| Type | Saturated velocity \(v_{sat}\) | Critical field \(\mathcal{E}_c\) |
|---|---|---|
| Electrons | \(10^5\) m/s | 1 V/\(\mu m\) |
| Holes | \(8 \times 10^4\) m/s | 3 V/\(\mu m\) |
Analog Integrated Circuits Design using the Inversion Coefficient
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5 The Short-channel MOSFET Model
5.1 Introduction
In the previous Chapter, the channel was assumed to be long, allowing for a one-dimensional analysis using the gradual channel approximation. This Chapter is devoted to the effects appearing when reducing the length of the transistor to dimensions that get close to the depletion width. In such a situation, the one-dimensional approach is no more valid and a two-dimensional analysis is required. Furthermore, the terminal voltages are not scaled down proportionally to the device length reduction, the longitudinal electric field increases beyond a certain critical field above which the velocity starts to saturate. This velocity saturation (VS) effect is presented in Section 5.3 using different velocity-field relations. Another short-channel effect that strongly limits the performance (particularly the voltage gain) of analog circuits is the channel length modulation (CLM) described in Section 5.4. When the device length gets small the surface potential in the channel region is no more defined uniquely by the vertical field, but becomes influenced by the drain (or source) voltage. This effect is called the drain induced barrier lowering (DIBL) and is presented in Section 5.5. Short-channel effects such as VS and CLM not only impact the current, but also the thermal noise. A short-channel thermal noise model including the effects of VS is presented in Section 5.6. Finally , the EKV model in saturation and including VS is called the simplified EKV model or sEKV. It is presented in Section 5.7 where the model is compared to measurements made on transistors from various technologies. It is shown that the sEKV, although initially developed for bulk technologies, the sEKV model also works very well for advanced FDSOI and FinFET technologies.
5.2 Mobility reduction mechanisms
The previous Chapter presented the ideal MOS transistor having a wide and long channel and a constant mobility in the channel region. Of course in a more advanced model, the mobility can no more be considered as constant and various scattering mechanisms need to be accounted for. As illustrated in Figure 1, there are mainly two different mobility reduction mechanisms: the first is due to the vertical electric field \(\mathcal{E}_z\), while the second is due to the longitudinal electric field \(\mathcal{E}_x\) (along the channel direction).
The mobility reduction due to the vertical field \(\mathcal{E}_z\) is caused by several scattering mechanisms, namely:
- Coulomb scattering: related to the interaction of mobile carrier with ionized impurity atoms (occurs at low field).
- Phonon scattering: related to the interaction with the lattice vibrations (occurs at medium field).
- Surface roughness: interaction between the mobile carrier and the Si-SiO2 interface (occurs at high field).
The mobility reduction due to the longitudinal field \(\mathcal{E}_x\) is caused by the saturation of the carrier drift velocity. While the mobility due to the vertical field is not restricted to short-channel devices but also affects long-channel devices in strong inversion where the vertical field is maximum. On the other hand, as the channel length gets smaller, the longitudinal field increases and the mobility degrades. The mobility reduction due to the longitudinal field \(\mathcal{E}_x\) is therefore an important (if not the most important) short-channel effect.
Among all effects related to the reduction of the device geometry we can distinguish effects that are related to the reduction of the channel length leading to short-channel effects (SCE) which include:
- Velocity saturation (VS),
- Channel length modulation (CLM),
- Charge sharing,
- Drain induced barrier lowering (DIBL) and
- Reverse short-channel effect.
The reduction of the transistor width also leads to narrow-channel effects, whereas the reduction of the oxide thickness gives rise to the gate leakage current.
Among all the SCE listed above, we will consider the velocity saturation (VS), which is probably the most important SCE, the channel length modulation (CLM) and the drain induced barrier lowering (DIBL). They are discussed in the following sections.
5.3 Velocity saturation
5.3.1 Velocity versus electric field models
An important effect that appears when the longitudinal electric field \(\mathcal{E}_x\) within the device starts to become large is the saturation of the drift velocity. The drift velocity \(v_{drift}\) of electrons and holes in bulk silicon is plotted versus \(\mathcal{E}_x\) in Figure 2. At low longitudinal electric field, the velocity is proportional to the electric field with a proportionality factor equal to the mobility \(\mu_z\) at low longitudinal field. When \(\mathcal{E}_x\) becomes larger than the critical field \(\mathcal{E}_c\), the velocity starts to saturate to a maximum value \(v_{sat}\). The shape of the velocity-field relation in silicon is slightly different for electrons and holes. Typical values for \(\mathcal{E}_c\) and \(v_{sat}\) at room temperature for electrons and holes are given in Table 1. The critical field \(\mathcal{E}_c\) is related to the saturated drift velocity and the mobility at low longitudinal field by \[\begin{equation} \mathcal{E}_c \triangleq \frac{v_{sat}}{\mu_z}. \end{equation}\] Note that the mobility at low longitudinal field \(\mu_z\) actually depends on the vertical field \(\mathcal{E}_z\). The larger the vertical field, the smaller \(\mu_z\) and the larger the critical field, since \(v_{sat}\) is constant for a given type of silicon and a given doping.
As shown in Figure 3, different velocity-field models can be considered to analyze the effect of velocity saturation on the drain current and on the transconductances.
The simplest model (Model 1) to describe the velocity-field dependence is to consider the velocity proportional to the longitudinal field with a constant slope up to the critical field, above which it stays constant and equal to the saturated velocity. This model is described by the piecewise linear model defined by \[\begin{equation}\label{eqn:vdrift_model1} \nu(e) \triangleq \frac{v_{drift}}{v_{sat}} = \begin{cases} e & \textsf{for $e \leq 1$}\\ 1 & \textsf{for $e > 1$}, \end{cases} \end{equation}\] where \(e\) is the longitudinal electric field \(\mathcal{E}_x\) normalized to the critical field \(\mathcal{E}_c\) \[\begin{equation} e \triangleq \frac{|\mathcal{E}_x|}{\mathcal{E}_c}. \end{equation}\] The corresponding effective mobility \(\mu_{eff}\) is then simply given by \[\begin{equation} \mu_{eff}(\mathcal{E}_x) \triangleq \frac{v_{drift}}{|\mathcal{E}_x|} = \begin{cases} \mu_z & \textsf{for $\mathcal{E}_x < \mathcal{E}_c$}\\ v_{sat}/|\mathcal{E}_x| & \textsf{for $\mathcal{E}_x \geq \mathcal{E}_c$}, \end{cases} \end{equation}\] or in a normalized form \[\begin{equation} u(e) \triangleq \frac{\mu_{eff}}{\mu_z} = \begin{cases} 1 & \textsf{for $e < 1$}\\ 1/e & \textsf{for $e \geq 1$}. \end{cases} \end{equation}\] The main advantage of this model is obviously its simplicity, allowing to get a first understanding of the physical phenomenon. But on the other hand, it has discontinuous derivatives at \(e=1\) that may induce a bad behavior of the model.
A continuous model (Model 2) also accounting for the difference between the velocity-field characteristics of electrons and holes as illustrated in Figure 3 is defined in normalized form as \[\begin{equation}\label{eqn:vdrift_model2} \nu(e) \triangleq \frac{v_{drift}}{v_{sat}} = \frac{e}{\left(1 + e^\alpha \right)^{\frac{1}{\alpha}}}. \end{equation}\] where \(\alpha=2\) for electrons and \(\alpha=1\) for holes. Note that this continuous model has been used in many compact models with the approximation that \(\alpha\) is equal to unity for both holes and electrons. The corresponding effective mobility is then given by \[\begin{equation} \mu_{eff}(\mathcal{E}_x) \triangleq \frac{vdrift}{|\mathcal{E}_x|} = \frac{\mu_z}{1 + |\mathcal{E}_x| / \mathcal{E}_c}, \end{equation}\] which can also be written in normalized form as \[\begin{equation} u(e) \triangleq \frac{\mu_{eff}}{\mu_z} = \frac{1}{1 + e}. \end{equation}\]
Although the continuous velocity-field model 2 insures the continuity of the current and the output conductance versus the drain voltage, it requires the electric field to become infinity at the drain for the velocity and hence the current to saturate, which is not physical.
The two velocity-field models presented above are plotted in Figure 3. Note also that the shape of the velocity-field curve will strongly affect the current and output conductance versus drain voltage. We will now evaluate the impact of velocity saturation on the drain current and the transconductances. For simplicity we will be using Model 1.
5.3.2 Effect of velocity saturation on the drain current
5.3.2.1 Analysis in strong inversion
We will start evaluating the impact of velocity saturation in strong inversion considering that the current in weak inversion is carried mostly by diffusion and the surface potential gradient along the channel is close to zero and hence the longitudinal electric field is smaller than the critical field. We also will ignore the effect of the vertical field on the mobility and consider \(\mu_z=\mu_0\) as constant. The drift component of the drain current is proportional to the velocity and can be written as [1] \[\begin{equation} I_D = W \cdot (-Q_i) \cdot v_{drift} = W \cdot (-Q_i) \cdot \mu_{eff} \cdot |\mathcal{E}_x| = W \cdot (-Q_i) \cdot \mu_{eff} \cdot \frac{d \Psi_s}{dx}, \end{equation}\] or using the normalized variables defined above [1] \[\begin{equation}\label{eqn:id_norm_si} i_d = 2 q_i \cdot \frac{\nu}{\lambda_c} = 2 q_i \cdot \frac{u \cdot e}{\lambda_c} = u \cdot q_i \cdot \frac{d \psi_s}{d \xi}, \end{equation}\] where the normalized variables \(i_d\), \(q_i\), \(\psi_s\) and \(\xi\) have their usual meaning. The velocity saturation parameter \(\lambda_c\) accounts for the velocity saturation effect and depends on the transistor length \(L\) according to [1] \[\begin{equation}\label{eqn:lambdac} \lambda_c \triangleq \frac{L_{sat}}{L} \end{equation}\] where [1] \[\begin{equation}\label{eqn:Lsat} L_{sat} \triangleq \frac{2 \mu_0 \cdot U_T}{v_{sat}} = \frac{2 U_T}{\mathcal{E}_c} \end{equation}\] The velocity saturation parameter \(\lambda_c\) corresponds to the parameter \(\zeta\) defined in [2] [3] as \[\begin{equation} \zeta = \frac{\lambda_c}{2} = \frac{\mu_0 \cdot U_T}{L \cdot v_{sat}} = \frac{U_T}{L \cdot \mathcal{E}_c} = \frac{v_{diff}}{v_{sat}}, \end{equation}\] where \(v_{diff}\) is the diffusion velocity defined as [2] [3] \[\begin{equation} v_{diff} = \frac{\mu_0 \cdot U_T}{L} = \frac{D_n}{L} \end{equation}\] with \(D_n = \mu_0 \cdot U_T\) the diffusivity coefficient for electron in silicon [4]. Parameter \(\zeta\) can therefore be interpreted as the ratio of the diffusion velocity to the saturated velocity. \(\lambda_c\) and \(\zeta\) are key parameters for short-channel devices that scale like \(1/L\) and hence tend to zero for very long channel devices. Setting them to zero therefore corresponds to ignoring the effect of velocity saturation. Typical values of \(\lambda_c\) for different channel lengths are given in Table 2.
| \(L\) | 1 \(\mu m\) | 0.5 \(\mu m\) | 0.17 \(\mu m\) | 0.1 \(\mu m\) |
|---|---|---|---|---|
| \(\lambda_c\) | 0.05 | 0.1 | 0.3 | 0.5 |
Using the inversion charge linearization with respect to \(\Psi_s\) gives a relation between the surface potential gradient and the inversion charge gradient [1] \[\begin{equation} \frac{d \Psi_s}{dx} = \frac{1}{n \cdot C_{ox}} \cdot \frac{d Q_i}{dx}, \end{equation}\] or in normalized form [1] \[\begin{equation}\label{eqn:dpsis_dxi} \frac{d \psi_s}{d \xi} = -2 \cdot \frac{d q_i}{d \xi}. \end{equation}\] Replacing \(\eqref{eqn:dpsis_dxi}\) into \(\eqref{eqn:id_norm_si}\) results in [1] \[\begin{equation}\label{eqn:id_mu_qi_si} i_d = -2 u \cdot q_i \cdot \frac{d q_i}{d \xi}. \end{equation}\] Compared to the constant mobility expression in strong inversion, the above expression includes now a field-dependent mobility term \(u\) which depends on the chosen velocity-field model.
The inversion charge density at the drain \(-Q_{iD}\) (or its normalized form \(q_d\)) plays a particular role in the presence of velocity saturation. When the longitudinal field \(\mathcal{E}_x\) becomes equal to the critical field \(\mathcal{E}_c\) right at the drain, the drift velocity saturates right at the drain, \(v_{drift}=v_{sat}\) at \(x=L\) (or in normalized form \(\nu = 1\) at \(\xi = 1\)). The drain current cannot increase anymore and is then limited to the saturation value \(i_{d_{sat}}\) given by \(\eqref{eqn:id_norm_si}\) evaluated at \(\xi = 1\) with \(\nu = 1\) and \(q_i = q_{d_{sat}}\) [1] \[\begin{equation}\label{eqn:idsat_qdsat} i_{d_{sat}} \triangleq \frac{2}{\lambda_c} \cdot q_{d_{sat}} = \frac{q_{d_{sat}}}{\zeta}, \end{equation}\] where \(q_{d_{sat}}\) is the value of the inversion charge density at the drain which is required to sustain the drain current when the carrier velocity is saturated right at the drain. The main difference compared to the long-channel situation is that the charge density at the drain \(-Q_{iD}\) (or its normalized form \(q_d\)) does not vanish to zero as it does at the onset of saturation for long-channel devices when \(v_d = v_p\), but it has to be finite in order for the current to flow despite the saturated velocity. To account for this saturation of the drain charge, the normalized drain charge in strong inversion has to be modified according to \[\begin{equation}\label{eqn:qd_qdsat} q_d = \begin{cases} \dfrac{v_p-v_d}{2} & \textsf{for $v_d < v_{d_{sat}}$}\\ q_{d_{sat}} & \textsf{for $v_d \geq v_{d_{sat}}$}, \end{cases} \end{equation}\] where the drain saturation voltage \(v_{d_{sat}}\) is the value of the drain voltage at which \(\mathcal{E}_x=\mathcal{E}_c\) and hence the current and the drain charge saturate. It is obtained by replacing \(q_d\) and \(v_d\) in \(q_d = (v_p-v_d)/2\) by \(q_{d_{sat}}\) and \(v_{d_{sat}}\) respectively, resulting in [1] \[\begin{equation}\label{eqn:vdsat} v_{d_{sat}} = v_p - 2 q_{d_{sat}}. \end{equation}\]
As illustrated in Figure 6, due to velocity saturation, \(v_{d_{sat}}\) is always smaller than the pinch-off voltage \(v_p\) corresponding to the saturation voltage when velocity saturation is not present.
