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Double electromagnetically induced transparency in a four-level lambda atomic system with doppler broadening 具有多普勒增宽的四级λ原子系统中的双电磁诱导透明度
Pub Date : 2023-12-04 DOI: 10.15625/0868-3166/18214
Hiền Nguyễn Thị Thu, Bang Nguyen Huy, Doai Le Van, D. Hoang Minh
In this paper, we study the formation of two electromagnetically induced transparency (EIT) windows in a four-level lambda atomic system with Doppler broadening. The depth and the width of the EIT windows are easily changed by adjusting the intensity of the controlling laser fields. Meanwhile, the position of the EIT windows is also easily shifted by changing the frequency of the laser fields. In particular, by turning on or off one of the two coupling laser fields, the probe field response can be switched between one or two EIT window regimes, i.e., it is possible to switch between absorption and transparency regimes, and vice versa. In addition, our analytical model also allows one to investigate the influence of temperature (or Doppler width) on EIT windows, which is necessary for experimental observations as well as related applications at room temperature.
本文研究了具有多普勒展宽的四能级λ原子体系中两个电致透明(EIT)窗口的形成。通过调节控制激光场的强度,可以很容易地改变EIT窗口的深度和宽度。同时,通过改变激光场的频率,可以很容易地改变EIT窗口的位置。特别是,通过打开或关闭两个耦合激光场中的一个,探针场响应可以在一个或两个EIT窗口区域之间切换,即可以在吸收和透明区域之间切换,反之亦然。此外,我们的分析模型还允许人们研究温度(或多普勒宽度)对EIT窗口的影响,这对于实验观察以及室温下的相关应用是必要的。
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引用次数: 0
Studying the Luminosity Function of Lyman Alpha Emitters Selected Behind 17 Lensing Clusters from Multi-Unit Spectroscopic Explorer (MUSE/VLT) Observations. 研究从多单元光谱探测器(MUSE/VLT)观测中选取的 17 个 Lensing 星团背后的莱曼阿尔法发射器的光度函数。
Pub Date : 2023-12-04 DOI: 10.15625/0868-3166/17734
Tran Thi Thai, Tuan Anh Pham, ROSER PELLO, Ilias Goovaerts, Muse Consortium
Studying the Luminosity Function of Lyman Alpha Emitters Selected Behind 17 Lensing Clusters from Multi-Unit Spectroscopic Explorer (MUSE/VLT) Observations.
研究多单元光谱探测器(MUSE/VLT)观测中17个透镜星团后莱曼α发射体的光度函数。
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引用次数: 0
Development of the segmented plastic scintillation detector GARi for studying $r$-process nucleosynthesis at RIBF 开发分段式塑料闪烁探测器 GARi,用于研究 RIBF 的 $r$ 过程核合成
Pub Date : 2023-12-04 DOI: 10.15625/0868-3166/17704
Minh Hue Bui, Ho Phong Vi, Shunji Nishimura
(beta)-decay properties of very neutron-rich nuclei, such as the half-life and the (beta)-delayed neutron emission probabilities, play an essential role in the astrophysical rapid neutron capture process (r-process), where elements heavier than iron may be synthesized. Investigating those crucial properties has been one of the main objectives of the experimental programs at the RIKEN RI Beam Factory (RIBF). Recently, the development of a fast-timing detector system comprising a highly segmented plastic scintillation detector GARi (Gas-cell Active detector for Radioisotope decay), a neutron time-of-flight detector array, and a LaBrtextsubscript{3} detector array is being conducted for the measurement of (beta)-delayed neutron emission and other related (beta)-decay properties of neutron-rich nuclei at the F11 decay station of RIBF. The GARi detector has been constructed from a fast, segmented plastic scintillator coupled with nine multi-anode photomultiplier tubes (PMTs), resulting in enhanced position sensitivity. Therefore, this detector can be employed as an implantation detector and can also serve as a trigger signal in neutron time-of-flight experiments. This work details the development of the GARi detector and the results tested with the radioactive sources.
