# Noise Parameter Analysis of SiGe HBTs for Different Sizes in the Breakdown Region

Authors: Chie-In Lee; Yan-Ting Lin; Wei-Cheng Lin
Journal: Active and Passive Electronic Components
 (2016)

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## Abstract

Noise parameters of silicon germanium (SiGe) heterojunction bipolar transistors (HBTs) for different sizes are investigated in the breakdown region for the first time. When the emitter length of SiGe HBTs shortens, minimum noise figure at breakdown decreases. In addition, narrower emitter width also decreases noise figure of SiGe HBTs in the avalanche region. Reduction of noise performance for smaller emitter length and width of SiGe HBTs at breakdown resulted from the lower noise spectral density resulting from the breakdown mechanism. Good agreement between experimental and simulated noise performance at breakdown is achieved for different sized SiGe HBTs. The presented analysis can benefit the RF circuits operating in the breakdown region.


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## Body

## 1. Introduction

Characterization of high frequency noise for a transistor [1, 2] is essential to radio-frequency (RF) circuit designs because generated noise from transistors can determine the minimum signal strength that can be detected. Noise characteristics of a transistor can be dependent on device geometry [3, 4]. There are some literatures [3, 4] that report geometry dependence of noise parameters for SiGe HBTs under the normal operating condition. RF circuits are usually prevented from operating in the high electric field region because noise performance can be degraded at breakdown. Nevertheless, high output power is demanded for some applications of voltage-controlled oscillators (VCOs) mentioned in [5–7]. Circuit designers can increase supply voltage of above collector-emitter breakdown voltage (BVCEO) for VCOs [8] to achieve high-power microwave source. For this RF circuit application in the impact ionization region, noise performance of SiGe HBTs needs to be considered because the breakdown mechanism can produce excess noise. In [9, 10], noise parameters of SiGe HBTs above BVCEO have been characterized. However, investigation of noise parameters of SiGe HBTs in the breakdown region has not been reported for different sizes.Our previous research focused on breakdown noise modeling for SiGe HBTs [11]. In this work, we extend to the analysis of device geometry of noise parameters for SiGe HBTs in the avalanche region. Noise performance dependence on emitter size is reported in the impact ionization. Multiplication factors of SiGe HBTs are also analyzed for different sizes. This study with respect to device size can benefit the RF circuit applications in the breakdown region.


## 2. Method

Noise parameters of SiGe HBTs can be dependent on device geometry [3, 4]. In order to extend geometry analysis from the normal operating region [3, 4] to the breakdown regime suitable for high-power VCO applications [5–7], we aim to study the emitter size dependence of noise parameters in the avalanche region in this work. This work utilizes the RF measurements to obtain the RF noise model for different sized devices and to analyze emitter size dependence of noise performance at breakdown. In [3], the DC measurements are employed to extract the equivalent circuit parameters of their noise model for geometry analysis in the normal operating region. On the other hand, for the breakdown operation, the literatures [9, 10] characterize the avalanche noise sources by using DC measurements for a fixed device size as shown in Table 1.Table 1
Comparison between extracted and calculated breakdown noise spectral density atVBE=1.1 V and VCE=3.6 V for different sized SiGe HBTs.
Operating region ⁢Characterization method DC RF Avalanche region [9, 10]∗ This work Normal region [3] [3, 4] ∗Fixed device size.Different from the conventional characterization approach by the DC measurements, the presented RF measurement based method can be utilized to further reveal the RF phase delay of the breakdown mechanism. In the literature [3, 4], they also apply the RF measurements for noise characterization of SiGe HBTs. However, their analysis of noise parameters for different sized SiGe HBTs only focuses on the normal operating regime as shown in Table 1. This work first studies the emitter size dependence of noise parameters in the avalanche region. The diagram of devices used in this study of noise parameter dependence on emitter size is shown in Figure 1. Similar to [12] where four different emitter sizes of transistors are employed, four different emitter sizes comprising 1.7 × 0.2 μm2 (total emitter area = 1.36 μm2 and total emitter periphery = 15.2 μm), 1.7 × 0.6 μm2 (total emitter area = 4.08 μm2 and total emitter periphery = 18.4 μm), 10.2 × 0.2 μm2 (total emitter area = 8.16 μm2 and total emitter periphery = 83.2 μm), and 10.2 × 0.6 μm2 (total emitter area = 24.48 μm2 and total emitter periphery = 86.4 μm) with the same emitter finger of 4 are selected in this work in order to study noise performance under extreme conditions.Figure 1
The flowchart of the presented analysis. The cross section of the SiGe HBTs with the diagram for different emitter lengths and emitter widths is also shown. The RF noise model including the inductive breakdown network is also presented. Although this noise model presented here for the sake of completeness is the same as [11], this work further extends to noise characterization for different sizes.The selected geometry of devices is the allowable smallest and largest cases from the foundry design kit. The number of emitter fingers is fixed as 4. The difference between this work and [12] is that we focus on noise parameter investigation at breakdown. In Figure 1, the SiGe HBT noise model for the presented investigation of noise parameter dependence on device size at breakdown is shown. Although the equivalent circuit model can be referred to [11], the description of each element is presented here for the sake of completeness. The avalanche noise sources iava,n2¯ and iava,p2¯ in the breakdown network are employed to describe the excess noise originated from random phenomena of the electron and hole avalanche multiplication mechanism, respectively. The noise spectral density is given as [11](1)Sibd=2qIBCM21-1-kM-1M2.Furthermore, the electron breakdown inductanceLjc,n and resistance Rjc,n model the RF avalanche delay mechanism of electrons. Reverse base current caused by holes [13] is described by the avalanche transconductance gm2 corresponding to hole conductance Rjc,p-1 in the avalanche network. In addition, Ljc,p describes the RF avalanche delay mechanism of holes. Cbe and Cbc represent the base-emitter and base-collector junction capacitance, respectively. Rpi is the base-emitter junction resistance. Gm with time constant τ is the transconductance. Ro is the output resistance. Rbi is the intrinsic base resistance. iB2¯ and iC2¯ represent the base current shot noise and collector current shot noise, respectively. Their noise correlation is also considered in the noise model. Equivalent circuit element and noise source determination of the presented RF noise model employ the procedure [14, 15] where the measured results at RF are fitted. The difference is that the RF avalanche network is further considered in this RF noise model in order to study the noise parameter dependence on emitter size in the impact ionization region.