We now will evaluate the impact of velocity saturation in strong inversion using the simplest velocity-field model, namely Model 1. The normalized drain current is obtained as before by integrating \(\eqref{eqn:id_norm_si}\) from source to drain. For \(v_d < v_{d_{sat}}\), the longitudinal field remains smaller than the critical field and according to the velocity-field Model 1 relation, there is no saturation of the carrier velocity. The effective mobility is then equal to \(\mu_z=\mu_0\) (or in normalized form \(u=1\)). The drain current for \(v_d < v_{d_{sat}}\) and \(q_d>q_{d_{sat}}\) is identical to what was obtained earlier for the long-channel transistor in strong inversion \[\begin{equation} i_d = i_f -i_r, \end{equation}\] with \[\begin{align} i_f &= q_s^2,\\ i_r &= q_d^2, \end{align}\] where \(q_s\) and \(q_d\) are the inversion charge densities at the source and drain, respectively. In strong inversion and assuming there is no velocity saturation at the source, they are related to the voltages according to \[\begin{align} q_s &\triangleq q_i(\xi=0) = \frac{v_p-v_s}{2},\\ q_d &\triangleq q_i(\xi=1) = \frac{v_p-v_d}{2}. \end{align}\]
In the case of a long-channel transistor, the drain current saturates when \(v_d=v_p\) and the drain charge becomes \(q_d=0\). For a short-channel transistor, when the drain voltage reaches the saturation voltage \(v_d=v_{d_{sat}}\), the drain charge does not vanish to zero but saturates to \(q_{d_{sat}}\). The reverse current \(i_r\) then also saturates to \(i_{r_{sat}}=q_{d_{sat}}^2\). The source and drain charges for \(v_d = v_{d_{sat}}\) are then given by \[\begin{align} q_s &= \frac{v_p-v_s}{2},\\ q_{d_{sat}} &= \frac{v_p-v_{d_{sat}}}{2},\label{eqn:qdsat_vdsat_mod1_si} \end{align}\] whereas the forward and reverse currents are given by \[\begin{align} i_f &= q_s^2,\label{eqn:if_qdsat_mod1_si}\\ i_{r_{sat}} &= q_{d_{sat}}^2.\label{eqn:ir_qdsat_mod1_si} \end{align}\] The drain current in saturation then becomes \[\begin{equation}\label{eqn:idsat_qs_qd_mod1_si} i_{d_{sat}} = i_f - i_{r_{sat}} = q_s^2 - q_{d_{sat}}^2. \end{equation}\] In order to express \(q_{d_{sat}}\), \(i_{r_{sat}}\), \(i_{d_{sat}}\) and \(v_{d_{sat}}\) in terms of \(q_s\), we can solve \(\eqref{eqn:idsat_qs_qd_mod1_si}\), \(\eqref{eqn:idsat_qdsat}\), \(\eqref{eqn:qdsat_vdsat_mod1_si}\), \(\eqref{eqn:if_qdsat_mod1_si}\) and \(\eqref{eqn:ir_qdsat_mod1_si}\) for \(q_{d_{sat}}\), \(i_f\), \(i_r\), \(i_{d_{sat}}\) and \(v_{d_{sat}}\), resulting in [1] \[\begin{align} q_{d_{sat}} &= \frac{1}{\lambda_c} \cdot \left[\sqrt{1+(\lambda_c\,q_s)^2}-1\right] = \frac{\lambda_c\,q_s^2}{1+\sqrt{1+(\lambda_c\,q_s)^2}},\label{eqn:qdsat_qs_mod1_si}\\ i_f &= q_s^2,\\ i_{r_{sat}} &= q_{d_{sat}}^2 = \frac{1}{\lambda_c^2} \cdot \left[\sqrt{1+(\lambda_c\,q_s)^2}-1\right]^2 =q_s^2 - \frac{2}{\lambda_c^2} \cdot \left[\sqrt{1+(\lambda_c\,q_s)^2}-1\right],\\ i_{d_{sat}} &= \frac{2}{\lambda_c} \cdot q_{d_{sat}} = i_f - i_{r_{sat}} = \frac{2}{\lambda_c^2} \cdot \left[\sqrt{1+(\lambda_c\,q_s)^2}-1\right] = \frac{2q_s^2}{1+\sqrt{1+(\lambda_c\,q_s)^2}},\label{eqn:idsat_qs_mod1_si}\\ v_{d_{sat}} &= v_p - 2 q_{d_{sat}} = v_p - \frac{2\lambda_c\,q_s^2}{1+\sqrt{1+(\lambda_c\,q_s)^2}}.\label{eqn:vdsat_qs_mod1_si} \end{align}\]
The normalized charges \(q_s\) and \(q_d\) are plotted versus \(v_d\) in Figure 4 ilustrating the saturation of \(q_d\) to \(q_{d_{sat}}\) for \(v_d > v_{d_{sat}}\). While the source charge remains constant because it does not depend on \(v_d\), the drain charge decreases linearly with \(v_d\). For a long-channel transistor its decreases until it reaches zero at \(v_d = v_p\). For a short-channel transistor it stops decreasing when \(v_d\) reaches \(v_{d_{sat}}\), point at which the longitudinal field \(\mathcal{E}_x\) gets equal to the critical field \(\mathcal{E}_c\) and the drift velocity starts to saturate
Figure 5 shows the impact of velocity saturation on the currents. While the forward current \(i_f\) remains unchanged, because of velocity saturation, for \(v_d>v_{d_{sat}}\), the reverse current saturates to \(i_{r_{sat}}=q_{d_{sat}}^2\) instead of zero as it would for a long-channel transistor. The drain current in saturation is therefore \(i_{r_{sat}}\) lower than the long-channel current in saturation \(i_f\). Note that, as expected, \(i_{r_{sat}}\) tends to zero when there is no velocity saturation (i.e. \(\lambda_c=0\)). Notice the discontinuity of the 1st-order derivative of \(i_d\) wrt \(v_d\) (which is simply the output conductance \(g_{ds}\)) at \(v_d=v_{d_{sat}}\) due to the discontinuous derivative of the drain charge.
The drain saturation voltage \(\eqref{eqn:vdsat_qs_mod1_si}\) is plotted versus the pinch-off voltage in Figure 6, which shows that \(v_{d_{sat}}\) can be substantially smaller than \(v_p\).
Figure 7 shows the forward, reverse and drain currents in saturation versus the pinch-off voltage. The blue curve corresponds to the normalized drain current \(i_d\) in saturation for a long-channel device for which velocity saturation can be ignored. In such a case the drain charge and the reverse current are both zero and the drain current \(i_d\) is simply equal to the forward current \(i_f\). When velocity saturation is present, the drain charge \(q_d\) in saturation is no more zero but equal to \(q_{d_{sat}}\) making the reverse current larger than zero as shown by the green curve in Figure 7. The drain current accounting for velocity saturation is then reduced by \(i_r\) resulting in the red curve in Figure 7. Notice also that the drain current being the difference between two quadratic functions of \(q_s\) and hence of \(v_p-v_s\), it becomes a linear function of \(v_p\). Indeed, in very strong inversion under strong velocity saturation (\(\lambda_c\,q_s \gg 1\)), from \(\eqref{eqn:idsat_qs_mod1_si}\) we get \[\begin{align} q_{d_{sat}} &\cong q_s,\label{eqn:qdsat_si_asym}\\ i_{d_{sat}} &\cong \frac{2q_s}{\lambda_c} = \frac{v_p-v_s}{\lambda_c}.\label{eqn:idsat_si_asym} \end{align}\] From \(\eqref{eqn:qdsat_si_asym}\) we observe that the inversion charge is constant along the channel and equal to \(q_s\) and from \(\eqref{eqn:idsat_si_asym}\) that the current is no more proportional to \(q_s^2\) but to \(q_s\) and hence to \(v_p-v_s\).
Figure 8 shows the normalized current \(i_d=IC\) versus the overdrive voltage \(V_G-V_{T0}\) measured on a long-channel and a minimum-length nMOS transistors from a 40 nm bulk CMOS process. The blue curve in Figure 8 (a) corresponds to \(\sqrt{IC}\) which, as expected, is proportional to the overdrive voltage \(V_G-V_{T0}\) which validates the quadratic dependence for long-channel devices. The blue curve in Figure 8 (b) corresponds to \(IC\) and shows to be proportional to the overdrive voltage \(V_G-V_{T0}\). This is a clear sign of velocity saturation. Indeed, in strong inversion and for a minimum channel length, \(\lambda_c\,q_s \gg 1\) and \(\eqref{eqn:idsat_qs_mod1_si}\) simplifies to \[\begin{equation}\label{eqn:idsat_si} i_{d_{sat}} \cong \frac{2 q_s}{\lambda_c} \cong \frac{v_p-v_s}{\lambda_c}, \end{equation}\] which, after denormalization, simplifies to \[\begin{equation}\label{eqn:IDsat1} I_{D_{sat}} \cong n \cdot W \cdot C_{ox} \cdot v_{sat} \cdot (V_P-v_s) \cong W \cdot C_{ox} \cdot v_{sat} \cdot (V_G-V_{T0} - n \cdot v_s). \end{equation}\] Equation \(\eqref{eqn:IDsat1}\) shows that when the channel is under strong velocity saturation conditions, the drain current in saturation does not depend on the channel length anymore and varies linearly instead of quadratically with respect to the overdrive voltage. This can be explained by the fact that in such condition on one hand the inversion charge becomes almost uniform along the channel from source to drain and equal to the value taken at the source and on the other hand that the carriers are moving at their maximum velocity which is constant along the channel. The charge moving from source to drain per unit time corresponding to the drain current is therefore constant and independent of the channel length \(L\) for a given \(W\) and \(V_P-v_s\).
5.3.2.2 Analysis valid in all regions of inversion
The above analysis can be extended to also include the moderate and weak inversion regions [5] [6] [7] [8]. In order to do this we start with the drain current expression \[\begin{equation} I_D = \mu_{eff} \cdot Q_i \cdot \mathcal{E}_x + \mu_{eff} \cdot U_T \cdot \frac{dQ_i}{dx} \end{equation}\] which can be written in normalized form as \[\begin{equation}\label{eqn:id_u_e_dqi_dxi} i_d = 2 q_i \cdot \frac{u \cdot e}{\lambda_c} - u \cdot \frac{dq_i}{d\xi}. \end{equation}\] The inversion charge linearization equation \(\eqref{eqn:dPsis_dx}\) gives a relation between the longitudinal field and the inversion charge gradient \[\begin{equation} |\mathcal{E}_x| = \frac{d\Psi_s}{dx} = \frac{1}{n C_{ox}} \cdot \frac{dQ_i}{dx} \end{equation}\] which can be written in normalized form as \[\begin{equation}\label{eqn:e_dqidxi} e = -\lambda_c \cdot \frac{dq_i}{d\xi}. \end{equation}\] Substituting \(\eqref{eqn:e_dqidxi}\) in \(\eqref{eqn:id_u_e_dqi_dxi}\) results in \[\begin{equation}\label{eqn:id_u_dqi_dxi} i_d = -u \cdot (2q_i+1) \cdot \frac{dq_i}{d\xi}. \end{equation}\]
To derive the model that is valid in all modes of inversion but includes the effect of velocity saturation, we use the simplest velocity-field model, namely Model 1. Integrating \(\eqref{eqn:id_u_dqi_dxi}\) from source to drain assuming first that there is no velocity saturation at the drain (i.e. \(v_d < v_{d_{sat}}\) or \(q_d > q_{d_{sat}}\) and hence \(u=1\) in \(\eqref{eqn:id_u_dqi_dxi}\)), we get the earlier long-channel result \[\begin{equation}\label{eqn:id_no_vs} i_d = q_s^2-q_d^2+q_s-q_d. \end{equation}\] where \(q_s^2-q_d^2\) corresponds to the drift current, whereas \(q_s-q_d\) corresponds to the diffusion current. For a long-channel device in saturation we have \(q_d \ll q_s\) and the drain current in saturation is then simply given by \[\begin{equation}\label{eqn:idsat_long} i_{d_{sat}} = q_s^2+q_s. \end{equation}\] For a short-channel device, velocity saturation needs to be accounted for in the drift part of the drain current in saturation by replacing \(q_d\) by \(q_{d_{sat}}\). In weak inversion, the longitudinal electric field \(\mathcal{E}_x\) usually stays smaller than the critical filed \(\mathcal{E}_c\) and the current should therefore not be affected by velocity saturation. Hence, the \(q_d\) term in the diffusion part of the current \(\eqref{eqn:id_no_vs}\) should not be replaced by \(q_{d_{sat}}\) and can simply be neglected in saturation. Therefore, as soon as velocity saturation starts to happen right at the drain, the current in saturation becomes \[\begin{equation}\label{eqn:idsat_qs_qdsat} i_{d_{sat}} = q_s^2 - q_{d_{sat}}^2 + q_s. \end{equation}\]
In the original model proposed in [5] [6] [7] [8], the drain current in saturation \(i_{d_{sat}}\) was actually affected by velocity saturation in weak inversion, because the \(q_d\) term of the diffusion current was also replaced by \(q_{d_{sat}}\).However, the difference between this model and the original model presented in [5] [6] [7] [8] remains very small particularly for small values of \(\lambda_c\).
