A Flexible RFIC Architecture for High-Sensitivity Reception and Compressed-Sampling Wideband Detection

Compressed sensing (CS) is a new signal processing approach that has disrupted the Shannon-Nyquist limit based design methodology and has opened promising avenues for building energy-efficient radio frequency integrated circuits (RFICs) for detecting and estimating particular classes (i.e. sparse) of signals. Whether in application domains where naturally occurring signals are sparse or where representations of signals subject to the fidelity limits or configuration settings of the radio equipment are often found to be sparse, the emergence of CS has forced us to re-imagine the radio receiver. While realizing some of the potential benefits promised by theory, CS-RFIC architectures proposed in earlier research were not particularly suitable for mass-market applications. This thesis demonstrates how to take a new signal processing technique all the way to the hardware level. So far, the main focus in literature has been how CS offers a significant advantage for signal processing. This work will show how CS techniques drive novel architectures down to the integrated circuit level. This requires close collaboration between communication system developers, integrated circuit designers and signal processing experts. The trans-disciplinary approach presented here has led to the unification of CS-inspired architectures for wideband signal detection with robust, legacy architectures for high-sensitivity signal reception. The result is a functionally flexible and rapidly reconfigurable CMOS RFIC compactly implemented on silicon with the potential to achieve the cost, size and power targets in mass-market applications. While the focus of this thesis is RF signal finding and reception in frequency, the CS-based RFIC design approach presented here is applicable to a wide range of other applications like direction-of-arrival and range finding. We begin by developing a signal-model driven approach for optimizing the performance of CS RF frontends (RFFEs). We consider sparse multiband signals with supports contained within a frequency span extending from fMIN to fMAX. The resulting quadrature analog-to-information converter (QAIC) is a flexible-bandwidth, blind sub-Nyquist sampling architecture optimized for energy consumption and sensitivity performance. The QAIC addresses key drawbacks of earlier CS RFFE architectures like the modulated wideband converter (MWC) that implement frequency spans extending from 0 to fMAX. While these earlier architectures, a direct implementation of CS signal processing theory, have several beneficial properties, the true cost of their proposed analog frontend significantly diminishes the sensitivity performance and energy savings that CS methods have the potential to deliver. They use periodic pseudo-random bit sequence (PRBS) generators where the clock frequency fPRBS scales up with the maximum signal frequency fMAX. In contrast, fPRBS in the QAIC RFFE scales up with the instantaneous bandwidth IBW, where IBW = ( fMAX − fMIN ). This results in significant performance advantages in terms of energy consumption and sensitivity performance. The QAIC uncouples fPRBS from fMAX by performing wideband quadrature downconversion ahead of analog mixing with PRBSs at an intermediate frequency (IF). However, the dual heterodyne architecture of the QAIC suffers from spurious responses at IF caused by gain and phase imbalance in its wideband downconverter. We then show how the direct RF-to-information converter (DRF2IC) compactly adds CS wideband detection to a direct conversion frequency-translational noise-cancelling (FTNC) receiver by introducing pseudo-random modulation of the local oscillator (LO) signals and by consolidating multiple CS measurements into one hardware branch. The DRF2IC inherits benefits of the FTNC receiver in signal reception mode. In CS wideband detection mode, the DRF2IC inherits key advantages from both the earlier lowpass CS architectures and the QAIC while avoiding the drawbacks of both. It uncouples fPRBS from fMAX in contrast with the MWC. In contrast with the QAIC, the DRF2IC employs a direct conversion RF chain with narrow bandwidth analog components at baseband thereby avoiding frequency-dependent gain and phase imbalance. The DRF2IC chip occupies 0.56mm2 area in 65nm CMOS. In reception mode, it consumes 46.5mW from 1.15V and delivers 40MHz RF bandwidth, 41.5dB conversion gain, 3.6dB noise figure (NF) and -2dBm blocker 1dB compression point (B1dB). In CS wideband detection mode, 66dB operational dynamic range, 40dB instantaneous dynamic range and 1.43GHz instantaneous bandwidth are demonstrated and 6 interferers each 10MHz wide scattered over a 1.27GHz span are detected in 1.2us consuming 58.5mW

