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Novel Scattering Mechanisms for Nanotube-Silicon Devices
Slava V. Rotkin
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Surface Polariton in SiO2
Specifics of surface polaritons: electric field is not normal to the surface (at 45o) electric field decays exponentially from the surface (not a uniform solution of Maxwell equations) existence of a surface mode essentially depends on existence of the anomalous dispersion region e<0 Surface phonons in polar dielectrics: due to the dielectric function difference between the substrate and the air, a surface e.m.w. could exist dielectric function of the polar insulator has a singularity at the frequency of LO phonon surface wave with a strong decay of the electric field in the air appears and interacts with the NT charges
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Maxwell equations in free space
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Maxwell equations in free space are solved by anzatz
E ~ eikz algebraic form of Maxwell equations in free space E q H surface requires that: all field components (but one) can be found from BC:
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"a" for air E q H in non-retarded limit the frequency of SPP mode is found from "b" for bulk
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E H "a" for air J E q H in non-retarded limit the frequency of SPP mode is found from "b" for bulk
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last component of the field can be found only with QM/QED
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Charge Scattering: Short Introduction
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Boltzmann Transport Equation (0)
Equilibrium distribution function is Fermi-Dirac function: E e.d.f. is symmetric and thus j = 0 k asymmetric non-e.d.f. provides: j > 0 (both in ballistic and diffusive model) Quantum-mechanical calculation of the conductivity may be reduced to the Drude formula electron velocity enters the formula
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Conductivity: van Hove singularities
Scattering rate is proportional to the velocity which diverges at the subband edge. Thus, the Drude conductivity has peculiarities at vHs. Prof. T. Ando
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Surface Phonon Polariton
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Introduction q j Vd q~area~nm2 channel heating due to Joule losses and low thermal coupling to leads It exists, however, a relaxation mechanism which transfers the energy directly to the substrate without intermediate exchange with the SWNT lattice (phonons) which is an inelastic remote optical phonon scattering Pioneering work by K. Hess and P. Vogl – back to 1972 – RIP-S in Si. The mechanism appeared to be ineffective for Si MOS-FETs and was almost forgotten for decades...
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Remote Polariton Scattering
Interaction potential (e-dipole) where the (dipole) polarization is calculated following Mahan et al. here q is the SPP wavenumber; x is normal to the surface F is related to Froehlich constant: and wSO is the SPP frequency
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Surface Polariton in SiO2
Surface phonons in polar dielectrics: due to the dielectric function difference between the substrate and the air, a surface e.m.w. could exist dielectric function of the polar insulator has a singularity at the frequency of LO phonon surface wave with a strong decay of the electric field in the air appears and interacts with the NT charges for vF~108 cm/s and wSO~150meV : e ~ 105 V/cm
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Saturation Regime and Heat Dissipation Problem
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Introduction Scattering in 1D systems is weak due to restricted phase space available for the electron: k -> -k. However, scattering at high (drift) electric field is inevitable due to emission of an optical phonon. Which provides a fast relaxation mechanism for the hot electrons (and holes). Inelastic scattering rates have been calculated for SWNTs earlier: However, recent optics experiments showed faster relaxation rates for the hot electron, which suggests a new scattering mechanism.
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Introduction Inelastic optical phonon relaxation scattering is likely a factor determining the saturation current in SWNTs : The hot electron energy is transferred to the SWNT phonon subsystem. The energy dissipation depends on the environment (thermal coupling).
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Remote Polariton Scattering
T=0K - therefore, only SO-phonon emission is included Dm=0 - intra-subband transitions Dm=1 - inter-subband transitions (neglecting higher m's) q~1/l (forward) and q~2k (backward) scattering
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Remote Polariton Scattering
RPS rate varies for intra-subband and inter-subband scattering RPS has maximum at the van Hove singularities (for semiconductor-SWNT)
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Conductivity: van Hove singularities
Scattering rate is proportional to the velocity which diverges at the subband edge. Thus, the Drude conductivity has peculiarities at vHs. reminder Prof. T. Ando
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Remote Polariton Scattering
RPS rate varies for intra-subband and inter-subband scattering RPS has maximum at the van Hove singularities (for semiconductor-SWNT) inter-subband transitions are negligible due to non-zero angular momentum transfer
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Remote Polariton Scattering
0.02 0.04 0.06 0.08 0.1 0.65 0.75 0.8 0.85 E(k), eV k, 1/A Scattering rate = lifetime ~ 30 meV No sharp transition could happen Selfconsistent calculation of the lifetime of the... RP-polaron
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Surface Polariton Scattering (2)
To correct many-body picture the phonon renormalization of the electron spectrum was computed. As a result of Quantum Mechanical calculation we obtain new scattering rate : scattering is averaged near the vHs but it is still a fast process. q~1/l forward scattering q~2k : backward scattering for vF~108 cm/s and wSO~140meV : l~40 nm 2ki ~ 2p/a ~ 1/nm
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Remote SPP Scattering Rate
for the SiO2 (quartz) substrate the RPS is likely prevailing over inelastic scattering by NT (own) optical phonons for the small distance to the polar substrate < l ~ 40 nm; the effect is even stronger for high-k dielectrics due to increase of the Froehlich constant : x20 and more; the effect is independent of the radius of the NT, thus for narrow NTs it will dominate over the other 1/R mechanisms
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Remote SPP Scattering Rate
scattering rate increases with the electric field strength because of stronger warming of the electron distribution function
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Remote SPP Scattering IVCs with and without taking into account SPP mechanism The saturation regime is clearly seen at larger bias (larger field) for SPP scattering Inset: mobility vs. field
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Remote SPP Scattering overheating of the channel : neglecting the thermal sink in the leads where two scattering mechanisms : SPP phonons take the heat directly into bulk substrate; NT phonons warm the lattice but are inefficient Joule losses - IsF are for the total energy loss; while NT phonons take only a small fraction of that
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Remote SPP Scattering ratio of "real"-to-expected losses for two tubes (R~0.5 and 1.0 nm) at two to= 77 and 300K inset: data collapse for (linear) dependence on the electron concentration (0.1 and 0.2 e/nm) different temperature dependence for two scattering mechanisms
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