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      Renormalized Energies of Superfluorescent Bursts from an Electron-Hole Magneto-plasma with High Gain in InGaAs Quantum Wells

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          Abstract

          We study light emission properties of a population-inverted 2D electron-hole plasma in a quantizing magnetic field. We observe a series of superfluorescent bursts, discrete both in time and energy, corresponding to the cooperative recombination of electron-hole pairs from different Landau levels. The emission energies are strongly renormalized due to many-body interactions among the photogenerated carriers, exhibiting red-shifts as large as 20 meV at 15 T. However, the magnetic field dependence of the lowest Landau level emission line remains excitonic at all magnetic fields. Interestingly, our time-resolved measurements show that this lowest-energy burst occurs only after all upper states become empty, suggesting that this excitonic stability is related to the `hidden symmetry' of 2D magneto-excitons expected in the magnetic quantum limit.

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          Author and article information

          Journal
          2010-09-15
          2012-05-28
          Article
          10.1103/PhysRevB.87.045304
          1009.3067
          e1540d6f-4c5e-4d33-b98b-e73e761d82c8

          http://arxiv.org/licenses/nonexclusive-distrib/1.0/

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          Custom metadata
          Physical Review B 87, 045304 (2013)
          5 pages, 4 figures
          cond-mat.mes-hall

          Nanophysics
          Nanophysics

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