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Miniquasars in the Dark Ages: Cosmological simulations of black holes with radiative transfer

Miniquasars in the Dark Ages: Cosmological simulations of black holes with radiative transfer
黑暗时代的小类星体:具有辐射传输的黑洞的宇宙学模拟
批准号:
1009781
负责人:
Tiziana Di Matteo
金额:
$43.48万
依托单位:
依托单位国家:
美国
项目类别:
Standard Grant
财政年份:
2010
资助国家:
美国
项目状态:
已结题
起止时间:
2010-09-15 至 2016-08-31

项目摘要

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中文摘要
翻译
再电离之前和期间的时代即将通过红外线和无线电仪器以及精细尺度微波背景实验的组合而在观测上变得可用。 因此,了解在黑暗时代结束时重新加热和重新电离星系际介质的源的性质是至关重要的。 该项目将研究类星体在高红移宇宙中的作用,结合类星体和星系形成和生长的从头算宇宙学模拟与高分辨率辐射传输,以执行该时代的第一个完全自洽的建模。 类星体通过热反馈和电离辐射的贡献,到目前为止在理论预测中基本上缺失,很可能在早期阶段占主导地位,并大大修改中性氢中看到的大尺度结构。 这些模拟将揭示硬X射线源预电离和恒星源贡献的复杂相互作用,研究星系际气体的物理状态,并对射电源的数量和性质进行详细的物理预测。这些结果对以后看到的从类星体和超大质量黑洞到矮星系追踪的大尺度结构具有重要意义。 由于对黑暗时代的第一次观测研究即将到来,成为一个新的新兴领域的一部分将使参与研究的研究生和本科生受益。 研究结果将纳入现有的外展计划,与来自代表性不足群体的中学生合作,并纳入本科课程项目。
英文摘要
The epoch before and during reionization is about to become accessible observationally through a combination of infrared and radio instruments and fine scale microwave background experiments. Understanding the nature of sources that reheated and reionized the intergalactic medium at the end of the dark ages is therefore crucial. This project will investigate the role of quasars in the high redshift Universe, combining ab initio cosmological simulations of quasar and galaxy formation and growth with high resolution radiative transfer to perform the first fully self consistent modeling of this epoch. The contribution of quasars through both thermal feedback and ionizing radiation, so far largely missing in theoretical predictions, is likely to dominate the early stages and substantially modify the large scale structure seen in neutral hydrogen. The simulations will reveal the complex interplay of pre-ionization by hard X-ray sources and the contribution of stellar sources, study the physical state of intergalactic gas, and make detailed physically motivated predictions of the number and character of radio sources.These results have major implications for what is seen later, from quasars and supermassive black holes to the large-scale structure traced by dwarf galaxies. As the first observational studies of the dark ages are just on the horizon, being part of a new, emerging field will benefit the graduate student and undergraduates involved in the research. The results will be incorporated in an existing outreach program working with middle school students from underrepresented groups, and included in undergraduate coursework projects.
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The First Billion Years: a Petascale Universe of Galaxies and Quasars
  • 批准号:
    1614853
  • 项目类别:
    Standard Grant
  • 资助金额:
    $4.0万
  • 财政年份:
    2016
  • 负责人:
    Tiziana Di Matteo
  • 依托单位:
Quasars and Large Scale Structure: Gigaparsec-scale simulations confront Large Survey Data
  • 批准号:
    1616168
  • 项目类别:
    Continuing Grant
  • 资助金额:
    $50.78万
  • 财政年份:
    2016
  • 负责人:
    Tiziana Di Matteo
  • 依托单位:
Petascale Cosmology with Gadget: Modeling the formation of the First Quasars with Blue Waters
  • 批准号:
    1036211
  • 项目类别:
    Standard Grant
  • 资助金额:
    $0.45万
  • 财政年份:
    2013
  • 负责人:
    Tiziana Di Matteo
  • 依托单位:
Toward Petascale Cosmology with GADGET
  • 批准号:
    0749212
  • 项目类别:
    Standard Grant
  • 资助金额:
    $81.48万
  • 财政年份:
    2007
  • 负责人:
    Tiziana Di Matteo
  • 依托单位:
国内基金
海外基金
Baryogenesis, Dark Matter and Nanohertz Gravitational Waves from a Dark Supercooled Phase Transition
  • 批准号:
    24ZR1429700
  • 项目类别:
    省市级项目
  • 资助金额:
    --
  • 批准年份:
    2024
  • 负责人:
    YUICHIRO NAKAI
  • 依托单位:
微波有源Scattering dark state粒子的理论及应用研究
  • 批准号:
    61701437
  • 项目类别:
    青年科学基金项目
  • 资助金额:
    28.0万元
  • 批准年份:
    2017
  • 负责人:
    李欢
  • 依托单位: