Dark energy: redshift-bin exclusion
Sensitivity of evolving-dark-energy preferences to the exclusion of redshift intervals.
Latest record: 09 Oct 2026
Results
Scientific results
Scientific questions grouped by method and hypothesis. Each family preserves its original runs, conditions and statuses.
Latest record date in this public snapshot: 9 October 2026. It does not represent current research activity.
Surveys are identified by textual mentions in summaries; this does not establish direct dataset usage. The stage filter appears when more than one approved status is available.
Displayed records
24 of 35 questions/families shown · 169 execution records
BAO priors and dark-energy robustness
Variations in the BAO scale, Ωm prior and exclusion conditions.
Latest record: 09 Oct 2026
Dependence on BAO tracer families
Persistence of cosmological preferences when BAO tracer families or blocks are excluded.
Latest record: 09 Oct 2026
Redshift localisation of the signal
Tests of whether particular redshift intervals dominate supernova comparisons.
Latest record: 09 Oct 2026
DESI DR1 versus DR2: BAO release dependence
Comparison of cosmological preferences when switching BAO releases.
Latest record: 09 Oct 2026
Fit direction and BAO components
Impact of galaxy and Lyα forest subsets on the fit.
Latest record: 09 Oct 2026
Individual exclusions and matter priors
Persistence of dynamical-dark-energy preferences when regions are removed separately.
Latest record: 09 Oct 2026
DESI DR1 tracers and CPL parameters
Fixed-CPL point comparisons across tracers and redshifts.
Latest record: 09 Oct 2026
Growth under fixed CPL expansion
Growth-observable tests under fixed expansion parameters.
Latest record: 09 Oct 2026
Does R = 1 follow from the classical derivation of the effective theory?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026
Is the eROSITA S8–redshift trend dominated by a single bin?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026
Is the preference for evolving dark energy spread across the supernova data or concentrated in one redshift range?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026
Do quantum corrections preserve R = 1 in the minimal bosonic model?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026
Does the literature contain a physically equivalent precedent for the complete theoretical chain?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026
If the growth suppression associated with S8 is physical, can the data determine when it began?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026
In Pantheon+ and DES-SN5YR, with Ωm = 0.315 ± 0.03, does the preference for dynamical dark energy persist after the exclusion of each of the six BAO tracer groups?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026
In DES-SN5YR and Union3, 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
Is one dark-matter self-interaction law compatible with both dwarf galaxies and clusters?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026
In Pantheon+ and DES-SN5YR, with Ωm = 0.3 ± 0.01, does the preference for dynamical dark energy persist after the exclusion of each of the six BAO tracer groups?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026
Does the literature already contain the chain linking holography, the meV scale and a protected local effective theory?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026
In Pantheon+ and DES-SN5YR, with Ωm = 0.33 ± 0.01, does the preference for dynamical dark energy persist after the exclusion of each of the six BAO tracer groups?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026
Does searching references and citations support the potential novelty of the full theoretical chain?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026
In Pantheon+ and Union3, with Ωm = 0.33 ± 0.01, 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
In Pantheon+ and Union3, with Ωm = 0.315 ± 0.03, does the preference for dynamical dark energy persist after the exclusion of each of the six BAO tracer groups?
Individual public-manifest question. The method and limitations are in its record.
Latest record: 09 Oct 2026