• 한국재료학회지
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• 제20권5호
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• pp.278-288
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• 2010

High Pressure High Temperature (HPHT) treatment can significantly change the color of diamonds. We studied the variation of the optical properties according to the nitrogen arrangement in natural brown diamonds of various types (type IaAB, type IaB, type IaA > B, type IaA < B, IaA = B) after HPHT treatment. The diamonds with different arrangements of nitrogen were annealed at temperatures in the range $1700-1800^{\circ}C$ under a stabilizing pressure of 5 GPa. HPHT treated samples were analyzed using UV-Vis-NIR, FT-IR, and PL spectroscopy. The absorption and luminescence spectra were measured to compare the variations of nitrogen arrangement in the natural brown diamonds before and after HPHT treatment. After HPHT treatment, the brown coloration in all types of diamonds was reduced and a decrease in the peaks related to the A-aggregate of nitrogen was more predominant than the B-aggregate. Furthermore, the peaks related to N3 (415.4 nm), H4 (496.4 nm), and platelet decreased and the peaks related to H3 (503.2 nm) and G-band increased after HPHT treatment. In conclusion, spectroscopic analysis of natural brown diamonds after HPHT treatment showed that a yellow color was produced by absorption in the H3 centers and a green color was generated by interaction between absorptions of the H3 and H2 centers.

• 대한화학회지
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• 제38권9호
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• pp.653-659
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• 1994

pH 7인 수용액에서 2-thenoyltrifluoroacetone(TTA), n-octanol과 Triton X-100의 존재하에서 유로퓸과 사마륨의 형광세기가 크게 증가하였다. 또한 이 착물에 과량의 $La^{3+}$을 첨가할 때 형광세기가 100배 이상 증가하였다. 유로퓸과 사마륨의 최대 들뜨기 파장은 각각 345 nm과 380 nm이고, 최대 형광파장은 각각 617 nm, 567 nm 이었다. 유로퓸과 사마륨의 형광세기는 농도가 각각 $1{\times}10^{-7}∼1{\tiems}10^{-9}\;M,\;1{\tiems}10^{-5}∼1{\times}10^{-7}\;M$에서 직선적으로 증가하였고, 유로퓸은 $1{\times}10^{-11}\;M$ 그리고 사마륨은 $1{\times}10^{-8}\;M$까지 검출할 수 있었다.

• 대한화학회지
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• 제55권6호
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• pp.932-935
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• 2011

Using tetrabutyl titanate as precursor, $Eu^{3+}$ doped $TiO_2$ nano-powder was prepared by sol-gel method, the nature of luminescence of nano-powder was studied. The interaction of chlorpyrifos with $Eu^{3+}$ doped $TiO_2$ was studied by absorption and fluorescence spectroscopy. The results indicated the fluorescence intensity of $Eu^{3+}$ doped $TiO_2$ was quenched by chlorpyrifos and the quenching rate constant ($k_q$) was $1.24{\times}10^{11}\;L/mol{\cdot}s$ according to the Stern-Volmer equation. The dynamics of photoinduced electron transfer from chlorpyrifos to conduction band of $TiO_2$ nanoparticle was observed and the mechanism of electron transfer had been confirmed by the calculation of free energy change (${\Delta}G_{et}$) by applying Rehm-Weller equation as well as energy level diagram. A new rapid method for detection of chlorpyrifos was established according to the fluorescence intensity of $Eu^{3+}$ doped $TiO_2$ was proportional to chlorpyrifos concentration. The range of detection was $5.0{\times}10^{-10}-2.5{\times}10^{-7}mol/L$ and the election limit ($3{\sigma}$) was $3.2{\times}10^{-11}$ mol/L.

