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Record W4414860802 · doi:10.1103/w9pk-xsk7

Constraints on neutrino physics from DESI DR2 BAO and DR1 full shape

2025· article· en· W4414860802 on OpenAlexaff
Willem Elbers, Alejandro Avilés, H. E. Noriega, D. Chebat, A. Menegas, Carlos S. Frenk, C. García-Quintero, D. Gonzalez, Mustapha Ishak, O. Lahav, Krishna Naidoo, Gustavo Niz, C. Yèche, A. G. Adame, S. P. Ahlen, O. Alves, U. Andrade, J. Behera, S. BenZvi, D. Bianchi, S. Brieden, A. Brodzeller, D. Brooks, E. Burtin, R. Calderón, R. E. A. Canning, A. Carnero Rosell, Lidia Casas, F. J. Castander, M. Charles, E. Chaussidon, J. Chaves-Montero, T. Claybaugh, S. Cole, Andrew P. Cooper, Andrei Cuceu, Kyle Dawson, Axel de la Macorra, Arnaud de Mattia, N. Deiosso, Arjun Dey, Biprateep Dey, Z. Ding, Peter Doel, D. J. Eisenstein, Simone Ferraro, Andreu Font-Ribera, J. E. Forero-Romero, L. H. Garrison, E. Gaztañaga, Héctor Gil-Marín, Satya Gontcho A Gontcho, Alma X. González‐Morales, G. Gutiérrez, S. He, M. Herbold, H. K. Herrera-Alcantar, Cullan Howlett, Dragan Huterer, S. Juneau, R. Kehoe, D. Kirkby, Theodore Kisner, C. Lamman, Martin Landriau, L. Le Guillou, Alexie Leauthaud, M. E. Levi, Qiong Li, K. Lodha, C. Magneville, Marc Manera, William L. Matthewson, Aaron Meisner, J. Mena-Fernández, R. Miquel, John Moustakas, S. Nadathur, Jeffrey A. Newman, E. Paillas, N. Palanque‐Delabrouille, Will J. Percival, Matthew M. Pieri, C. Poppett, F. Prada, Ignasi Pérez-Ràfols, D. Rabinowitz, C. Ramírez-Pérez, M. Rashkovetskyi, C. Ravoux, H. Rivera-Morales, J. Rohlf, Ashley J. Ross, Graziano Rossi, V. Ruhlmann-Kleider, Lado Samushia, E. Sánchez, David J. Schlegel, M. Schubnell, Hee‐Jong Seo, Francesco Sinigaglia, D. Sprayberry, T. Tan, G. Tarlé, Peter L. Taylor, W. Turner, M. Vargas-Magaña, Licia Verde, Michael Walther, B. A. Weaver, Abbé M Whitford, Molly Wolfson, Pauline Zarrouk, Cheng Zhao, Rongpu Zhou, Hu Zou

Bibliographic record

VenuePhysical review. D/Physical review. D. · 2025
Typearticle
Languageen
FieldPhysics and Astronomy
TopicAstrophysics and Cosmic Phenomena
Canadian institutionsCoast Mountain CollegePerimeter InstituteUniversity of WaterlooUniversity of Toronto
FundersHigh Energy PhysicsDivision of Astronomical SciencesScience and Technology Facilities CouncilOffice of ScienceCommissariat à l'Énergie Atomique et aux Énergies AlternativesDurham UniversityNational Science FoundationRoyal SocietyNational Energy Research Scientific Computing CenterEuropean Research CouncilMinisterio de Ciencia, Innovación y UniversidadesGordon and Betty Moore FoundationHeising-Simons FoundationConsejo Nacional de Ciencia y TecnologíaSpace Telescope Science InstituteDepartment for Business, Energy and Industrial Strategy, UK GovernmentU.S. Department of EnergyNational Aeronautics and Space Administration
KeywordsNeutrinoNeutrino oscillationCosmic microwave backgroundCosmologyDark energyMeasurements of neutrino speedCosmic background radiationLimit (mathematics)RedshiftPhysics beyond the Standard Model

