Exploration of the Non-normal Students’ Attitude to Taking Part in the Teacher Qualification Examination in China

As the teacher qualification examination has been extensively spread in China in recent years, a "national examination fever" is rising among non-normal students. A large number of non-normal college students have obtained the teacher certification by taking the qualification exam. It is found that there are all kinds of attitudes to the students’ participating in this exam. Firstly, they once had to choose a non-normal major on account of different reasons, although they expect to be teachers. Secondly, they hold a blind attitude that all their friends take part in it. Thirdly, it is a practical way to have a job choice after graduation. Therefore, we have a responsibility to remind the students to treat the examination rationally, because it can’t ensure them the capabilities required for a qualified teacher even if they have passed three or four subjects. Meanwhile, those who participate in the exam only plan to increase the possibility of getting employed instead of genuine enthusiasm for education can hardly enjoy satisfaction and happiness. Therefore, the non-normal students should recognize and understand the true purpose of the examination and make a rational career planning. At the same time, the government needs to improve the teacher qualification examination system

Integrated all-optical logic discriminators based on plasmonic bandgap engineering

Optical computing uses photons as information carriers, opening up the possibility for ultrahigh-speed and ultrawide-band information processing. Integrated all-optical logic devices are indispensible core components of optical computing systems. However, up to now, little experimental progress has been made in nanoscale all-optical logic discriminators, which have the function of discriminating and encoding incident light signals according to wavelength. Here, we report a strategy to realize a nanoscale all-optical logic discriminator based on plasmonic bandgap engineering in a planar plasmonic microstructure. Light signals falling within different operating wavelength ranges are differentiated and endowed with different logic state encodings. Compared with values previously reported, the operating bandwidth is enlarged by one order of magnitude. Also the SPP light source is integrated with the logic device while retaining its ultracompact size. This opens up a way to construct on-chip all-optical information processors and artificial intelligence systems.Comment: 4 figures 201

Ultrawide-band Unidirectional Surface Plasmon Polariton Launchers

Plasmonic devices and circuits, bridging the gap between integrated photonic and microelectronic technology, are promising candidates to realize on-chip ultrawide-band and ultrahigh-speed information processing. Unfortunately, the wideband surface plasmon source, one of the most important core components of integrated plasmonic circuits, is still unavailable up to now. This has seriously restricted the practical applications of plasmonic circuits. Here, we report an ultrawide-band unidirectional surface plasmon polariton launcher with high launching efficiency ratio and large extinction ratio, realized by combining plasmonic bandgap engineering and linear interference effect. This device offers excellent performances over an ultrabroad wavelength range from 690 to 900 nm, together with a high average launching efficiency ratio of 1.25, large average extinction ratio of 30 dB, and ultracompact lateral dimension of less than 4 um. Compared with previous reports, the operating bandwidth is enlarged 210 folds, while the largest launching efficiency ratio, largest extinction ratio, and small feature size are maintained simultaneously. This provides a strategy for constructing on-chip surface plasmon source, and also paving the way for the study of integrated plasmonic circuits.Comment: 4 figure

Supernova calibration by gravitational wave

Hubble tension is one of the most important problems in cosmology. Although the local measurements on the Hubble constant with Type Ia supernovae (SNe Ia) are independent of cosmological models, they suffer the problem of zero-point calibration of the luminosity distance. The observations of gravitational waves (GWs) with space-based GW detectors can measure the luminosity distance of the GW source with high precision. By assuming that massive binary black hole mergers and SNe Ia occur in the same host galaxy, we study the possibility of re-calibrating the luminosity distances of SNe Ia by GWs. Then we use low-redshift re-calibrated SNe Ia to determine the local Hubble constant. We find that we need at least 7 SNe Ia with their luminosity distances re-calibrated by GWs to reach a 2\% precision of the local Hubble constant. The value of the local Hubble constant is free from the problems of zero-point calibration and model dependence, so the result can shed light on the Hubble tension.Comment: 22 pages, 5 figures, 2 tables; Comments are welcom