Weighing Black Holes with The Australian Dark Energy Survey

通过澳大利亚暗能量调查测量黑洞的重量

• 批准号: DP160100930
• 负责人: Prof Tamara Davis
• 金额: $ 25.35万
• 依托单位: The University of Queensland
• 依托单位国家: 澳大利亚
• 项目类别: Discovery Projects
• 财政年份: 2016
• 资助国家: 澳大利亚
• 起止时间: 2016-01-01 至 2019-12-31
• 项目状态: 已结题
• 来源: https://dataportal.arc.gov.au/RGS/Web/Grants/DP160100930
• 关键词: Weighing; Black; Holes; Australian; Dark

This project plans to measure how supermassive black holes have evolved over the last 12 billion years. Direct measurements of central black hole masses only exist for about 40 relatively nearby galaxies. The unique time-lapse observations and five-year baseline of the Australian Dark Energy Survey will enable us to measure masses for about 400 black holes, an order of magnitude more than previously possible. In addition to weighing black holes, recent results show that with precision measurement these systems may provide a standard candle, a new fundamental yardstick for cosmology. Unlike supernova observations that discovered dark energy, our measurements are practical to distances stretching back across 90 per cent of the observable universe.

该项目计划衡量过去120亿年中超级质量的黑洞如何发展。中央黑洞质量的直接测量仅存在于大约40个相对银河系附近。澳大利亚黑暗能源调查的独特延时观测和五年的基线将使我们能够测量约400个黑洞的质量，这是比以前更多的数量级。除了加权黑洞外，最近的结果还表明，通过精确测量，这些系统可能会提供标准的蜡烛，这是一种新的宇宙学基本尺寸。与发现暗能量的超新星观测值不同，我们的测量方法对延伸到90％可观察到的宇宙的距离是实用的。