An improved velocity-space carrier transport model is presented, based on a direct solution of the Boltzmann Transport Equation. This model attempts to achieve the computational efficiency required for device simulation, while still solving for the distribution function itself. This preserves critical fine structure effects due a non-ideal band structure and forward scattering mechanisms. The model includes a numerically efficient representation of three dimensional k-space formulated around a 1D velocity-space variable, and the particle energy. The number of empirical parameters in the model is reduced to a single constant per scattering mechanism. A physically intuitive solution algorithm is developed which repeatedly shifts and shapes the estimate of the distribution until convergence. Results are presented for the steady-state homogeneous case in silicon and GaAs, which are of comparable computational cost as drift-diffusion simulations.
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Imperial Coll London, Dept Phys, London SW7 2AZ, England
ESAC, European Space Agcy, E-28692 Madrid, SpainUniv Calabria, Dipartimento Fis, I-87036 Cosenza, Italy
Perrone, D.
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Valentini, F.
Sorriso-Valvo, L.
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Nanotec CNR, I-87036 Arcavacata Di Rende, ItalyUniv Calabria, Dipartimento Fis, I-87036 Cosenza, Italy
Sorriso-Valvo, L.
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Greco, A.
Matthaeus, W. H.
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Univ Delaware, Bartol Res Inst, Newark, DC 19716 USA
Univ Delaware, Dept Phys & Astron, Newark, DC 19716 USAUniv Calabria, Dipartimento Fis, I-87036 Cosenza, Italy
Matthaeus, W. H.
Veltri, P.
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Univ Calabria, Dipartimento Fis, I-87036 Cosenza, ItalyUniv Calabria, Dipartimento Fis, I-87036 Cosenza, Italy