• 방사선산업학회지
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• 제6권2호
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• pp.119-123
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• 2012

The detection properties of gamma-irradiated (0~10 kGy) dried seaweed, dried shrimp, and seasoned dried filefish were investigated by photo-stimulated luminescence (PSL) and electron spin resonance (ESR). PSL could be used as a detection method on irradiated dried seaweed and dried shrimp as they showed photon counts greater than 5,000 counts/60 s (positive) in the irradiated samples with doses above l kGy. However, PSL could not be applied to detect irradiated seasoned dried filefish, because gamma-irradiated sample at 10 kGy even yielded photon counts less than 700 counts/60 s (negative). The ESR spectroscopy for only dried shrimp revealed specific signals derived from free radicals captured in the shell of shrimp. As a result, it is considered that PSL or ESR methods for detection of gamma-irradiated dried shrimp and only PSL can be used to detect gamma-irradiated seaweed. Furthermore, it is considered that hydrocarbon analysis of seasoned dried filefish containing fat by GC/MS and Thermo Luminance (TL) analysis of dried seaweed should be studied for detection of irradiation.

• 한국진공학회지
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• 제20권4호
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• pp.288-293
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• 2011

본 논문은 InGaN/GaN 다중양자우물 구조를 가지는 녹색 발광다이오드의 활성층 내 인듐(In) 조성비와 piezoelectric field에 대한 전계 흡수 현상을 연구하였다. 활성층 내 결정학적 성질과 In 조성비는 double crystal X-ray diffraction 측정으로 분석하였으며, $1{\times}1\;mm^2$ 대면적 칩을 제작하여 발광특성을 조사하였다. 또한, 활성층 내 piezoelectric field는 electro-reflectance spectroscopy로부터 측정한 compensation voltage를 이용해 계산하였고, 인가전압에 따른 photocurrent의 변화를 측정함으로써 녹색 발광 소자의 전기 광학적 특성을 분석하였다.

• Journal of Astronomy and Space Sciences
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• 제36권1호
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• pp.21-33
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• 2019

This paper focuses on the interpretation of radiation fluxes from active galactic nuclei. The advantage of positron annihilation spectroscopy over other methods of spectral diagnostics of active galactic nuclei (therefore AGN) is demonstrated. A relationship between regular and random components in both bolometric and spectral composition of fluxes of quanta and particles generated in AGN is found. We consider their diffuse component separately and also detect radiative feedback after the passage of high-velocity cosmic rays and hard quanta through gas-and-dust aggregates surrounding massive black holes in AGN. The motion of relativistic positrons and electrons in such complex systems produces secondary radiation throughout the whole investigated region of active galactic nuclei in form of cylinder with radius R= 400-1000 pc and height H=200-400 pc, thus causing their visible luminescence across all spectral bands. We obtain radiation and electron energy distribution functions depending on the spatial distribution of the investigated bulk of matter in AGN. Radiation luminescence of the non-central part of AGN is a response to the effects of particles and quanta falling from its center created by atoms, molecules and dust of its diffuse component. The cross-sections for the single-photon annihilation of positrons of different energies with atoms in these active galactic nuclei are determined. For the first time we use the data on the change in chemical composition due to spallation reactions induced by high-energy particles. We establish or define more accurately how the energies of the incident positron, emitted ${\gamma}-quantum$ and recoiling nucleus correlate with the atomic number and weight of the target nucleus. For light elements, we provide detailed tables of all indicated parameters. A new criterion is proposed, based on the use of the ratio of the fluxes of ${\gamma}-quanta$ formed in one- and two-photon annihilation of positrons in a diffuse medium. It is concluded that, as is the case in young supernova remnants, the two-photon annihilation tends to occur in solid-state grains as a result of active loss of kinetic energy of positrons due to ionisation down to thermal energy of free electrons. The single-photon annihilation of positrons manifests itself in the gas component of active galactic nuclei. Such annihilation occurs as interaction between positrons and K-shell electrons; hence, it is suitable for identification of the chemical state of substances comprising the gas component of the investigated media. Specific physical media producing high fluxes of positrons are discussed; it allowed a significant reduction in the number of reaction channels generating positrons. We estimate the brightness distribution in the ${\gamma}-ray$ spectra of the gas-and-dust media through which positron fluxes travel with the energy range similar to that recorded by the Payload for Antimatter Matter Exploration and Light-nuclei Astrophysics (PAMELA) research module. Based on the results of our calculations, we analyse the reasons for such a high power of positrons to penetrate through gas-and-dust aggregates. The energy loss of positrons by ionisation is compared to the production of secondary positrons by high-energy cosmic rays in order to determine the depth of their penetration into gas-and-dust aggregations clustered in active galactic nuclei. The relationship between the energy of ${\gamma}-quanta$ emitted upon the single-photon annihilation and the energy of incident electrons is established. The obtained cross sections for positron interactions with bound electrons of the diffuse component of the non-central, peripheral AGN regions allowed us to obtain new spectroscopic characteristics of the atoms involved in single-photon annihilation.