Switchable wideband receiver frontend for 5G and satellite applications

Modern day communication architectures provides the requirement for interconnected devices offering very high data rate (more than 10 Gbps), low latency, and support for multiple service integration across existing communication generations with wideband spectrum coverage. An integrated satellite and 5G architecture switchable receiver frontend is presented in this thesis, consisting of a single pole double throw (SPDT) switch and two low noise amplifiers (LNAs) spanning X-band and K/Ka-band frequencies. The independent X-band LNA (8-12 GHz) has a gain of 38 dB at a centre design frequency of 9.8 GHz, while the K/Ka-band (23-28 GHz) has a gain of 29 GHz at a centre design frequency of 25.4 GHz. Both LNAs are a three-stage cascaded design with separated gate and drain lines for each transistor stage. The broadband high isolation single pole double throw (SPDT) switch based on a 0.15 μm gate length Indium Gallium Arsenide (InGaAs) pseudomorphic high electron transistor (pHEMT) is designed to operate at the frequency range of DC-50 GHz with less than 3 dB insertion loss and more than 40 dB isolation. The switch is designed to improve the overall stability of the system and the gain. A gain of about 25 dB is achieved at 9.8 GHz when the X-band arm is turned on and the K/Ka-band is turned off. A gain of about 23 dB is achieved at 25.4 GHz when the K/Ka-band arm is turned on and the X-band arm is off. This presented switchable receiver frontend is suitable for radar applications, 5G mobile applications, and future broadband receivers in the millimetre wave frequency range

Feedback methods for inductorless bandwidth extension and linearisation of post-amplifiers in optical receiver frontends

Optical communication is increasingly important in today's telecommunications. It is not only a key component in long-haul infrastructure, but is also being brought into new applications within the datacentre, at the circuit board and integrated circuit level, and in next generation mobile networks. This thesis proposes feedback tuning approaches in order to address two challenges within optical receiver analog frontend circuits: a) the dynamic response of a prior bandwidth extension technique; and b) linearity optimisation. To address dynamic response, we begin with an inductorless method of bandwidth extension using positive feedback loops. In a multi-stage post-amplifier with local positive feedback loops, we propose an approach which tunes each positive feedback gain separately, and demonstrate that this achieves better dynamic response and eye opening than the prior equal-feedback-gain approach. We additionally propose root-locus analysis as a means of characterising dynamic response, and suggest some design guidelines based on this analysis. To address linearity optimisation, we propose the use of an interleaving negative-feedback post-amplifier topology, previously proposed only for bandwidth extension. We investigate the relationship between the feedback gains and linearity and develop a design approach for linearity optimisation. We then designed and fabricated two 70 dB 6 GHz optical receiver circuits, making use of two different post-amplifiers, in order to compare different design approaches. We achieved a linearity of 0.08 dBVrms OIP3 (quasi-static) and a THD of 0.195\% at 1 GHz

HIGH PERFORMANCE CMOS WIDE-BAND RF FRONT-END WITH SUBTHRESHOLD OUT OF BAND SENSING

In future, the radar/satellite wireless communication devices must support multiple standards and should be designed in the form of system-on-chip (SoC) so that a significant reduction happen on cost, area, pins, and power etc. However, in such device, the design of a fully on-chip CMOS wideband receiver front-end that can process several radar/satellite signal simultaneously becomes a multifold complex problem. Further, the inherent high-power out-of-band (OB) blockers in radio spectrum will make the receiver more non-linear, even sometimes saturate the receiver. Therefore, the proper blocker rejection techniques need to be incorporated. The primary focus of this research work is the development of a CMOS high-performance low noise wideband receiver architecture with a subthreshold out of band sensing receiver. Further, the various reconfigurable mixer architectures are proposed for performance adaptability of a wideband receiver for incoming standards. Firstly, a high-performance low- noise bandwidthenhanced fully differential receiver is proposed. The receiver composed of a composite transistor pair noise canceled low noise amplifier (LNA), multi-gate-transistor (MGTR) trans-conductor amplifier, and passive switching quad followed by Tow Thomas bi-quad second order filter based tarns-impedance amplifier. An inductive degenerative technique with low-VT CMOS architecture in LNA helps to improve the bandwidth and noise figure of the receiver. The full receiver system is designed in UMC 65nm CMOS technology and measured. The packaged LNA provides a power gain 12dB (including buffer) with a 3dB bandwidth of 0.3G – 3G, noise figure of 1.8 dB having a power consumption of 18.75mW with an active area of 1.2mm*1mm. The measured receiver shows 37dB gain at 5MHz IF frequency with 1.85dB noise figure and IIP3 of +6dBm, occupies 2mm*1.2mm area with 44.5mW of power consumption. Secondly, a 3GHz-5GHz auxiliary subthreshold receiver is proposed to estimate the out of blocker power. As a redundant block in the system, the cost and power minimization of the auxiliary receiver are achieved via subthreshold circuit design techniques and implementing the design in higher technology node (180nm CMOS). The packaged auxiliary receiver gives a voltage gain of 20dB gain, the noise figure of 8.9dB noise figure, IIP3 of -10dBm and 2G-5GHz bandwidth with 3.02mW power consumption. As per the knowledge, the measured results of proposed main-high-performancereceiver and auxiliary-subthreshold-receiver are best in state of art design. Finally, the various viii reconfigurable mixers architectures are proposed to reconfigure the main-receiver performance according to the requirement of the selected communication standard. The down conversion mixers configurability are in the form of active/passive and Input (RF) and output (IF) bandwidth reconfigurability. All designs are simulated in 65nm CMOS technology. To validate the concept, the active/ passive reconfigurable mixer configuration is fabricated and measured. Measured result shows a conversion gain of 29.2 dB and 25.5 dB, noise figure of 7.7 dB and 10.2 dB, IIP3 of -11.9 dBm and 6.5 dBm in active and passive mode respectively. It consumes a power 9.24mW and 9.36mW in passive and active case with a bandwidth of 1 to 5.5 GHz and 0.5 to 5.1 GHz for active/passive case respectively