Solving \(\eqref{eqn:idsat_qs_qdsat}\) and \(\eqref{eqn:idsat_qdsat}\) for \(q_{d_{sat}}\) and \(i_{d_{sat}}\) results in \[\begin{align} q_{d_{sat}} &= \frac{1}{\lambda_c} \cdot \left[\sqrt{1+\lambda_c^2\,(q_s^2+q_s)}-1\right] = \frac{\lambda_c(q_s^2+q_s)}{1+\sqrt{1+\lambda_c^2\,(q_s^2+q_s)}},\label{eqn:qdsat_qs_mod1}\\ i_f &= q_s^2+q_s,\\ i_{r_{sat}} &= q_{d_{sat}}^2 = \frac{1}{\lambda_c^2} \cdot \left[\sqrt{1+\lambda_c^2\,(q_s^2+q_s)}-1\right]^2 =q_s^2 +q_s - \frac{2}{\lambda_c^2} \cdot \left[\sqrt{1+\lambda_c^2\,(q_s^2+q_s)}-1\right],\\ i_{d_{sat}} &= \frac{2}{\lambda_c} \cdot q_{d_{sat}} = i_f - i_{r_{sat}} = \frac{2}{\lambda_c^2} \cdot \left[\sqrt{1+\lambda_c^2\,(q_s^2+q_s)}-1\right] = \frac{2(q_s^2+q_s)}{1+\sqrt{1+\lambda_c^2\,(q_s^2+q_s)}},\label{eqn:idsat_qs_mod1}\\ v_{d_{sat}} &= v_p - 2 q_{d_{sat}} = v_p - \frac{2}{\lambda_c} \cdot \left[\sqrt{1+\lambda_c^2\,(q_s^2+q_s)}-1\right].\label{eqn:vdsat_qs_mod1} \end{align}\]
From \(\eqref{eqn:qdsat_qs_mod1}\) and \(\eqref{eqn:idsat_qs_mod1}\), we see that for \(\lambda_c=0\) (no velocity saturation), we fall back to the long-channel equations with \(q_{d_{sat}}=0\), \(i_{r_{sat}}=0\) (saturation) and \(i_{d_{sat}}=q_s^2+q_s\). In strong inversion (\(q_s \gg 1\)) we get the earlier result \(\eqref{eqn:qdsat_qs_mod1_si}\) and \(\eqref{eqn:idsat_qs_mod1_si}\) found for Model 1. In very strong inversion under velocity saturation (\(\lambda_c\,q_s \gg 1\)), we get the strong inversion asymptotes \(\eqref{eqn:idsat_si_asym}\). As expected and contrary to the original model presented in [5] [6] [7] [8], in weak inversion we do not observe any impact of velocity saturation. Indeed, for \(q_s \ll 1\), \(\eqref{eqn:qdsat_qs_mod1}\) and \(\eqref{eqn:idsat_qs_mod1}\) reduce to \[\begin{align} q_{d_{sat}} &\cong \frac{\lambda_c}{2} \cdot q_s \ll 1,\\ i_{d_{sat}} &\cong q_s. \end{align}\]
5.3.3 Effect of velocity saturation on the transconductances
5.3.3.1 Analysis in strong inversion
The impact of velocity saturation on the transconductances in saturation can be derived from the above analysis by rewriting the normalized source transconductance in saturation as \[\begin{equation}\label{eqn:gms_dqs_dvs_si} g_{ms_{sat}} \triangleq - \frac{\partial i_{d_{sat}}}{\partial v_s} = - \frac{\partial i_{d_{sat}}}{\partial q_s} \cdot \frac{\partial q_s}{\partial v_s}. \end{equation}\]
We first will derive \(g_{ms_{sat}}\) in strong inversion in which case \[\begin{equation} \frac{\partial q_s}{\partial v_s} = -\frac{1}{2}. \end{equation}\]
For Model 1, the derivative \(\partial i_{d_{sat}}/\partial q_s\) is simply obtained by differentiating \(\eqref{eqn:idsat_qs_mod1_si}\) resulting in \[\begin{equation} \frac{\partial i_{d_{sat}}}{\partial q_s} = \frac{2 q_s}{\sqrt{1+(\lambda_c\,q_s)^2}}. \end{equation}\] The normalized source transconductance in strong inversion and saturation is then given by \[\begin{equation}\label{eqn:gmssat_qs_mod1_si} g_{ms_{sat}} = \frac{q_s}{\sqrt{1+(\lambda_c\,q_s)^2}}. \end{equation}\] For circuit design it is more useful to have \(g_{ms}\) expressed in term of the inversion coefficient \(IC=i_{d_{sat}}\). This can be done by solving \(\eqref{eqn:idsat_qs_mod1_si}\) for \(q_s\) which results in \[\begin{equation} q_s = \sqrt{IC} \cdot \sqrt{1+\left(\tfrac{\lambda_c}{2}\right)^2\,IC}. \end{equation}\] \(g_{ms_{sat}}\) is then given by \[\begin{equation}\label{eqn:gmssat_ic_mod1_si} g_{ms_{sat}} = \sqrt{IC} \cdot \frac{\sqrt{4+\lambda_c^2\,IC}}{2+\lambda_c^2\,IC}. \end{equation}\]
In very strong inversion (\(q_s \gg 1\) or \(IC \gg 1\)), \(\eqref{eqn:gmssat_qs_mod1_si}\) and \(\eqref{eqn:gmssat_ic_mod1_si}\) reduce to \[\begin{equation}\label{eqn:gmssat_si} g_{ms_{sat}} \cong \frac{1}{\lambda_c} = \frac{L}{L_{sat}}. \end{equation}\] Instead of increasing as \(\sqrt{IC}\), as it does for long-channel devices, for short-channel transistors with heavy velocity saturation, the normalized source transconductance \(g_{ms_{sat}}\) saturates to \(1/\lambda_c\). Parameter \(\lambda_c\) therefore sets the maximum normalized source transconductance that can be achieved by a short-channel device for a given technology.
From \(\eqref{eqn:gmssat_si}\) it seems that the transconductance scales like \(L\), however this is not correct. Indeed, if we write the transconductance in denormalized form, we get \[\begin{equation}\label{eqn:Gmssat_si} G_{ms_{sat}} \cong \frac{G_{spec}}{\lambda_c} = n\,W\,C_{ox}\,v_{sat} \end{equation}\] and hence \[\begin{equation}\label{eqn:Gmsat_si} G_{m_{sat}} \cong \frac{G_{ms_{sat}}}{n} = W\,C_{ox}\,v_{sat}. \end{equation}\] From \(\eqref{eqn:Gmssat_si}\) and \(\eqref{eqn:Gmsat_si}\), we see that in strong inversion with heavy velocity saturation, the source and gate transconductances become actually independent of the transistor length \(L\) and independent of the current! They only depend on the transistor width \(W\) and the saturated drift velocity \(v_{sat}\). This means that increasing the bias current does not help increasing the transconductance and the only way to increase \(G_{ms_{sat}}\) and \(G_{m_{sat}}\) is to increase the transistor width.
5.3.3.2 Analysis valid in all regions of inversion
We now will derive an expression of the normalized source transconductance in saturation that is valid in all modes of inversion using the simplest velocity-field model, namely Model 1. To do this we first rewrite the source transconductance as \[\begin{equation}\label{eqn:gms_dqs_dvs} g_{ms_{sat}} \triangleq - \frac{\partial i_{d_{sat}}}{\partial v_s} = \frac{\partial i_{d_{sat}}}{\partial q_s} \cdot \left(\frac{\partial v_s}{\partial q_s}\right)^{-1}. \end{equation}\]
Recalling the relation between the saturation voltage and the source charge which allows to write the source voltage in terms of the source charge at a given gate and pinch-off voltage as \[\begin{equation}\label{eqn:vs_vp_qs} v_s = v_p-2q_s-\ln(q_s). \end{equation}\] Differentiating \(\eqref{eqn:vs_vp_qs}\) we get \[\begin{equation} \frac{\partial v_s}{\partial q_s} = -\frac{2q_s+1}{q_s}. \end{equation}\]
For Model 1, the derivative \(\partial i_{d_{sat}}/\partial q_s\) is simply obtained by differentiating \(\eqref{eqn:idsat_qs_mod1}\) resulting in \[\begin{equation} \frac{\partial i_{d_{sat}}}{\partial q_s} = \frac{2q_s+1}{\sqrt{1+\lambda_c^2\,(q_s^2+q_s)}} \end{equation}\] The normalized source transconductance in saturation for Model 1 is then given by \[\begin{equation}\label{eqn:gmssat_qs_mod1_new} g_{ms_{sat}} = \frac{q_s}{\sqrt{1+\lambda_c^2\,(q_s^2+q_s)}}, \end{equation}\] which has the following asymptotes in weak and strong inversion \[\begin{equation} g_{ms_{sat}} \cong \begin{cases} q_s &\textsf{in weak inversion ($q_s \ll 1$)}\label{eqn:gmssat_wi_mod1_new}\\ \frac{q_s}{\sqrt{1+(\lambda_c\,q_s)^2}} \cong \frac{1}{\lambda_c}&\textsf{in strong inversion ($q_s \gg 1$)}. \end{cases} \end{equation}\]
Without velocity saturation (\(\lambda_c = 0\)), \(\eqref{eqn:gmssat_qs_mod1_new}\) reduces to the long-channel expression \(g_{ms_{sat}} \cong q_s\). In strong inversion (\(q_s \gg 1\)) we get the earlier result \(\eqref{eqn:gmssat_qs_mod1_si}\) found in the strong inversion model. In very strong inversion under velocity saturation (\(\lambda_c\,q_s \gg 1\)), we get the strong inversion asymptote \(\eqref{eqn:gmssat_si}\). In weak inversion, as expected velocity saturation has no impact as shown by \(\eqref{eqn:gmssat_wi_mod1_new}\) contrary to the original model presented in [5] [6] [7] [8]} which shows some dependence on \(\lambda_c\).
As above, we can also express \(g_{ms_{sat}}\) in terms of the inversion coefficient \(i_{d_{sat}}=IC\) by solving \(\eqref{eqn:idsat_qs_mod1}\) for \(q_s\) resulting in \[\begin{equation}\label{eqn:qs_ic_mod1} q_s = \tfrac{1}{2}\,\left(\sqrt{4IC+1+(\lambda_c\,IC)^2}-1\right). \end{equation}\] Replacing \(\eqref{eqn:qs_ic_mod1}\) in \(\eqref{eqn:gmssat_qs_mod1_new}\) results in \[\begin{equation}\label{eqn:gmssat_ic_mod1_new} g_{ms_{sat}} = \frac{\sqrt{4IC+1+(\lambda_c\,IC)^2}-1}{2+\lambda_c^2\,IC} = \frac{2IC\,\left[1+\left(\frac{\lambda_c}{2}\right)^2\,IC\right]}{\left(1+\frac{\lambda_c^2}{2}\,IC\right)\left(1+\sqrt{4 IC+1+(\lambda_c\,IC)^2}\right)}. \end{equation}\] Again without velocity saturation (\(\lambda_c = 0\)), \(\eqref{eqn:gmssat_ic_mod1_new}\) reduces to the long-channel expressions \[\begin{equation} g_{ms_{sat}} = \frac{\sqrt{4IC+1}-1}{2} = \frac{2IC}{1+\sqrt{4IC+1}}. \end{equation}\] The asymptotes in weak and strong inversion are given by \[\begin{equation} g_{ms_{sat}} \cong \begin{cases} IC &\textsf{in weak inversion ($IC \ll 1$)}\\ \sqrt{IC} \cdot \frac{\sqrt{4+\lambda_c^2\,IC}}{2+\lambda_c^2\,IC} \cong \frac{1}{\lambda_c} &\textsf{in strong inversion ($IC \gg 1$)}. \end{cases} \end{equation}\] We see that the source transconductance in weak inversion and in saturation for short-channel devices is not affected by velocity saturation and remains proportional to the inversion coefficient and hence to the drain current.
5.3.4 Effect of velocity saturation on the \(G_m/I_D\) ratio
We can now easily derive an expression for the \(G_m/I_D\) FoM that accounts for velocity saturation and is valid from weak to strong inversion. The normalized \(G_m/I_D\) FoM is obtained by dividing \(\eqref{eqn:gmssat_ic_mod1_new}\) by \(IC\) resulting in \[\begin{equation}\label{eqn:gmid_ic_mod1} \frac{g_{ms}}{IC} = \frac{G_{ms}\,U_T}{I_D} = \frac{G_m\,n\,U_T}{I_D} = \frac{\sqrt{4IC+1+(\lambda_c\,IC)^2}-1}{IC\,(2+\lambda_c^2\,IC)} = \begin{cases} 1 & \textsf{in WI and sat.}\\ \dfrac{1}{\lambda_c IC} & \textsf{in SI and sat.} \end{cases} \end{equation}\]
Equation \(\eqref{eqn:gmid_ic_mod1}\) is plotted versus \(IC\) in red in Figure 10 and compared to the long-channel behavior corresponding to the dashed red curve. We clearly see that for a given current budget, the impact of velocity saturation in strong inversion is dramatic for low-power design since it reduces the current efficiency by a factor \(\lambda_c \sqrt{IC}\). For example, for \(\lambda_c=0.5\) and \(IC=100\), the current efficiency is reduced by a factor 5, which is considerable. This means that the transistor needs to be five times larger to recover the same transconductance for a given current budget. On the other hand, the normalized \(G_m/I_D\) ratio remains invariant (i.e. \(g_{ms}/IC=1\)) in weak inversion, irrespective of the channel length. This is simply due to the fact that in weak inversion the source transconductance remains proportional to the current and additionally velocity saturation has no effect on \(g_{ms}\). As shown in Figure 10, the inversion coefficient for which the strong inversion asymptote of a short-channel device crosses the horizontal unity line is equal to \(1/\lambda_c\). This is actually how the parameter \(\lambda_c\) can be extracted from measurements of a short-channel device.
We actually don’t need to go to very deep-submicron CMOS technologies to see the effect of velocity saturation. Figure 11 shows the current efficiency measured on a minimum length nMOS transistor from a 130 nm bulk CMOS process and which already shows a loss of efficiency in strong inversion. It also illustrates how the \(\lambda_c\) parameter can be extracted from the intersection of the \(1/IC\) asymptote with the horizontal unity line giving \(1/\lambda_c=3\) and hence \(\lambda_c =1/3\). Figure 11 also highlights the very good match between the simple expression \(\eqref{eqn:gmid_ic_mod1}\) and the measured data.
