• 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.

• Journal of the Korean Wood Science and Technology
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• 제38권4호
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• pp.333-340
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• 2010

한반도 남부 일대에서 자생하는 황칠나무(Dendropanax morbifera Lev.) 수액으로부터 추출한 천연 도료인 황칠도료(Korean Dendropanax lacquer)는 예로부터 귀중한 예술품이나 투구, 화살, 활 등의 전쟁도구를 찬란한 황금색으로 도장하는데 사용되어 왔다. 경화 후 황금색의 투명한 도막을 형성하여 우수한 색상특성을 지니고 있을 뿐만 아니라 내후성, 내수성, 내식성 등이 우수하여, 보호도장으로써도 훌륭한 가치를 지니고 있다. 그러나 이러한 많은 장점에도 불구하고, 현대적인 여러 적용분야에 사용되지 못하고 있는 이유는 황칠도료의 생산량이 적고, 이로 인하여 가격이 매우 고가이고, 장시간의 경화시간이 소요되는 문제도 큰 원인으로 작용하고 있다. 한편 황칠 내에 광중합이 가능한 conjugated diene을 포함한 모노머가 있으며, 이러한 모노머는 일광 조사 조건등에 의하여 짧은 시간에 단단하고 황금색을 띠는 도막을 형성할 수 있음이 보고된 바가 있다. 따라서 본 연구에 서는 전통적인 황칠도료의 경화방법을 개선하고 경화속도를 촉진하기 위하여, 열개시제를 도입하여 열경화를 촉진하는 방법과 열개시제 및 광개시제를 동시에 도입하고 이중경화(dual curing)에 의해서 경화속도를 촉진하고자 하였다. 이러한 경화 속도 및 경화 거동은 적외선분광분석기(FT-IR)을 이용하여 -C=C- 이중결합 특성피크의 변화를 관찰하거나, 진자경도계(pendulum hardness tester)를 이용하여 표면 경도의 변화를 관찰함으로써 평가하였다. 또한 강체진자물성측정기(RPT)에 spot UV curing 장비를 도입하여 이중경화에 의한 경화 속도 진을 평가하였다. 본 연구의 결과 열개시제에 의하여 열경화가 촉진될 수 있을 뿐만 아니라, 이중경화에 의하여 경화속도를 향상시킬 수 있음을 확인하였다. 또한 이러한 황칠도료 경화 속도 촉진 방법을 활용하여 전통적인 역에만 사용되어온 황칠도료를 현대적인 여러 적용분야에도 확대하여 사용할 수 있는 가능성을 제시하였다.