Ultra-wideband and highly linear 43-97 GHz receiver front-end

This research presents a wideband mmWave receiver front-end that covers the frequency range from 43 to 97 GHz, supporting the operation in the major parts of the V-, E- and W-bands. The front-end incorporates a passive mixer-first topology to achieve high linearity and wideband performance along with an optimum operational instantaneous bandwidth. In addition, it implements the multi-gate gm3 cancellation technique at the IF amplifiers to preserve the linearity and provide gain at the IF section. Image rejection capabilities using a current mode transformer based IF 90o coupler is implemented on chip and demonstrated with measurements. The front-end is fabricated on the Globelfoundries 22nm FD-SOI CMOS process and demonstrates an ultra-wideband performance across the frequency range 43-97 GHz (2.25:1 bandwidth) with image rejection of up to 32 dB, IIP3 of 1.6-5.2 dBm and gain of 15 dB. Furthermore, the measurement results show that the front-end supports high speed modulated signals of up to 6 Gbps 64QAM modulation data.M.S

A CMOS spectrum analyzer frontend for cognitive radio achieving +25dBm IIP3 and −169 dBm/Hz DANL

A dual RF-receiver preceded by discrete-step attenuators is implemented in 65nm CMOS and operates from 0.3– 1.0 GHz. The noise of the receivers is reduced by cross-correlating the two receiver outputs in the digital baseband, allowing attenuation of the RF input signal to increase linearity. With this technique a displayed average noise level below -169 dBm/Hz is obtained with +25 dBm IIP3, giving a spurious-free dynamic range of 89 dB in 1 MHz resolution bandwidth

Current reuse topology in UWB CMOS LNA

Non

Technology Advances for Radio Astronomy

The field of radio astronomy continues to provide fundamental contributions to the understanding of the evolution, and inner workings of, our universe. It has done so from its humble beginnings, where single antennas and receivers were used for observation, to today's focal plane arrays and interferometers. The number of receiving elements (pixels) in these instruments is quickly growing, currently approaching one hundred. For the instruments of tomorrow, the number of receiving elements will be in the thousands. Such instruments will enable researchers to peer deeper into the fabric of our universe and do so at faster survey speeds. They will provide enormous capability, both for unraveling today's mysteries as well as for the discovery of new phenomena. Among other challenges, producing the large numbers of low-noise amplifiers required for these instruments will be no easy task. The work described in this thesis advances the state of the art in three critical areas, technological advancements necessary for the future design and manufacturing of thousands of low-noise amplifiers. These areas being: the automated, cryogenic, probing of \diameter100 mm indium phosphide wafers; a system for measuring the noise parameters of devices at cryogenic temperatures; and the development of low-noise, silicon germanium amplifiers for terahertz mixer receivers. The four chapters that comprise the body of this work detail the background, design, assembly, and testing involved in these contributions. Also included is a brief survey of noise parameters, the knowledge of which is fundamental to the design of low-noise amplifiers and the optimization of the system noise temperature for large, dense, interferometers.</p

Amplifiers in Biomedical Engineering: A Review from Application Perspectives

Continuous monitoring and treatment of various diseases with biomedical technologies and wearable electronics has become significantly important. The healthcare area is an important, evolving field that, among other things, requires electronic and micro-electromechanical technologies. Designed circuits and smart devices can lead to reduced hospitalization time and hospitals equipped with high-quality equipment. Some of these devices can also be implanted inside the body. Recently, various implanted electronic devices for monitoring and diagnosing diseases have been presented. These instruments require communication links through wireless technologies. In the transmitters of these devices, power amplifiers are the most important components and their performance plays important roles. This paper is devoted to collecting and providing a comprehensive review on the various designed implanted amplifiers for advanced biomedical applications. The reported amplifiers vary with respect to the class/type of amplifier, implemented CMOS technology, frequency band, output power, and the overall efficiency of the designs. The purpose of the authors is to provide a general view of the available solutions, and any researcher can obtain suitable circuit designs that can be selected for their problem by reading this survey