The impact of velocity saturation is also illustrated in Figure 14 which shows the current efficiency measured on a long-channel (Figure 14 (a)) and short-channel device (Figure 14 (b)) from a 40 nm bulk CMOS process. It actually corresponds to the derivatives of the large-signal \(IC\) versus \(V_G-V_{T0}\) characteristics shown in Figure 8. We clearly see the strong degradation introduced by velocity saturation on the current efficient of the short-channel transistor in Figure 14 (b). We also see a reasonable fit between the simple analytical expression of the normalized \(G_m/I_D\) and the measurements.
Figure 13 shows the current efficiency measured on different devices having the same width but three different lengths for the same 40 nm bulk CMOS technology. The blue curve corresponds to the long-channel asymptote (\(L=2\,\mu m\)), the green curve corresponds to a medium channel length (\(L=120\,nm\)) but already affected by velocity saturation and finally the red curve corresponds to the minimum channel length (\(L=40\,nm\)) which is strongly affected by velocity saturation. We observe that the cross-point between the \(1/IC\) asymptote which should scale like \(L\) indeed decreases and hence moves to the left. Additional measurements performed on more advanced bulk, FDSOI and FinFET technologies are presented in .
The model used in this Section, assumed that velocity saturation occurs when \(v_d=v_{d_{sat}}\) and that the drain charge and current in saturation (for \(v_d>v_{d_{sat}}\)) remain constant. In reality this is not the case because of the effects of channel length modulation (CLM) and drain induced barrier lowering (DIBL) which are discussed in the next Sections.
5.4 Channel length modulation (CLM)
5.4.1 Channel length reduction
In the previous Section, velocity saturation starts when the longitudinal field \(\mathcal{E}_x\) becomes equal to the critical field \(\mathcal{E}_c\) right at the drain limit of the channel. At this point, the drain voltage becomes equal to the saturation voltage \(V_{D_{sat}}\). As the drain voltage gets larger than the saturation voltage \(V_{D_{sat}}\), the saturation point moves away from the drain into the channel. As illustrated in Figure 14 (a), this is creating a velocity saturated region (VSR) in which the carriers are traveling at their maximum saturated velocity \(v_{sat}\). Using a quasi-2D analysis applied to the VSR shown in Figure 14 (b), it can be shown that the channel length reduction \(\Delta L\) is given by [9] [10] [11] [12] [13] \[\begin{equation} \Delta L \triangleq L-L_{eff} = \ell \cdot \ln\left(u+\sqrt{u^2+1}\right), \end{equation}\] where \(u\) is defined as \[\begin{equation}\label{eqn:u} u \triangleq \frac{V_{DS}-V_{DS_{sat}}}{\ell\,\mathcal{E}_{sat}} = \frac{v_d-V_{D_{sat}}}{\ell\,\mathcal{E}_{sat}}. \end{equation}\] \(V_{DS_{sat}} = V_{D_{sat}}-v_s\) is the drain-to-source saturation voltage accounting for velocity saturation. If we use Model 1 the normalized value of \(V_{D_{sat}}\) is given by \(\eqref{eqn:vdsat_qs_mod1_si}\) \[\begin{equation*} v_{d_{sat}} = v_p - \frac{2\lambda_c \cdot q_s^2}{1+\sqrt{1+(\lambda_c\,q_s)^2}}. \end{equation*}\] Parameter \(\ell\) (which has length unit) is defined as [11] [12] [13] \[\begin{equation} \ell \triangleq \sqrt{\frac{\epsilon_{si}\,x_j}{C_{ox}}} \end{equation}\] where \(x_j\) is the junction depth and \(C_{ox}\) the oxide capacitance per unit area. Parameter \(\mathcal{E}_{sat}\) is defined as the longitudinal electric field at the pinch-off point which is actually equal to the critical field \(\mathcal{E}_c\) defined in the velocity saturation model \[\begin{equation} \mathcal{E}_{sat} = \mathcal{E}_c = \frac{v_{sat}}{\mu_0} = \frac{2 U_T}{L_{sat}}. \end{equation}\] We can then rewrite \(\eqref{eqn:u}\) in terms of the normalized drain and saturation voltages according to \[\begin{equation} u = \frac{L_{sat}}{2 \ell} \cdot (v_d-v_{d_{sat}}). \end{equation}\] In the above model, \(L_{sat}\) appears in the VS parameter \(\lambda_c = L_{sat}/L\) that is used for the computation of the drain current in saturation, but also in \(u\) to scale the voltage that is used for the calculation of \(\Delta L\). For \(u \ll 1\), the channel length reduction simplifies to \[\begin{equation}\label{eqn:DeltaL_ekv} \Delta L \cong \ell \cdot \ln(1+u) = \ell \cdot \ln\left(1+\frac{v_d-v_{d_{sat}}}{v_{dclm}}\right), \end{equation}\] where \(v_{dclm} = 2\ell/L_{sat}\) is considered an additional fitting parameter. This simpler model was initially proposed by Arora [12] [13] and used in the EKV v2.6 compact model [14]. We will use this model below to investigate the impact of CLM on the drain current in saturation.
5.4.2 Impact of CLM on the drain current in saturation
5.4.2.1 Analysis in strong inversion
CLM has obviously an impact on the drain current in saturation which can no more be considered as constant. Since the impact of VS is dominant in strong inversion, we first analyze the impact of CLM in strong inversion.
When accounting for VS, the transistor enters into saturation when the longitudinal field \(\mathcal{E}_x\) becomes equal to the critical field \(\mathcal{E}_c\) which happens when \(v_d=V_{D_{sat}}\) (or in normalized form \(v_d=v_{d_{sat}}\)). At this point the channel length is still equal to \(L\) and the drain current is given by \[\begin{equation} I_{D_{sat0}} = I_{spec} \cdot i_{d_{sat0}} \end{equation}\] with \[\begin{equation}\label{eqn:clm_ispec} I_{spec} \triangleq I_{spec\Box} \cdot \frac{W}{L} \end{equation}\] and \[\begin{equation} i_{d_{sat0}} = \frac{2 q_s^2}{1+\sqrt{1+(\lambda_{c0}\,q_s)^2}} \end{equation}\] where the VS parameter \(\lambda_{c0}\) is defined as \[\begin{equation} \lambda_{c0} \triangleq \frac{L_{sat}}{L}. \end{equation}\] The \(0\) in the subscript indicates that the operating point corresponds to the onset of saturation for which \(v_d=v_{d_{sat}}\) and the length is still equal to \(L\) (or \(\Delta v_d = v_d-v_{d_{sat}} = 0\) and \(\Delta L=0\)).
When the drain voltage is increased above \(V_{D_{sat}}\) (or \(v_d > V_{D_{sat}}\)), the pinch-off point (defined as the point along the channel at which \(\mathcal{E}_x = \mathcal{E}_c\) or \(V_{ch}=V_{D_{sat}}\)) moves in the direction of the source reducing the channel length by \(\Delta L\). The drain current in saturation for \(v_d>V_{D_{sat}}\) is then given by \[\begin{equation} I_{D_{sat}} = I_{spec\Box} \cdot \frac{W}{L_{eff}} \cdot i_{clm} \end{equation}\] where \(L\) has been replaced by the effective length \(L_{eff} \triangleq L-\Delta L\) in \(I_{spec}\). The term \(i_{clm}\) accounts for the dependency of \(\lambda_{c0}\) on \(L\) in \(i_{d_{sat0}}\) where \(L\) also needs to replaced by \(L_{eff}\). \(i_{clm}\) is defined as \[\begin{equation} i_{clm} = \frac{2 q_s^2}{1+\sqrt{1+(\lambda_c\,q_s)^2}} \end{equation}\] where the VS parameter \(\lambda_c\) is now defined as \[\begin{equation} \lambda_c \triangleq \frac{L_{sat}}{L_{eff}}. \end{equation}\]
We actually can keep the original definition of \(I_{spec}\) given by \(\eqref{eqn:clm_ispec}\) by rewriting \(I_{D_{sat}}\) as \[\begin{equation} \begin{split} I_{D_{sat}} &= I_{spec\Box} \cdot \frac{W}{L_{eff}} \cdot i_{clm} = I_{spec\Box} \cdot \frac{W}{L} \cdot \frac{L}{L_{eff}} \cdot i_{clm}\\ &= I_{spec} \cdot \frac{L}{L-\Delta L} \cdot i_{clm} = I_{spec} \cdot f_{clm} \cdot i_{clm} \end{split} \end{equation}\] where \(f_{clm}\) is defined as \[\begin{equation}\label{eqn:fclm_def} f_{clm} \triangleq \frac{L}{L_{eff}} = \frac{L}{L-\Delta L} = \frac{1}{1-\Delta L/L}. \end{equation}\]
The VS saturation parameter \(\lambda_c\) can then also be written in terms of \(f_{clm}\) as \[\begin{equation}\label{eqn:lambdac_lambdac0_fclm} \lambda_c \triangleq \frac{L_{sat}}{L_{eff}} = \frac{L_{sat}}{L-\Delta L} = \frac{L_{sat}}{L} \cdot \frac{L}{L-\Delta L} = \frac{L_{sat}}{L} \cdot \frac{1}{1-\Delta L/L} = \lambda_{c0} \cdot f_{clm}. \end{equation}\]
The normalized drain current in saturation \(i_{d_{sat}}\) is then simply given by \[\begin{equation}\label{eqn:idsat_fclm_iclm} i_{d_{sat}} \triangleq \frac{I_{D_{sat}}}{I_{spec}} = f_{clm} \cdot i_{clm}. \end{equation}\] where \(I_{spec}\) is constant and given by \(\eqref{eqn:clm_ispec}\).
CLM is impacting the drain current in saturation \(i_{d_{sat}}\) in two ways. First, \(i_{d_{sat}}\) increases due to the increase of \(f_{clm}\). Second, the latter increase of \(f_{clm}\) also increases \(\lambda_c\) which reduces the drain current. This current decrease is captured by \(i_{clm}\). There are therefore two antagonist effects induced by CLM that need to be carefully accounted for, particularly when deriving the output conductance.
In strong inversion (\(q_s\gg 1\)), and for strong VS (\(\lambda_c\,q_s \gg 1\)), the drain current at saturation is given by \[\begin{equation} i_{d_{sat0}} \cong \frac{2}{\lambda_{c0}}\,q_s. \end{equation}\] Similarly, the \(i_{clm}\) term becomes \[\begin{equation} i_{clm} \cong \frac{2}{\lambda_c}\,q_s = \frac{2}{\lambda_{c0}\,f_{clm}}\,q_s. \end{equation}\] The normalized drain current in saturation then becomes \[\begin{equation} i_{d_{sat}} = f_{clm} \cdot i_{clm} \cong f_{clm} \cdot \frac{2}{\lambda_{c0}\,f_{clm}}\,q_s = i_{d_{sat0}}. \end{equation}\] In this case, CLM has no impact on the drain current because \(i_{clm}\) fully compensates \(f_{clm}\) and the drain current stays constant and equal to \(i_{d_{sat0}}\).
This behavior is specific to short-channel devices. However, as it will be established below, for short-channel transistors, DIBL actually dominates CLM. We therefore need to focus on the impact of CLM on long-channel devices.
5.4.2.2 Long-channel expression in strong inversion
For long-channel transistors, we can ignore the impact of CLM on the \(i_{clm}\) term because \(\lambda_{c0}\) becomes very small and \(\lambda_c\) also remains small because \(f_{clm}\) does not increase much for long-channel devices. Therefore, for long-channel transistors, \(i_{clm}\) can be considered to be equal to the long-channel current \(i_{clm} \cong q_s^2\). The drain current in strong inversion and in saturation for a long-channel transistor is then only impacted by \(f_{clm}\) according to \[\begin{equation} i_{d_{sat}} \cong f_{clm} \cdot q_s^2. \end{equation}\]
5.4.2.3 Linear dependence and empirical model
In the measurements presented below, we see that the output characteristic in saturation can be approximated by a linear function. Such a linear dependence of \(i_{d_{sat}}\) on \(v_d\) can be obtained from the model of \(\Delta L\) versus \(v_d\) described in \(\eqref{eqn:DeltaL_ekv}\) if parameter \(v_{dclm}\) and the maximum drain voltage are such that \(\Delta v_d = v_d - v_{d_{sat}} \ll v_{dclm}\). Then \(\Delta L/L\) becomes \[\begin{equation} \frac{\Delta L}{L} = \frac{\ell}{L} \cdot \ln\left(1+\frac{v_d-v_{d_{sat}}}{v_{dclm}}\right) \cong \frac{\ell}{L} \cdot \frac{v_d - v_{d_{sat}}}{v_{dclm}} = \frac{L_{clm}}{L} \cdot (v_d - v_{d_{sat}}) \end{equation}\] with \(L_{clm} \triangleq \ell/v_{dclm}\). If we additionally can consider that \(\ell<L\), then \(\Delta L/L \ll 1\) and \(f_{clm}\) simplifies to \[\begin{equation} f_{clm} = \frac{1}{1-\Delta L/L} \cong 1+\frac{\Delta L}{L} \cong 1 + \frac{\ell}{L} \cdot \frac{v_d - v_{d_{sat}}}{v_{dclm}} = 1 + \frac{L_{clm}}{L} \cdot (v_d - v_{d_{sat}}). \end{equation}\]
Under the assumption that \(\Delta L/L \ll 1\), the impact of \(f_{clm}\) on \(\lambda_c\) can be neglected and \(\lambda_c\) can be replaced by \(\lambda_{c0}\) which is independent of \(v_d\). The drain current in saturation \(i_{d_{sat}}\) then writes \[\begin{equation}\label{eqn:clm_idsat_linear} i_{d_{sat}} \cong \left(1+\frac{\Delta L}{L}\right) \cdot i_{d_{sat0}} \cong \left(1+\frac{\ell}{L} \cdot \frac{v_d - v_{d_{sat}}}{v_{dclm}}\right) \cdot i_{d_{sat0}} = \left[1+\frac{L_{clm}}{L} \cdot (v_d - v_{d_{sat}})\right] \cdot i_{d_{sat0}}, \end{equation}\] which has now the desired linear behavior with respect to \(v_d\).
