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Ernesto Limiti

E.E.Dept . head, University of Rome “Tor Vergata”, Rome, Italy limiti@ing.uniroma2.it. HEMTs in Europe ( GaAs HEMT low-noise technologies , design techniques, characterization and modeling). Ernesto Limiti. Who and Where we are. University of Roma “Tor Vergata” Founded in 1982

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Ernesto Limiti

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  1. E.E.Dept. head, University of Rome “Tor Vergata”, Rome, Italy limiti@ing.uniroma2.it HEMTs in Europe (GaAs HEMT low-noise technologies, design techniques, characterization and modeling) Ernesto Limiti

  2. Who and Where we are • University of Roma “Tor Vergata” • Founded in 1982 • 600 hectares of Campus • 6 Faculties & 35k students • Electronic Engineering Department • Founded in 1983 • 150 people • MiMEG Group • 2 Full & 3 Associate Prof. • 5 Researchers • 1 Technicians • 5 PhD Students • 3 Post Docs

  3. Characterization Modelling Methodologies & Designs What we do at MiMEG Small-Signal (bias-dependent, scalable) Noise Large-Signal Small-Signal Large-Signal Noise Time Domain High-Efficiency Power Amplification & Linearization Techniques Linear Amplification (Gain blocks, LNA …) Nonlinear functionalities (MIXER, Multipliers, Dividers, VCO…) Advanced Functions (Core Chip, DigiPS, DigiATT) MMIC and MIC Subsystem Integration (SCFE, Tx/Rx modules) From 250kHz up to 120 GHz (extending to 300GHz) and in many technologies

  4. Low-NoiseGaAs HEMT technologies in Europe

  5. OMMIC reaches G-band frequencies thanks to its 40nm GaAs process (D004MH). UMS offers a GaAs low-noise 100nm process (PH10) suitable up to V-band Europe GaAs HEMTs (100nm or smaller) +LNF INDUSTRIES R&D labs GaAs mHEMT (down to 20nm) technologies are available and have been presented in open literature.

  6. OMMIC MetamorphicHEMTs(high indiumcontent in the channel, 70%)

  7. OMMIC

  8. Fraunhofer IAF … and 20nm

  9. Fraunhofer IAF InxGa1-xAs mHEMT

  10. Low-NoiseDesign Techniques

  11. Design Techniques for LNAs Very powerful derivations regarding the effect of feedback on the noise and gain of amplifiers were published by Haus and Alder back in the 60’s. These papers are not easily understood and are often ignoredin current literature. They are the cornerstone of accurate low-noise amplifier synthesis. Appropriate design methodologies leverage the transistor’s capabilities. Finally, differentdesign techniques apply to differentoperatingfrequencies. millimetre-wave • Transistor gain is not enough to conceal the noise contribution on subsequent stages. The correct figure of merit for the transistor/technology is the noise measure, M. • Design effort is put upon obtaining low NF and adequate Gain. M takes into account both terms. microwave • Very high transistor gain, enough to conceal the noise contribution from following stages • Design effort is put upon I/O match

  12. LNA designers often struggle to simultaneously satisfy gain, noise and I/O matching requirements. To this purpose a NOVEL DESIGN TECHNIQUE for multi stage low-noise amplifiers has been developed to obtain conjugate LNA I/O match. Design Techniques for microwave LNAs LNA Gain Feedback Inductance LNA interstagematch Feedback Inductance Look for Author E. Limiti (et al.) in IEEExplore

  13. Design Techniques for millimetre-wave LNAs Optimum terminations in the source plane have been identified and discussed. The effect of feedback has been carefully analyzed. Feedback eases the noise/gain trade-off, especially at higher frequencies. The importance of Noise Measure (M) has been highlighted when designing millimetre-wave LNAs since the 1st stage’s FET available gain (Ge) is not enough to conceal the following stage’s noise contribution. feedback reduces gain… but also NFMINis reduced. ….so MMIN is constant! Look for Author E. Limiti (et al.) in IEEExplore

  14. Several LNAs have been designed in-house lately In European Industrial Grade Technology… OMMIC’s mHEMT GaAs process NF of GaAs in-house designed MMIC LNAs 70 nm 40 nm EuMC 2017 EuMC 2008 MOTL 2018 Indicates Relative BW % MOTL 2019 Min 15 % - Max 40% JSSC 2010 Gain > 20dB NF = 10*log(1+TN/T0) Look for Author “E. Limiti” (et al.) in IEEExplore and Wiley Interscience

  15. E-Band 71-86 GHz LNA with NF < 2.5dB • OMMIC D007IH 70nm GaAs Industrial process • Four-stage, single ended MICROSTRIP • MMIC Size: 3.0 x 1.6 mm2 • Gain 22dB - NF 2.3 dB TYP. OP1dB +4dBm OIP3 +16 dBm

  16. D-Band 125-155 GHz LNA with NF ≈ 5.0 dB • OMMIC D004IH 40nm GaAs process • Four-stage, single ended COPLANAR • MMIC Size: 2.0 x 1.0 mm2 • Gain 17dB - NF 5 dB typ.

