2014
DOI: 10.1016/j.physe.2013.08.008
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High field transport properties of a bilayer graphene

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Cited by 24 publications
(46 citation statements)
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“…6 (Figure 7 inset). We emphasize that this n −1.5 e dependence in bilayer graphene, due to its parabolic dispersion relation at low energies [11], is very different from the n −0.5 e dependence for monolayer graphene which has been theoretically predicted [14] and already experimentally observed [6]. As a comparison, the carrier density dependence of α in monolayer graphene is plotted in the same figure. Below the crossing point corresponding to a carrier density of approximately 1.86 × 10 12 cm −2 and at carrier temperatures between 1.4 K and 100 K, hot carriers in bilayer graphene will be able to lose energy faster than those in monolayer and vice versa.…”
Section: Energy Loss Rate and Electron-phonon Relaxation Time In Bilamentioning
confidence: 84%
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“…6 (Figure 7 inset). We emphasize that this n −1.5 e dependence in bilayer graphene, due to its parabolic dispersion relation at low energies [11], is very different from the n −0.5 e dependence for monolayer graphene which has been theoretically predicted [14] and already experimentally observed [6]. As a comparison, the carrier density dependence of α in monolayer graphene is plotted in the same figure. Below the crossing point corresponding to a carrier density of approximately 1.86 × 10 12 cm −2 and at carrier temperatures between 1.4 K and 100 K, hot carriers in bilayer graphene will be able to lose energy faster than those in monolayer and vice versa.…”
Section: Energy Loss Rate and Electron-phonon Relaxation Time In Bilamentioning
confidence: 84%
“…So far, no theoretical extension of the "supercollisions" to bilayer graphene has been reported and our results show no evidence of the transition to a T 3 dependence as observed in monolayer graphene. Another possible cooling mechanism to retain the energy loss rate increasing as T 4 in a substrate supported bilayer graphene sample could be the interaction between hot electrons and surface polar phonons (SPPs) [11][12][13], combined with hot phonon effects which occur when the hot phonon decay rate is not as fast as the phonon emission rate. However, theoretical calculations based on a SiC substrate suggest the contribution from SPPs can only be clearly observed for electron temperatures higher than 100 K [13], due to the relatively low dielectric constant and high surface polar phonon energies of SiC, compared with substrates such as HfO 2 .…”
Section: Energy Loss Rate and Electron-phonon Relaxation Time In Bilamentioning
confidence: 99%
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“…We suggest, in order to see the VP coupling contribution to the hot electron cooling power, measurements need to be made over the large range of n s covering the cross over region.. It is to be noted that the BG regime studies in conventional in 2DEG [22],TMDs [23] and bilayer graphene (unscreened DP coupling) [18], with the parabolic dispersion of electron energy, show n s -3/2 dependence. But the n s -1/2 dependence of VP coupling in BLG, with the same parabolic dispersion for electrons, is due to the explicit dependence of its matrix element on electron energy (see Eq.…”
Section: Electron Concentration Dependence Of F(tn S )mentioning
confidence: 99%
“…Electron heating by photons finds potential applications in bolometry and calorimetry. Hot electron cooling is extensively studied, theoretically and experimentally, in bulk semiconductors , conventional two‐dimensional electron gas (2DEG) of low‐dimensional semiconductor heterostructures , graphene and in monolayer MoS 2 . Also, there exists a study of cooling of hot carriers on the surface of topological insulator Bi 2 Se 3 .…”
Section: Introductionmentioning
confidence: 99%