The drain current in saturation can therefore be expressed using an empirical model with a linear function having a slope equal to the output conductance \(G_{ds}\) and an Early voltage \(V_E\) (which is negative) \[\begin{equation}\label{eqn:clm_idsat_empirical_model} I_{D_{sat}} \cong G_{ds} \cdot (v_d-V_E) \end{equation}\] or in normalized form \[\begin{equation} i_{d_{sat}} \cong g_{ds} \cdot (v_d-v_e). \end{equation}\]
\(g_{ds}\) and \(v_e\) are related to the parameters in \(\eqref{eqn:clm_idsat_linear}\) by \[\begin{align} g_{ds} &= \frac{L_{clm}}{L} \cdot i_{d_{sat0}},\\ -v_e &= \frac{i_{d_{sat0}}}{g_{ds}}-V_{D_{sat}}. \end{align}\]
5.4.3 Output conductance in saturation due to CLM
The output conductance in saturation is defined as \[\begin{equation}\label{eqn:Gds_sat_def} G_{ds} = \left.\frac{\partial I_{D_{sat}}}{\partial V_{DS}}\right|_{V_G,v_s,v_d}. \end{equation}\] or in normalized form \[\begin{equation} g_{ds} \triangleq \frac{G_{ds}}{G_{spec}} = \frac{\partial i_{d_{sat}}}{\partial v_{ds}} \end{equation}\] with \[\begin{equation} G_{spec} \triangleq \frac{I_{spec}}{U_T}. \end{equation}\] In this derivation we will consider that \(v_s\) is constant, therefore \[\begin{equation}\label{eqn:gds_sat_def} g_{ds} = \frac{\partial i_{d_{sat}}}{\partial v_{ds}} = \frac{\partial i_{d_{sat}}}{\partial v_d}. \end{equation}\] It can be shown that \(g_{ds}\) is actually proportional to the saturation current \(i_{d_{sat}}\) and can be written as \[\begin{equation}\label{eqn:clm_gdssat_empirical_model} g_{ds} = \frac{i_{d_{sat}}}{v_{clm}} \end{equation}\] where \(v_{clm}\) is the CLM voltage given by \[\begin{equation} \frac{1}{v_{clm}} = \frac{g_{ds}}{i_{d_{sat}}} = g_1 \cdot g_2, \end{equation}\] where \(g_1\) accounts for the dependence of \(f_{clm}\) to \(v_d\), whereas \(g_2\) is due to the change of \(\lambda_c\) with respect to \(v_d\) \[\begin{align} g_1 &\triangleq \frac{\ell}{L} \cdot \frac{f_{clm}}{v_{dclm} + v_d - v_{dsat}} = \frac{L_{clm}}{L} \cdot \frac{f_{clm}}{1+\frac{v_d-v_{dsat}}{v_{dclm}}},\label{eqn:g1_def}\\ g_2 &\triangleq 1 - \frac{\lambda_c^2}{2} \cdot \frac{i_{clm}}{\sqrt{1+(\lambda_c \, q_s)^2}}\label{eqn:g2_def}. \end{align}\]
For a long-channel transistor, we can neglect the change of the drain current due to a change of \(\lambda_c\) and hence \(g_2 \cong 1\), which leads to \[\begin{equation}\label{eqn:oneovervclm_approx1} \frac{1}{v_{clm}} \cong g_1 = \frac{\ell}{L} \cdot \frac{f_{clm}}{v_{dclm}+v_d-v_{d_{sat}}} = \frac{L_{clm}}{L} \cdot \frac{f_{clm}}{1+\frac{v_d-v_{d_{sat}}}{v_{dclm}}}. \end{equation}\] In the case of the linear model we can assume that \(v_d-v_{d_{sat}} \ll v_{dclm}\) for which \[\begin{equation}\label{eqn:oneovervclm_approx2} \frac{1}{v_{clm}} \cong \frac{L_{clm}}{L} \end{equation}\] which scales as \(1/L\) but is now bias independent. This means that for long-channel transistors, most of the bias dependence of \(g_{ds}\) due to CLM for a long-channel transistor is actually captured by \(i_{d_{sat}}\) and \(v_{clm}\) can be considered as approximately bias independent and proportionnal to \(L\).
5.4.4 Experimental validation
As will be discussed below, the output characteristic and output conductance for short-channel transistors are dominated by DIBL. For this reason we will focus on a long-channel transistor in order to validate the model derived above. Figure 15 shows the output characteristic and output conductance measured in strong inversion on a very wide and long nMOS transistor (\(W=3\,\mu m\), \(L=1\,\mu m\)) from a 28 nm bulk CMOS technology. Despite the long channel, we see that the output conductance does not vanish to zero in saturation. The finite output conductance shown in Figure 15 is then clearly due to CLM.
In order to perform the normalization and validation, the sEKV parameters have first been extracted from the \(I_D\)-\(V_G\) characteristics, resulting in the values presented in Table 3. We see that parameter \(\lambda_c\) is very small, justifying the long-channel approximation used above.
| \(W\) | \(L\) | \(V_{T0}\) | \(n\) | \(I_{spec}\) | \(\lambda_c\) |
|---|---|---|---|---|---|
| 3 \(\mu m\) | 1 \(\mu m\) | 0.427 V | 1.176 | 2.43 \(\mu A\) | 0.03 |
Figure 16 shows the fit of the normalized measured output characteristic of this long-channel transistor for three different gate bias voltages. For long-channel the normalized current is about equal to \(f_{clm}\) which is calculated in Figure 16 using the channel length reduction expression given in \(\eqref{eqn:DeltaL_ekv}\). We see that a very good fit is obtained for values of the parameters \(v_{dclm} = 17.7\) (\(V_{DCLM}=0.46\,V\)) and \(\ell = 17.6\,\mu m\). We can also observe from Figure 16 that the output characteristic for a long-channel transistor is close to a linear dependence on \(\Delta v_d\). We can therefore extract the parameters \(G_{ds}\) and \(V_E\) for each gate voltage resulting in the linear approximation shown in Figure 17. The parameters have been extracted using a linear regression using a saturation voltage slightly higher than the long-channel value \(V_P\) in order to have a better approximation of the output conductance in the saturation region.
The empirical linear model can also be used in weak and moderate inversion as shown in Figure 18. From Figure 18, we observe that the parameter \(V_M\) used in the output conductance expression does not vary too much. Figure 19 shows the fit to the output conductance in saturation over all bias obtained using a single value of \(V_M=30\,V\). We can conclude that the simple model given by \(\eqref{eqn:clm_gdssat_empirical_model}\) provides a reasonable estimation of the output conductance in saturation due to CLM for long-channel transistors.
5.5 Drain induced barrier lowering (DIBL)
5.5.1 Physical description
The drain current was derived assuming the gradual channel approximation which states that the change in the electric field along the channel direction is much smaller than the change along the vertical direction. This assumption allows to reduce the Poisson equation to a one dimensional differential equation depending only on the vertical direction. As a consequence, the charge density in silicon \(Q_{si}\) only depended on the vertical electric field at the surface of the silicon (just below the oxide). This approximation is no more valid for short-channel transistors, and a more thorough analysis accounting for the variation of the longitudinal field \(\mathcal{E}_x\) must be included in the calculation of \(Q_{si}\). This analysis allows to model the influence of the source and drain voltages on the channel surface potential which tends to be larger than what would be obtained from the long-channel model using the gradual channel approximation. This effect is called drain induced barrier lowering (DIBL) because it basically corresponds to the drain (source) voltage(s) lowering the potential barrier or increasing the surface potential in the channel, resulting in a drain current that is larger than what is obtained from the long-channel approximation.
The DIBL effect is illustrated in Figure 20 which plots the surface potential along the channel versus the normalized distance \(\xi=x/L\) for different transistor lengths and for \(V_S = 0\), \(V_D = 2\;V\) with a junction built-in voltage \(V_{bi} \cong 1\;V\). The corresponding surface potential obtained from the long-channel approximation is then \(\Psi_{sL} = 0.283\;V\). The green curve corresponds to a long-channel device (\(L = 10\;\mu m\)). It starts at the built-in voltage \(V_{bi}\) of about 1 V at the source and then immediately drops to the long-channel value \(\Psi_{sL}\). It then stays constant along the channel up to the drain where it jumps to \(V_{bi} + V_D = 3\;V\). For a shorter channel of \(L=0.5\;\mu m\), we already see the influence of the source and particularly the drain voltage on the value of the surface potential close to the source and drain junctions. The surface potential reaches the long-channel only in the middle of the channel. For an even shorter channel (\(L=0.2\;\mu m\)), the surface potential now does not even reach the long-channel value anymore. The current is then significantly larger than the one that would be predicted by the long-channel approximation, particularly in weak and moderate inversion.
DIBL has to be accounted for in short-channel device and we will show in the next Section how it can be modeled as a change of the threshold or the pinch-off voltage.
5.5.2 Modeling DIBL in the threshold or pinch-off voltage
Since DIBL increases the current as the length is reduced for a given set of terminal voltages, it has traditionally been modeled in compact models as a reduction of the threshold voltage according to [15] [2] [3] \[\begin{equation}\label{eqn:vt_dibl} V_T \cong V_{T0} -\sigma_d \cdot (V_D + V_S) \end{equation}\] where \(\sigma_d\) is a unitless parameter that has a strong dependence on the channel length according to [15] \[\begin{equation}\label{eqn:sigmad} \sigma_d = \frac{1}{2[\cosh(\xi) - 1]}, \end{equation}\] where \[\begin{equation} \xi \triangleq \frac{L}{2 L_c}. \end{equation}\] \(L_c\) is the characteristic length defined as [15] \[\begin{equation} L_c \triangleq \sqrt{\frac{\epsilon_{si} \, t_d}{C_{ox}}}, \end{equation}\] where \(t_d\) is an average value of the depletion thickness which is assumed to be constant. Note that for FDSOI, \(t_d\) would actually correspond to the silicon channel thickness. The scaling of \(\sigma_d\) with respect to \(\xi \triangleq L/(2 L_c)\) is plotted in Figure 21 together with the asymptotes given by \[\begin{equation}\label{eqn:dibl_sigmad_asymptotes} \sigma_d \cong \begin{cases} \frac{1}{\xi^2} = \left(\frac{2 L_c}{L}\right)^2 &\text{for $\xi \ll 1$}\\ e^{-\xi} &\text{for $\xi \gg 1$}. \end{cases} \end{equation}\] For \(L \ll 2 L_c\) (or \(\xi \ll 1\)), \(\sigma_d\) scales as \(1/L^2\), but for \(2 L_c \ll L\) (\(\xi \gg 1\)), \(\sigma_d\) decreases very fast. According to \(\eqref{eqn:vt_dibl}\), \(V_T\) decreases as the drain voltage increases and therefore the drain current in saturation will increase with \(V_D\) instead of staying constant. Similarly to CLM, DIBL also introduces an output conductance. Because the output conductance due to CLM scales as \(1/L\), for long-channel transistors, DIBL can be ignored so that the output conductance is mainly due to CLM. For this reason we will evaluate the impact of DIBL on the drain current and output conductance focusing on short-channel transistors.
In the EKV model, the DIBL effect can easily be included in the pinch-off voltage which is now redefined as [16] [17] \[\begin{equation} V_P' = V_P + \frac{\sigma_d}{n} \cdot (V_D+V_S) \end{equation}\] or in normalized form \[\begin{equation}\label{eqn:vpprime_def} v_p' = v_p + \frac{\sigma_d}{n} \cdot (v_d+v_s) = v_p + \Delta v_p, \end{equation}\] where \(\Delta v_p\) is the increase of the pinch-off voltage due to DIBL given by \[\begin{equation}\label{eqn:Dvp_def} \Delta v_p = \frac{\sigma_d}{n} \cdot (v_d+v_s). \end{equation}\] In addition of depending on the gate voltage, the pinch-off voltage including DIBL \(v_p'\) now depends also on the drain and source voltages \(v_d\) and \(v_s\). At a given gate and source voltages, if the drain voltage is increased, the pinch-off voltage \(v_p'\) also increases resulting in an increase of the drain current that can be observed from the linear to the saturation region.
Let’s now analyze the impact of DIBL on the drain current first without considering the effect of VS.
5.5.3 Impact of DIBL on the drain current without VS
In this section we will investigate the impact of DIBL on the charges and currents in strong inversion. In a first step, for the sake of clarity and simplicity, we will ignore the effect of velocity saturation (VS). Of course this is not correct because DIBL affects short-channel transistors for which velocity saturation cannot be ignored. The combined effects of DIBL and VS are examined in a separate Notebook.
Since DIBL can be modelled as a reduction of the threshold voltage due to \(v_s\) and \(v_d\), it basically will increase the drain current and shift the \(I_D\)-\(V_G\) transfer characteristic to the left. However it will introduce a non-zero output conductance in the \(I_D\)-\(V_D\) output characteristic. We will start analyzing the strong inversion case in the next Section.
5.5.3.1 Analysis in strong inversion without VS
We will start analyzing the impact of DIBL on the drain current in strong inversion and in the linear region, ignoring the effect of velocity saturation and CLM. The normalized drain current in strong inversion and in the linear region is given by \[\begin{equation}\label{eqn:id_if_ir} i_d = i_f - i_r. \end{equation}\] where the forward and reverse currents are given by \[\begin{align} i_f &= q_s^2,\label{eqn:id_qs_si}\\ i_r &= q_d^2. \end{align}\] The normalized source and drain charges in strong inversion including DIBL are now given by \[\begin{align} q_s &= \frac{v_p'-v_s}{2} = \tfrac{1}{2} \cdot \left[v_p - v_s + \frac{\sigma_d}{n} \cdot (v_d+v_s)\right]\\ &= \frac{v_p-v_s}{2} + \frac{\sigma_d}{n} \cdot \frac{v_d+v_s}{2} = q_{s,nodibl} + \frac{\Delta v_p}{2},\label{eqn:qs_vpprime_vs_vd}\\ q_d &= \frac{v_p'-v_d}{2} = \tfrac{1}{2} \cdot \left[v_p - v_d + \frac{\sigma_d}{n} \cdot (v_d+v_s)\right]\\ &= \frac{v_p-v_d}{2} + \frac{\sigma_d}{n} \cdot \frac{v_d+v_s}{2} = q_{d,nodibl} + \frac{\Delta v_p}{2}.\label{eqn:qd_vpprime_vs_vd} \end{align}\] where \(q_{s,nodibl}\) and \(q_{d,nodibl}\) are the source and drain charges without DIBL \[\begin{align} q_{s,nodibl} &= \frac{v_p-v_s}{2},\\ q_{d,nodibl} &= \frac{v_p-v_d}{2} \end{align}\] and \(\Delta v_p\) is given by \(\eqref{eqn:Dvp_def}\). The normalized source and drain charges are increased by \(\Delta v_p/2\) due to DIBL. This will obviously have an impact on the currents and transconductances. Notice that contrary to the long-channel case where \(q_s\) depends on \(v_p-v_s\) and \(q_d\) on \(v_p-v_d\), now both \(q_s\) and \(q_d\) depend on \(v_p\), \(v_s\) and \(v_d\).
