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Skyrmions and the crossover from the integer to fractional quantum Hall effect at small Zeeman energies
981
Citations
19
References
1993
Year
Quantum Lattice SystemEngineeringMany-body Quantum PhysicStrongly Correlated Electron SystemsTopological Quantum StateZeeman EnergyQuantum MaterialsSmall Zeeman EnergiesHigh Magnetic FieldQuantum ScienceMajorana FermionPhysicsQuantum Field TheoryCondensed Matter TheoryQuantum MagnetismSpintronicsNatural SciencesCondensed Matter PhysicsApplied PhysicsDisordered Quantum SystemSecond OrderSkyrmions
The study investigates a two‑dimensional electron gas at ν=1 in a high magnetic field, varying the Zeeman‑to‑interaction energy ratio. The authors analyze the system by varying this ratio and discuss extensions to other odd‑integer and fractional filling factors. They find that a gap persists even at zero Zeeman energy, that quasiparticles are perturbative for large Zeeman energy but become skyrmions below a critical ratio, and that in GaAs heterojunctions the gap is dominated by correlations, implying skyrmionic quasiparticles.
We study the two-dimensional electron gas in a high magnetic field at filling factor \ensuremath{\nu}=1 for an arbitrary ratio of the Zeeman energy g${\mathrm{\ensuremath{\mu}}}_{\mathit{B}}$B to the typical interaction energy. We find that the system always has a gap, even when the one-particle gap vanishes, i.e., when g=0. When g is sufficiently large, the quasiparticles are perturbatively related to those in the noninteracting limit; we compute their energies to second order in the Coulomb interaction. For g smaller than a critical value ${\mathit{g}}_{\mathit{c}}$ the quasiparticles change character; in the limit of g\ensuremath{\rightarrow}0, they are skyrmions---spatially unbounded objects with infinite spin. In GaAs heterojunctions, the gap is unambiguously predominantly due to correlation effects; indeed, we tentatively conclude that g is always smaller than ${\mathit{g}}_{\mathit{c}}$, so the relevant quasiparticles are the skyrmions. The generalization to other odd-integer filling factors, and to \ensuremath{\nu}=1/3 and 1/5, is discussed.
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