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| Auteurs principaux: | , , , , , |
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| Format: | Preprint |
| Publié: |
2025
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| Sujets: | |
| Accès en ligne: | https://arxiv.org/abs/2503.10841 |
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| _version_ | 1866910928880009216 |
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| author | Tang, Xiao-Xiao Wang, Peng Wang, Wei Sheng, Ming-Jie Yu, Hao-Ran Xu, Haojie |
| author_facet | Tang, Xiao-Xiao Wang, Peng Wang, Wei Sheng, Ming-Jie Yu, Hao-Ran Xu, Haojie |
| contents | In the cosmic web, filaments play a crucial role in connecting walls to clusters and also act as an important stage for galaxy formation and evolution. Recent observational studies claim that filaments have spin. In this study, we examined the potential impact of diversity in filament identification algorithms and galaxy survey datasets on the quantification of filament spin. The results of this study demonstrate qualitative agreement with previous research, suggesting that a reliable filament spin signal is detectable when the viewing angle of filament spine larger than 80 degrees under a rough estimation. The detected filament spin signal is intricately linked to the viewing angle, dynamic temperature, etc. The quantitative difference of filament spin signal among samples is slightly dependent on the filament identification algorithms, while the value is relatively greater dependent on the redshift space distortion effect in the galaxy sample. |
| format | Preprint |
| id |
arxiv_https___arxiv_org_abs_2503_10841 |
| institution | arXiv |
| publishDate | 2025 |
| record_format | arxiv |
| spellingShingle | Cosmic filament spin -- I: a comparative study in observation Tang, Xiao-Xiao Wang, Peng Wang, Wei Sheng, Ming-Jie Yu, Hao-Ran Xu, Haojie Cosmology and Nongalactic Astrophysics In the cosmic web, filaments play a crucial role in connecting walls to clusters and also act as an important stage for galaxy formation and evolution. Recent observational studies claim that filaments have spin. In this study, we examined the potential impact of diversity in filament identification algorithms and galaxy survey datasets on the quantification of filament spin. The results of this study demonstrate qualitative agreement with previous research, suggesting that a reliable filament spin signal is detectable when the viewing angle of filament spine larger than 80 degrees under a rough estimation. The detected filament spin signal is intricately linked to the viewing angle, dynamic temperature, etc. The quantitative difference of filament spin signal among samples is slightly dependent on the filament identification algorithms, while the value is relatively greater dependent on the redshift space distortion effect in the galaxy sample. |
| title | Cosmic filament spin -- I: a comparative study in observation |
| topic | Cosmology and Nongalactic Astrophysics |
| url | https://arxiv.org/abs/2503.10841 |