Thermal & electrical simulation for the development of solid-phase polycrystalline silicon TFTs

Solid phase crystallization (SPC) is a processing technique used for conversion of amorphous silicon (a-Si) to polycrystalline silicon (poly-Si). SPC can potentially be used as an alternative to excimer laser annealing to fabricate the semiconductor layer for thin-film transistors (TFTs) in active-matrix liquid crystal display (AMLCD). It is a technique suitable for large-area applications since it involves easily scalable thermal processes in the form of rapid thermal annealing (RTA) and furnace annealing (FA). The SPC parameter space involves the time and temperature of the FA, and the time, temperature, and number of pulses in the RTA process. In developing new process flows for thin-film transistors (TFTs) using SPC, thermal and electrical device simulation are invaluable tools. Comsol® was utilized to explore this SPC experimental parameter space, and provided important insight on temperature conditions not directly measureable on glass substrates (see Fig. 1). Silvaco\u27s Atlas® was utilized to evaluate the TFT response variables of sub-threshold slope (SS), threshold voltage (VT), and maximum current (Imax). Further, a procedure for fitting TFT device characteristics using Atlas was developed. From this simulation fit (see Fig. 2), theoretical trap state distributions for the semiconducting film can be extracted, as well as the trap state distributions at the oxide-semiconductor interfaces

Germanium on Silicon Avalanche Photodiode for High-Speed fiber Communication

Silicon photonics is one of the promising technologies for high-speed optical fiber communications. Among various silicon photonic devices, germanium on silicon avalanche photodiode (Ge/Si APDs) received tremendous attentions because of its superior performance and integration compatibility. In 2016, normal incidence Ge/Si APD demonstrated a NRZ 10−12 sensitivity of −23.5 dBm at 25 Gb/s; more recently, a waveguide-integrated Ge/Si APD receiver presents a 106Gb/s PAM4 sensitivity of −18.9 dBm. These results are best reported performance among all APD-based devices, and these breakthroughs are mainly benefited from Ge/Si APD’s structure and material characteristics. Ge/Si APD adopts a separated charge-absorption-multiplication (SCAM) structure with a pure Ge absorber and an intrinsic Si avalanche layer. Since, Si is one of well-known best avalanche materials with large gain-bandwidth products and low ionization noise ratio, which make Ge/Si APDs demonstrating superior performance at high data rates. Moreover, this Si-based device is manufactured by standard CMOS foundries and is process-compatible with other silicon photonic devices including silicon-based waveguides, demux, hybrid, etc. This advantage simplifies the assembly of photonic systems and makes a large-scale integrated silicon photonic chip possible, which provides compact solutions for high-density communication systems. In this chapter, we review recent progresses on Ge/Si APD structure design, material, and performance

Synergies between interstellar dust and heliospheric science with an Interstellar Probe

We discuss the synergies between heliospheric and dust science, the open science questions, the technological endeavors and programmatic aspects that are important to maintain or develop in the decade to come. In particular, we illustrate how we can use interstellar dust in the solar system as a tracer for the (dynamic) heliosphere properties, and emphasize the fairly unexplored, but potentially important science question of the role of cosmic dust in heliospheric and astrospheric physics. We show that an Interstellar Probe mission with a dedicated dust suite would bring unprecedented advances to interstellar dust research, and can also contribute-through measuring dust - to heliospheric science. This can, in particular, be done well if we work in synergy with other missions inside the solar system, thereby using multiple vantage points in space to measure the dust as it `rolls' into the heliosphere. Such synergies between missions inside the solar system and far out are crucial for disentangling the spatially and temporally varying dust flow. Finally, we highlight the relevant instrumentation and its suitability for contributing to finding answers to the research questions.Comment: 18 pages, 7 Figures, 5 Tables. Originally submitted as white paper for the National Academies Decadal Survey for Solar and Space Physics 2024-203

Contents

Step-by-step configuration instructions for the BladeCente