Analysis of carrier injection under high temperature AC operation in top gate IGZO TFTs

Abstract– With the development of high-quality displays, metal oxides gradually become a popular active layer in TFTs [1]. In this work, InGaZnO thin film transistors with double-layer oxide are investigated. The oxide layer is divided into top and bottom layers. We improve the characteristics and reliability of the device through the design of double-layer oxide stack structure. The bottom oxide layer is deposited with a lower SiH4 flow rate, and the top oxide layer is deposited with a higher SiH4 flow rate. By increasing the SiH4 flow rate of the top oxide layer, two effects can be achieved. Firstly, it is beneficial for speeding up the film deposition process. Furthermore, the hydrogen residue passivates the dangling bonds in the oxide layer and increases the bonding amount of silanol groups, SiO-H, and achieve hydrogen channel doping [2]. By modulating the SiH4 flow rate of the top oxide layer, the basic characteristics of the devices and the reliability under alternating current (AC) operation are improved. In this work, we use three waveform types of switch process to analyze the degradation under AC stress, and the physic mechanism is proposed subsequently [3-4]. After AC stress, the top oxide layer with higher SiH4 flow rate has a smaller threshold voltage right shift, and the reliability is significantly improved. Please click Download on the upper right corner to see the full abstract

Yield enhancement of recombinant α-Amylases in Bacillus amyloliquefaciens by ARTP mutagenesis-screening and medium optimization

α-Amylase is the most extensively applied enzyme in industry. There is an urgent need for improvement on the yield of α-amylases currently. Herein, a strategy which combined Atmospheric and Room Temperature Plasma (ARTP) mutagenesis tool for construction of mutant library of Bacillus amyloliquefaciens with a 24-well plates screening technique was adopted to improve the yield of recombinant Bacillus amyloliquefaciens α-amylases (BAA). A mutant strain named B. amyloliquefaciens ZN mut-7# was obtained, and the activity of BAA produced by this mutant strain was 86.92% higher than that of the original strain. B. amyloliquefaciens ZN mut-7# has an unchanged BAA gene and genetic stability. This successful application proved that ARTP can be applied to the genetically engineering strains that contain recombinant plasmid. Furthermore, response surface methodology offers an achievable and efficient strategy to optimize the composition of medium used to generate BAA in B. amyloliquefaciens ZN mut-7#. A 1.28-fold increase had been obtained compared to the production of non-optimized fermentation medium. This study demonstrates that ARTP mutagenesis and medium optimization are efficient and feasible methods for increasing recombinant enzyme production in the genetically engineering strains

Empirical modeling of the stellar spectrum of galaxies

An empirical method of modeling the stellar spectrum of galaxies is proposed, based on two successive applications of Principal Component Analysis (PCA). PCA is first applied to the newly available stellar library STELIB, supplemented by the J, H and K$_{s}$ magnitudes taken mainly from the 2 Micron All Sky Survey (2MASS). Next the resultant eigen-spectra are used to fit the observed spectra of a sample of 1016 galaxies selected from the Sloan Digital Sky Survey Data Release One (SDSS DR1). PCA is again applied, to the fitted spectra to construct the eigen-spectra of galaxies with zero velocity dispersion. The first 9 galactic eigen-spectra so obtained are then used to model the stellar spectrum of the galaxies in SDSS DR1, and synchronously to estimate the stellar velocity dispersion, the spectral type, the near-infrared SED, and the average reddening. Extensive tests show that the spectra of different type galaxies can be modeled quite accurately using these eigen-spectra. The method can yield stellar velocity dispersion with accuracies better than 10%, for the spectra of typical S/N ratios in SDSS DR1.Comment: 34 pages with 18 figures, submitted to A

Hybrid nature of 0846+51W1: a BL Lac object with a narrow line Seyfert 1 nucleus

We have found a NLS1 nucleus in the extensively studied eruptive BL Lac, 0846+51W1, out of a large sample of NLS1 compiled from the spectroscopic dataset of SDSS DR1. Its optical spectrum can be well decomposed into three components, a power law component from the relativistic jet, a stellar component from the host galaxy, and a component from a typical NLS1 nucleus. The emission line properties of 0846+51W1, FWHM(Hbeta) ~ 1710 km s^-1 and [OIII]5007/Hbeta ~ 0.32 when it was in faint state, fulfil the conventional definition of NLS1. Strong FeII emission is detected in the SDSS spectrum, which is also typical of NLS1s. We try to estimate its central black hole mass using various techniques and find that 0846+51W1 is very likely emitting at a few times 10% L_Edd. We speculate that Seyfert-like nuclei, including NLS1s, might be concealed in a significant fraction of BL Lacs but have not been sufficiently explored due to the fact that, by definition, the optical-UV continuum of such kind of objects are often overwhelmed by the synchrotron emission.Comment: ChJAA accepte