Challenging the standard cosmological model

挑战标准宇宙学模型

• 批准号: RGPIN-2020-06115
• 负责人: Scott, Douglas
• 金额: $ 5.46万
• 依托单位: University of British Columbia
• 依托单位国家: 加拿大
• 项目类别: Discovery Grants Program - Individual
• 财政年份: 2022
• 资助国家: 加拿大
• 起止时间: 2022-01-01 至 2023-12-31
• 项目状态: 已结题
• 来源: https://www.nserc-crsng.gc.ca/ase-oro/Details-Detailles_eng.asp?id=763085
• 关键词: Challenging; standard; cosmological; model

The standard model of cosmology successfully explains a wide set of precise data, with a few simplifying assumptions and just seven free parameters. It has remained essentially unchanged for about 25 years. However, it is purely phenomenological and contains several unexplained aspects, e.g. there is no explanation for the nature of the dark matter or dark energy, or for the origin of the initial density perturbations. The model is far from being elegant, and additionally there is no expectation that it can be complete. Moreover, despite its successes, there are some apparent chinks in the armour of the standard cosmological model, variously called "anomalies", "curiosities" or "tensions" - it is currently unclear which of them may point the way towards new physics, which are caused by unidentified systematic effects, and which are just statistical fluctuations. Of course the obvious way to make progress is through obtaining much more sensitive data from future experiments with the goal of discovering that new parameters may be needed (such as a component of primordial gravitational waves, a non-trivial kind of dark energy, or observable effects from massive neutrinos). I am involved in such ambitious cosmic microwave background (CMB) experiments, but the results are not expected soon. For the 5 years of research proposed here, I will explore 4 separate ways to extend the cosmological model, each involving students in attempts to more immediately challenge the standard cosmology. First, some existing anomalies can be directly investigated with new data, e.g. probing large-scale curiosities using CMB polarization or lensing data.  Second, parameter tensions can be explored in the context of modified-gravity ideas or adding other novel physics ingredients to the model. Third, we can use cross-correlations between CMB "secondary" signals and other astrophysical survey data to extract additional cosmological information from existing data and confront this with the predictions of the standard model. Last, we can search for structures that would be difficult to explain within the standard picture, particularly proto-clusters of galaxies at high redshift. Through a combination of these interrelated research thrusts, this proposal will examine how the standard cosmological model needs to evolve to fully describe future cosmological data.

宇宙学的标准模型成功地解释了大量精确的数据，只有一些简化的假设和七个自由参数。25年来，它基本上没有变化。然而，它是纯粹的现象学，包含了一些无法解释的方面，例如，没有解释暗物质或暗能量的性质，或者初始密度扰动的起源。该模型远非优雅，而且也没有期望它可以完成。此外，尽管它取得了成功，但标准宇宙学模型的盔甲上有一些明显的裂缝，被称为“异常”，“好奇心”或“张力”-目前还不清楚它们中的哪一个可能指向新的物理学，这是由未知的系统效应引起的，而这只是统计波动。当然，取得进展的明显方式是通过从未来的实验中获得更敏感的数据，目的是发现可能需要的新参数（例如原始引力波的成分，一种非平凡的暗能量，或来自大质量中微子的可观测效应）。我参与了这样雄心勃勃的宇宙微波背景（CMB）实验，但结果不会很快出现。在这里提出的5年研究中，我将探索4种不同的方法来扩展宇宙学模型，每种方法都让学生尝试更直接地挑战标准宇宙学。首先，一些现有的异常可以直接调查新的数据，例如探测大规模的好奇心使用CMB偏振或透镜数据。 第二，参数张力可以在修改的重力思想或在模型中添加其他新的物理成分的背景下进行探索。第三，我们可以利用CMB“次级”信号和其他天体物理调查数据之间的互相关，从现有数据中提取额外的宇宙学信息，并将其与标准模型的预测相对抗。最后，我们可以寻找在标准图像中难以解释的结构，特别是高红移的原星系团。通过结合这些相互关联的研究重点，该提案将研究标准宇宙学模型需要如何演变，以充分描述未来的宇宙学数据。