  17. Low-NoiseAnalysis, characterization and modelling capabilities

  18. Analysis, characterization and modelling capabilities • I – Available instrumentation • II – Advanced measurement approaches • Calibrations • Test-benches • III – Model extraction • Passive devices • Active devices • IV – On-wafer non-linear measurements

  19. Available instrumentation • 4Vector Network Analysers (HP 8510C 0.05-50 GHz; Anritsu Lightning(37397B), 0.05-65 GHz, extending to 110 GHz; Anritsu VectorStar (MS4640B) up to 125 GHz; KeysightE5061B, down to 1 Hz) • 2 Spectrum Analyser (HP 70000 DC-40 GHz, Agilent PSA E4448A 3Hz-50GHz) • Noise Measurement System (HP8970B-HP8971C DC-26.5 GHz, with proprietary amplified SSB extension to 40 GHz; pre-amplifiers, LO frequency multipliers, isolators, waveguide switches, waveguide filters and noise sources to extend the hot/cold or cold-source SSB measurement range up to 75 GHz) • 2 Elettromechanical Tuners (Focus 0.08-18 GHz and 3-50 GHz) • Digital Sampling Oscilloscope (TekTronix up to 50 GHz) • I-V PulsedMeasurement System (GaAs Code) • PowerAmplifier (AR 0.8-4.2 GHz - 25 W) • SynthesisedSources (2 Anritsu MG3692A 2-20 GHz,HP 83640A up to 40 GHz, Agilent MXG N5183A up to 40 GHz, HP 83651A up to 50 GHz) • Vector Signal Source (Agilent E4438C 250 kHz-6 GHz) • Probe Stations (CascadeMicrotechRF-1, SussMicrotec PM8, Cascade M150, allequipped with anti-vibratingtables) • Cryogenic Probe Station (down to 20 K, proprietary) • Test-fixtures (Wiltron, Agilent, …)

  20. Calibrations • Calibration approaches: • Commercial substrates vs custom substrates • SOLT vs TRL-like • Modeling at microwaves and up requires calibration on the same substrate as the devices • The accuracy to which the standards are known is of course low with custom calibration kits • On high-loss substrates, a combination of commercial and custom substrates may be required (two-tier) to extract Zc • Contribution of the access lines fully removed • Line propagation constant obtained as a by-product • Line characteristic impedance easily obtained also on low-loss substrates

  21. Calibrations • The typical method for determining the characteristic impedance of the line standards in TRL-like calibrations is the “capacitance method” [1]. • This is based, however, on the hypothesis that the substrate loss is negligible. • With lossy substrates, such as Silicon, the method fails: often this appears as over-unity magnitudes for reflection coefficients of passive (but highly reactive) loads. • The “calibration comparison method” comes in handy in these cases [2]. • In this example (OMMIC D01GH, Run A) it is shown how the S11 of HEMT devices, which is highly reactive at low frequencies, may easily appear to feature over-unity magnitude when it is renormalized based on the capacitance method Zc. • This artifact is eliminated by using the calibration comparison method Zc. S11 (capacitance method) S11 (calibration comparison method) Zc extraction [1] Williams D. F. & Marks R. B., “Transmission line capacitance measurement.” IEEE Microwave and Guided Wave Letters, 1991, 1, 243-245 [2] Williams D. F., ArzU. & GrabinskiH., “Characteristic-impedance measurement error on lossysubstrates.” IEEE Microwave and Wireless Components Letters, 2001, 11, 299-301

  22. Test-benches: Noisefactormeasurements Typical noise test bench for on-wafer measurements Block 1 Block 2a Block 2b SOLT TRL Two-tier Two-tier One-tier Term Bias-Tee Bias-Tee Rcvr DUT • Can be eliminated by means of a full receiver calibration • Fixed or source pull

