2026 preprint: DESI Lyman-alpha geometry and dark-energy inference
Research context
development · proposed · As of 2026-10-10
preprint · 2026-07-29
- Study design
- Blinded Lyman-alpha anisotropy analysis with metal/absorber/continuum controls and comparisons to external CMB/supernova likelihoods.
- Reported result
- The preprint reports geometric constraints and dataset-dependent preferences in an extended dark-energy model.
- Limitations
- Dataset combinations and prior/model choices affect preference; it does not determine the physical cause of acceleration.
DESI DR2 Lyman-alpha Alcock–Paczyński measurements add redshift-dependent geometry information with blinded validation and contaminant controls.
Key knowledge
DESI DR2 Lyman-alpha Alcock–Paczyński measurements add redshift-dependent geometry information with blinded validation and contaminant controls. Dark-energy preferences differ across CMB/supernova combinations and parameterizations; the result does not establish a unique changing dark-energy field.
Conditions and scope
- First submitted 29 July 2026; v3 dated 4 August; no accepted-journal status established in this inspection.
- Selected analysis and cosmological-results sections inspected; inference remains conditional on covariance, contaminants and chosen cosmology.
Sources · 1
References
Sources retain their recorded scope. A source link alone does not establish verification of every statement.
Evidence and review
DESI DR2 Results IV: Lyman-alpha Alcock–Paczyński measurements: Sections III–VII: contaminants, blinded validation and model-dependent constraints (selected source body inspected).
2026-10-10 · Bounded source check of the recorded statement and conditions. This does not certify a unique physical model, reproduce the cited study or replace independent branch review.
Entry details
Permanent link to this entry ↗- Record identity
- research-earth-desi-2026-preprint
- Revision
- research.1
- Structured reference record
- Postgraduate & research reference