1995
DOI: 10.1103/physrevb.52.4728
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Hot-phonon effects in femtosecond luminescence spectra of electron-hole plasmas in CdS

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Cited by 71 publications
(104 citation statements)
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“…Here T is the common electron/hole temperature, m is the electron momentum relaxation time due to phonon-or carrier-induced scattering processes, and E ៝ is an electric field that arises from charge density imbalance e͑N h − N e ͒ and from J. The space-charge and current sources produce scalar ͑⌽͒ and vector potentials ͑A͒ which can be calculated using Green function techniques 17 for the appropriate boundary conditions; the electric field is then given by E =−١⌽ − ‫ץ‬A / ‫ץ‬t. For our experiments where the illuminated spot sizes are W ϳ 100 m full width at half maximum ͑FWHM͒ in diameter and the relative dielectric constants 15 are ⑀ = 9.3 ͑8.7͒ for CdSe ͑CdS͒, respectively; the time scales ͑ϳ100 fs͒ for current evolution areϽW ͱ ⑀ / c therefore the electrostatic approximation is inappropriate; and the electric field arises mainly from current sources through A if one uses the Coulomb gauge.…”
Section: B Current Evolutionmentioning
confidence: 99%
“…Here T is the common electron/hole temperature, m is the electron momentum relaxation time due to phonon-or carrier-induced scattering processes, and E ៝ is an electric field that arises from charge density imbalance e͑N h − N e ͒ and from J. The space-charge and current sources produce scalar ͑⌽͒ and vector potentials ͑A͒ which can be calculated using Green function techniques 17 for the appropriate boundary conditions; the electric field is then given by E =−١⌽ − ‫ץ‬A / ‫ץ‬t. For our experiments where the illuminated spot sizes are W ϳ 100 m full width at half maximum ͑FWHM͒ in diameter and the relative dielectric constants 15 are ⑀ = 9.3 ͑8.7͒ for CdSe ͑CdS͒, respectively; the time scales ͑ϳ100 fs͒ for current evolution areϽW ͱ ⑀ / c therefore the electrostatic approximation is inappropriate; and the electric field arises mainly from current sources through A if one uses the Coulomb gauge.…”
Section: B Current Evolutionmentioning
confidence: 99%
“…3. Estimations show that the threshhold for saturation of the EЈ(2 2 ) phonon mode is at carrier densities of ϳ5ϫ10 16 cm Ϫ3 , which is in the range of the excitation densities used in the present experiments.…”
Section: A Carrier Cooling Dynamicsmentioning
confidence: 95%
“…The free-exciton formation rate is determined by the exciton binding energy (E B X ϭ19 meV in GaSe͒ and the thermal energy of the carriers 3 2 k B T C . When the thermal energy of the carriers becomes smaller than the exciton binding energy, the attractive Coulomb interaction between electrons and holes is strong enough to bind them into excitons and prevent the thermal dissociation of the exciton.…”
Section: B Exciton Formation Dynamicsmentioning
confidence: 99%
“…Furthermore, it is well-known that the highly excited carriers rapidly relax energy toward the LO-phonon system, creating large nonequilibrium phonon populations. A build-up of the nonequilibrium phonons creates a bottleneck in the relaxation channel carrier-phonon LO that may influence considerably the carriers' cooling rate [2,[5][6][7][8][9][10][11]. The diminished effectiveness of the process of relaxation in the carrier system, with an accompanied slowing down in the rate of energy loss has been mainly ascribed to this so-called hotphonon effect [12].…”
Section: Introductionmentioning
confidence: 98%