6211$$aDE-HGF$$bForschungsbereich Materie$$lVon Materie zu Materialien und Leben$$vIn-house research on the structure, dynamics and function of matter$$x0
000453253 9131_ $$0G:(DE-HGF)POF3-622$$1G:(DE-HGF)POF3-620$$2G:(DE-HGF)POF3-600$$3G:(DE-HGF)POF3$$4G:(DE-HGF)POF$$9G:(DE-HGF)POF3-6G3$$aDE-HGF$$bForschungsbereich Materie$$lVon Materie zu Materialien und Leben$$vFacility topic: Research on Matter with Brilliant Light Sources$$x1
000453253 9141_ $$y2020
000453253 915__ $$0StatID:(DE-HGF)0200$$2StatID$$aDBCoverage$$bSCOPUS$$d2020-08-32
000453253 915__ $$0StatID:(DE-HGF)0160$$2StatID$$aDBCoverage$$bEssential Science Indicators$$d2020-08-32
000453253 915__ $$0StatID:(DE-HGF)1230$$2StatID$$aDBCoverage$$bCurrent Contents - Electronics and Telecommunications Collection$$d2020-08-32
000453253 915__ $$0LIC:(DE-HGF)CCBY4$$2HGFVOC$$aCreative Commons Attribution CC BY 4.0
000453253 915__ $$0StatID:(DE-HGF)0600$$2StatID$$aDBCoverage$$bEbsco Academic Search$$d2020-08-32
000453253 915__ $$0StatID:(DE-HGF)0100$$2StatID$$aJCR$$bPHYS REV LETT : 2018$$d2020-08-32
000453253 915__ $$0StatID:(DE-HGF)9905$$2StatID$$aIF >= 5$$bPHYS REV LETT : 2018$$d2020-08-32
000453253 915__ $$0StatID:(DE-HGF)0113$$2StatID$$aWoS$$bScience Citation Index Expanded$$d2020-08-32
000453253 915__ $$0StatID:(DE-HGF)0199$$2StatID$$aDBCoverage$$bClarivate Analytics Master Journal List$$d2020-08-32
000453253 915__ $$0StatID:(DE-HGF)0150$$2StatID$$aDBCoverage$$bWeb of Science Core Collection$$d2020-08-32
000453253 915__ $$0StatID:(DE-HGF)0510$$2StatID$$aOpenAccess
000453253 915__ $$0StatID:(DE-HGF)0571$$2StatID$$aDBCoverage$$bSCOAP3 sponsored Journal$$d2020-08-32
000453253 915__ $$0StatID:(DE-HGF)1150$$2StatID$$aDBCoverage$$bCurrent Contents - Physical, Chemical and Earth Sciences$$d2020-08-32
000453253 915__ $$0StatID:(DE-HGF)0300$$2StatID$$aDBCoverage$$bMedline$$d2020-08-32
000453253 915__ $$0StatID:(DE-HGF)0420$$2StatID$$aNationallizenz$$d2020-08-32$$wger
000453253 915__ $$0StatID:(DE-HGF)0030$$2StatID$$aPeer Review$$bASC$$d2020-08-32
000453253 9201_ $$0I:(DE-H253)HAS-User-20120731$$kDOOR ; HAS-User$$lDOOR-User$$x0
000453253 9201_ $$0I:(DE-H253)FS-PET-S-20190712$$kFS-PET-S$$lExperimentebetreuung PETRA III$$x1
000453253 980__ $$ajournal
000453253 980__ $$aVDB
000453253 980__ $$aUNRESTRICTED
000453253 980__ $$aI:(DE-H253)HAS-User-20120731
000453253 980__ $$aI:(DE-H253)FS-PET-S-20190712
000453253 9801_ $$aFullTexts