(beta)-中子非常丰富的原子核的衰变特性,如半衰期和(beta) -延迟中子发射概率,在天体物理快中子捕获过程(r-过程)中起着至关重要的作用,在这个过程中可以合成比铁重的元素。研究这些关键特性一直是RIKEN束流工厂(RIBF)实验项目的主要目标之一。近年来,为了测量富中子核的(beta) -延迟中子发射及其他相关的(beta) -衰变特性,在RIBF F11衰变站研制了一个由高节段塑料闪烁探测器GARi (Gas-cell Active detector for radioactive isotope decay)、中子飞行时间探测器阵列和LaBr textsubscript{3}探测器阵列组成的快速定时探测器系统。GARi探测器是由一个快速的、分段的塑料闪烁体与9个多阳极光电倍增管(pmt)耦合而成,从而提高了位置灵敏度。因此,该探测器既可以作为注入探测器,也可以作为中子飞行时间实验的触发信号。这项工作详细介绍了GARi探测器的发展和用放射源测试的结果。
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引用次数: 0
Circumgalactic Enrichment in Local Dwarf Galaxies as Probed by Star-Formation Driven Outflows 恒星形成驱动外流探测到的本地矮星系的环银河富集现象
Pub Date : 2023-12-04 DOI: 10.15625/0868-3166/17728
Michael Romano
Galactic feedback driven by massive stars and active galactic nuclei plays a fundamen-tal role in regulating galaxy formation and evolution. In particular, intense starburst episodes can generate strong outflows able to suppress star formation by expelling large amount of dust and metals out of the galaxies, possibly enriching their circum (or even inter) galactic media. Local dwarf galaxies are particularly sensitive to feedback processes and offer a unique opportunity to study these phenomena in great details. We search for outflow signatures in a sample of ∼ 30 lo-cal dwarf galaxies drawn from the Dwarf Galaxy Survey. We make use of Herschel/PACS archival data to detect atomic outflows in the broad wings of observed [CII] 158 µm line profiles. We find that atomic outflows in these galaxies have typical mass-loading factors consistent with unity and velocities high enough to bring gas and dust outward. Our results can be used as input for chemical models, posing new constraints on the processes of dust growth and destruction in the interstellar medium of galaxies.
由大质量恒星和活动星系核驱动的星系反馈在调节星系的形成和演化中起着重要的作用。特别是,强烈的星暴事件可以产生强烈的流出物,通过将大量的尘埃和金属排出星系,可能丰富它们的环(甚至是星系间)介质,从而抑制恒星的形成。局部矮星系对反馈过程特别敏感,为详细研究这些现象提供了独特的机会。我们从矮星系调查中提取的¼30低卡矮星系样本中寻找流出信号。我们利用赫歇尔/PACS档案数据来探测观测到的[CII] 158 µm谱线宽翼中的原子流出。我们发现这些星系中的原子外流具有典型的质量加载因子,与单位一致,并且速度足够高,可以向外携带气体和尘埃。我们的结果可以作为化学模型的输入,对星系星际介质中尘埃生长和破坏的过程提出新的限制。
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引用次数: 0
Big-bang Nucleosynthesis on a bubble universe nucleated in Kerr-AdS5. 在 Kerr-AdS5 中成核的气泡宇宙上的大爆炸核合成。
Pub Date : 2023-12-04 DOI: 10.15625/0868-3166/17900
Issei Koga, Akira Dohi, Naritaka Oshita, Kazushige Ueda
Modelling the Galactic chemical evolution (GCE) of short-lived radioisotopes (SLRs, with half-lives of the order of million years) can provide timing information on recent nucleosynthesis. The knowledge of their spatial distribution throughout the interstellar medium (ISM) is crucial. We are using a three-dimensional GCE model to investigate the evolution of four SLRs: (^{53})Mn from supernovae of type Ia (SNeIa), (^{60})Fe from core-collapse supernovae (CCSNe), (^{182})Hf from stellar winds from intermediate mass stars (IMSs), and (^{244})Pu from neutron star mergers (NSMs) to explain the recent (within the last $approx 1 -- 20$ Myr) deposition of live SLRs into deep-sea reservoirs. We find that although these SLRs are produced at very different nucleosynthetic sites, they are deposited on Earth conjointly.
