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3
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85037875371
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We cool the liquid nitrogen to 69 K by pumping its vapor down to 250 torr, then repressurize the cryostat with helium gas. The liquid nitrogen will then evaporate, rather than boil, and remain below 71 K for the duration of the experiment.
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We cool the liquid nitrogen to 69 K by pumping its vapor down to 250 torr, then repressurize the cryostat with helium gas. The liquid nitrogen will then evaporate, rather than boil, and remain below 71 K for the duration of the experiment.
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4
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85037888805
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The theoretical energy distributions of hot carriers undergoing phonon relaxation and Auger decay is not a trivial problem and will be considered in a future paper.
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The theoretical energy distributions of hot carriers undergoing phonon relaxation and Auger decay is not a trivial problem and will be considered in a future paper.
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10
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0000682033
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T. Goto, M.Y. Shen, S. Koyama, and T. Yokouchi, Phys. Rev. B 55, 7609 (1997).
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(1997)
Phys. Rev. B
, vol.55
, pp. 7609
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Goto, T.1
Shen, M.Y.2
Koyama, S.3
Yokouchi, T.4
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11
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0029726494
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N. Naka, S. Kono, M. Hasuo, and N. Nagasawa, Prog. Cryst. Growth Charact. Mater. 33, 89 (1996).
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(1996)
Prog. Cryst. Growth Charact. Mater.
, vol.33
, pp. 89
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Naka, N.1
Kono, S.2
Hasuo, M.3
Nagasawa, N.4
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12
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0001726747
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M.Y. Shen, T. Yokouchi, S. Koyama, and T. Goto, Phys. Rev. B 56, 13 066 (1997).
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(1997)
Phys. Rev. B
, vol.56
, pp. 13 066
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Shen, M.Y.1
Yokouchi, T.2
Koyama, S.3
Goto, T.4
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18
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85037898995
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Trauernicht et al. report an Auger constant (Formula presented) for paraexcitons confined to a Gaussian cloud by a strain well. This value must be multiplied by the appropriate volume—(Formula presented) using Eq. (10) later in this paper and the description of the strain well by Trauernicht et al.— and divided by 2 due to a difference in definitions.
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Trauernicht et al. report an Auger constant (Formula presented) for paraexcitons confined to a Gaussian cloud by a strain well. This value must be multiplied by the appropriate volume—(Formula presented) using Eq. (10) later in this paper and the description of the strain well by Trauernicht et al.— and divided by 2 due to a difference in definitions.
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20
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85037876010
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The density approaches steady state as (Formula presented) so to reach this steady-state value within a pulse of length T requires (Formula presented)
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The density approaches steady state as (Formula presented) so to reach this steady-state value within a pulse of length T requires (Formula presented)
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21
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85037893168
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To the extent that the Auger cross section for ortho-para collisions may be larger than that for ortho-ortho collisions, Auger recombination would drive the paraexciton number lower, keeping the magnitude of the effect of paraexcitons the same.
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To the extent that the Auger cross section for ortho-para collisions may be larger than that for ortho-ortho collisions, Auger recombination would drive the paraexciton number lower, keeping the magnitude of the effect of paraexcitons the same.
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24
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84952278885
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B. Karlsson, C.G. Ribbing, A. Roos, E. Valkonen, and T. Karlsson, Phys. Scr. 25, 826 (1982).
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(1982)
Phys. Scr.
, vol.25
, pp. 826
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Karlsson, B.1
Ribbing, C.G.2
Roos, A.3
Valkonen, E.4
Karlsson, T.5
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25
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85037918891
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The actual situation in (Formula presented) is somewhat more complicated. The optical transitions in question are phonon assisted, so we must consider the energies of the optical phonons created or destroyed. We balance the redshifted absorption—seen in Fig. 5(b)—with the redshifted luminescence. Letting (Formula presented) denote the occupation number of the (Formula presented) optical phonon, the rate for this redshifted absorption is (Formula presented)and the luminescence rate is (Formula presented)The energies of the photon and exciton are not equal; the total energy of the exciton is lower than that of the photon by one (Formula presented) phonon energy. Since in equilibrium all the (Formula presented)’s are Planck functions, we have the following identity: (Formula presented)So the final result is the same as Eq. (6) in the text.
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The actual situation in (Formula presented) is somewhat more complicated. The optical transitions in question are phonon assisted, so we must consider the energies of the optical phonons created or destroyed. We balance the redshifted absorption—seen in Fig. 5(b)—with the redshifted luminescence. Letting (Formula presented) denote the occupation number of the (Formula presented) optical phonon, the rate for this redshifted absorption is (Formula presented)and the luminescence rate is (Formula presented)The energies of the photon and exciton are not equal; the total energy of the exciton is lower than that of the photon by one (Formula presented) phonon energy. Since in equilibrium all the (Formula presented)’s are Planck functions, we have the following identity: (Formula presented)So the final result is the same as Eq. (6) in the text.
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28
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85037910783
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Reference 12 reported (Formula presented) and Ref. 11 reports a cross section which implies that (Formula presented) in order of magnitude.
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Reference 12 reported (Formula presented) and Ref. 11 reports a cross section which implies that (Formula presented) in order of magnitude.
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