  23. Test-benches: Noisecharacterization and modelling • Several methods of noise characterization available: • Y-factor [1] • Cold-source [1] • Source pull [1,2] • Source/load pull [3,4] • noise-temperature model • of the transistor • black-box characterization • of the whole noise parameter set • NF Y-factor measurement on the 4×35 µm device • at VDS = 5 V, JD = 250 mA/mm. • Notice the similarity in Gav and Gav,hc, with a possible exception around 31 GHz. • Cold-source measurement do not offer an analogous check. • [1] Limiti E., Ciccognani W. & Colangeli S., “Characterization and modeling of high-frequency active devices oriented to high-sensitivity subsystems design,” in Microwave de-embedding - From theory to applications, Elsevier, 2013, 97-150 • [2] Lane R. Q., “The determination of device noise parameters,” Proceedings of the IEEE, 1969, 57, 1461-1462 • [3] CiccognaniW., Colangeli S., SerinoA., LonghiP. E. & Limiti E. “Generalized extraction of the noise parameters by means of Source- and Load-Pull noise power measurements,” IEEE Transactions on Microwave Theory and Techniques, 2018, 66, 2258-2264 • [4] RandaJ., “Comparison of noise-parameter measurement strategies: Simulation results for amplifiers,” 84th ARFTG Microwave Measurement Conference, 2014, 1-8

  24. Test-benches: Source/load pull Better conditioned system of equations resulting in reduced uncertainty in the estimation of Fminand Rn.

  25. Test-benches:SSB measurements at higherfrequency (Q, V … W) Q-band Mixer: SAGE SFB-22-E2, 33 to 50 GHz, DC to 17 GHz IF, +3 dBm LO Power, WR-22 Waveguide, Q Band Externally Biased Balanced Mixer LNA: LOW NOISE FACTORY LNF-LNR28_52WB, 28-52 GHz Low pass filter: SAGE SWF-50354340-22-L1, 30 to 50 GHz, 40 dB Rejection from DC to 25 GHz and 56 to 100 GHz, Q Band, WR-22 Waveguide WR22 DPDT switch: SAGE SWJ-22-TS, 33 to 50 GHz, 60 dB Isolation, WR-22 Waveguide, Q Band DPDT MotorizedSwitch WR22/V transition: SAGE SWC-22VM-E1, WR-22 Waveguide to 1.85 mm V(M) Coax Adapter, End Launch Biastee: SHF BT65 (high voltage option), 1.85 mm V(M)-DCRF, 1.85 mm V(F)-RF Frequencymultiplier: QUINSTAR QPM-42052Q, passive multiplier, X2, input k-female output WR-22, UG-383 LO driver: Quinstar QPI-K0238JO KA-Fullbandamplifier, input k-female, output k-male Noisesource: QUINSTAR QNS-FB15LQ, noise source with isolator

  26. Model Extraction • Available modeling approaches: • Black-box vsequivalent circuit • Geometry-specific vsscalable • Measurements at lower frequencies can be performed, and the model extrapolated • Physical behavior guaranteed by construction • Possible fitting to extract the internal parameters, not to compute the external behavior • Scalability can be exploited during extraction to enhance model robustness: especially useful for active devices • Scalable models are required anyway

  27. Model Extraction • Standard equivalent circuit topology • CPW devices: no need for de-embedding via holes • μ-strip devices: EM simulation of the via holes • S11,4x50μm • Measurements up to 60 GHz • Models up to 110 GHz • S11,4x100μm

  28. Active devices - OMMIC D01GH process Noise temperature extraction • Γopt • ΓS • [1] Colangeli S., Ciccognani W., Cleriti R, Palomba M. & Limiti E., “Optimization-based approach for scalable small-signal and noise model extraction of GaN-on-SiC HEMTs,” International Journal of Numerical Modelling: Electronic Networks, Devices and Fields, 2017, 30, e2135 • [2] PospieszalskiM. W., “Modeling of noise parameters of MESFETs and MODFETs and their frequency and temperature dependence,” IEEE Transactions on Microwave Theory and Techniques, 1989, 37, 1340-1350 • [3] Mokari M. E. & Patience W., “A new method of noise parameter calculation using direct matrix analysis,” IEEE Transactions on Circuits and Systems I: Fundamental Theory and Applications, 1992, 39, 767-771 • Rn • Closed-form least-squares fit of the 4×35 µm device noise factor at VDS = 5 V, JD  = 250mA/mm: • Tg ≈ 314 K, Td≈ 2798 K • NFmin ≈ 1.4 dB at 35 GHz • NFmin

  29. Active devices - OMMIC D004IH process Characterization and modelling activities performed within the framework of the TeraSCREEN and ULTRAWAVE projects. • Typical maximum gm: 80÷85 mS • DC measurements at a reference bias to assess the uniformity of the process and to select the most representative cells for the subsequent characterization and modelling activities. • Figures refer to measurements performed on a preliminary TeraSCREEN wafer

