Paper Citation Record · LEDGER

Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

As of 4 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 27 inbound Pith citation observations for arXiv:2407.18047.

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pith.paper-citation-record.v1
2407.18047 v2

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Pith citing papers itemized under the disclosed page cap.

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Pith citing papers

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Updated Cosmological Constraints in Extended Parameter Space with Planck PR4, DESI Baryon Acoustic Oscillations, and Supernovae: Dynamical Dark Energy, Neutrino Masses, Lensing Anomaly, and the Hubble Tension cites this paper.

Updated Cosmological Constraints in Extended Parameter Space with Planck PR4, DESI Baryon Acoustic Oscillations, and Supernovae: Dynamical Dark Energy, Neutrino Masses, Lensing Anomaly, and the Hubble Tension Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 37

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NuFit-6.0: Updated global analysis of three-flavor neutrino oscillations cites this paper.

NuFit-6.0: Updated global analysis of three-flavor neutrino oscillations Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 32

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Observation 8a5e55ad-0fa8-4f8d-9e67-65081b3adf42 · inbound

DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements cites this paper.

DESI 2024 VII: Cosmological Constraints from the Full-Shape Modeling of Clustering Measurements Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 180

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Observation 725396a5-35f0-4947-9e5e-0a3b2b85cecb · inbound

Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape cites this paper.

Constraints on Neutrino Physics from DESI DR2 BAO and DR1 Full Shape Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 80

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Observation 6c7822d4-4ec5-4670-b0b6-8e46a73e25a1 · inbound

Beyond CPL: Evidence for dynamical dark energy in three-parameter models cites this paper.

Beyond CPL: Evidence for dynamical dark energy in three-parameter models Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 40

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Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder cites this paper.

Model-independent late-universe measurements of $H_0$ and $\Omega_K$ with the parametrization based on cosmic age-improved inverse distance ladder Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 112

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Observational constraints on early time non-phantom behaviour of dynamical dark energy cites this paper.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 40

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Observation 4bdb685b-990d-4daf-909b-13986c02e189 · inbound

Joint Constraints on Neutrinos and Dynamical Dark Energy in Minimally Modified Gravity cites this paper.

Joint Constraints on Neutrinos and Dynamical Dark Energy in Minimally Modified Gravity Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 76

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Observation 97d33669-187a-4821-bc86-1ef3497ce7ed · inbound

Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy cites this paper.

Reanalyzing DESI DR1: 4. Percent-Level Cosmological Constraints from Combined Probes and Robust Evidence for the Normal Neutrino Mass Hierarchy Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 27

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Evidence for deviation in gravitational light deflection from general relativity at cosmological scales with KiDS-Legacy and CMB lensing cites this paper.

Evidence for deviation in gravitational light deflection from general relativity at cosmological scales with KiDS-Legacy and CMB lensing Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 48

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Observation 66de5c22-224e-4048-b4d9-199ae18f48bd · inbound

Neutrino mass limits and decaying dark matter: background evolution versus perturbations cites this paper.

Neutrino mass limits and decaying dark matter: background evolution versus perturbations Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 17

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Measuring neutrino mass in light of ACT DR6 and DESI DR2 cites this paper.

Measuring neutrino mass in light of ACT DR6 and DESI DR2 Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 114

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Observation c3f82918-87d1-45fb-a3c9-66bbc5be9b3f · inbound

Breaking Free from the Swampland of Impossible Universes through the DESI Portal cites this paper.

Breaking Free from the Swampland of Impossible Universes through the DESI Portal Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 74

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Observation 2a78cd58-7c92-47f9-b9f2-2d836037a96c · inbound

Two-loop neutrino mass model with modular $S_4$ symmetry cites this paper.

Two-loop neutrino mass model with modular $S_4$ symmetry Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 119

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Observation 7bd75b37-b763-47fd-9f24-1b333cb8b72f · inbound

Probing the small-scale primordial power spectrum via relic neutrinos and acoustic reheating cites this paper.

Probing the small-scale primordial power spectrum via relic neutrinos and acoustic reheating Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 72

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Observation 26659808-64ff-4b5a-a031-ef3e43644b20 · inbound

Negative neutrino mass or negative dark energy? cites this paper.

Negative neutrino mass or negative dark energy? Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 20

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A Minimal Dark $SU(2)$ Origin of a Massless Dirac Neutrino cites this paper.

A Minimal Dark $SU(2)$ Origin of a Massless Dirac Neutrino Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 44

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Neutrino mass constraints in interacting dark energy models after DESI DR2 cites this paper.

Neutrino mass constraints in interacting dark energy models after DESI DR2 Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 130

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Observation ddf23d2a-7339-4364-9356-46781fdf4abc · inbound

The Future of Lepton Flavor cites this paper.

The Future of Lepton Flavor Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 44

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Observation 44a59eb4-9c2a-4c56-9dc1-c71aa0115b83 · inbound

Mass-Varying Neutrinos from an Inverse Symmetron cites this paper.

Mass-Varying Neutrinos from an Inverse Symmetron Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 9

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Are Cosmological Data Excluding Sterile Neutrinos or Only the Fully Thermalized Limit? cites this paper.

Are Cosmological Data Excluding Sterile Neutrinos or Only the Fully Thermalized Limit? Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 12

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First full-shape joint analysis of the two- and three-point correlation functions on real data: $\Lambda$CDM cosmological constraints from BOSS DR12 cites this paper.

First full-shape joint analysis of the two- and three-point correlation functions on real data: $\Lambda$CDM cosmological constraints from BOSS DR12 Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 119

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Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation cites this paper.

Intertwined Constraints in Extended Cosmologies: Dark Energy, Curvature, Neutrinos, and Inflation Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 172

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Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data cites this paper.

Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 208

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Imprint of swampland-inspired coupled early dark energy cites this paper.

Imprint of swampland-inspired coupled early dark energy Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 32

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Observation 8bf86ef0-81cc-43fc-aaf6-e9f8450b3822 · inbound

Late-time cosmological constraints on three holographic dark energy models with DESI DR2 BAO and Type Ia supernovae cites this paper.

Late-time cosmological constraints on three holographic dark energy models with DESI DR2 BAO and Type Ia supernovae Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 37

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Observation d5e2f9e5-cdb5-44e6-a470-5146baf67817 · inbound

Hubble tension: the shape wall cites this paper.

Hubble tension: the shape wall Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 279

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