1985
DOI: 10.1103/physrevb.32.2407
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Electron-hole plasma expansion in the direct-band-gap semiconductors CdS and CdSe

Abstract: The properties of the electron-hole plasma in direct-band-gap semiconductors are investigated by exciteand probe-beam techniques with use of CdS and CdSe as examples. By spatially resolved transmission and reflection spectroscopy and by using samples of different thicknesses, the diffusion length and other data of the plasma are determined. A "slow drift" is found, i.e. , the drift velocity is smaller than the Fermi velocities of electrons and holes. The drift distances are of the order of 10 pm with some sign… Show more

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Cited by 100 publications
(16 citation statements)
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“…While the absolute energy of the 1s exciton stays nearly unchanged in bulk samples over a wide range of carrier densities its oscillator strength disappears due to band gap shrinkage. This was proved in many experiments [1][2][3] and explained qualitatively by strong compensation of gap shrinkage and weakening of the Coulomb interaction due to screening inspecting the effective Wannier equation of an exciton embedded in a thermal plasma [4][5][6][7]. The situation is rather different in quantum wells, where a blueshift of the exciton with increasing density was observed [8,9].…”
mentioning
confidence: 84%
“…While the absolute energy of the 1s exciton stays nearly unchanged in bulk samples over a wide range of carrier densities its oscillator strength disappears due to band gap shrinkage. This was proved in many experiments [1][2][3] and explained qualitatively by strong compensation of gap shrinkage and weakening of the Coulomb interaction due to screening inspecting the effective Wannier equation of an exciton embedded in a thermal plasma [4][5][6][7]. The situation is rather different in quantum wells, where a blueshift of the exciton with increasing density was observed [8,9].…”
mentioning
confidence: 84%
“…With increasing stripe length or increasing carrier concentration, g(hw) deviates from I,,(hw) along with q and the gain becomes negative on the high-energy side Next, we considered the gain spectrum (curve 5 in Fig. l b ) at higher excitation (1.1 MW/cm2) but for the same stripe length as above and fitted it with the electron-hole plasma model described in [3]. The optical amplification g(ho) in a direct-band gap semiconductor, where all excitonic correlations are screened in an EHP of sufficiently high carrier concentration, can be described simply by the square-root dependence of the combined density of states above the reduced band gap Ei(np), modulated by the Fermi functions of electrons and holes, j , and f,, as given in [3],…”
Section: 34mentioning
confidence: 99%
“…A gain spectrum calculated according to (3) and modified with the k concervation model and energy-depending damping as described in [3] is shown in Fig. 3a together with the experimental one where the exciton-exciton scattering processes are strongly saturated.…”
Section: 34mentioning
confidence: 99%
“…[8,13]) have been reported. With respect to the plasma expansion velocity, u p , one can distinguish two kinds of behaviour:`slow' expansion with u p µ 10 6 cm s ¡1 [6,7,12,17,21,22] or`fast' , with u p > 10 6 cm s ¡1 [8± 10, 13± 16, 23]. In the latter case a mechanism of stimulated emission recombination, optical transport and reabsorption has been proposed to explain the observed ultrafast carrier diå usion.…”
Section: Introductionmentioning
confidence: 98%
“…Expansion lengths as low as ¹20 mm (e.g. [6,12]) and as high as ¹100 mm (e.g. [8,13]) have been reported.…”
Section: Introductionmentioning
confidence: 98%