Abstract

fetched live from OpenAlex

The Dark Energy Spectroscopic Instrument (DESI) Collaboration has obtained robust measurements of baryon acoustic oscillations in the redshift range 0.1 < z < 4.2 , based on the Lyman- α forest and galaxies from data release 2. We combine these measurements with cosmic microwave background (CMB) data from and the Atacama Cosmology Telescope to place our tightest constraints yet on the sum of neutrino masses. Assuming the cosmological Λ CDM model and three degenerate neutrino states, we find ∑ m ν < 0.0642 eV (95%) with a marginalized error of σ ( ∑ m ν ) = 0.020 eV . We also constrain the effective number of neutrino species, finding N eff = 3.2 3 − 0.34 + 0.35 (95%), in line with the Standard Model prediction. When accounting for neutrino oscillation constraints, we find a preference for the normal mass ordering and an upper limit on the lightest neutrino mass of m l < 0.023 eV (95%). However, we determine using frequentist and Bayesian methods that our constraints are in tension with the lower limits derived from neutrino oscillations. Correcting for the physical boundary at zero mass, we report a 95% Feldman-Cousins upper limit of ∑ m ν < 0.053 eV , breaching the lower limit from neutrino oscillations. Considering a more general Bayesian analysis with an effective cosmological neutrino mass parameter, ∑ m ν , eff , that allows for negative energy densities and removes unsatisfactory prior weight effects, we derive constraints that are in 3 σ tension with the same oscillation limit, while the error rises to σ ( ∑ m ν , eff ) = 0.053 eV . In the absence of unknown systematics, this finding could be interpreted as a hint of new physics not necessarily related to neutrinos. The preference of DESI and CMB data for an evolving dark energy model offers one possible solution. In the w 0 w a CDM model, we find ∑ m ν < 0.163 eV (95%), relaxing the neutrino tension. These constraints all rely on the effects of neutrinos on the cosmic expansion history. Using full-shape power spectrum measurements of data release 1 galaxies, we place complementary constraints that rely on neutrino free streaming. Our strongest such limit in Λ CDM , using selected CMB priors, is ∑ m ν < 0.193 eV (95%).

Fetched live from OpenAlex and de-inverted. Abstracts are not stored in this database: the inverted indexes are 8.6 GB of the frame’s 9.3 GB of text, and the host has 13 GB free.

How this classification was reachedexpand

Full frame machine prediction

Teacher imitation

Not calibrated prevalence, not ground truth. Human validation pending. The Gemma side is a direct model label for every work in the frame, read from the title-only record. The Codex side is a classifier learned from the 10,348 direct Codex labels and calibrated to design-weighted sample rates; fields without enough sample support carry no Codex call. Candidate is the union of the two sides; consensus is their intersection. These outputs are machine_predicted_unvalidated and are not human labels.

metaresearch head score (Codex)0.003
metaresearch head score (Gemma)0.006
Version: metacan-v3-hybrid-931329e0061cValidation status: machine_predicted_unvalidated
Candidate categoriesnone
Consensus categoriesnone
DomainCandidate signal: none · Consensus signal: none
Study designCandidate signal: Observational · Consensus signal: Observational
GenreCandidate signal: Empirical · Consensus signal: Empirical
Teacher disagreement score0.016
Threshold uncertainty score0.055

Distilled classifier scores by category (both heads)

CategoryCodexGemma
Metaresearch0.0030.006
Meta-epidemiology (narrow)0.0010.001
Meta-epidemiology (broad)0.0010.001
Bibliometrics0.0020.002
Science and technology studies0.0010.000
Scholarly communication0.0040.002
Open science0.0010.002
Research integrity0.0010.002
Insufficient payload (model declined to judge)0.0160.004

Machine scores (provisional)

The two teacher heads of the student model, read on this work. A score orders the frame for review; it never asserts a category, and the validation status ships verbatim with every row.

Baseline scores from an immature model (maturity gate not passed, 7 training rounds). Scores rank; they never assert a category.

Opus teacher head0.014
GPT teacher head0.366
Teacher spread0.353 · how far apart the two teachers sit on this one work
Validation statusscore_only:v0-immature-baseline · verbatim from the scoring run: score_only means the number may rank works, and no category label ships from it

Classification

machine, unvalidated

Machine predicted; a candidate call from one source (direct Gemma or distilled Codex), not a consensus.

The models applied no category: nothing in the taxonomy fit this work.
Study designObservational
Domainnot available
GenreEmpirical

How this classification was reached, model by model and score by score, is at the end of the page under "How this classification was reached".

Quick stats

Citations58
Published2025
Admission routes1
Has abstractyes

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