Research family

BAO priors and dark-energy robustness

Variations in the BAO scale, Ωm prior and exclusion conditions.

24 execution records · Latest record: 09 Oct 2026

Editorial grouping by research question. Each record preserves its original identifier, priors, method, result and status. Values have not been combined, and a signal in a single run is not a global detection.

Runs and variants

T-0062706e5bd5Candidate
With a BAO scale-parameter prior of 30 ± 2 and Ωm = 0.315 ± 0.007, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?
The preference for dynamical dark energy retained the same direction in every tested group exclusion. This stability is limited to the analyzed data, priors and groupings; it does not establish a globally significant detection.
09 Oct 2026Method, limits and provenance · T-0062706e5bd5
T-0633897944c1Candidate
With a BAO scale-parameter prior of 30 ± 2 and Ωm = 0.315 ± 0.02, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?
The group exclusions produced unequal responses in the fit. The comparison established neither independence of the preference from every group nor exclusive dependence on any one group.
09 Oct 2026Method, limits and provenance · T-0633897944c1
T-10b57651447bCandidate
With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.3 ± 0.01, does the preference for dynamical dark energy in Pantheon+ and Union3 persist after excluding each tracer block?
The group exclusions produced unequal responses in the fit. The comparison established neither independence of the preference from every group nor exclusive dependence on any one group.
09 Oct 2026Method, limits and provenance · T-10b57651447b
T-14ccbc39849eCandidate
With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.315 ± 0.007, does the preference for dynamical dark energy in Pantheon+ and DES-SN5YR persist after excluding each tracer block?
The preference for dynamical dark energy retained the same direction in every tested group exclusion. This stability is limited to the analyzed data, priors and groupings; it does not establish a globally significant detection.
09 Oct 2026Method, limits and provenance · T-14ccbc39849e
T-1b7542e82bf0Candidate
With a BAO scale-parameter prior of 30 ± 2 and Ωm = 0.3 ± 0.01, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?
The group exclusions produced unequal responses in the fit. The comparison established neither independence of the preference from every group nor exclusive dependence on any one group.
09 Oct 2026Method, limits and provenance · T-1b7542e82bf0
T-2402743e1bc5Candidate
With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.3 ± 0.01, does the preference for dynamical dark energy in Pantheon+ and DES-SN5YR persist after excluding each tracer block?
The group exclusions produced unequal responses in the fit. The comparison established neither independence of the preference from every group nor exclusive dependence on any one group.
09 Oct 2026Method, limits and provenance · T-2402743e1bc5
T-2a468105a961Candidate
With a BAO scale-parameter prior of 30 ± 4 and Ωm = 0.3 ± 0.01, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?
The group exclusions produced unequal responses in the fit. The comparison established neither independence of the preference from every group nor exclusive dependence on any one group.
09 Oct 2026Method, limits and provenance · T-2a468105a961
T-430e5c51bfaeCandidate
With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.3 ± 0.01, does the preference for dynamical dark energy in DES-SN5YR and Union3 persist after excluding each tracer block?
The group exclusions produced unequal responses in the fit. The comparison established neither independence of the preference from every group nor exclusive dependence on any one group.
09 Oct 2026Method, limits and provenance · T-430e5c51bfae
T-43f34932b319Candidate
With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.33 ± 0.01, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?
The preference for dynamical dark energy retained the same direction in every tested group exclusion. This stability is limited to the analyzed data, priors and groupings; it does not establish a globally significant detection.
09 Oct 2026Method, limits and provenance · T-43f34932b319
T-4547bf250443Candidate
With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.3 ± 0.01, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?
The group exclusions produced unequal responses in the fit. The comparison established neither independence of the preference from every group nor exclusive dependence on any one group.
09 Oct 2026Method, limits and provenance · T-4547bf250443
T-4906aac18658Candidate
With a BAO scale-parameter prior of 30 ± 4 and Ωm = 0.315 ± 0.02, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?
The group exclusions produced unequal responses in the fit. The comparison established neither independence of the preference from every group nor exclusive dependence on any one group.
09 Oct 2026Method, limits and provenance · T-4906aac18658
T-66ccf03dc95aCandidate
With a BAO scale-parameter prior of 30 ± 4 and Ωm = 0.3 ± 0.01, does the preference for dynamical dark energy in Pantheon+ and Union3 persist after excluding each tracer block?
The group exclusions produced unequal responses in the fit. The comparison established neither independence of the preference from every group nor exclusive dependence on any one group.
09 Oct 2026Method, limits and provenance · T-66ccf03dc95a
