• 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.

• 한국가스학회지
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• 제26권3호
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• pp.45-53
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• 2022

디젤엔진의 배출물 개선을 위해 탄소수가 낮은 천연가스를 혼합하여 사용하는 천연가스-디젤 혼소 연소가 각광받고 있다. 특히 자발화 특성에 차이가 있는 디젤과 천연가스의 특성을 이용한 반응성 제어 압축착화(reactivity controlled compression ignition, RCCI) 연소 전략을 통해 기존 디젤엔진의 효율과 배출가스를 동시에 개선시키는 연구가 활발하게 진행되어 왔다. 상사점보다 앞당겨진 디젤 직접 분사시기 적용을 통해 실린더 전체 영역의 균일 혼합기를 형성하여 전체적으로 희박한 자발화 기반 연소를 달성함으로써 질소산화물 (NOx) 및 입자상물질 (PM) 저감과 제동열효율 개선을 동시에 달성할 수 있다. 하지만 매우 희박한 저부하 영역에서 불완전 연소량이 증가하는 단점이 존재하며, 안정적인 연소 구현을 위해 디젤 분사시기가 민감하게 제어되어야 하는 어려움도 존재한다. 본 연구에서는 앞서 언급된 저부하 영역에서의 천연가스-디젤 혼소 엔진의 효율 및 배기 개선을 확인하고, 동시에 발전용 엔진 구동 영역에서 디젤 분사시기에 따른 연소안정성을 평가하였다. 실험에는 6 L급 상용디젤 엔진이 사용되었으며, 1,800 rpm, 50% 부하 영역 (~50 kW)에서 실험이 진행되었다. 제동효율 및 연소안정성을 개선하기 위한 전략으로 분무 패턴이 다른 2개의 인젝터를 적용하였으며, 천연가스/디젤 비율과 디젤 분사시기를 바꿔가면서 실험이 진행되었다. 실험 결과, 협각 분사가 추가된 수정 인젝터에서 제동 열효율이 증가하는 것을 확인하였다. 또한 연소안정성 및 출력, 그리고 강화된 배기 규제를 고려하였을 때 수정 인젝터의 분무 패턴이 예혼합연소 형성에 적합하였고 이를 통해 질소산화물 배출량을 Tier-V 기준치인 0.4 g/kWh 이하로 저감함으로써 RCCI 연소 가능 영역을 확장할 수 있음을 실험적으로 확인하였다.