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Volumn 81, Issue 15, 2010, Pages

Cooperative recombination of electron-hole pairs in semiconductor quantum wells under quantizing magnetic fields

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EID: 77955394308     PISSN: 10980121     EISSN: 1550235X     Source Type: Journal    
DOI: 10.1103/PhysRevB.81.155314     Document Type: Article
Times cited : (26)

References (42)
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  • 31
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    • The high-field Landau notation is used to specify a QW electron-hole plasma in a magnetic field; for low-field-high-field correspondence, see, e.g., 10.1103/PhysRevB.33.8336
    • The high-field Landau notation is used to specify a QW electron-hole plasma in a magnetic field; for low-field-high-field correspondence, see, e.g., A. H. MacDonald and D. S. Ritchie, Phys. Rev. B 33, 8336 (1986). 10.1103/PhysRevB.33.8336
    • (1986) Phys. Rev. B , vol.33 , pp. 8336
    • MacDonald, A.H.1    Ritchie, D.S.2
  • 32
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    • Although the very initial stage of SF requires full quantum electrodynamic analysis, the semiclassical approximation becomes valid as soon as the number of photons per mode becomes larger than one
    • Although the very initial stage of SF requires full quantum electrodynamic analysis, the semiclassical approximation becomes valid as soon as the number of photons per mode becomes larger than one.
  • 33
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    • ΩR also contains nonresonant "local field" corrections from screened Coulomb interactions. However, we will neglect them here, assuming ΩR =dA/2 where the dipole moment d/e0.5nm. The local field effect can be important for SF of a dense small sample of size much smaller than the wavelength. In our case it creates only a small correction to the SF dynamics
    • Ω R also contains nonresonant "local field" corrections from screened Coulomb interactions. However, we will neglect them here, assuming Ω R = d A / 2 where the dipole moment d / e0.5nm. The local field effect can be important for SF of a dense small sample of size much smaller than the wavelength. In our case it creates only a small correction to the SF dynamics.
  • 35
    • 0001226806 scopus 로고    scopus 로고
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    • 10.1103/PhysRevB.66.085337
    • H. Zhao, S. Wachter, and H. Kalt, Phys. Rev. B 66, 085337 (2002). 10.1103/PhysRevB.66.085337
    • (2002) Phys. Rev. B , vol.66 , pp. 085337
    • Zhao, H.1    Wachter, S.2    Kalt, H.3


* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.