  30. Active devices - OMMIC D004IH process S11 S22 Characterization and modelling activities performed within the framework of the TeraSCREEN and ULTRAWAVE projects. dB(S21) • Scattering parameters measurements at a reference bias to assess the uniformity of the process and to select the most representative cells for the subsequent characterization and modelling activities. • Figures refer to measurements performed on a preliminary TeraSCREEN wafer

  31. Active devices - OMMIC D004IH process • Comparison between measurement and scalable model for a 2x20 µm DS15 devices • Bias ID max = 625 mA/mm ; VDS = 1 V; ID = 20% IDmax = 50 mA Characterization and modelling activities performed within the framework of the TeraSCREEN and ULTRAWAVE projects. Fmeas vs Fmod S11 S22 dB(S21) NFmin, Rn

  32. Conclusions • Europe offers research & production-gradeGaAs mHEMTs technologies for millimeter-wave low-noise systems, comparable to overseas InP ones. • Technology alone does not solve any issue: device characterization and modelling, appropriate design methodologies are key elements.

  33. E.E.Dept. head, University of Rome “Tor Vergata”, Rome, Italy limiti@ing.uniroma2.it HEMTs in Europe (GaAs HEMT low-noise technologies, design techniques, characterization and modeling) Ernesto Limiti

  34. References • Low-Noise Amplifier Design Techniques Ciccognani, W., Longhi, P.E., Colangeli, S., Limiti, E., “Constant mismatch circles and application to low-noise microwave amplifier design”, IEEE Transactions on Microwave Theory and Techniques, 61(12),6662458, pp. 4154-4167, 2013. Ciccognani, W., Colangeli, S., Limiti, E., Longhi, P. “Noise measure-based design methodology for simultaneously matched multi-stage low-noise amplifiers”, IET Circuits, Devices and Systems, 6(1), pp. 63-70, 2012. Colangeli, S., Ciccognani, W., Salvucci, A., Limiti, E., “Deterministic design of simultaneously matched, two-stage low-noise amplifiers”, Asia-Pacific Microwave Conference Proceedings, pp. 558-561, 2018. • Low-Noise Active Devices Characterization & Modeling Ciccognani, W., Colangeli, S., Serino, A., Longhi, P.E., Limiti, E., “Generalized Extraction of the Noise Parameters by Means of Source-and Load-Pull Noise Power Measurements” IEEE Transactions on Microwave Theory and Techniques, 66(5), pp. 2258-2264, 2018. Colangeli, S., Ciccognani, W., Palomba, M., Limiti, E., “Automated extraction of device noise parameters based on multi-frequency, source-pull data”, International Journal of Microwave and Wireless Technologies, 6(1), pp. 63-72, 2014. Cleriti, R., Ciccognani, W., Colangeli, S., (...), Frijlink, P., Renvoisé, M., “Characterization and modelling of 40 nm mHEMT process up to 110 GHz”, 11th European Microwave Integrated Circuits Conference, pp. 353-356, 2016 Cleriti, R., Colangeli, S., Ciccognani, W., Palomba, M., Limiti, E., “Cold-source cryogenic characterization and modeling of a mHEMTprocess”, European Microwave Week, pp. 41-44, 2015.

  35. Reference • Millimetre-wave GaAs LNAs Ciccognani, W., Colangeli, S., Longhi, P.E., Limiti, E., “Design of a MMIC low-noise amplifier in industrial gallium arsenide technology for E-band 5G transceivers”, Microwave and Optical Technology Letters 61(1), pp. 205-210, 2019. Ciccognani, W., Longhi, P.E., Colangeli, S., Limiti, E. “Q/V band LNA for satellite on-board space applications using a 70 nanometers GaAs mHEMT commercial technology”, Microwave and Optical Technology Letters 60(9), pp. 2185-2190, 2018. Cleriti, R., Ciccognani, W., Colangeli, S., et al.., “D-band LNA using a 40-nm GaAs mHEMTtechnology”, 12th European Microwave Integrated Circuits Conference, pp. 105-108, 2017. Ciccognani, W., Colangeli, S., Limiti, E., Scucchia, L., “Millimeter wave low noise amplifier for satellite and radio-astronomy applications”, IEEE 1st AESS European Conference on Satellite Telecommunications, ESTEL 2012. Ciccognani, W., Limiti, E., Longhi, P.E., Renvoisè, M., “MMIC LNAs for radioastronomy applications using advanced industrial 70 nm metamorphic technology” IEEE Journal of Solid-State Circuits, 45(10), pp. 2008-2015, 2010. Ciccognani, W., Giannini, F., Limiti, E., Longhi, P.E., “Full W-band high-gain LNA in mHEMTmmictechnology” European Microwave Integrated Circuit Conference, EuMIC2008, pp. 314-317, 2008.

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