T-8d164854842aCandidate
With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.33 ± 0.01, does the preference for dynamical dark energy in DES-SN5YR and Union3 persist after excluding each tracer block?
The preference for dynamical dark energy retained the same direction in every tested group exclusion. This stability is limited to the analyzed data, priors and groupings; it does not establish a globally significant detection.
09 Oct 2026Method, limits and provenance · T-8d164854842a
T-986bac19c5ceCandidate
With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.33 ± 0.01, does the preference for dynamical dark energy in Pantheon+ and Union3 persist after excluding each tracer block?
The preference for dynamical dark energy retained the same direction in every tested group exclusion. This stability is limited to the analyzed data, priors and groupings; it does not establish a globally significant detection.
09 Oct 2026Method, limits and provenance · T-986bac19c5ce
T-b3ab99a53562Candidate
With a BAO scale-parameter prior of 30 ± 4 and Ωm = 0.3 ± 0.01, does the preference for dynamical dark energy in Pantheon+ and DES-SN5YR persist after excluding each tracer block?
The group exclusions produced unequal responses in the fit. The comparison established neither independence of the preference from every group nor exclusive dependence on any one group.
09 Oct 2026Method, limits and provenance · T-b3ab99a53562
T-c1a3e0fb9f26Candidate
With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.315 ± 0.007, does the preference for dynamical dark energy in DES-SN5YR and Union3 persist after excluding each tracer block?
The preference for dynamical dark energy retained the same direction in every tested group exclusion. This stability is limited to the analyzed data, priors and groupings; it does not establish a globally significant detection.
09 Oct 2026Method, limits and provenance · T-c1a3e0fb9f26
T-c2a28f6f2e5eCandidate
With a BAO scale-parameter prior of 30 ± 4 and Ωm = 0.3 ± 0.01, does the preference for dynamical dark energy in DES-SN5YR and Union3 persist after excluding each tracer block?
The group exclusions produced unequal responses in the fit. The comparison established neither independence of the preference from every group nor exclusive dependence on any one group.
09 Oct 2026Method, limits and provenance · T-c2a28f6f2e5e
T-c98114e25884Candidate
With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.33 ± 0.01, does the preference for dynamical dark energy in Pantheon+ and DES-SN5YR persist after excluding each tracer block?
The preference for dynamical dark energy retained the same direction in every tested group exclusion. This stability is limited to the analyzed data, priors and groupings; it does not establish a globally significant detection.
09 Oct 2026Method, limits and provenance · T-c98114e25884
T-d0ee3e41d250Candidate
With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.315 ± 0.007, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?
The preference for dynamical dark energy retained the same direction in every tested group exclusion. This stability is limited to the analyzed data, priors and groupings; it does not establish a globally significant detection.
09 Oct 2026Method, limits and provenance · T-d0ee3e41d250
T-ea488de163c3Candidate
With a BAO scale-parameter prior of 30 ± 4 and Ωm = 0.33 ± 0.01, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?
The preference for dynamical dark energy retained the same direction in every tested group exclusion. This stability is limited to the analyzed data, priors and groupings; it does not establish a globally significant detection.
09 Oct 2026Method, limits and provenance · T-ea488de163c3
T-ed9ca90519ffCandidate
With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.315 ± 0.007, does the preference for dynamical dark energy in Pantheon+ and Union3 persist after excluding each tracer block?
The preference for dynamical dark energy retained the same direction in every tested group exclusion. This stability is limited to the analyzed data, priors and groupings; it does not establish a globally significant detection.
09 Oct 2026Method, limits and provenance · T-ed9ca90519ff
T-f901477a215fCandidate
With a BAO scale-parameter prior of 30 ± 2 and Ωm = 0.33 ± 0.01, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?
The preference for dynamical dark energy retained the same direction in every tested group exclusion. This stability is limited to the analyzed data, priors and groupings; it does not establish a globally significant detection.
09 Oct 2026Method, limits and provenance · T-f901477a215f
T-fd3fcefa6269Candidate
With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.315 ± 0.02, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?
The group exclusions produced unequal responses in the fit. The comparison established neither independence of the preference from every group nor exclusive dependence on any one group.
09 Oct 2026Method, limits and provenance · T-fd3fcefa6269
T-fe29e9f5a9a2Candidate
With a BAO scale-parameter prior of 30 ± 4 and Ωm = 0.315 ± 0.007, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?
The preference for dynamical dark energy retained the same direction in every tested group exclusion. This stability is limited to the analyzed data, priors and groupings; it does not establish a globally significant detection.
09 Oct 2026Method, limits and provenance · T-fe29e9f5a9a2

