Numerical Simulations of Non-Equilibrium Plasmas and Their Spectra

AST-0307720费兰我们对宇宙化学演化的许多理解都来自于对星际气体中产生的发射或吸收线的分析。该项目是对从附近的HII区域延伸到发光类星体的几个广泛战线的同时攻击，其共同主题是开发绘制其化学演化所需的工具。大部分工作集中在大规模等离子体模拟程序Cloudy的开发和应用上。这是一个多管齐下的努力，结合了观测天体物理学，数值模拟，原子和分子物理学。这些步骤强烈地交织在一起，从猎户座星云，到巨大的河外H II区30剑鱼座，最终到遥远类星体光谱中的吸收线所看到的介入系统。从中性氢分子的完整模型开始，通过完全自洽的光谱模拟，该项目将扩展到类氦物种，并首次应用于原始氦丰度。 通过其他扩展，结果应该是完全自洽的描述气体如何从其完全分子状态流动，最终进入通过光电离形成离子的区域，从而导致整个环境的几乎无参数描述。 这些模型将与猎户座星云和剑鱼座30（最近的巨大河外HII区域）的非常深的光谱进行测试。该项目核心的光谱模拟代码被其他研究人员用于每年产生100多篇论文的工作。 因此，在学生的大力参与下，包括作为其博士论文的一部分，代码开发对社区产生了非常广泛的影响。 从这个项目的结果也将被研究人员用来协助正在开发的计划，这将带来在职教师从中央肯塔基州到他的大学校园的研究简报和教学策略的讨论。

AST-0307720FerlandMuch of our understanding of the chemical evolution of the cosmos comes from the analysis of emission or absorption lines produced in interstellar gas. This project is a simultaneous attack on several broad fronts extending from nearby HII regions to luminous quasars with the common theme of developing the tools needed to chart their chemical evolution. Much of this work centers on the development and application of the large-scale plasma simulation code Cloudy. This is a multi-pronged effort that combines observational astrophysics, numerical simulations, and atomic and molecular physics. These steps are strongly interwoven and progress from the Orion Nebula, to the giant extragalactic H II region 30 Doradus, and eventually to the intervening systems seen by their absorption lines in spectra of distant quasars. Starting with a complete model of the neutral hydrogen molecule, with a fully self-consistent spectral simulation, the project will then extend to helium-like species, with an important first application to the primordial helium abundance. With other extensions, the result should be a fully self-consistent description of how gas flows from its fully molecular state, eventually into regions where ions are formed by photo-ionization, resulting in an almost parameter-free description of the entire environment. The models will be tested against very deep optical spectroscopy of the Orion Nebula and of 30 Doradus, the nearest giant extragalactic HII region.The spectral simulation code at the heart of this project is used by other researchers in work that produces over a hundred papers a year. Code development, with strong involvement by students, including as parts of their doctoral theses, therefore has a very wide impact on the community. Results from this project will also be used by the researcher to assist with a scheme under development which will bring in-service teachers from central Kentucky to his University campus for research briefings and teaching strategy discussions.