2012
DOI: 10.1016/j.jlumin.2012.06.004
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On the radiative lifetime of free-moving two-dimensional excitons

Abstract: A simple microscopic mechanism explaining the linear dependence of the radiative lifetime of freemoving two-dimensional excitons on their effective temperature is suggested. It is shown that there exists a characteristic effective temperature (of about few Kelvin) defined by the exciton-acoustic phonon interaction at which the radiative lifetime is minimal. Below this temperature the lifetime starts to increase with decreasing temperature. The correspondence with previous theoretical and experimental results i… Show more

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Cited by 4 publications
(3 citation statements)
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References 11 publications
(29 reference statements)
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“…For example, T* % 3.6 K, in GaAs quantum well. 30 Therefore, one typically observes the well-known linear dependence of s R (T) / T. However, the S-series emission lines in hBN are attributed to the recombination of Frenkel excitons. [26][27][28][29] The Bohr radius of a Frenkel exciton is expected to be a few lattice constants.…”
mentioning
confidence: 99%
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“…For example, T* % 3.6 K, in GaAs quantum well. 30 Therefore, one typically observes the well-known linear dependence of s R (T) / T. However, the S-series emission lines in hBN are attributed to the recombination of Frenkel excitons. [26][27][28][29] The Bohr radius of a Frenkel exciton is expected to be a few lattice constants.…”
mentioning
confidence: 99%
“…26 The four main emission peaks located at 5.771 (S4), 5.799 (S3), 5.869 (S2), and 5.897 (S1) eV were attributed to the four Frenkel class free exciton levels originated from the doubly degenerated dipole-forbidden (dark) and dipole-allowed (bright) exciton states, in which the dark exciton state becomes allowed either due to the spontaneous symmetry breaking caused by energy transfer from bright exciton band as a result of the zero-point vibration of the lattice 27,28 or a strong spin-orbital interaction due to 2D layered structure. 29 For 2D excitons, Paraskevov 30 suggests that because of the momentum conservation light emission resulting from direct exciton recombination in directions other than that of in-plane is induced by the exciton-acoustic phonon interaction. Based on this concept, the dependence of the exciton radiative lifetime s R on the effective temperature of the exciton system was derived.…”
mentioning
confidence: 99%
“…Time resolved photoluminescence (PL) measurements on the other hand would rely on the exciton-trion energy eigenstates to relax down to the light cone before they can recombine radiatively with high efficiency [32]. This relaxation process is generally bottlenecked by phonon scattering times which are usually much slower (around a few picoseconds) than the radiative lifetimes inside the light cone [33][34][35][36]. In addition, as discussed in this paper, PL collected from both peaks in the emission/absorption spectra of doped 2D materials are from states that are superpositions of exciton and trion states and contribute to PL from both inside and outside the light cone.…”
Section: Discussionmentioning
confidence: 99%