Hubble tension environment correction (reproducible pipeline)
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| Natura: | Recurso digital |
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Zenodo
2026
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| _version_ | 1866901991886684160 |
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| author | Baiyi Wang |
| author_facet | Baiyi Wang |
| contents | <p>Summary: H0(δ)=H0_ref(1-β·δ). Reproducible fit: β≈0.171 (MC 16/50/84: 0.139/0.169/0.201)</p> <p>Reproduce (3 commands): python -m pip install -r requirements.txt python math/hubble_env_scan/run_hubble_env_scan_v1.py python math/spectral_graph/run_relational_hubble_beta_poisson_3d_v0.py</p> <p>Key outputs: math/hubble_env_scan/plot_v1.png math/hubble_env_scan/results_v1.json</p> |
| format | Recurso digital |
| id | zenodo_https___doi_org_10_5281_zenodo_18482429 |
| institution | Zenodo |
| language | |
| publishDate | 2026 |
| publisher | Zenodo |
| record_format | zenodo |
| spellingShingle | Hubble tension environment correction (reproducible pipeline) Baiyi Wang cosmology hubble tension observer environment local H0 bias density contrast reproducibility <p>Summary: H0(δ)=H0_ref(1-β·δ). Reproducible fit: β≈0.171 (MC 16/50/84: 0.139/0.169/0.201)</p> <p>Reproduce (3 commands): python -m pip install -r requirements.txt python math/hubble_env_scan/run_hubble_env_scan_v1.py python math/spectral_graph/run_relational_hubble_beta_poisson_3d_v0.py</p> <p>Key outputs: math/hubble_env_scan/plot_v1.png math/hubble_env_scan/results_v1.json</p> |
| title | Hubble tension environment correction (reproducible pipeline) |
| topic | cosmology hubble tension observer environment local H0 bias density contrast reproducibility |
| url | https://doi.org/10.5281/zenodo.18482429 |