## 3. Results and Discussion

SiGe HBTs with various emitter sizes were manufactured through the Taiwan Semiconductor Manufacturing Company by using the 0.18μm BiCMOS technology node. Noise parameters including the minimum noise figure NFmin, optimum source admittance Yopt, and equivalent noise resistance Rn for different sized SiGe HBTs in the breakdown regime were measured through the ATN NP5B noise measurement system. The calibration procedure for the noise parameter measurement is performed from 1 to 18 GHz by this ATN system as in [16]. In Figures 2 and 3, measured and simulated noise parameters are compared for SiGe HBTs with various emitter sizes, and good agreement is achieved, validating the presented RF noise model for different sizes.Figure 2
Measured (symbols) and simulated (lines) minimum noise figure and equivalent noise resistance atVBE = 1.1 V and VCE = 3.6 V in the breakdown region for different emitter widths. The emitter length is fixed as 1.7 μm. Solid and dash lines depict the results obtained from the noise model with and without considering the breakdown network, respectively. In the inset, the results for different emitter lengths as the emitter width is fixed as 0.6 μm are shown. (a) Minimum noise figure. (b) Equivalent noise resistance.
(a) (b)Figure 3
Measured (symbols) and simulated (lines) real part of optimal source impedance versusVCE for different emitter widths. VBE is at 1.1 V. The operating frequency is at 2 GHz. The emitter length is fixed as 10.2 μm. Solid and dash lines depict the results obtained from the noise model with and without considering the breakdown network, respectively. In the inset, the results for different emitter lengths as the emitter width is fixed as 0.6 μm are shown.In Figure2(a), as the emitter length is fixed as 1.7 μm, NFmin decreases with decreasing emitter width from 0.6 μm to 0.2 μm. In addition, equivalent noise resistance of SiGe HBTs also decreases with reducing emitter width from 0.6 μm to 0.2 μm as shown in Figure 2(b). In Table 2, the determined breakdown noise spectral density is shown. Sibdn and Sibdp are avalanche noise spectral density resulting from iava,n2¯ and iava,p2¯, respectively. Sib and Sic are shot noise spectral density resulting from iB2¯ and iC2¯, respectively. As the emitter length is fixed as 1.7 μm, the spectral density decreases with decreasing emitter width. This lower Sibd reduces noise performance for the narrower emitter width SiGe HBT, and thus, NFmin and Rn become lower as shown in Figure 2. In addition, the signal-to-noise ratio (SNR) increases for the narrower emitter width as shown in Table 3 due to lower Sibd mentioned above. The high SNR represents low noise performance [17]. On the other hand, when the emitter width is fixed as 0.6 μm, NFmin and Rn decrease and SNR increases with decreasing emitter length from 10.2 μm to 1.7 μm as shown in the inset of Figures 2(a) and 2(b) and Table 3 due to the reduced breakdown noise spectral density for the shorter emitter length shown in Table 2. The analysis of NFmin and Rn dependence on emitter length and width indicates that the smaller emitter size can reduce noise for SiGe HBTs operating in the breakdown region. This is explained as follows. The smaller emitter size can decrease the device current. As base-collector current of SiGe HBTs decreases, the noise spectral density can reduce [18]. Therefore, noise performance reduces with lowering the emitter size. Large Rn can introduce difficulty of achieving minimum noise matching [19]. SiGe HBTs with narrow emitter width and short emitter length have smaller Rn than the wide width and long length HBTs as shown in Figure 2(b). Therefore, small size of SiGe HBTs appears to be a way for obtaining the condition of minimum noise matching in low noise RF circuit designs.Table 2
Comparison between extracted and calculated breakdown noise spectral density atVBE=1.1 V and VCE=3.6 V for different sized SiGe HBTs.
S i b d n / S i b d p from calculation (×10−22 A2 s) S i b d n / S i b d p from presented noise model (×10−22 A2 s) 0.2μm × 1.7 μm 0.72/0.62 0.69–0.74/0.60–0.65 0.6μm × 1.7 μm 0.80/0.70 0.78–0.84/0.67–0.73 0.2μm × 10.2 μm 0.85/0.71 0.83–0.89/0.69–0.74 0.6μm × 10.2 μm 0.92/0.75 0.90–0.95/0.73–0.77Table 3
