2014
DOI: 10.1103/physrevb.90.125424
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Phonon-assisted radiative recombination of excitons confined in strongly anisotropic nanostructures

Abstract: The influence of acoustic phonons on the emission spectra of quantum dashes (QDashes), that are quasi-zerodimensional epitaxial nanostructures with significant shape anisotropy, is investigated both experimentally and theoretically. Photoluminescence (PL) spectra of single InAs/InGaAlAs/InP (001) QDashes exhibit sidebands of the main emission peak, clearly indicating the contribution of phonon-assisted emission to the exciton luminescence, which dominates the PL line shape at higher temperatures (between 50 an… Show more

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Cited by 22 publications
(19 citation statements)
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“…While the energy shift is mainly driven by the change in the energy gap of the CQD material, the broadening of the emission line is related to the increase of the phonon reservoir and therefore enhanced the exciton-acoustic phonon coupling in the system. 33 The full picture of the temperature evolution of the X* emission line in the range of 5-80 K is presented in Fig. 3.…”
Section: 30mentioning
confidence: 99%
“…While the energy shift is mainly driven by the change in the energy gap of the CQD material, the broadening of the emission line is related to the increase of the phonon reservoir and therefore enhanced the exciton-acoustic phonon coupling in the system. 33 The full picture of the temperature evolution of the X* emission line in the range of 5-80 K is presented in Fig. 3.…”
Section: 30mentioning
confidence: 99%
“…A temperature series were recorded and analyzed. Emission from single QDs is observed for temperatures in the range of 100 K, comparable to 80 K obtained in this spectral range for InAs/GaAs QDs on a metamorphic buffer layer [ 113 ], InAs/InGaAlAs/InP quantum dashes [ 114 ] and low-density InAs/InP QDs [ 88 ], as well as 100 K for InAs/InP quantum-LED [ 50 ]. For all the emission lines, typical thermally-induced behavior of the emission spectra is observed: a systematic redshift of the emission energy, linewidth broadening, and monotonic decrease of emission intensity (exemplary spectra presented in Figure 7 a).…”
Section: Resultsmentioning
confidence: 68%
“…However, with increasing temperature, the FWHM increases to the range of 55–68 meV at . This behavior is related to the carrier-phonon-induced broadening of an optical transition [ 55 ] without a strong signature of the carrier redistribution process, which typically results in a complicated functional form of the FWHM( T ) [ 53 , 54 , 56 ]. The indication of the carrier re-excitation process influencing the FWHM is possibly observed for the PL band A.…”
Section: Resultsmentioning
confidence: 99%