2011
DOI: 10.1143/jjap.50.094001
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Effect of Heating and Cooling of Photogenerated Electron–Hole Plasma in Optically Pumped Graphene on Population Inversion

Abstract: We study the characteristics of photogenerated electron-hole plasma in optically pumped graphene layers at elevated (room) temperatures when the interband and intraband processes of emission and absorption of optical phonons play a crucial role. The electron-hole plasma heating and cooling as well as the effect of nonequilibrium optical phonons are taken into account. The dependences of the quasi-Fermi energy and effective temperature of optically pumped graphene layers on the intensity of pumping radiation ar… Show more

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Cited by 38 publications
(34 citation statements)
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“…The rate of the optical phonon-assisted interband transitions (recombination rate) R inter 0 and the rate of the intraband energy relaxation associated with optical phonons R intra 0 can be calculated using the following simplified formulas [9,16] (see, also Ref. [20]:…”
Section: Equations Of the Modelmentioning
confidence: 99%
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“…The rate of the optical phonon-assisted interband transitions (recombination rate) R inter 0 and the rate of the intraband energy relaxation associated with optical phonons R intra 0 can be calculated using the following simplified formulas [9,16] (see, also Ref. [20]:…”
Section: Equations Of the Modelmentioning
confidence: 99%
“…The η 0 − µ and η 0 − T dependences are associated with the linearity of the density of states in GLs as a function of energy. To a good approximation these dependences can be described [16] by function (10) is given by…”
Section: Equations Of the Modelmentioning
confidence: 99%
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“…In the case of strong pumping, the effective temperature of the electron-hole plasma can be much higher than the lattice temperature [23]. As a result, the electron-hole plasma can become nondegenerate, so that µ e = µ < 0 while µ h = −µ > 0.…”
mentioning
confidence: 99%
“…In the case of pumping of intrinsic GLs, µ e = −µ h = µ = 0. In the latter case, T can differ from the lattice temperature T l being both higher than T l or lower [23].Considering in the following the case Σ d (x, y) = 0 and assuming that the fluctuations are not too strong (e|ϕ| < k B T ), Eq. (1) can be linearized: ∆ϕ = ϕ r s ln 1 + e µ/k B T − 4π e ae Σ i · δ(z),…”
mentioning
confidence: 99%