• 방사선산업학회지
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• 제6권4호
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• pp.305-310
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• 2012

This study examined radiation detection properties of imported perilla seeds, almonds, and soybeans. Food samples were irradiated at doses of 0.5, 1, 2, and 4 kGy and analyzed by photo-stimulated luminescence (PSL), thermoluminescence (TL), and electron spin resonance (ESR). The results of PSL showed that photon counts of irradiated perilla seeds and soybeans were $32,959counts{\cdot}60sec^{-1}$ and $7,234counts{\cdot}60sec^{-1}$, respectively, at an irradiation dose of 0.5 kGy, and the photon count of irradiated almonds was $5,581counts{\cdot}60sec^{-1}$ at an irradiation dose of 1 kGy. The results of TL showed that this technique is useful for detecting irradiated samples; the TL ratios ($TL_1/TL_2$) measured for the food samples at an irradiation dose of 0.5 kGy were 0.2301 for perilla seeds, 0.4595 for almonds, and 0.4827 for soy beans. Lastly, results of ESR spectroscopy for only soybeans revealed specific signals derived from free radicals captured in the cellulose. In conclusion, PSL, TL, and ESR methods can be used for the detection of gamma-irradiated soybean samples, whereas gamma-irradiated perilla seeds and almonds can be confirmed by a serial detection with a TL method after PSL.

• 공업화학
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• 제19권3호
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• pp.299-303
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• 2008

열경화가 가능한 PPV유도체인 poly[(2,5-dimethoxy-1,4-phenylenevinylene)-alt-(1,4-phenylenevinylene)] (Cross-PPV)를 Heck coupling 반응을 이용하여 합성하였다. Cross-PPV 박막은 $200^{\circ}C$에서 경화 시키면 일반적인 유기용매에 용해되지 않는 불용성의 고분자 박막이 된다. 열경화 전 후의 Cross-PPV의 구조는 FT-IR로 확인하였으며 구조의 차이는 크지 않았다. 경화된 Cross-PPV는 일반적인 유기용매에 대하여 내용매성이 강하다. 순환전압전류법과 흡수분광법으로 측정한 경화된 Cross-PPV의 호모 및 루모 에너지 준위는 각각 -5.11 eV와 -2.56 eV으로 ITO로 부터의 정공주입장벽(hole injection barrier)이 작아(약 0.1 eV) 정공주입층으로 효과적으로 사용 할 수 있다. 호모 및 루모 에너지 준위가 각각 -5.44 eV, -3.48 eV인 poly(1,4-phenylenevinylene-(4-dicyanomethylene-4H-pyran)-2,6-vinylene-1,4-phenylene-vinylene-2,5-bis(dodecyloxy)-1,4-phenylenevinylene) (PM-PPV)을 발광층으로 사용하여 두층의 구조(bilayer structure)를 갖는 소자(ITO/crosslinked Cross-PPV/PM-PPV/Al)를 제작, 특성을 평가한 결과 최대 효율은 0.024 cd/A, 최대 발광세기는 $45cd/m^2$으로 단층형 소자(ITO/PM-PPV/Al)(최대 효율 = 0.003 cd/A, 최대 발광세기 = $3cd/m^2$)에 비하여 매우 월등한 성능을 나타냄을 확인하였다. 또한 두층의 구조를 가지는 다층형 소자의 발광스펙트럼은 단층형 소자의 발광 스펙트럼과 동일하다. 이러한 사실들로 보아 ITO 및 Al에서 주입된 전자는 모두 발광층인 PM-PPV층에서 재결합(recombination)되어 여기자(exciton)가 형성되는 것으로 사료된다.