The drain current in strong inversion can then be written as \[\begin{equation} \begin{split} i_d &= \left[v_p+\left(\frac{\sigma_d}{n}-\frac{1}{2}\right)\,v_d+\left(\frac{\sigma_d}{n}-\frac{1}{2}\right)\,v_s\right] \cdot \frac{v_d-v_s}{2} \\ &= \left[v_p-\frac{v_d+v_s}{2}+\frac{\sigma_d}{n}\,(v_d+v_s)\right] \cdot \frac{v_d-v_s}{2} \\ &= \left[v_p-\frac{v_d+v_s}{2}\right] \cdot \frac{v_d-v_s}{2} + \frac{\sigma_d}{n} \cdot \frac{v_d^2-v_s^2}{2} \\ &= i_{d,no\;dibl} + \frac{\sigma_d}{n} \cdot \frac{v_d^2-v_s^2}{2}. \end{split} \end{equation}\] where \[\begin{equation} i_{d,no\;dibl} \triangleq \left[v_p-\frac{v_d+v_s}{2}\right] \cdot \frac{v_d-v_s}{2} \end{equation}\] is the drain current in the linear region without DIBL. The drain current in the linear region including DIBL increases faster with \(v_d\) than without DIBL with the difference growing as \(v_d^2\).
If velocity saturation is ignored, saturation is reached when \(q_d=0\). We can find the saturation voltage \(v_{d_{sat}}\) defined as the drain voltage for which \(q_d=0\) which is given by \[\begin{equation}\label{eqn:vdsat_dibl} v_{d_{sat}} = \frac{v_p+\frac{\sigma_d}{n}\,v_s}{1-\frac{\sigma_d}{n}}. \end{equation}\] For \(v_s=0\), the saturation voltage is \(1/(1-\frac{\sigma_d}{n})\) larger than \(v_p\).
In saturation (i.e. for \(v_{d_{sat}}< v_d\)), \(i_r=0\) and the drain current is given by \[\begin{equation}\label{eqn:idsat_vd_si} \begin{split} i_{d_{sat}} &= i_f = q_s^2 = \left(\frac{v_p'-v_s}{2}\right)^2 = \tfrac{1}{4} \cdot \left[v_p-v_s+\frac{\sigma_d}{n} \cdot (v_d+v_s)\right]^2 \\ &= \tfrac{1}{4} \cdot (v_p-v_s)^2 + \frac{\sigma_d}{n} \cdot \frac{v_d+v_s}{2} \cdot \left[v_p-v_s+\frac{\sigma_d}{n} \cdot \frac{v_d+v_s}{2}\right]\\ &= i_{d_{sat},nodibl} + \frac{\Delta v_p}{2} \cdot \left[v_p-v_s+\frac{\Delta v_p}{2}\right]. \end{split} \end{equation}\] where \[\begin{equation} i_{d_{sat},nodibl} \triangleq \left(\frac{v_p-v_s}{2}\right)^2 \end{equation}\] is the drain current in saturation without DIBL. Because of DIBL, the drain current in saturation increases quadratically with \(v_d\). Since usually \(\sigma_d \ll 1\), \(v_p-v_s \gg \sigma_d/n\;(v_d+v_s)/2\) and the drain current in saturation is approximately given by \[\begin{equation} i_{d_{sat}} \cong i_{d_{sat},nodibl} + \frac{\sigma_d}{n} \cdot \frac{v_d+v_s}{2} \cdot (v_p-v_s) = i_{d_{sat},nodibl} + \frac{\Delta v_p}{2} \cdot (v_p-v_s), \end{equation}\] which grows now linearly with \(v_d\).
The normalized charges \(q_s\) and \(q_d\) are plotted versus \(v_d\) in Figure 22 for \(v_s=0\), \(n=1.3\) and \(\sigma_d=0.217\) for which the normalized saturation voltage is increased from \(v_p=50\) to \(v_{d_{sat}}=60\). We see that \(q_s\) increases with respect to \(v_d\) instead of staying constant as it would for the long-channel case without DIBL. On the other hand, \(q_d\) decreases until it reaches zero at the onset of saturation. We observe that, because of DIBL, the saturation voltage given by \(\eqref{eqn:vdsat_dibl}\) is higher than \(v_p\). Note that \(\sigma_d=0.217\) is already a fairly large value that has been used in Figure 22 to increase the saturation voltage by 10 \(U_T\).
The normalized forward, reverse and drain currents are plotted versus \(v_d\) in Figure 23 for the same value \(\sigma_d=0.217\). We see that the forward current increases with respect to \(v_d\) instead of remaining constant as it would in the long-channel case without DIBL. The reverse current is also slightly higher than the reverse current without DIBL. It decreases until reaching zero at \(v_d=v_{d_{sat}}\). The drain current is larger than its value without DIBL and continues to increase in saturation for \(v_{d_{sat}}<v_d\).
5.5.3.2 Analysis in weak inversion without VS
The forward and reverse currents in weak inversion are given by \[\begin{align} i_f &= q_s,\\ i_r &= q_d, \end{align}\] with the normalized source and drain charges \(q_s\) and \(q_d\) given by \[\begin{align} q_s &= e^{v_p'-v_s} = e^{v_p-v_s+\frac{\sigma_d}{n} \cdot (v_d+v_s)} = e^{\frac{\sigma_d}{n} \cdot (v_d+v_s)} \cdot e^{v_p-v_s} = e^{\Delta v_p} \cdot q_{s,nodibl},\\ q_d &= e^{v_p'-v_d} = e^{v_p-v_d+\frac{\sigma_d}{n} \cdot (v_d+v_s)} = e^{\frac{\sigma_d}{n} \cdot (v_d+v_s)} \cdot e^{v_p-v_d} = e^{\Delta v_p} \cdot q_{d,nodibl}, \end{align}\] where \(q_{s,nodibl}\) and \(q_{d,nodibl}\) are the source and drain charges without DIBL \[\begin{align} q_{s,nodibl} &= e^{v_p-v_s},\\ q_{d,nodibl} &= e^{v_p-v_d}. \end{align}\]
DIBL has a significant effect on the source and drain charges since they are multiplied by \(exp[\Delta v_p]\).
The drain current in weak inversion is then given by \[\begin{equation} i_d = i_f-i_r = q_s-q_d = e^{\frac{\sigma_d}{n} \cdot (v_d+v_s)} \cdot \left[e^{v_p-v_s}-e^{v_p-v_d}\right] = e^{\Delta v_p} \cdot i_{d,nodibl} \end{equation}\] The drain current in weak inversion is multiplied by \(exp[\Delta v_p]\). The normalized forward, reverse and drain currents are plotted versus \(v_d\) in Figure 24 in weak inversion for \(\sigma_d=0.15\). We see that the forward current \(i_f\) and drain current \(i_d\) increase in saturation because of DIBL. The impact of DIBL on the drain current ignoring VS is strong, significantly degrading the output characteristic for short-channel devices.
5.5.3.3 Analysis in all regions of inversion without VS
The normalized forward and reverse currents in all modes of inversion but ignoring VS are given by \[\begin{align} i_f &= q_s^2+q_s,\\ i_r &= q_d^2+q_d. \end{align}\] The relation between charges and voltages are given by \[\begin{align} v_p'-v_s &= 2 q_s + \ln(q_s),\label{eqn:qs_dibl_all_regions}\\ v_p'-v_d &= 2 q_d + \ln(q_d), \end{align}\] with \(v_p'\) given by \(\eqref{eqn:vpprime_def}\).
The normalized forward, reverse and drain currents are plotted versus \(v_d\) in Figure 25 in moderate inversion for \(\sigma_d=0.15\). We see that the forward current \(i_f\) and drain current \(i_d\) increase in saturation because of DIBL but the impact is less than in weak inversion for the same value of \(\sigma_d\).
We see that DIBL can have a dramatic impact on the output characteristic in weak inversion where the current can increase exponentially with \(v_d\). The above DIBL model valid in all regions of inversion is checked against measurements in the next Section.
5.5.3.4 Experimental validation
The above model of DIBL is validated on a short nMOS transistor from a 28 nm bulk CMOS technology. Figure 26 shows the \(I_D\)-\(V_D\) characteristic measured in strong inversion. We can observe that the simple DIBL model can fit the measurements very well provided an additional scaling parameter \(i_{scale}\) is added. This additional parameter is needed to compensate for the fact that the sEKV parameter \(I_{spec}\) has been extracted at the highest drain voltage \(V_D=1.1\,V\) (\(V_D=42.5\)). It also accounts for the current reduction in saturation due to VS which is not accounted for in this simple model. The corresponding output conductance are shown in Figure 27}. We can observe that the model predicts an increase of \(g_{ds}\) wrt \(v_d\) which is actually not observed in the measured data. This is due to the fact that according to \(\eqref{eqn:idsat_vd_si}\), the drain current in saturation increases with the square of \(v_d\) and hence the output conductance with \(v_d\). A better model of the output conductance will be derived in the Notebook dedicated to the output conductance.
Figure 28 shows the \(I_D\)-\(V_D\) characteristic measured in weak inversion. We can see the very strong impact that DIBL can have on short transistors in weak inversion. Note that such an output characteristic is almost unusable for analog circuit. For this reason a non-minimum channel length should be chosen when biasing the transistor in weak inversion. Things improve slightly when moving to moderate inversion as shown in Figure 29. However, the output conductance is still huge and the minimum length device will perform poorly in an analog circuit when biased in moderate inversion. Again, this can be circumvented by choosing a non-minimum length
5.5.4 Impact of DIBL on the transconductances in saturation without VS
5.5.4.1 General expression valid in saturation from weak to strong inversion
The gate transconductance in saturation is given by \[\begin{equation} g_{m_{sat}} = \frac{\partial i_{d_{sat}}}{\partial v_g} = \frac{1}{n} \cdot \frac{\partial i_{d_{sat}}}{\partial v_p}. \end{equation}\] Without VS, in saturation, \(i_{d_{sat}} \cong i_f\) and hence \[\begin{equation} g_{m_{sat}} = \frac{1}{n} \cdot \frac{\partial i_f}{\partial v_p} = \frac{1}{n} \cdot \frac{\partial i_f}{\partial q_s} \cdot \left(\frac{\partial v_p}{\partial q_s}\right)^{-1}. \end{equation}\] with \[\begin{equation} i_f = q_s^2+q_s. \end{equation}\] The normalized source charge \(q_s\) is related to \(v_p\), \(v_s\) and \(v_d\) according to \[\begin{equation} v_p'-v_s = 2 q_s + \ln(q_s) \end{equation}\] with \[\begin{equation} v_p' = v_p + \Delta v_p. \end{equation}\] where \(\Delta v_p\) is given by \(\eqref{eqn:Dvp_def}\). The pinch-off voltage is then given by \[\begin{equation} v_p = v_s - \Delta v_p + 2 q_s + \ln(q_s). \end{equation}\] We therefore have \[\begin{equation} \frac{\partial i_f}{\partial q_s} = 2 q_s+1 \end{equation}\] and \[\begin{equation} \frac{\partial v_p}{\partial q_s} = 2 + \frac{1}{q_s} = \frac{2 q_s+1}{q_s}. \end{equation}\] The gate transconductance is then given by \[\begin{equation}\label{eqn:gmsat_dibl} g_{m_{sat}} = \frac{q_s}{n}. \end{equation}\]
The source transconductance is given by \[\begin{equation} g_{ms} = -\frac{\partial i_{d_{sat}}}{\partial v_s} \cong -\frac{\partial i_f}{\partial v_s} = -\frac{\partial i_f}{\partial q_s} \cdot \frac{\partial q_s}{\partial v_s} = -\frac{\partial i_f}{\partial q_s} \cdot \left(\frac{\partial v_s}{\partial q_s}\right)^{-1}. \end{equation}\] The source voltage including DIBL is given by \[\begin{equation} v_s = \frac{1}{1-\frac{\sigma_d}{n}} \cdot \left[v_p+\frac{\sigma_d}{n}\,v_d-2 q_s-\ln(q_s)\right] \end{equation}\] from which we get \[\begin{equation} \frac{\partial v_s}{\partial q_s} = -\frac{1}{1-\frac{\sigma_d}{n}} \cdot \frac{2 q_s+1}{q_s}. \end{equation}\] The source transconductance in strong inversion is then given by \[\begin{align} g_{ms} = \left(1-\frac{\sigma_d}{n}\right) \cdot q_s. \end{align}\] The ratio \(g_{ms}/g_m\) in strong inversion and saturation is no more equal simply to \(n\) but \[\begin{equation} \frac{g_{ms}}{g_m} = n\,\left(1-\frac{\sigma_d}{n}\right) = n - \sigma_d, \end{equation}\] which is lower than \(n\).
5.5.4.2 Analysis in strong inversion and saturation
We assume that \(v_{d_{sat}} < v_d\) where the saturation voltage \(v_{d_{sat}}\) is slightly larger then \(v_p\) according to \(\eqref{eqn:vdsat_dibl}\). Using the general derivation, the gate transconductance in strong inversion and saturation without VS is then given by \[\begin{equation}\label{eqn:gmsat_dibl_si_novs} g_{m_{sat}} = \frac{q_s}{n} = \frac{1}{n} \cdot \left[\frac{v_p-v_s}{2} + \frac{\sigma_d}{n} \cdot \frac{v_d+v_s}{2}\right] = g_{m_{sat},nodibl} + \Delta g_{m_{sat},dibl}, \end{equation}\] where \(g_{m_{sat},nodibl}\) is the gate transconductance in strong inversion and saturation without DIBL \[\begin{equation} g_{m_{sat},nodibl} = \frac{1}{n} \cdot \frac{v_p-v_s}{2} \end{equation}\] and \(\Delta g_{m_{sat}}\) is the transconductance increase due to DIBL \[\begin{equation} \Delta g_{m_{sat},dibl} = \frac{\sigma_d}{n^2} \cdot \frac{v_d+v_s}{2} = \frac{\Delta v_p}{2 n}. \end{equation}\] The impact of DIBL on the gate transconductance is an increase \(\Delta g_{m_{sat}} = \Delta v_p/(2 n)\).
