Show simple item record

Files in this item

Thumbnail

Item metadata

dc.contributor.authorClose, Tom
dc.contributor.authorFadugba, Femi
dc.contributor.authorBenjamin, Simon C.
dc.contributor.authorFitzsimons, Joseph
dc.contributor.authorLovett, Brendon W.
dc.date.accessioned2014-08-21T09:31:02Z
dc.date.available2014-08-21T09:31:02Z
dc.date.issued2011-04-22
dc.identifier79639158
dc.identifier06ee166a-5b44-4bc6-8157-cf12fe536b78
dc.identifier000290097500016
dc.identifier79960620415
dc.identifier.citationClose , T , Fadugba , F , Benjamin , S C , Fitzsimons , J & Lovett , B W 2011 , ' Rapid and Robust Spin State Amplification ' , Physical Review Letters , vol. 106 , no. 16 , 167204 . https://doi.org/10.1103/PhysRevLett.106.167204en
dc.identifier.issn0031-9007
dc.identifier.otherORCID: /0000-0001-5142-9585/work/47136540
dc.identifier.urihttps://hdl.handle.net/10023/5204
dc.descriptionThis work was supported by the EPSRC, the National Research Foundation and Ministry of Education, Singapore, and the Royal Society.en
dc.description.abstractElectron and nuclear spins have been employed in many of the early demonstrations of quantum technology. However, applications in real world quantum technology are limited by the difficulty of measuring single spins. Here we show that it is possible to rapidly and robustly amplify a spin state using a lattice of ancillary spins. The model we employ corresponds to an extremely simple experimental system: a homogenous Ising-coupled spin lattice in one, two, or three dimensions, driven by a continuous microwave field. We establish that the process can operate at finite temperature (imperfect initial polarization) and under the effects of various forms of decoherence.
dc.format.extent4
dc.format.extent206585
dc.language.isoeng
dc.relation.ispartofPhysical Review Lettersen
dc.subjectSingle-shot readouten
dc.subjectElectron-spinen
dc.subjectQuantum-doten
dc.subjectQC Physicsen
dc.subject.lccQCen
dc.titleRapid and Robust Spin State Amplificationen
dc.typeJournal articleen
dc.contributor.institutionUniversity of St Andrews. School of Physics and Astronomyen
dc.contributor.institutionUniversity of St Andrews. Condensed Matter Physicsen
dc.identifier.doi10.1103/PhysRevLett.106.167204
dc.description.statusPeer revieweden


This item appears in the following Collection(s)

Show simple item record