The signal-to-noise ratio (SNR) of SiGe HBTs with different area atVBE=1.1 V and VCE=3.6 V in the breakdown region. The operating frequency is at 2 GHz.
Emitter width = 0.2μm Emitter width = 0.6μm Emitter length = 1.7μm 85.6 dB 84.7 dB Emitter length = 10.2μm 85.2 dB 78.6 dBThe real part of optimal source impedance Re(Zopt) shown in Figure 3 is used to investigate the geometry dependence of optimal source condition for noise matching of RF circuits as in [4]. Figure 3 shows that the narrower emitter width can increase Re(Zopt). This is explained as follows. Re(Zopt) can be proportional to the resistance seen at the input because the optimal source impedance is an input noise matching characteristic [4]. When the emitter width declines from 0.6 μm to 0.2 μm, the breakdown resistance seen at the input increases from 98 Ω to 126 Ω for the fixed emitter length of 10.2 μm. This higher breakdown resistance seen at the input raises Re(Zopt) for the narrower emitter width SiGe HBTs. On the other hand, when the emitter width is fixed as 0.6 μm, Re(Zopt) increases with decreasing emitter length as shown in the inset of Figure 3 due to the higher breakdown resistance for the shorter emitter length SiGe HBTs. The breakdown resistance increases from 98 Ω to 156 Ω for emitter length decreased from 10.2 μm to 1.7 μm. Conventional analysis for the real part of optimal source impedance for different device sizes focuses on the normal operating region [4]. This work further investigates the real part of optimal source impedance dependence on device size in the avalanche region. This analysis demonstrates that the smaller emitter size can increase real part of optimal source impedance in the avalanche region due to increased breakdown resistance which can influence the input noise matching characteristic.The simulated results by using the conventional noise model without considering the presented RF avalanche network are compared in the impact ionization region and a deviation is found for different sized SiGe HBTs as shown in Figures2 and 3. Larger deviation of Sib and Sic in the conventional model is observed for the longer emitter length and wider emitter width sized devices as shown in Table 4 because the breakdown noise spectral density is more pronounced for large sized SiGe HBTs as reported in Table 2. Instead, the obtained Sib and Sic from our RF noise model are close to the calculated values. In addition, the extracted breakdown noise spectral density can agree well with the theoretical results using (1) for different sized SiGe HBTs.Table 4
Determined base and collector noise spectral density for different sized SiGe HBTs in the breakdown region ofVBE=1.1 V and VCE=3.6 V. The results obtained from the presented noise model, calculation, and conventional model are compared. The variation is indicated for the results obtained from the presented model as the deviation of noise performance fitting is within 1%.
S i b / S i c from presented noise model (×10−24 A2 s) S i b / S i c from calculation (×10−24 A2 s) S i b / S i c from conventional noise model (×10−24 A2 s)∗ 0.2μm × 1.7 μm 5.44–5.97/42.83–43.32 5.64/43.11 6.11/43.36 0.6μm × 1.7 μm 7.21–7.76/46.3–47.0 7.41/46.76 8.01/47.33 0.2μm × 10.2 μm 8.54–8.90/48.87–49.36 8.86/49.12 9.41/49.89 0.6μm × 10.2 μm 11.01–11.72/55.68–56.19 11.65/55.89 12.87/56.93 ∗It is difficult to achieve error below 1% by the conventional noise model so that the determined values deviate from calculation results.


## 4. Conclusions

In this paper, the investigation of noise parameter dependence on device geometry for SiGe HBTs operating in the avalanche region is presented for the first time. SiGe HBT minimum noise figure at breakdown decreases with decreasing the emitter length. In addition, narrower emitter width reduces noise figure in the avalanche region. Decreased noise with decreasing device size at breakdown is found to be due to the low breakdown noise spectral density for smaller devices which have lower current than larger devices. Good agreement between experiment and simulation results of noise performance at breakdown is obtained for different sized SiGe HBTs. This study with respect to device size can benefit the RF circuit applications in the breakdown region.



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