Can DESI DR1 geometry and observational selection support a three-dimensional map without introducing artificial structures?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026
Results
Scientific results
Scientific questions grouped by method and hypothesis. Each family preserves its original runs, conditions and statuses.
Questions 25–35 of 35 · page 2 of 2
Do anomalies attributed to cold dark matter point to the same new property after accounting for baryonic effects and measurement uncertainties?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026
Can suppression of growth on intermediate scales reduce the S8 difference between Planck and lensing surveys?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026
Does holography predict the 2.3 meV scale independently of cosmological observations?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026
Do the Lyman-alpha forest and satellite galaxies favor a cutoff scale compatible with warm or ultralight dark matter?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026
Do the citation networks of partial precedents contain a paper that combines the full proposal?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026
In Pantheon+ and Union3, with Ωm = 0.315 ± 0.007, does the preference for dynamical dark energy persist after excluding each of the seven DESI DR2 BAO bins?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026
Does supersymmetry protect the relation R = 1 without requiring new fine-tuning?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026
In Pantheon+ and Union3, with Ωm = 0.315 ± 0.03, does the preference for dynamical dark energy persist after excluding each of the seven DESI DR2 BAO bins?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026
Can velocity-dependent dark-matter self-interaction satisfy small-galaxy and cluster constraints simultaneously?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026
Do the DES, KiDS and HSC weak-lensing mass calibrations used by eROSITA show tension at high redshift?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026