Testing General Relativity with Galaxy Surveys

用星系巡天测试广义相对论

• 批准号: 1713791
• 负责人: Martin White
• 金额: $ 45.81万
• 依托单位: University of California-Berkeley
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2017
• 资助国家: 美国
• 起止时间: 2017-08-15 至 2022-07-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1713791&HistoricalAwards=false
• 关键词: Testing; General; Relativity; Galaxy; Surveys

Cosmology has made tremendous advances in the last decade, and we now have a highly predictive model for the emergence of structure in the Universe, which draws upon a rich set of ideas from high energy physics, gravitation theory, and astrophysics. However, this model requires one very surprising ingredient, an accelerating expansion of the Universe. This acceleration poses the most profound question in physical science today with even the most prosaic explanations demanding the existence of a new constituent ("dark energy") with exotic physical properties. More extreme alternatives include extra spatial dimensions or a breakdown of General Relativity on cosmological scales. Luckily, the motion of galaxies allows us to probe dark energy and to test General Relativity. Turning this realization into a precision tool is the goal of this project.The project aims to develop the insight that large-scale structure can provide as a probe of dark energy and modified gravity. By combining state-of-the-art modeling and new analysis methods with the massive new data sets being accumulated from redshift surveys, it is possible to simultaneously measure the growth rate of cosmic structure and the cosmological geometry using redshift-space distortions. The investigators will validate and apply models rooted in perturbation theory to the most constraining subsets of existing near-future data sets to generate a consistent meta-analysis of the current state of the field.

宇宙学在过去的十年里取得了巨大的进步，我们现在有了一个高度可预测的宇宙结构出现的模型，它借鉴了高能物理学、引力理论和天体物理学的丰富思想。然而，这个模型需要一个非常令人惊讶的因素，宇宙的加速膨胀。这种加速提出了当今物理科学中最深刻的问题，即使是最平淡无奇的解释也要求存在一种具有奇异物理特性的新成分（“暗能量”）。更极端的选择包括额外的空间维度或广义相对论在宇宙尺度上的崩溃。幸运的是，星系的运动使我们能够探测暗能量并检验广义相对论。将这种实现转化为精密工具是本项目的目标。该项目旨在发展大规模结构的洞察力，可以作为暗能量和修正重力的探测器。通过将最先进的建模和新的分析方法与从红移调查中积累的大量新数据集相结合，可以同时测量宇宙结构的增长率和利用红移空间扭曲的宇宙几何形状。研究人员将验证并应用基于微扰理论的模型，将其应用于现有近期数据集的最约束子集，以生成该领域当前状态的一致元分析。

项目成果

Biased tracers of two fluids in the Lagrangian picture

• DOI: 10.1088/1475-7516/2019/06/006
• 发表时间: 2019-03
• 期刊: Journal of Cosmology and Astroparticle Physics
• 影响因子: 6.4
• 作者: Shi-Fan Chen;E. Castorina;M. White

Synergies between radio, optical and microwave observations at high redshift

• DOI: 10.1088/1475-7516/2019/07/023
• 发表时间: 2018-10
• 期刊: Journal of Cosmology and Astroparticle Physics
• 影响因子: 6.4
• 作者: Shi-Fan Chen;E. Castorina;M. White;A. Slosar

Measuring the growth of structure with intensity mapping surveys

• DOI: 10.1088/1475-7516/2019/06/025
• 发表时间: 2019-02
• 期刊: Journal of Cosmology and Astroparticle Physics
• 影响因子: 6.4
• 作者: E. Castorina;M. White

CosmoDC2: A Synthetic Sky Catalog for Dark Energy Science with LSST

• DOI: 10.3847/1538-4365/ab510c
• 发表时间: 2019-07
• 期刊: The Astrophysical Journal Supplement Series
• 作者: D. Korytov;Andrew P. Hearin;E. Kovacs;P. Larsen;Esteban Rangel;J. Hollowed;A. Benson;K. Heitmann;Yao-Yuan Mao;A. Bahmanyar;Chihway L. Chang;D. Campbell;J. DeRose;H. Finkel;N. Frontiere;E. Gawiser;S. Habib;B. Joachimi;F. Lanusse;Nan Li;R. Mandelbaum;C. Morrison;J. Newman;A. Pope;E. Rykoff;M. Simet;C. To;V. Vikraman;R. Wechsler;M. White

Consistent modeling of velocity statistics and redshift-space distortions in one-loop perturbation theory

• DOI: 10.1088/1475-7516/2020/07/062
• 发表时间: 2020-05
• 期刊: Journal of Cosmology and Astroparticle Physics
• 影响因子: 6.4
• 作者: Shi-Fan Chen;Z. Vlah;M. White