Spin-orbit splitting of image states

dc.creatorMcLaughlan, J R
dc.creatorLlewellyn-Samuel, E M
dc.creatorCrampin, S
dc.date2004-07-08
dc.date.accessioned2026-07-07T02:59:06Z
dc.date.available2026-07-07T02:59:06Z
dc.descriptionWe quantify the effect of the spin-orbit interaction on the Rydberg-like series of image state electrons at the (111) and (001) surface of Ir, Pt and Au. Using relativistic multiple-scattering methods we find Rashba-like dispersions with Delta E(K)=gamma K with values of gamma for n=1 states in the range 38-88 meV Angstrom. Extending the phase-accumulation model to include spin-orbit scattering we find that the splittings vary like 1/(n+a)^3 where a is the quantum defect and that they are related to the probability of spin-flip scattering at the surface. The splittings should be observable experimentally being larger in magnitude than some exchange-splittings that have been resolved by inverse photoemission, and are comparable to linewidths from inelastic lifetimes.
dc.description10 pages, 4 figures
dc.identifierhttps://arxiv.org/abs/cond-mat/0407211
dc.identifierhttp://arxiv.org/abs/cond-mat/0407211
dc.identifierJ. Phys.: Condens. Matter 16 (2004) 6841-6849
dc.identifierdoi:10.1088/0953-8984/16/39/017
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/24381
dc.subjectMaterials Science
dc.titleSpin-orbit splitting of image states
dc.typetext

Files

Collections