• 분석과학
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• 제14권2호
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• pp.159-166
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• 2001

한외여과법을 이용하여 휴믹산(Aldrich Co.)을 분자량 별로 3개의 소부분($F_1$: 1,000-10,000 daltons; $F_2$: 10,000-50,000 daltons; $F_3$: 100,000-300,000 daltons)으로 분리한 뒤, 적외선 분광법과 고체상태 C-13 핵자기공명 분광법을 이용하여 각 소부분의 구조적 특성을 규명하였고, pH 적정법을 이용하여 각 소부분의 카르복실산 작용기 함량을 결정하였다. 휴믹산과 금속이온과의 착물 반응 특성을 규명하기 위하여, Eu(III)과 각 소부분 휴믹산과의 착화합물($[Eu(III)]=1.0{\times}10^{-4}mol\;L^{-1}$, $(HA)=470-970mg\;L^{-1}$, at pH 5.0)을 Eu(III)의 $^7F_0-{^5}D_0$ 전이를 이용한 여기 스펙트럼으로 관찰하였다. 적외선 스펙트럼과 C-13 핵자기공명 스펙트럼 분석 결과, 100,000 dalton 이상의 고분자량의 휴믹산 분자는($F_3$) 높은 지방족 탄소함량을 가지며, 50,000 daltons 이하의 저 분자량의 휴믹산($F_1$, $F_2$) 분자는 상대적으로 높은 방향족 탄소 함량을 가짐을 확인하였다. pH 적정 결과 휴믹산은 분자의 크기가 커질수록 더 낮은 카르복실기 함량을 가짐을 확인하였다. Eu(III)-휴믹산 착물의 여기스펙트럼을 Lorenzian-Gaussian 식을 이용하여 분석한 결과, 휴믹산 분자의 크기가 커질수록 최대피크의 파장 위치가 더 낮은 에너지 방향으로 이동하였다. 이러한 피크 이동의 결과는 휴믹산 분자의 크기가 커질수록 Eu(III)과 결합하는 분자내 카르복실산의 배위수가 증가함을 나타내는 것으로서, C-13 NMR 스펙트럼 분석에서 밝혀진 휴믹산 분자의 구조적인 요인과의 관련성을 밝혔다.

• 한국식품영양과학회지
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• 제37권11호
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• pp.1529-1533
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• 2008

한약재의 방사선 조사여부를 확인하기 위해 도라지와 오가피에 $0{\sim}10\;kGy$의 감마선을 조사하고 PSL, TL 및 ERS 특성을 비교 검토하였다. PSL을 측정한 결과 비 조사된 한약재에서 한계치($T_1$)인 700보다 낮은 photon count 값을 보이면서 negative로 판정되었고, 0.15 kGy 이상 조사구는 한계치($T_2$)인 5,000보다 높은 photon count 값을 나타내면서 positive로 표시되어 방사선 조사된 것을 확인할 수 있었다. 또한 시료로부터 mineral을 분리하여 TL의 glow curve와 TL ratio($TL_1/TL_2$)를 확인하였다. 방사선 조사가 되지 않은 도라지와 오가피는 TL ratio가 0.007 이하의 값을 나타내었으며, 조사구(1.0 kGy 이상)에서는 0.314 이상의 TL ratio를 나타내었다. 도라지와 오가피는 본 연구에서 설정한 TL ratio의 한계치 0.1보다 높은 수치를 나타내어 방사선 조사여부 확인이 가능하였다. ESR 측정을 통한 방사선 조사 한약재 검지에서는 cellulose 라디칼에서 유래된 특이한 라디칼 신호를 보여주었고, 이는 도라지 시료에서 더욱 뚜렷하게 확인할 수 있었다. 이상의 결과에서 PSL, TL 및 ESR 분석은 도라지와 오가피의 방사선 조사 여부 확인에 적합한 방법임을 확인할 수 있었다