对短寿命放射性同位素(SLRs,半衰期为百万年)的银河系化学演化(GCE)进行建模,可以提供最近核合成的时间信息。了解它们在星际介质(ISM)中的空间分布是至关重要的。我们使用三维GCE模型来研究四种slr的演化:(^{53})来自Ia型超新星(SNeIa)的Mn, (^{60})来自核心坍缩超新星(CCSNe)的Fe, (^{182})来自中质量恒星(IMSs)的恒星风的Hf,以及(^{244})来自中子星合并(nsm)的Pu,以解释最近(在最后$approx 1 -- 20$ Myr内)活slr沉积到深海储层中的原因。我们发现,虽然这些单反是在不同的核合成位点产生的,但它们是共同沉积在地球上的。
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引用次数: 0
Galactic Chemical Evolution with the short lived radioisotopes (^{53}textbf{Mn}), (^{60}textbf{Fe}), (^{182}textbf{Hf}), and (^{244}textbf{Pu}) 使用短寿命放射性同位素((^{53}textbf{Mn})、((^{60}textbf{Fe})、((^{182}textbf{Hf})和((^{244}textbf{Pu})的银河化学演变
Pub Date : 2023-09-18 DOI: 10.15625/0868-3166/17727
Benjamin Wehmeyer, Andr´es Yag¨ue L´opez, Benoit Cˆot´e, Maria K. Pet˝o, Chiaki Kobayashi, Maria Lugaro
Modelling the Galactic chemical evolution (GCE) of short-lived radioisotopes (SLRs, with half-lives of the order of million years) can provide timing information on recent nucleosynthesis. The knowledge of their spatial distribution throughout the interstellar medium (ISM) is crucial. We are using a three-dimensional GCE model to investigate the evolution of four SLRs: (^{53})Mn from supernovae of type Ia (SNeIa), (^{60})Fe from core-collapse supernovae (CCSNe), (^{182})Hf from stellar winds from intermediate mass stars (IMSs), and (^{244})Pu from neutron star mergers (NSMs) to explain the recent (within the last $approx 1 -- 20$ Myr) deposition of live SLRs into deep-sea reservoirs. We find that although these SLRs are produced at very different nucleosynthetic sites, they are deposited on Earth conjointly.
建立短寿命放射性同位素(SLR,半衰期约为百万年)的银河化学演化(GCE)模型可以提供有关近期核合成的时间信息。了解它们在整个星际介质(ISM)中的空间分布至关重要。我们正在使用一个三维 GCE 模型来研究四种 SLR 的演化:(^{53})Mn来自Ia型超新星(SNeIa),(^{60})Fe来自核坍缩超新星(CCSNe),(^{182})Hf来自中等质量恒星(IMSs)的恒星风、和来自中子星合并(NSMs)的(^{244})Pu来解释最近(在过去大约1-20百万年内)活的SLRs沉积到深海储层的现象。我们发现,尽管这些SLR是在非常不同的核合成地点产生的,但它们是共同沉积在地球上的。
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引用次数: 0
Investigation of Elemental Deposition in Lamdong Province (Vietnam) by the Moss Biomonitoring Method and Neutron Activation Analysis 利用苔藓生物监测方法和中子活化分析研究越南兰东省的元素沉积
Pub Date : 2023-09-05 DOI: 10.15625/0868-3166/18266
Thi Minh Sang Nguyen, Anh Son Nguyen, L. Khiem, Thi Thanh Tran Le, Tuan Anh Tran, Huu Thang Ho, I. Zinicovscaia, M. Frontasyeva, Dai Nam Le, Thi Xuan Thai Nguyen
The results of an investigation of heavy metal air pollution in Lamdong province (Vietnam) using the moss biomonitoring method are presented in this paper. Barbula Indica moss samples were collected at 30 different locations in Dalat and Baoloc, two major cities of Lamdong province. The concentrations of 10 heavy metal and metalloid elements, Sc, V, Cr, Mn, Fe, Co, Zn, As, Hf, and Ta in the collected moss samples, were determined by the neutron activation analysis method using the nuclear reactor at the Nuclear Research Institute in Dalat. The results show that the air in Lamdong province may be polluted by Mn and is moderately polluted by Sc, V, Cr, Fe, Co, Zn, As, Hf and Ta. The main sources of heavy metal pollution in the Lamdong atmosphere may be soil dust, traffic emissions, industry, bauxite mining and refining, chemical fertilizers and pesticides, and combustion of coal and oil. By comparing heavy element concentrations in the moss from Lamdong with that of Hanoi, Thainguyen, and several European countries, it is found that heavy metal air pollution in Lamdong is much lower than in Hanoi and Thainguyen and much higher than in the European countries.
本文介绍了利用苔藓生物监测方法对越南兰东省大气重金属污染进行调查的结果。在澜东省两个主要城市大叻和宝洛克的30个不同地点采集了印度斑纹苔藓样本。利用大拉特核研究所的核反应堆,采用中子活化分析法测定了收集的苔藓样品中Sc、V、Cr、Mn、Fe、Co、Zn、As、Hf、Ta等10种重金属和类金属元素的浓度。结果表明:兰东省大气中存在Mn污染,Sc、V、Cr、Fe、Co、Zn、As、Hf、Ta污染较为严重;蓝东大气中重金属污染的主要来源可能是土壤粉尘、交通排放、工业、铝土矿开采和精炼、化肥和农药以及煤和石油的燃烧。通过与河内、坦茵和几个欧洲国家苔藓中重金属浓度的比较,发现兰东的重金属空气污染远低于河内和坦茵,远高于欧洲国家。
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引用次数: 0
Adsorption capacity of a hydrogen atom on the 2D silicon carbide surface 二维碳化硅表面氢原子的吸附能力
Pub Date : 2023-09-05 DOI: 10.15625/0868-3166/18091
T. T. Hanh
Hydrogen adsorption on two-dimensional (2D) silicon carbide (SiC) was studied using molecular dynamics and ab initio calculations. By investigating a converged density functional theory (DFT) calculation, the stable adsorption sites of a hydrogen atom on the 2D SiC were found at the top sites (T­Si and T­C, of which the most stable adsorption site is T­Si). The adsorption of a hydrogen atom on 2D silicon carbide led to local structural changes in silicon carbide.
