Integration of polarised 3He infrastructure with sample environment equipment

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dc.contributor.authorD'Adam, TMen_AU
dc.contributor.authorBooth, Nen_AU
dc.contributor.authorDavidson, Gen_AU
dc.contributor.authorLee, Sen_AU
dc.contributor.authorManning, AGen_AU
dc.contributor.authorTimperon, Nen_AU
dc.contributor.authorImperia, Pen_AU
dc.date.accessioned2022-08-29T22:26:56Zen_AU
dc.date.available2022-08-29T22:26:56Zen_AU
dc.date.issued2017-01-31en_AU
dc.date.statistics2021-09-24en_AU
dc.description.abstractMany challenges exist when attempting to integrate polarised 3He infrastructure with neutron beam instruments. This is often due to its sensitivity to the magnetic environment and also due to the compact geometry of many beam lines. One additional consideration is the effect that Sample Environment equipment can have on the functionality of a particular polarised neutron setup. We have been able to provide incident beam polarisation with two separate magnets providing fields at the sample position of up to 2 T. In addition, full polarisation analysis is possible over a temperature range of 30 mK to 800 K. To enable this, some pieces of Sample Environment equipment must be designed specifically for use with polarised 3He and in many cases modifications are necessary to accommodate the sensitive gas. We are also in the process of procuring an 8 T shielded asymmetric magnet suitable for use with polarised 3He infrastructure.en_AU
dc.identifier.citationD'Adam, T., Booth, N., Davidson, G., Lee, S., Manning, A., Timperon, N., & Imperia, P. (2017). Integration of polarised 3He infrastructure with sample environment equipment. Poster presented to the 41st Annual Condensed Matter and Materials Meeting, 31st January - 3rd February 2017 Charles Sturt University Wagga Wagga, NSW, Australia. (pp. 77). Retrieved from: https://physics.org.au/wp-content/uploads/cmm/2017/Wagga_2017_Conference_Handbook.pdfen_AU
dc.identifier.conferenceenddate3 February 2017en_AU
dc.identifier.conferencenameAustralian and New Zealand Institutes of Physics 41st Annual Condensed Matter and Materials Meetingen_AU
dc.identifier.conferenceplaceWagga Wagga, NSWen_AU
dc.identifier.conferencestartdate31 January 2017en_AU
dc.identifier.otherTP1en_AU
dc.identifier.pagination77en_AU
dc.identifier.urihttps://physics.org.au/wp-content/uploads/cmm/2017/Wagga_2017_Conference_Handbook.pdfen_AU
dc.identifier.urihttps://apo.ansto.gov.au/dspace/handle/10238/13658en_AU
dc.language.isoenen_AU
dc.publisherAustralian Institute of Physicsen_AU
dc.subjectBeamsen_AU
dc.subjectEven-odd nucleien_AU
dc.subjectHelium isotopesen_AU
dc.subjectIsotopesen_AU
dc.subjectLight nucleien_AU
dc.subjectNucleien_AU
dc.subjectNucleon beamsen_AU
dc.subjectParticle beamsen_AU
dc.subjectStable isotopesen_AU
dc.titleIntegration of polarised 3He infrastructure with sample environment equipmenten_AU
dc.typeConference Posteren_AU
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