标题： 宇宙微波测绘在宇宙学和基本物理领域的最新成果与展望 显示英文标题

标题： Recent results and perspectives on cosmology and fundamental physics from microwave surveys

摘要： 最近的宇宙微波背景辐射在温度和极化方面的数据已经达到了高精度，能够估计描述当前所谓标准宇宙学模型的所有参数。 从宇宙微波背景各向异性、星系巡天及其交叉相关性中得出的积分萨克斯-沃尔夫效应的最新结果被提出。 通过观察宇宙微波背景中的细微特征，如低多极矩处的功率缺失、原初功率谱以及非高斯性的限制，并结合星系巡天，我们讨论了暴胀物理和早期宇宙中原初扰动的产生。 回顾了粒子物理中的三个重要课题，即由宇宙学数据得出的中微子质量与参数、热暗物质质量以及中子寿命的限制，并关注其与实验室实验结果的比较。 提出了旨在检验爱因斯坦等效原理的宇宙极化旋转分析的最新结果。 最后，我们讨论了下一代射电设施在改进未来宇宙微波背景光谱畸变实验分析方面的前景。 显示英文摘要

摘要： Recent cosmic microwave background data in temperature and polarization have reached high precision in estimating all the parameters that describe the current so-called standard cosmological model. Recent results about the integrated Sachs-Wolfe effect from cosmic microwave background anisotropies, galaxy surveys, and their cross-correlations are presented. Looking at fine signatures in the cosmic microwave background, such as the lack of power at low multipoles, the primordial power spectrum and the bounds on non-Gaussianities, complemented by galaxy surveys, we discuss inflationary physics and the generation of primordial perturbations in the early Universe. Three important topics in particle physics, the bounds on neutrinos masses and parameters, on thermal axion mass and on the neutron lifetime derived from cosmological data are reviewed, with attention to the comparison with laboratory experiment results. Recent results from cosmic polarization rotation analyses aimed at testing the Einstein equivalence principle are presented. Finally, we discuss the perspectives of next radio facilities for the improvement of the analysis of future cosmic microwave background spectral distortion experiments.