• 한국자기학회지
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• 제18권6호
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• pp.211-216
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• 2008

Si이 체심입방구조(body centered cubic; bcc) Fe에 불순물로 포함된 경우에 Fe의 전자구조와 자성에 미치는 영향을 스핀-궤도 상호작용(spin-orbit coupling, SOC)을 고려한 제일원리방법을 통하여 연구하였다. Si 불순물의 효과를 기술하기 위하여 27개의 원자가 포함된 bcc Fe 초격자 구조를 고려하였다. 제일원리방법은 전전자 총퍼텐셜선형보강평면파(all-electron full-potential linearized augmented plane wave, FLAPW) 방법을 일반기울기 근사(generalized gradient approximation, GGA) 하에서 계산하였다. 스핀-궤도 상호작용은 스핀대각항 만을 고려한 이차변분방법을 이용하여 자체충족적으로 계산하였다. SOC를 고려하지 않은 강자성(ferromagnetic, FM) 상태의 경우 Si 불순물의 경우에는 $-0.143{\mu}B$의 스핀 자기모멘트가 계산되었으며, Fe 원자가 Si 불순물에서 멀어지면서 각각 $2.214{\mu}B$, $2.327{\mu}B$, 및 $2.354{\mu}B$의 값을 얻었다. 그러나, SOC를 고려한 경우 Si 불순물의 스핀 자기모멘트는 $-0.144{\mu}B$로 계산되어 SOC의 효과가 크지 않았으나, Fe 원자의 경우 각각 $2.189{\mu}B$, $2.310{\mu}B$, 및 $2.325{\mu}B$로 계산되어 SOC를 고려한 경우 스핀 자기모멘트 값이 줄어드는 것을 알 수 있었다. 총전하 및 스핀밀도의 비교와 상태밀도의 비교를 통하여 이러한 현상은 Si 불순물에 의한 영향을 가리는데 참여하는 Fe 원자의 $t_{2g}$ 전자 궤도의 변형의 효과로서 SOC를 고려할 때만 얻을 수 있다.

• 한국진공학회:학술대회논문집
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• 한국진공학회 2016년도 제50회 동계 정기학술대회 초록집
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• pp.420.1-420.1
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• 2016

Colloidal quantum dot (CQD) is emerging as a promising active material for next-generation solar cell applications because of its inexpensive and solution-processable characteristics as well as unique properties such as a tunable band-gap due to the quantum-size effect and multiple exciton generation. However, the most widely used spin-coating method for the formation of the quantum dot (QD) active layers is generally hard to be adopted for high productivity and large-area process. Instead, the spray-coating technique may potentially be utilized for high-throughput production of the CQD solar cells (CQDSCs) because it can be adapted to continuous process and large-area deposition on various substrates although the cell efficiency is still lower than that of the devices fabricated with spin-coating method. In this work, we observed that the subsequent treatment of two different ligands, halide ion and butanedithiol, on the lead sulfide (PbS) QD layer significantly enhanced the cell efficiency of the spray CQDSCs. The maximum power conversion efficiency was 5.3%, comparable to that of the spin-coating CQDSCs.

• 한국세라믹학회지
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• 제53권3호
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• pp.338-342
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• 2016

ZnO thin film co-doped with F and Al was prepared on a glass substrate via simple non-alkoxide sol-gel spin coating. For a fixed F concentration, the addition of Al co-dopant was shown to reduce the resistivity mainly due to an increase in electrical carrier density compared with ZnO doped with F only, especially after the second post-heat-treatment in a reducing environment. There was no effective positive contribution to the reduction in resistivity due to the mobility enhancement by the addition of Al co-dopant. Optical transmittance of the ZnO thin film co-doped with F and Al in the visible light domain was shown to be higher than that of the ZnO thin film doped with F only.

• 한국해안해양공학회지
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• 제13권4호
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• pp.273-281
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• 2001

본 연구에서는 종횡비가 2인 직사각형 용기에 대한 스핀업 유동을 실험과 수치해석으로 연구하였다. 수치해석에서는 1차-, 2차- 에크만 펌핑 모형을 사용한 경우와 평정을 무시한 경우에 관해 유동장을 구하였으며, 실험에서는 고전적인 PIV 방법을 통하여 속도장을 구하였다. 연구결과, 1차-, 2차- 에크만 펌핑 모형은 실험과 유사하게 나타났으며, 펌핑을 무시한 경우는 상이한 유동양상을 보였다.

• 전기학회논문지P
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• 제51권2호
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• pp.82-86
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• 2002

A series of $Ni_xZn_yFe_{3-x-y}O_4$ films were prepared by spin-spray ferrite plating on glass substrates from aqueous solution at $90[^{\circ}C]$. The magnetic properties in terms of contents of Ni and Zn in the plated films are presented. All the films are polycrystalline with spinel structure. At x+y=0.58, the film presents preferential orientation. As composition of y in the films increases grain size and void in the films increases, while saturation magnetization and coercive force of the films decrease.

