Rotation Field of the Cosmic Microwave Background Joint Validation v1.42

Rotation Field Joint Validation v1.42 This dataset analyzes directional rotation patterns in the Cosmic Microwave Background using Planck 2018 data. Version 1.42 applies a dependence aware joint significance test to determine whether the observed anisotropy could arise from noise. The results show that the anisotropic rotation signal is real and stable across independent tests. Condit, Amy. 2025. Rotation Field Joint Validation v1.42. Zenodo. DOI 10.5281/zenodo.17553829. Files: _replication_bundle_v142_20251107_173949.zip joint_result_20251107_171919.json

旋转场联合验证数据集v1.42
本数据集利用普朗克2018（Planck 2018）观测数据，分析宇宙微波背景（Cosmic Microwave Background）中的定向旋转模式。版本1.42采用依赖感知联合显著性检验（dependence aware joint significance test），以确定观测到的各向异性是否源于噪声。研究结果表明，各向异性旋转信号真实存在，且在多组独立检验中均表现出稳定性。本数据集由Amy Condit于2025年发布，相关元数据存储于Zenodo平台，DOI为10.5281/zenodo.17553829。数据集包含以下文件：_replication_bundle_v142_20251107_173949.zip、joint_result_20251107_171919.json。