Runs and variants

With a BAO scale-parameter prior of 30 ± 2 and Ωm = 0.315 ± 0.007, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?

With a BAO scale-parameter prior of 30 ± 2 and Ωm = 0.315 ± 0.02, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?

With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.3 ± 0.01, does the preference for dynamical dark energy in Pantheon+ and Union3 persist after excluding each tracer block?

With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.315 ± 0.007, does the preference for dynamical dark energy in Pantheon+ and DES-SN5YR persist after excluding each tracer block?

With a BAO scale-parameter prior of 30 ± 2 and Ωm = 0.3 ± 0.01, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?

With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.3 ± 0.01, does the preference for dynamical dark energy in Pantheon+ and DES-SN5YR persist after excluding each tracer block?

With a BAO scale-parameter prior of 30 ± 4 and Ωm = 0.3 ± 0.01, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?

With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.3 ± 0.01, does the preference for dynamical dark energy in DES-SN5YR and Union3 persist after excluding each tracer block?

With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.33 ± 0.01, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?

With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.3 ± 0.01, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?

With a BAO scale-parameter prior of 30 ± 4 and Ωm = 0.315 ± 0.02, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?

With a BAO scale-parameter prior of 30 ± 4 and Ωm = 0.3 ± 0.01, does the preference for dynamical dark energy in Pantheon+ and Union3 persist after excluding each tracer block?

With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.33 ± 0.01, does the preference for dynamical dark energy in DES-SN5YR and Union3 persist after excluding each tracer block?

With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.33 ± 0.01, does the preference for dynamical dark energy in Pantheon+ and Union3 persist after excluding each tracer block?

With a BAO scale-parameter prior of 30 ± 4 and Ωm = 0.3 ± 0.01, does the preference for dynamical dark energy in Pantheon+ and DES-SN5YR persist after excluding each tracer block?

With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.315 ± 0.007, does the preference for dynamical dark energy in DES-SN5YR and Union3 persist after excluding each tracer block?

With a BAO scale-parameter prior of 30 ± 4 and Ωm = 0.3 ± 0.01, does the preference for dynamical dark energy in DES-SN5YR and Union3 persist after excluding each tracer block?

With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.33 ± 0.01, does the preference for dynamical dark energy in Pantheon+ and DES-SN5YR persist after excluding each tracer block?

With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.315 ± 0.007, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?

With a BAO scale-parameter prior of 30 ± 4 and Ωm = 0.33 ± 0.01, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?

With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.315 ± 0.007, does the preference for dynamical dark energy in Pantheon+ and Union3 persist after excluding each tracer block?

With a BAO scale-parameter prior of 30 ± 2 and Ωm = 0.33 ± 0.01, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?

With a BAO scale-parameter prior of 30 ± 8 and Ωm = 0.315 ± 0.02, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?

With a BAO scale-parameter prior of 30 ± 4 and Ωm = 0.315 ± 0.007, does the preference for dynamical dark energy in Pantheon+, DES-SN5YR and Union3 persist after excluding each tracer block?