Using the above general derivation, the source transconductance in strong inversion and saturation is then given by \[\begin{equation} g_{ms} = \left(1-\frac{\sigma_d}{n}\right) \cdot q_s = \frac{v_p-v_s}{2} + \frac{\sigma_d}{n} \cdot \left[\left(1-\frac{\sigma_d}{n}\right)\,\frac{v_d+v_s}{2} - \frac{v_p-v_s}{2}\right] = g_{ms,nodibl} + \Delta g_{ms}, \end{equation}\] where \(g_{ms,nodibl}\) is the source transconductance without DIBL \[\begin{equation} g_{ms,nodibl} = \frac{v_p-v_s}{2} \end{equation}\] and \(\Delta g_{ms}\) is the increase in the source transconductance due to DIBL \[\begin{equation} \Delta g_{ms} = \frac{\sigma_d}{n} \cdot \left[\left(1-\frac{\sigma_d}{n}\right)\,\frac{v_d+v_s}{2} - \frac{v_p-v_s}{2}\right] = \frac{\sigma_d}{n} \cdot \left[\left(1-\frac{\sigma_d}{n}\right) \cdot \frac{v_d-v_{d_{sat}}}{2} + v_s\right]. \end{equation}\] The source transconductance in saturation including DIBL is increased by \(\Delta g_{ms}\).
5.5.4.3 Analysis in weak inversion and saturation
Because of DIBL, the normalized source charge \(q_s\), forward current \(i_f\) and drain current \(i_d\) are all multiplied by \(exp[\Delta v_p]\). Similarly, the gate transconductance in weak inversion and saturation is also multiplied by the factor \[\begin{equation} g_{m_{sat}} = \frac{q_s}{n} = \frac{i_f}{n} = e^{\Delta v_p} \cdot g_{m_{sat},nodibl}, \end{equation}\] where \(g_{m_{sat},nodibl}\) is the gate transconductance without DIBL.
The source transconductance in saturation including DIBL is multiplied by \((1-\sigma_d/n) \cdot exp[\Delta v_p]\). \[\begin{equation} g_{ms} = \left(1-\frac{\sigma_d}{n}\right) \cdot e^{\Delta v_p} \cdot g_{ms,nodibl}. \end{equation}\]
5.5.5 Output conductance in saturation due to DIBL without VS
5.5.5.1 General expression
From Figure 23 we see that the drain current in saturation does no more remain constant but increases with \(v_d\) because of DIBL. This is due to the forward current \(i_f\) which now increases with \(v_d\) due to DIBL instead of remaining constant. The output conductance is hence no more zero, which obviously affects the self-gain \(G_m/G_{ds}\). It is therefore important to be able to predict \(G_{ds}\) (or its normalized form \(g_{ds}\)) as accurately as possible.
Similarly to what was done in Section 5.4.3, we will consider \(v_s\) constant. The output conductance is then defined by \(\eqref{eqn:gds_sat_def}\). In saturation, the change of the forward current and hence of the drain current due to a change of the \(v_d\) voltage is due to DIBL through an increase of the pinch-off voltage \(v_p'\). We can then write \[\begin{equation} g_{ds} = \frac{\partial i_{d_{sat}}}{\partial v_d} = \frac{\partial i_{d_{sat}}}{\partial v_p'} \cdot \frac{\partial v_p'}{\partial v_d}. \end{equation}\] where \(v_p'\) is given by \(\eqref{eqn:vpprime_def}\). The derivative \(\partial v_p'/\partial v_d\) is therefore simply equal to \[\begin{equation} \frac{\partial v_p'}{\partial v_d} = \frac{\sigma_d}{n}. \end{equation}\] On the other hand, the derivative \(\partial i_{d_{sat}}/\partial v_p'\) is related to the transconductance according to \[\begin{equation} \frac{\partial i_{d_{sat}}}{\partial v_p'} = \frac{\partial i_{d_{sat}}}{\partial v_p} = \frac{\partial i_{d_{sat}}}{\partial v_g} \cdot \frac{\partial v_g}{\partial v_p} = n \cdot g_{m_{sat}}. \end{equation}\] The output conductance in saturation is therefore proportional to the gate transconductance in saturation \[\begin{equation}\label{eqn:gds_gmsat} g_{ds} = \sigma_d \cdot g_{m_{sat}}. \end{equation}\] Note that the above derivation is also valid when including VS as long as the transconductance expression accounts for both DIBL and VS. Note also that the above derivation is mostly valid in strong inversion. Indeed, the reverse current of a long-channel transistor in weak inversion is a function of \(v_d\) also in saturation, but usually the later can be neglected for short-channel devices compared to the contribution of DIBL.
The transistor self-gain due to DIBL without accounting for CLM and VS is then simply \[\begin{equation} A_{dc} = \frac{G_m}{G_{ds}} = \frac{g_m}{g_{ds}} = \frac{1}{\sigma_d}. \end{equation}\]
From the general expression of the gate transconductance \(\eqref{eqn:gmsat_dibl}\) accounting for DIBL (but not VS), we can write \[\begin{equation} g_{ds} = \frac{\sigma_d}{n} \cdot q_s. \end{equation}\]
The output conductance due to DIBL can then easily be calculated from the expression of the gate transconductance in saturation derived above.
Similarly to what is done for CLM, we can define a DIBL voltage as \[\begin{equation}\label{eqn:vdibl_novs} \frac{1}{v_{dibl}} = \frac{g_{ds}}{i_{d_{sat}}} = \sigma_d \cdot \frac{g_{m_{sat}}}{i_{d_{sat}}} = \frac{\sigma_d/n}{q_s}. \end{equation}\]
We see that \(1/v_{dibl}\) is proportional to the normalized \(G_m/I_D\) function in saturation which should include both DIBL and VS. Now, \(i_{d_{sat}}\) is nothing else than the inversion coefficient \(IC\) and hence \[\begin{equation} \frac{1}{v_{dibl}} = \frac{g_{ds}}{i_{d_{sat}}} = \frac{\sigma_d}{n} \cdot \frac{g_{ms}}{IC}, \end{equation}\] where \(g_{ms}\) is the normalized source transconductance including VS and DIBL.
To use the relation between the output conductance \(g_{ds}\) and the gate transconductance in saturation \(g_{m_{sat}}\) given by \(\eqref{eqn:gds_gmsat}\), we would need to derive the expression of the gate transconductance in strong inversion and saturation including both DIBL and VS. This is done the in the dedicated Notebook. Here we only will account for DIBL ignoring VS.
5.5.5.2 Analysis in strong inversion and saturation
From \(\eqref{eqn:gmsat_dibl_si_novs}\) we get the output conductance in strong inversion and saturation due to DIBL ignoring VS \[\begin{equation}\label{eqn:gds_dibl_si_novs} g_{ds} = \sigma_d \cdot g_{m_{sat}} = \frac{\sigma_d}{n} \cdot \left[\frac{v_p-v_s}{2} + \frac{\sigma_d}{n} \cdot \frac{v_d+v_s}{2}\right] = \frac{\sigma_d}{n} \cdot \left[\frac{v_p-v_s}{2} + \frac{\Delta v_p}{2}\right]. \end{equation}\] We see from \(\eqref{eqn:gds_dibl_si_novs}\) that the output conductance increases with \(v_p-v_s\) and also depends on \(v_d\). Usually \(\sigma_d \ll 1\) and hence \(v_p-v_s \gg \Delta v_p\). \(\eqref{eqn:gds_dibl_si_novs}\) can therefore be approximated by \[\begin{equation} g_{ds} \cong \frac{\sigma_d}{n} \cdot \frac{v_p-v_s}{2}. \end{equation}\]
5.5.5.3 Analysis in weak inversion and saturation
In weak inversion, the drain charge does not vanish to zero but decreases exponentially wrt \(v_d\). This gives a finite output conductance even without DIBL. If we account for this and add the effect of DIBL we get \[\begin{equation} g_{ds} = e^{\Delta v_p} \cdot e^{v_p} \cdot \left[\frac{\sigma_d}{n}\,e^{-v_s} + \left(1+\frac{\sigma_d}{n}\right) \cdot e^{-v_d}\right] \cong \frac{\sigma_d}{n} \cdot e^{\Delta v_p} \cdot e^{v_p-v_s}. \end{equation}\]
5.5.6 Impact of DIBL on the transconductances in saturation including VS
The derivation of the transconductances including both effects of DIBL and VS is tedious and is not presented here. The detailed analyisis given in the Notebook dedicated to DIBL shows that a good and simple approximation of the normalized gate transcondcutance \(g_m\) versus the inversion coefficient that is valid in all regions of inversion is obtained by simply reusing the short-channel expression of \(g_m\) accounting for VS only and replacing \(\lambda_c\) by \(\lambda_{dibl}\) \[\begin{equation}\label{eqn:gmsat_ic_vs_dibl_all_regions} g_{m_{sat}} = \frac{1}{n} \cdot \frac{\sqrt{4IC+1+(\lambda_{dibl}\,IC)^2}-1}{2+\lambda_{dibl}^2\,IC}, \end{equation}\] with \[\begin{equation} \frac{1}{\lambda_{dibl}} \triangleq \frac{1}{\lambda_c} + \frac{\Delta v_p}{2}. \end{equation}\]
This approximation is plotted in Figure 30 by the blue line which is very close to the full expression corresponding to the red dots. For \(IC \gg 1/\lambda_{dibl}\), \(\eqref{eqn:gmsat_ic_vs_dibl_all_regions}\) tends to \(1/\lambda_{dibl}\) which is higher that \(1/\lambda_c\) because of DIBL.
Finally, the normalized \(G_m/I_D\) characteristic \(n \cdot g_{m_{sat}}/IC\) is plotted versus \(IC\) in Figure 31. We see that the weak inversion asymptote remains at unity, while the strong inversion asymptote is shifted to higher inversion coefficient because of DIBL. The intersection of the strong inversion asymptote with the horizontal unity line is therefore shifted from \(1/\lambda_c\) to \(1/\lambda_{dibl}\) because of DIBL. We can reuse \(\eqref{eqn:gmsat_ic_vs_dibl_all_regions}\) to approximate the normalized \(G_m/I_D\) characteristic as \[\begin{equation}\label{eqn:gmsid_ic_vs_dibl_all_regions} \frac{n \cdot g_{m_{sat}}}{IC} = \frac{\sqrt{4i_{d_{sat}}+1+(\lambda_{dibl}\,IC)^2}-1}{IC \cdot (2+\lambda_{dibl}^2\,IC)}, \end{equation}\] which is plotted in Figure 31 as the dashed red line which is close to the red line corresponding to the full expression.
The fact that we can use the expression of the normalized gate transconductance \(g_m\) and of the normalized \(G_m/I_D\) including the effect of VS only and account for the additional DIBL effect by simply replacing \(\lambda_c\) by a slighlty higher value \(\lambda_{dibl}\) explains why we get very good fits of the transconductances and the normalized \(G_m/I_D\). The value extracted for \(\lambda_c\) actually corresponds to \(\lambda_{dibl}\) and hence also includes the effect of DIBL for short-channel transistors.
This Notebook proposes a more accurate output conductance model that is valid in saturation from weak to strong inversion and covers short to long-channel transistors. It also tries to answer the question: what is the minimum transistor length for avoiding a strong degradation of the intrinsic gain [18] ?
5.6 Short-channel effects on thermal noise
Noise represents the ultimate lower limit of signal resolution in analog signal processing. For this reason it is key for the circuit designer to evaluate the noise of analog circuits whether at low-frequency or at RF. In CMOS circuits, the most important contributor to noise is the MOSFET. At RF, the noise in linear circuits is essentially due to the transistors white noise. At low-frequency the MOSFET noise is dominated by flicker noise. However, the latter can be strongly reduced using circuit techniques such as chopper stabilization, autozero or correlated double (or multiple) sampling which are presented in Chapter ?? [19] [20]. The remaining noise is then the white noise which is either thermal noise if the transistor is biased in strong inversion, or shot noise if the transistor is biased in weak inversion, or a mix if the transistor is biased in the moderate inversion region [1].
The transistor white noise is characterized by its transconductance \(G_m\) and the thermal noise excess factor \(\gamma_n\), which is defined in ???. Since the transconductance also sets the gain and the bandwidth, it is essential for the designer to find the right \(G_m\) resulting from the trade-off between gain, bandwidth and noise. To this purpose the designer can use various figures-of-merit (FoMs) helping exploring the design space. The thermal noise excess factor \(\gamma_n\) is an essential FoM for the design of low-noise circuits since it evaluates how much noise is produced for a given transconductance. It can hence be used to derive the required transconductance needed for achieving a given input-referred noise or noise figure for a given thermal noise excess factor \(\gamma_n\). The \(G_m/I_D\) is another FoM that evaluates how much transconductance you get for a given current. It can then be used to derive the required bias current after having chosen the most appropriate region of operation using the inversion coefficient [21] [8].
As shown in ??? that for a long-channel transistor the thermal noise excess factor \(\gamma_n\) is close to unity and shows only a slight bias dependence. However, in advanced technologies, short channel devices biased in strong inversion show a \(\gamma_n\) that can become larger than one. Since the input-referred noise resistance is proportional to \(\gamma_n/G_m\), if \(\gamma_n\) increases, the transconductance has to be increased by the same amount in order to maintain the same input-referred noise resistance (or noise figure). This increase in \(G_m\) unavoidably results in an increase of the bias current and of the power consumption. It is therefore crucial for the designer to have a sufficiently accurate model of the thermal noise excess factor valid over a wide range of current (or inversion coefficient).
