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dc.contributor.advisorSantos, Michael B.,en_US
dc.contributor.authorMeyer, Robert.en_US
dc.date.accessioned2013-08-16T12:19:38Z
dc.date.available2013-08-16T12:19:38Z
dc.date.issued2005en_US
dc.identifier.urihttps://hdl.handle.net/11244/835
dc.description.abstractIn this study we looked at spin resolved cyclotron resonance in InSb quantum wells. InSb is an attractive material for this type of work due to its small electron effective mass (0.014 mo), high intrinsic electron mobility, large electron g-factor (-51), and non-parabolic conduction band. The energies of the spin resolved transitions agreed with calculated values, even though some discrepancies in the intensities were evident. We used this spin-resolved cyclotron resonance to observe and study four subband Landau level avoided level crossings. These observed avoided level crossings are associated with the lowest Landau levels of the ground and first excited subbands of the InSb quantum wells. It was found that the energy gaps associated with anti-crossings of the same spin Landau levels depend on the tilt of the sample with respect to the magnetic field direction. This result is consistent with earlier, non spin-resolved, studies of Landau level coupling in GaAs quantum wells. We also observed anti-crossings associated with Landau Levels of opposite spin, with energy gaps that are essentially independent of sample tilt angle. Opposite spin anti-crossings are not expected from the theory explaining the GaAs experiments. Although spin-orbit effects are strong in InSb, the origins of the opposite spin anti-crossings are not definitively identified.en_US
dc.format.extentvii, 183 leaves :en_US
dc.subjectCyclotron resonance.en_US
dc.subjectQuantum wells.en_US
dc.subjectPhysics, Condensed Matter.en_US
dc.titleSpin resolved cyclotron resonance in indium antimonide quantum wells.en_US
dc.typeThesisen_US
dc.thesis.degreePh.D.en_US
dc.thesis.degreeDisciplineHomer L. Dodge Department of Physics and Astronomyen_US
dc.noteSource: Dissertation Abstracts International, Volume: 66-01, Section: B, page: 0327.en_US
dc.noteAdviser: Michael B. Santos.en_US
ou.identifier(UMI)AAI3162829en_US
ou.groupCollege of Arts and Sciences::Homer L. Dodge Department of Physics and Astronomy


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