Model for tunneling transport

BS Boris V. Senkovskiy
AN Alexey V. Nenashev
SA Seyed K. Alavi
YF Yannic Falke
MH Martin Hell
PB Pantelis Bampoulis
DR Dmitry V. Rybkovskiy
DU Dmitry Yu. Usachov
AF Alexander V. Fedorov
AC Alexander I. Chernov
FG Florian Gebhard
KM Klaus Meerholz
DH Dirk Hertel
MA Masashi Arita
TO Taichi Okuda
KM Koji Miyamoto
KS Kenya Shimada
FF Felix R. Fischer
TM Thomas Michely
SB Sergei D. Baranovskii
KL Klas Lindfors
TS Thomas Szkopek
AG Alexander Grüneis
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To calculate the tunneling probability P(E) through a trapezoidal barrier, we used the following expression36:

This equation is valid only for the case when the tunneling occurs between the edges of the barrier, i.e., the tunneling length is equal to the geometrical length of the barrier d. This is the case if Φb − E > 0 and Φb − E − eV > 0. Depending on the sign of Vd, the barrier can either decrease or increase by the amount ∣eV∣ along the tunneling path. Since the situation is symmetrical with respect to the direction of the applied voltage, we will consider in the following the case of V ≥ 0. In the case Φb − E > 0 and Φb − E − eV < 0, the carrier has to tunnel under the triangular barrier and the transmission coefficient is described by the Fowler–Nordheim theory56. In Eq. (4), d indicates the barrier length, m is the charge carrier effective mass inside the barrier, φ(x,V) = Φb + (x/d) ⋅ (−eV) is the barrier height at coordinate x, V is the applied voltage, and Φb denotes the barrier height at x = 0. In the case of a triangular barrier, the integration over x in the exponent of Eq. (3) should be performed from zero till the value xc determined by the condition φ(xc, V) − E = 0. The expression for P(E) then reads,

in agreement with the exponent in Eq. (4) of ref. 32. The integral over E in Eq. (1) is to be calculated in the range E ≥ 0, E ≥ −eV. This integration was performed numerically. The position of the Fermi level EF in Eq. (1) is determined by the carrier concentration in the channel, which in turn is controlled by Vg. The carrier concentration n in the channel of the heterojunction FET is given by n = n0 + VgCg/e. Approximating the density of states by a constant ρ, we have nn0=ρ(EFEF0) where n − n0 is the change in the carrier concentration induced by the gate voltage and EFEF0 is the Fermi level shift induced by the gate voltage. Rearranging the above equation yields EF=EF0+(nn0)/ρ. Substituting n = n0 + VgCg, we get EF=EF0+CgVg/(eρ). We set α = Cg/(eρ) and take into account that the source–drain voltage also affects the gate potential at a given position along the channel. For instance, a barrier close to the source contact experiences a different potential than a barrier close to the drain contact. Thus, the gate voltage dependence is modeled in our fit as EF(Vg,Vd)=EF0(T)+α(T)(Vg+βVd). This relation assumes that the EF is a linear function of carrier concentration, which is always true for a sufficiently small range of EF, e.g., for a small gate voltage range. In all our fits of IdVd curves, the variation of EF0 was within 100 meV relative to band edge, i.e., small as compared to Φb. The product αβ accounts for the asymmetry between the source and drain contacts, with the former taken as the reference potential against which both gate potential Vg and drain potential Vd are applied.

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