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001035116 037__ $$aFZJ-2025-00212
001035116 041__ $$aEnglish
001035116 1001_ $$0P:(DE-Juel1)192187$$aFaatz, Nicolas$$b0$$eCorresponding author$$ufzj
001035116 1112_ $$aDPG Frühjahrstagung Sektion Atome, Moleküle, Quantenoptik und Photonik$$cFreiburg$$d2024-03-11 - 2024-03-15$$gSAMOP$$wGermany
001035116 245__ $$aA universal method to polarize beams and samples
001035116 260__ $$c2024
001035116 3367_ $$033$$2EndNote$$aConference Paper
001035116 3367_ $$2DataCite$$aOther
001035116 3367_ $$2BibTeX$$aINPROCEEDINGS
001035116 3367_ $$2DRIVER$$aconferenceObject
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001035116 3367_ $$0PUB:(DE-HGF)6$$2PUB:(DE-HGF)$$aConference Presentation$$bconf$$mconf$$s1736768467_16129$$xOther
001035116 502__ $$cFH Aachen, Campus Jülich
001035116 520__ $$aIn various applications a high nuclear polarisation, ideally a total alignment of all spins, is favourable, e.g. for sources and targets for fundamental research. The hereby presented method provides an inexpensive, fast, versatile and effective solution to produce highly polarised materials in reasonable amounts based on radio-wave pumping of hyperfine states and quantum interference effects. This method is theoretically understood and was experimentally proven for beams of metastable hydrogen atoms in the keV energy range. Thus, this technique opens the door for new applications as polarised tracers or even low-field MRI with even better spatial resolution in medicine or the production of polarised fuel to increase the energy output.
001035116 536__ $$0G:(DE-HGF)POF4-612$$a612 - Cosmic Matter in the Laboratory (POF4-612)$$cPOF4-612$$fPOF IV$$x0
001035116 536__ $$0G:(GEPRIS)533904660$$aDFG project G:(GEPRIS)533904660 - Eine vielseitige Polarisationsmethode für Teilchen mit einfachen Hyperfeinstrukturen (533904660)$$c533904660$$x1
001035116 65027 $$0V:(DE-MLZ)SciArea-200$$2V:(DE-HGF)$$aNuclear Physics$$x0
001035116 65017 $$0V:(DE-MLZ)GC-2001-2016$$2V:(DE-HGF)$$aNuclei and Particles$$x0
001035116 7001_ $$0P:(DE-Juel1)204381$$aEl-Kordy, Tarek$$b1$$eCollaboration author$$ufzj
001035116 7001_ $$0P:(DE-Juel1)131182$$aHanhart, Christoph$$b2$$eCollaboration author$$ufzj
001035116 7001_ $$0P:(DE-Juel1)178627$$aKannis, Chrysovalantis$$b3$$eCollaboration author$$ufzj
001035116 7001_ $$0P:(DE-Juel1)194961$$aKunkel, Lukas$$b4$$eCollaboration author
001035116 7001_ $$0P:(DE-Juel1)201229$$aPütz, Simon Jakob$$b5$$eCollaboration author
001035116 7001_ $$0P:(DE-Juel1)195614$$aSharma, Harsh$$b6$$eCollaboration author
001035116 7001_ $$0P:(DE-Juel1)194670$$aVerhoeven, Vincent Johannes$$b7$$ufzj
001035116 7001_ $$0P:(DE-Juel1)198732$$aWirtz, Jan$$b8$$eCollaboration author
001035116 909CO $$ooai:juser.fz-juelich.de:1035116$$pVDB
001035116 9101_ $$0I:(DE-588b)5008462-8$$6P:(DE-Juel1)192187$$aForschungszentrum Jülich$$b0$$kFZJ
001035116 9101_ $$0I:(DE-588b)5008462-8$$6P:(DE-Juel1)204381$$aForschungszentrum Jülich$$b1$$kFZJ
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001035116 9101_ $$0I:(DE-588b)36225-6$$6P:(DE-Juel1)194961$$aRWTH Aachen$$b4$$kRWTH
001035116 9101_ $$0I:(DE-HGF)0$$6P:(DE-Juel1)201229$$aGSI: Helmholtzzentrum für Scherionen GmbH$$b5
001035116 9101_ $$0I:(DE-HGF)0$$6P:(DE-Juel1)195614$$a FH Aachen, Campus Jülich$$b6
001035116 9101_ $$0I:(DE-588b)5008462-8$$6P:(DE-Juel1)194670$$aForschungszentrum Jülich$$b7$$kFZJ
001035116 9101_ $$0I:(DE-HGF)0$$6P:(DE-Juel1)198732$$a GSI: Helmholtzzentrum für Schwerionen$$b8
001035116 9131_ $$0G:(DE-HGF)POF4-612$$1G:(DE-HGF)POF4-610$$2G:(DE-HGF)POF4-600$$3G:(DE-HGF)POF4$$4G:(DE-HGF)POF$$aDE-HGF$$bForschungsbereich Materie$$lMatter and the Universe$$vCosmic Matter in the Laboratory$$x0
001035116 9141_ $$y2024
001035116 920__ $$lyes
001035116 9201_ $$0I:(DE-Juel1)IKP-2-20111104$$kIKP-2$$lExperimentelle Hadrondynamik$$x0
001035116 9201_ $$0I:(DE-Juel1)PGI-6-20110106$$kPGI-6$$lElektronische Eigenschaften$$x1
001035116 9201_ $$0I:(DE-Juel1)ZEA-1-20090406$$kZEA-1$$lZentralinstitut für Technologie$$x2
001035116 9201_ $$0I:(DE-Juel1)IAS-4-20090406$$kIAS-4$$lTheorie der Starken Wechselwirkung$$x3
001035116 980__ $$aconf
001035116 980__ $$aVDB
001035116 980__ $$aI:(DE-Juel1)IKP-2-20111104
001035116 980__ $$aI:(DE-Juel1)PGI-6-20110106
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