Studies of Interstellar Processes

星际过程研究

• 批准号: 9988126
• 负责人: Bruce Draine
• 金额: $ 36.37万
• 依托单位: Princeton University
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2000
• 资助国家: 美国
• 起止时间: 2000-07-01 至 2005-09-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=9988126&HistoricalAwards=false
• 关键词: Studies; Interstellar; Processes

Dr. Bruce Draine of Princeton University will lead studies of a variety of processes in the interstellar medium. He will investigate the size distribution of very small interstellar grains. With the constraints provided by the observed wavelength-dependent interstellar extinction, Dr. Draine expects to obtain the best determination to date of the size distribution of interstellar grains. New models of photo-dissociation regions will be developed, using improved estimates of photoelectric heating rates, and detailed modeling of radiative and collisional excitation/de-excitation of molecular hydrogen (H2). He will extend previous studies on spherical grains to consider nonspherical grain shapes in order to obtain realistic estimates for the net force on irregular interstellar grains. He will study the observable consequences if a gamma ray burst (GRB) takes place in a dense molecular cloud, including the destruction of dust, thermal emission from hot dust, the appearance of absorption features due to vibrationally-excited H2, and ultraviolet fluorescent emission from H2. Studies will be conducted into the role of "thermal flipping" and "thermal trapping" in the physics of interstellar grain alignment. Dr. Draine will attempt to improve the treatment of strongly-absorbing materials in the discrete dipole approximation (DDA). This would allow the DDA to be used to calculate the infrared absorption cross sections of irregular grains composed of materials like amorphous carbon. He also expects to continue to support and maintain the portable program DDSCAT, which is used by researchers in a number of disciplines to compute scattering and absorption by irregular targets.

普林斯顿大学的布鲁斯德莱恩博士将领导对星际介质中各种过程的研究。 他将研究非常小的星际颗粒的尺寸分布。 在观测到的波长依赖性星际消光提供的约束下，Draine博士希望获得迄今为止星际颗粒尺寸分布的最佳测定。 将开发新的模型的光解离区域，使用改进的光电加热速率的估计，和详细的建模的辐射和碰撞激发/去激发的分子氢（H2）。 他将扩展以前对球形颗粒的研究，考虑非球形颗粒的形状，以获得对不规则星际颗粒的净力的现实估计。 他将研究可观察到的后果，如果伽马射线暴（GRB）发生在一个密集的分子云，包括灰尘的破坏，热尘埃的热发射，由于振动激发的H2吸收功能的外观，和紫外荧光发射从H2。将研究“热翻转”和“热俘获”在星际颗粒排列物理学中的作用。 Dr. Draine将尝试改进离散偶极子近似（DDA）中强吸收材料的处理。这将允许DDA用于计算由无定形碳等材料组成的不规则颗粒的红外吸收截面。他还希望继续支持和维护便携式程序DDSCAT，该程序被许多学科的研究人员用于计算不规则目标的散射和吸收。