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85033020796
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note
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Similar equations, but with density-independent time constants, have been introduced previously to describe the exciton dynamics. See, for example, see Ref. 8.
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x can be found in J. Lee, E. S. Koteles, and M. O. Vassell, Phys. Rev. B 33, 5512 (1986); Y. J. Chen, E. S. Koteles, J. Lee, and B. S. Elman, Proc. SPIE 792, 162 (1987). At very low temperatures the exciton lifetime has a different form governed by intrinsic radiative lifetime, as obtained by L. C. Andreani, F. Tassone, and F. Bassani, Solid State Commun. 77, 641 (1991).
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x can be found in J. Lee, E. S. Koteles, and M. O. Vassell, Phys. Rev. B 33, 5512 (1986); Y. J. Chen, E. S. Koteles, J. Lee, and B. S. Elman, Proc. SPIE 792, 162 (1987). At very low temperatures the exciton lifetime has a different form governed by intrinsic radiative lifetime, as obtained by L. C. Andreani, F. Tassone, and F. Bassani, Solid State Commun. 77, 641 (1991).
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x can be found in J. Lee, E. S. Koteles, and M. O. Vassell, Phys. Rev. B 33, 5512 (1986); Y. J. Chen, E. S. Koteles, J. Lee, and B. S. Elman, Proc. SPIE 792, 162 (1987). At very low temperatures the exciton lifetime has a different form governed by intrinsic radiative lifetime, as obtained by L. C. Andreani, F. Tassone, and F. Bassani, Solid State Commun. 77, 641 (1991).
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85033030571
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note
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The dark exciton state at K also may be considered to be a linear combination of Slater determinant crystal states with a conduction-band electron at K and a valence-band vacancy at K-k for all possible k. We expect that the saturation value for large K exciton density imposed by the Fermi exclusion is much larger than the occupancy of dark excitons at K in our experiments. This may be justified on the grounds that the excited dark excitons distribute over the K space with a 2D degeneracy of motion whereas those at K≈0 have a much smaller phase space available.
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