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Zhi-Hao Chen

Publications and source records attributed to Zhi-Hao Chen.

3 recordsLinked to original sources

Mie-lithography: void-resonance-assisted femtosecond laser printing for deep-ultraviolet to near-infrared nano dispersion devices

Nanoscale control of optical dispersion is essential for applications ranging from miniaturized spectrometers to color printing, all of which demand broadband spectral tunability. However, the Kramers-Kronig relations impose a fundamental trade-off between dispersion and loss, strictly limiting the design ability of single-material devices across the deep ultraviolet (DUV) to near-infrared (NIR) regimes. Consequently, the fabrication of miniaturized dispersion devices heavily relies on costly nanofabrication or heterogeneous integration. Here we overcome these limitations by shifting the light-matter interaction from solid structure into air-filled voids. We introduce a fabrication strategy termed "Mie-lithography", in which laser printed seed nanocavities excite Mie resonances in air and the resulting localized field enhancement drives the self-assembly of three-dimensionally tunable void-type optical resonators. Because the resonant modes are primarily confined within air voids, this architecture effectively alleviates material-imposed dispersion-loss constraints, allowing on-demand customization of the broadband spectral response. This approach could enable single-step, high-throughput (>= 10^6 pixels/s) printing of dispersion units with a resolution of 63,500 DPI. As a proof of concept, we demonstrate a single-material nano dispersion device for spectral encoding from 200 to 800 nm, with spectral reconstruction using a camera. Our approach can be extended into a platform for ultra-broadband (DUV-NIR) nano devices fabrication and design, opening avenues for high-pixel-density displays and miniaturized spectrometers.

physics.optics↗

Find The Optimized Structure of 5CBs

We use density functional theory (DFT) to investigate the geometric and electronic structures of multiple 5CB molecules. There are three parts for this research, test of the arrangement property of the 5CB molecule, calculation of two 4-n-pentyl-4-cyanobiphenyl (5CB), and four molecules 5CB structure arrangement. First part reveals the result, which the two 5CBs pointing in opposite directions case possesses lower total energy, that has the same result of the optimized caused by the nematic property of 5CBs. In the result of two 5CBs calculation, two 5CBs optimized structures always appears at least one pair of parallel plains formed by the head benzene of one 5CB and the carbon chain. In the four 5CBs optimized structure case, we can find out several pairs of parallel plains consist of benzene plains and one parallel plain in two carbon chain.

cond-mat.mtrl-sci↗

The Tsinghua University-Ma Huateng Telescopes for Survey: Overview and Performance of the System

Over the past decade, time-domain astronomy in optical bands has developed rapidly with the operations of some wide-field survey facilities. However, most of these surveys are conducted with only a single band, and simultaneous color information is usually unavailable for the objects monitored during the survey. Here we present introductions to the system of Tsinghua University-Ma Huateng Telescopes for Survey (TMTS), which consists of an array of four optical telescopes installed on a single equatorial mount. Such a system is designed to get multiband photometry simultaneously for stars and transients discovered during the survey. The optics of each telescope is a modified Hamilton-Newtonian system, covering the wavelengths from 400 to 900 nm, with a field of view (FoV) of about 4.5 deg2 and a plate scale of 1.86"/pixel when combining with a 4K*4K QHY4040 CMOS detector. The TMTS system can have a FoV of about 9 deg2 when monitoring the sky with two bands (i.e., SDSS g and r filters) at the same time, and a maximum FoV of ~18 deg2 when four telescopes monitor different sky areas in monochromatic filter mode. For an exposure time of 60 s, the average 3σ detection limit of the TMTS system can reach at ~19.4 mag in Luminous filter and at ~18.7 mag in SDSS r filter. The preliminary discovery obtained during the first few months' survey is briefly discussed. As this telescope array is located at the Xinglong Observatory of NAOC, it can have an excellent synergy with the spectroscopic survey by the LAMOST (with a FoV of about 20 deg2) at the same site, which will benefit the studies of stellar and binary physics besides the transient sciences.

astro-ph.IM↗