采用分子动力学和从头算方法研究了二维(2D)碳化硅(SiC)对氢的吸附。通过收敛密度泛函理论(DFT)计算,发现二维SiC上氢原子的稳定吸附位点位于顶部(T-Si和T-C),其中最稳定的吸附位点是T-Si。一个氢原子在二维碳化硅上的吸附导致了碳化硅的局部结构变化。
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引用次数: 0
Size-controlled synthesis of ZnO nanorods for highly sensitive NO(_2) gas sensors 用于高灵敏度NO (_2)气体传感器的ZnO纳米棒的尺寸控制合成
Pub Date : 2023-08-15 DOI: 10.15625/0868-3166/18355
Lưu Hoàng Minh, Pham Thi Thuy Thu, Luong Minh Tuan, Bui Quang Thanh, Mai Thi Hue, Ta Thi Tho, Pham Van Tong
The nanostructure of zinc oxide has excellent potential in gas sensing applications to detect and monitor toxic gases in the atmosphere. Appropriate nanostructures can enhance the performance of gas sensors. In this study, we report the controlled fabrication of ZnO nanorods of different sizes by a simple hydrothermal method, which can be applied to detect NO2 toxic gas efficiently. The size of the nanorods was controlled by varying the amount of D-Glucose. The morphology and crystal structure of the materials were analyzed using advanced techniques such as field-emission scanning electron microscopy, X-ray diffraction patterns, and energy-dispersive X-ray spectroscopy. The sensor's response based on ZnO nanorods at 2 ppm NO2 is 13.3 and 18.8 times higher than that of 500 ppm CO and NH3, respectively. In addition, the sensor also exhibits good selectivity and repeatability for NO2 toxic gas; The optimum working temperature is about 150 oC.[H_2= H_1+ H_1 tag{1}] H2 hoac H2
氧化锌的纳米结构在大气中有毒气体的检测和监测方面具有良好的应用潜力。适当的纳米结构可以提高气体传感器的性能。在这项研究中,我们报道了用简单的水热法控制制备不同尺寸的ZnO纳米棒,该纳米棒可以有效地用于检测NO2有毒气体。通过改变d -葡萄糖的量来控制纳米棒的大小。利用场发射扫描电子显微镜、x射线衍射图和能量色散x射线光谱学等先进技术分析了材料的形态和晶体结构。基于ZnO纳米棒的传感器在2 ppm NO2条件下的响应分别是500 ppm CO和NH3条件下的13.3和18.8倍。此外,该传感器对NO2有毒气体也表现出良好的选择性和重复性;最佳工作温度为150℃左右。[H_2= H_1+ H_1 tag{1}] H2 hoac H2
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引用次数: 0
Effect of dipolar interaction on magnetic properties of magnetite nanoparticles system: a simulation study 偶极相互作用对磁铁矿纳米颗粒磁性能影响的模拟研究
Pub Date : 2023-08-12 DOI: 10.15625/0868-3166/17642
Hoang Thanh Nguyen, T. N. Lan, Tuan N. M.
Superparamagnetic iron oxide nanoparticles are a potential candidate for novel research. The inter-particle interactions play a significant role in determining the overall magnetic behavior of a magnetic nanoparticle assembly, especially in dipolar interaction. In this paper, we have synthesized a practical sample and then applied an atomistic spin model simulation study with input parameters obtained from experimental measurements to investigate the influence of the dipolar interaction on the magnetic properties of Fe3O4 magnetite nanoparticles. 
超顺磁性氧化铁纳米颗粒是一种潜在的新研究对象。粒子间的相互作用在决定磁性纳米粒子的整体磁性行为中起着重要的作用,特别是在偶极相互作用中。在本文中,我们合成了一个实际样品,然后应用原子自旋模型模拟研究了偶极相互作用对Fe3O4磁铁矿纳米颗粒磁性能的影响。
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引用次数: 0
期刊
Communications in Physics
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