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001035117 037__ $$aFZJ-2025-00213
001035117 041__ $$aEnglish
001035117 1001_ $$0P:(DE-Juel1)178627$$aKannis, Chrysovalantis$$b0$$eCorresponding author$$ufzj
001035117 1112_ $$aDPG Frühjahrstagung Sektion Atome, Moleküle, Quantenoptik und Photonik$$cFreiburg$$d2024-03-11 - 2024-03-15$$gSAMOP$$wGermany
001035117 245__ $$aA new polarization method and its applications
001035117 260__ $$c2024
001035117 3367_ $$033$$2EndNote$$aConference Paper
001035117 3367_ $$2DataCite$$aOther
001035117 3367_ $$2BibTeX$$aINPROCEEDINGS
001035117 3367_ $$2DRIVER$$aconferenceObject
001035117 3367_ $$2ORCID$$aLECTURE_SPEECH
001035117 3367_ $$0PUB:(DE-HGF)6$$2PUB:(DE-HGF)$$aConference Presentation$$bconf$$mconf$$s1736767574_12730$$xOther
001035117 520__ $$aSince the discovery of nuclear spin, scientific efforts have been focused on the production of non-equilibrium spin distributions, in which one of the possible spin projections prevails. Nuclear spin-polarization is advantageous for several fields of scientific (physics, chemistry, biology) and public (medicine) interest. Recently, our group developed a new polarization method based on radio-wave pumping at small magnetic fields that can be applied to particle beams and potentially to samples. Its advantages compared to conventional methods along with its limitations will be highlighted. Some exemplary applications are polarized sources and targets for the measurement of spin-dependent observables, polarized nuclear fusion, medical imaging diagnostics, etc.. Further developments and our future plans will be discussed.
001035117 536__ $$0G:(DE-HGF)POF4-612$$a612 - Cosmic Matter in the Laboratory (POF4-612)$$cPOF4-612$$fPOF IV$$x0
001035117 536__ $$0G:(GEPRIS)533904660$$aDFG project G:(GEPRIS)533904660 - Eine vielseitige Polarisationsmethode für Teilchen mit einfachen Hyperfeinstrukturen (533904660)$$c533904660$$x1
001035117 65027 $$0V:(DE-MLZ)SciArea-200$$2V:(DE-HGF)$$aNuclear Physics$$x0
001035117 65017 $$0V:(DE-MLZ)GC-2001-2016$$2V:(DE-HGF)$$aNuclei and Particles$$x0
001035117 7001_ $$0P:(DE-Juel1)131141$$aEngels, Ralf W.$$b1$$eCollaboration author$$ufzj
001035117 7001_ $$0P:(DE-Juel1)204381$$aEl-Kordy, Tarek$$b2$$eCollaboration author$$ufzj
001035117 7001_ $$0P:(DE-Juel1)192187$$aFaatz, Nicolas$$b3$$eCollaboration author$$ufzj
001035117 7001_ $$0P:(DE-Juel1)131182$$aHanhart, Christoph$$b4$$eCollaboration author$$ufzj
001035117 7001_ $$0P:(DE-Juel1)194961$$aKunkel, Lukas$$b5$$eCollaboration author
001035117 7001_ $$0P:(DE-Juel1)195614$$aSharma, Harsh$$b6$$eCollaboration author
001035117 7001_ $$0P:(DE-Juel1)131108$$aBüscher, Markus$$b7$$eCollaboration author$$ufzj
001035117 7001_ $$0P:(DE-Juel1)198732$$aWirtz, Jan$$b8$$eCollaboration author
001035117 909CO $$ooai:juser.fz-juelich.de:1035117$$pVDB
001035117 9101_ $$0I:(DE-588b)5008462-8$$6P:(DE-Juel1)178627$$aForschungszentrum Jülich$$b0$$kFZJ
001035117 9101_ $$0I:(DE-588b)5008462-8$$6P:(DE-Juel1)131141$$aForschungszentrum Jülich$$b1$$kFZJ
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001035117 9101_ $$0I:(DE-588b)36225-6$$6P:(DE-Juel1)194961$$aRWTH Aachen$$b5$$kRWTH
001035117 9101_ $$0I:(DE-HGF)0$$6P:(DE-Juel1)195614$$a FH Aachen, Campus Jülich$$b6
001035117 9101_ $$0I:(DE-588b)5008462-8$$6P:(DE-Juel1)131108$$aForschungszentrum Jülich$$b7$$kFZJ
001035117 9101_ $$0I:(DE-588b)36225-6$$6P:(DE-Juel1)198732$$aRWTH Aachen$$b8$$kRWTH
001035117 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
001035117 9141_ $$y2024
001035117 920__ $$lyes
001035117 9201_ $$0I:(DE-Juel1)IKP-2-20111104$$kIKP-2$$lExperimentelle Hadrondynamik$$x0
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001035117 980__ $$aI:(DE-Juel1)IKP-2-20111104
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