The long-channel thermal noise model derived in Chapter ?? assumed that the mobility was constant along the channel and that the channel length was sufficiently long so that velocity saturation and channel length modulation could be neglected. These assumptions are obviously not valid anymore for short-channel devices where velocity saturation and channel length modulation effects have to be accounted for. Mobility reduction due to the vertical field also greatly influences the thermal noise and has also to be included. Finally, the increase of the carrier temperature at high longitudinal field also needs to be accounted for. The impact of all these effects on short-channel transistor is described in details in [22] [23] [24] [25]. In this section we will derive a simple empirical model of the thermal noise excess factor for short-channel transistors in terms of the most important design parameter, namely the inversion coefficient.
5.6.1 Empirical model of the thermal noise excess factor for short-channel transistors
The thermal noise excess factor \(\gamma_n\) of short-channel transistor can increase significantly because of various short-channel effects like VS and CLM [22] [23] [24] [25]. The behavior of \(\gamma_n\) with respect to the inversion coefficient can be modeled by a simple empirical model given by [26] \[\begin{equation}\label{eqn:gammansat_empirical} \gamma_{n_{sat}} \cong \gamma_{nwi} \cdot (1 + \alpha_n \cdot IC). \end{equation}\] where \(\alpha_n\) is used as a fitting parameter but can be related to the velocity saturation parameter \(\lambda_c\) according to \[\begin{equation} \alpha_n = \frac{n}{2} \cdot \lambda_c^2. \end{equation}\] This empirical model has been validated on 5 different technologies from 240nm down to 40 nm. The empirical model \(\eqref{eqn:gammansat_empirical}\) is compared to measured data in Figure 32 after extraction of parameters \(\gamma_{nwi}\) and \(\alpha_n\) by curve fitting. We can extract the corresponding VS parameter according to \[\begin{equation}\label{eqn:lambdac_ext} \lambda_c = \sqrt{\frac{2 \alpha_n}{n}}. \end{equation}\]
The fitting parameters \(\gamma_{nwi}\) and \(\alpha_n\), the imposed slope factor \(n\) and the corresponding extracted value of \(\lambda_c\) are presented in Table 4. Figure 33 shows that \(\alpha_n\) is actually scaling as \(/1/L\).
| Techno | \(\gamma_{{nwi}}\) | \(\alpha_n\) | \(n\) | \(\lambda_c\) |
|---|---|---|---|---|
| 240nm | 0.837034 | 0.0138037 | 1.3 | 0.135665 |
| 180nm | 0.952055 | 0.0177346 | 1.3 | 0.153773 |
| 120nm | 1.26136 | 0.0216531 | 1.3 | 0.169914 |
| 100nm | 1.26643 | 0.0259371 | 1.3 | 0.185965 |
| 40nm | 1.0053 | 0.0679447 | 1.45 | 0.306132 |
5.7 The simplified EKV model
The simplified EKV mode (sEKV) correspnds to the normalized drain current in saturation given by \(\eqref{eqn:idsat_qs_mod1}\) \[\begin{equation}\label{eqn:sekv_ic_qs} IC = \frac{2(q_s^2+q_s)}{1+\sqrt{1+\lambda_c^2\,(q_s^2+q_s)}}, \end{equation}\] which is completed with the voltage-charge relation giving the normalized saturation voltage \(v_p-v_s\) in terms of the source charge \(q_s\) given by [1]} \[\begin{equation}\label{eqn:sekv_vps_qs} v_p-v_s = 2q_s + \ln(q_s), \end{equation}\] where \[\begin{equation} v_p = \frac{v_g-v_{t0}}{n}. \end{equation}\]
The inversion coefficient given by \(\eqref{eqn:sekv_ic_qs}\) can actually be solved to express \(q_s\) as a function of \(IC\) leading to \[\begin{equation}\label{eqn:sekv_qs_ic} q_s = \tfrac{1}{2}\,\left(\sqrt{4IC+1+(\lambda_c\,IC)^2}-1\right). \end{equation}\] which can then be replaced in \(\eqref{eqn:sekv_vps_qs}\) to obtain an expression of the saturation voltage \(v_p-v_s\) in terms of \(IC\). Unfortunately, the resulting equation cannot be inverted to express the inversion coefficient in terms of the saturation voltage \(v_p-v_s\). This is actually not a problem when we use \(IC\) as the main design parameter from which we can then compute the saturation voltage using \(\eqref{eqn:sekv_qs_ic}\) and \(\eqref{eqn:sekv_vps_qs}\).
The simplified EKV model only requires four parameters to fit the \(I_D\)-\(V_G\) transfer characteristic, namely:
- the slope factor \(n\),
- the specific current per square \(I_{spec\Box}\),
- the threshold voltage \(V_{T0}\) and
- the velocity saturation parameter \(\lambda_c\) (or \(L_{sat}\)).
| Type | \(n\) | \(I_{spec\Box}\) [nA] | \(V_{T0}\) [V] | \(L_{sat}\) [nm] |
|---|---|---|---|---|
| n-channel | 1.1 - 1.5 | 850 | 0.4 - 0.55 | 15 - 25 |
| p-channel | 1.1 - 1.5 | 350 | 0.35 - 0.5 | 15 - 25 |
The methodology to extract these parameters from measured data is sketched in a specialized Notebook. Typical values for these parameters for a 28 nm bulk CMOS process are given in Table 5.
Note that the sEKV model does not include the effect of mobility reduction due to the vertical field (MRV). The reason is that because of voltage scaling the gate voltage has been reduced considerably making MRV less important. However, for older technologies it can be shown that it can actually be covered to a certain extent by the VS parameter \(\lambda_c\).
Despite the very few number of parameters, the simplified EKV model can perfectly match data even from advanced CMOS processes as will be shown below.
5.7.1 Bulk technologies
The \(IC\) versus \(V_G\)-\(V_{T0}\) transfer characteristics are plotted in Figure 34 and compared to measurements made on wide and minimal length transistors from three different bulk CMOS processes, namely a 40 nm and two different 28 nm processes. Although the drain current is measured by sweeping the gate voltage, the sEKV model is calculated from the measured current by first normalizing it to the specific current for each transistor to get the inversion coefficient, from which the overdrive voltage is computed using \(\eqref{eqn:sekv_qs_ic}\) and \(\eqref{eqn:sekv_vps_qs}\). Despite the very few number of parameters, the simple model fits the measurements very well over more than 6 decades of current. Note that the extraction of the parameters \(I_{spec}\) and \(L_{sat}\) is done for several different geometries (in particular different length) illustrating the rather good scalability of the simplified model. Notice that the measured points and analytical models of the \(W=108\mu m\), \(L=30 nm\) (red circles) and \(W=108\mu m\), \(L=40 nm\) (green squares) transistors almost fall on top of each other, indicating that the normalization process almost completely strips off the technology dependence. The difference with the \(W=3\mu m\), \(L=30 nm\) (blue diamond) characteristic is due to a slightly larger value of \(\lambda_c\). In other words, the four parameters almost fully characterize the technology at least for the transfer characteristics in saturation and in the regions of operation used for analog circuit design.
The most important small-signal parameter is without doubt the gate transconductance \(G_m\). Remember that since in the EKV model the voltages are all referred to the bulk, we can define two other transconductances: the source transconductance \(G_{ms} \triangleq -\partial I_D/\partial V_S\) and the drain transconductance \(G_{md} \triangleq \partial I_D/\partial V_D\) [1]. Note that \(G_{md}\) should not be confused with the output conductance \(G_{ds}\). In saturation \(G_{md}=0\) and \(G_{ms}=n \cdot G_m\).
The normalized source transconductance in saturation \(G_{ms}\) is given by \(\eqref{eqn:gmssat_ic_mod1_new}\), which is repeated here for convenience \[\begin{equation*} g_{ms} \triangleq \frac{G_{ms}}{G_{spec}} = \frac{n \cdot G_m}{G_{spec}} = \frac{\sqrt{4IC+1+(\lambda_c\,IC)^2}-1}{2+\lambda_c^2\,IC}, \end{equation*}\] where \(G_{spec} \triangleq I_{spec}/U_T = 2n\beta U_T\) with \(\beta = \mu_0 C_{ox} W/L\). \(G_{ms}\) is plotted versus \(IC\) in Figure 35 and favorably compares to measurements obtained from the derivative of the characteristics shown in Figure 34 over a very wide range of bias (more than 4 decades of current). Note that for short-channel devices in strong inversion, the \(I_D\)-\(V_G\) transfer characteristic becomes a linear function of the gate voltage as illustrated in Figure 34 and hence the gate transconductance becomes independent of the drain current or the inversion coefficient and saturates to \[\begin{equation*} g_{ms} \cong \frac{1}{\lambda_c} = \frac{L}{L_{sat}}. \end{equation*}\] The source transconductance also becomes independent of the length and only depends on \(W\) and \(v_{sat}\) according to \(\eqref{eqn:Gmssat_si}\) \[\begin{equation*} G_{ms} \cong \frac{G_{spec}}{\lambda_c} = n W C_{ox} v_{sat}. \end{equation*}\]
Instead of increasing as \(\sqrt{IC}\), as it does for long-channel devices, for short-channel transistor with heavy velocity saturation, the normalized source transconductance \(G_{ms}\) saturates to \(1/\lambda_c\). The inverse of the velocity saturation parameter \(\lambda_c\) is therefore a key parameter since it gives the maximum normalized transconductance that can be achieved for a short-channel device in a given technology.
The transconductance efficiency \(G_m/I_D\), sometimes also called the current efficiency, is one of the most important FoM for low-power analog circuit design. It is a measure of how much transconductance is produced for a given bias current and is a function of \(IC\). The transconductance efficiency (or its inverse) appears in many expressions related to the optimization of analog circuits. In normalized form, the transconductance efficiency is defined as the actual transconductance obtained at a given \(IC\) with respect to the maximum transconductance \(G_m = I_D/(n\,U_T)\) reached in weak inversion and is given by \(\eqref{eqn:gmid_ic_mod1}\) which is repeated here for convenience \[\begin{equation}\label{eqn:sekv_gmid_ic} \frac{g_{ms}}{IC} = \frac{G_{ms} U_T}{I_D} = \frac{G_m n\,U_T}{I_D} = \frac{\sqrt{4IC+1+(\lambda_c\,IC)^2}-1}{IC\,(2+\lambda_c^2\,IC)} = \begin{cases} 1 &\textsf{in WI and sat.}\\ \dfrac{1}{\lambda_c IC} &\textsf{in SI and sat.} \end{cases} \end{equation}\] The normalized transconductance efficiency given by \(\eqref{eqn:sekv_gmid_ic}\) is compared to measurements in Figure 36 for the same devices shown in Figure 34 and Figure 35. Despite the normalized \(G_m n\,U_T/I_D\) only requires one parameter (\(\lambda_c\) or \(L_{sat}\)), the model fits very well to the data over more than 5 decades of \(IC\).
5.7.2 FDSOI technologies
The sEKV model was originally developed for the bulk MOS transistors. However, it can easily be extended to FDSOI process by making the threshold voltage depend on the back-gate voltage \(V_B\) [27]. The sEKV model has been successfully validated on a 28 nm FDSOI process [27]. After a proper parameter extraction, we get the \(I_D\)-\(V_G\) characteristic shown in Figure 37 demonstrating a good fit of the \(I_D\)-\(V_G\) characteristic in saturation for three different gate length ranging from \(L=300\,nm\) down to \(80\,nm\) and \(30\,nm\).
The normalized source transconductance \(g_{ms}\) is plotted versus \(IC\) in Figure 38 for the same devices than in Figure 37. We see that for the short-channel devices with \(L=80\,nm\) and \(L=30\,nm\), \(g_{ms}\) saturates to \(1/\lambda_c\). On the other hand the \(g_{ms}\) of the long-channel transistor with \(L=300\,nm\) continues to increase as \(\sqrt{IC}\). We also see that for the short devices, \(g_{ms}\) decreases at high \(IC\). This is the effect of mobility reduction due to the vertical field which has not been accoounted for in sEKV.
The normalized transconductance efficiency \(g_{ms}/IC\) is plotted versus \(IC\) for the same devices in Figure 39. We clearly see the strong impact of velocity saturation on the short-channel devices making \(g_{ms}/IC\) decrease sharply as \(1/(\lambda_c\,IC)\) in strong inversion. We also see some deviations for the short-channel devices at high \(IC\) due to mobility reduction due to the vertical field.
5.7.3 FinFET technologies
Even thought the FinFET transistor has a very different structure than the classical bulk transistor, the sEKV can also fit the I-V characteristics of FinFET transistors. This is illustrated in Figure 40 which shows the \(I_D\)-\(V_G\) characteristics of nMOS transistors for 3 different lengths (\(L=1\,\mu m\), \(70\,nm\) and \(30\,nm\)) from a 28 nm FinFET process. We see a very good fit for all transistor lengths over more than 6 decades of current. There is a small deviation at low gate voltage for the \(70\,nm\) transistor probably due to additional leakage current which is not accounted for in sEKV.
Figure 41 shows the normalized source transconductance versus the inversion coefficient for the same devices. An almost perfect fit is obtained over 5 decades of transconductance.
Finally, Figure 42 shows how the normalized \(G_m/I_D\) characteristic can be fitted versus the inversion coefficient over more than 5 decades with just a single parameter \(\lambda_c\).
5.7.4 Comparison on 28 nm bulk, 22 nm FDSOI and 16 nm FinFET
The sEKV model has also been validated on n- and p-channel transistors from a 28 nm bulk, 22 nm FDSOI and 16 nm FinFET technologies. The \(I_D\)-\(V_G\) characteristic of the three technologies are compared in
| Type | Technology | \(W\) [nm] | \(L\) [nm] | \(n\) | \(I_{spec\Box}\) [nA] | \(\lambda_c\) | \(V_{T0}\) [V] |
|---|---|---|---|---|---|---|---|
| nMOS | 28 nm bulk | 3000 | 30 | 1.46 | 599 | 0.271 | 0.478 |
| nMOS | 22 nm FDSOI | 1000 | 18 | 1.24 | 446 | 0.307 | 0.266 |
| nMOS | 16 nm FinFET | 58 | 16 | 1.13 | 1290 | 0.475 | 0.366 |
| pMOS | 28 nm bulk | 3000 | 30 | 1.74 | 446 | 0.253 | 0.501 |
| pMOS | 22 nm FDSOI | 1000 | 18 | 1.52 | 468 | 0.36 | 0.312 |
| pMOS | 16 nm FinFET | 58 | 16 | 1.12 | 995 | 0.331 | 0.431 |