• Bulletin of the Korean Chemical Society
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• 제26권3호
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• pp.418-422
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• 2005

By introducing spin-coating method to the evaporation induced self-assembly (EISA) process, a simple and reproducible route in controlling the mesophase of silica thin films has been developed for the first time in this work. When a comparatively solvent-rich Si-sol (The atomic ratio of TEOS : F127 : HCl : $H_2O$ : EtOH = 1 : 0.006 : 0.2 : 9.2 : 30) was used as coating solution, the mesophase of resultant silica films was selectively controlled by adjusting the spin-on speed. The cubic mesophase has been obtained from the coating at a low rpm, such as 600 rpm, while the 2-D hexagonal mesophase is formed at a high rpm, such as 2,500 rpm. At a medium coating speed, a mixture of cubic and hexagonal mesophase has been found in the fabricated films. The present results confirm that the evaporation rate of volatile components at initial step is critical for the determination of mesopore structures during the EISA process.

• 대한화학회지
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• 제25권1호
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• pp.13-20
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• 1981

Iminoxyl biradical은 biradical spin probe로 액체결정에 주입시켜 그 결정의 director분포에 관한 역학적성질을 조사하는데 유용한 물질이다. 새로운 방법으로 iminoxyl biradical을 합성하는 과정에서 각 단계의 합성중간 생성물들을 녹는점측정과 NMR, IR, UV 및 Mass 등과 같은 분광학적인 방법으로 확인하였다. 최종 생성물인 iminoxyl biradical은 EPR 분광법으로 확인하고 두 spin간의 상호작용도 EPR peaks로 고찰하였다.

• Bulletin of the Korean Chemical Society
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• 제34권1호
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• pp.179-187
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• 2013

We describe newly developed software named KPACK for relativistic electronic structure computation of molecules containing heavy elements that enables the two-component ab initio calculations in Kramers restricted and unrestricted formalisms in the framework of the relativistic effective core potential (RECP). The spin-orbit coupling as relativistic effect enters into the calculation at the Hartree-Fock (HF) stage and hence, is treated in a variational manner to generate two-component molecular spinors as one-electron wavefunctions for use in the correlated methods. As correlated methods, KPACK currently provides the two-component second-order M${\o}$ller-Plesset perturbation theory (MP2), configuration interaction (CI) and complete-active-space self-consistent field (CASSCF) methods. Test calculations were performed for the ground states of group-14 elements, for which the spin-orbit coupling greatly influences the determination of term symbols. A categorization of three procedures is suggested for the two-component methods on the basis of spin-orbit coupling manifested in the HF level.

• Journal of Advanced Marine Engineering and Technology
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• 제25권4호
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• pp.857-868
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• 2001

The aerodynamic forces and wake structures of the non-rotating downstream cylinder which is located behind the spinning upstream cylinder in tandem and staggered arrangement have been investigated by experimental method at Re= $1.32{\times}10^4$. The measurements of wake flow and pressure distributions of downstream cylinder are carried out in various spin parameters by combination of both longitudinal spacing rations L/d=1.5, 3.0, 4.5 and transverse spacing ratios T/d =0.0, -0.5, 0.5. For the present experiment, it has been found that the spin parameter of spinning upstream cylinder affect more easily the downstream cylinder in tandem arrangement than that in staggered arrangement.

• 천문학회보
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• 제40권1호
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• pp.85.2-86
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• 2015

The YORP effect is non-gravitational force that changes the spin-status of asteroid. So far this effect has been directly detected only from the Near-Earth asteroids (Taylor et al. 2007; Lowry et al. 2007, 2014; Breiter et al. 2011; Durech et al. 2008, 2012). Pravec at el. 2008 found the evidences for changing spin rate of small asteroids (3 - 15 km) by the YORP effect in the Main-Belt and Mars-crossing asteroids. The Mars-crossing asteroids (1.3 < q < 1.66 AU) are objects that cross orbit of the Mars. The Mars-crossing asteroids are regarded as one of the main sources for the Near-Earth asteroids. We expect that rotation of Mars-crossing asteroids would be influenced by the YORP effect. We try to search observational evidence of the YORP effect for the Mars-crossing asteroid. Our target 2078 Nanking is a population of the Mars-crossing asteroid. First light-curve of 2078 Nanking was obtained from Mohamed et al. 1994, and Warner et al. 2015 recently published new observational data. We observed this asteroid on 26th Nov. 2014 and 17th Jan. 2015 using SOAO (Sobaeksan Optical Astronomy Observatory) 0.61 m telescope with 4K CCD. Using light-curve inversion method (Kaasalainen & Torppa 2001; Kaasalainen et al. 2001), we try to determine the pole orientation and shape model of this asteroid based on the combination of our light-curve and literature photometric data. Knowing spin parameters, such as rotational period and spin axis, are essential for studying the YORP effect. In this presentation, we provide some preliminary results of our recent study: light-curve and processing of shape modeling of 2078 Nanking. We plan to find observational clue for the YORP effect on the Mars-crossing asteroids.