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

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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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The Neutrino Mass Bound from Leptogenesis Revisited cites this paper.

The Neutrino Mass Bound from Leptogenesis Revisited Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

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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

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Individual Neutrino Masses From a Supernova cites this paper.

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

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Origin of cosmological neutrino mass bounds: background $\textit{versus}$ perturbations cites this paper.

Origin of cosmological neutrino mass bounds: background $\textit{versus}$ perturbations Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 12

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New parameter region in sterile neutrino searches: a scenario to alleviate cosmological neutrino mass bound and its testability at oscillation experiments Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

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Revisiting the impact of neutrino mass hierarchies on neutrino mass constraints in light of recent DESI data Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

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Neutrino masses from large-scale structures: future sensitivity and theory dependence Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 47

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Observation 78745fd0-72b6-4e5c-800e-8b9f3a3b78b4 · inbound

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DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

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Reference 48

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Reference 262

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Can the sound horizon-free measurement of $H_0$ constrain early new physics? Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

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Dark energy and lensing anomaly in Planck CMB data Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

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Robustness of dark energy phenomenology across different parameterizations Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

Reference 69

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Can the universe experience an AdS landscape since matter-radiation equality? Neutrino cosmology after DESI: tightest mass upper limits, preference for the normal ordering, and tension with terrestrial observations

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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

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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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arxiv_id, observed 2026-05-13T02:42:08.607152Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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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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verified exact
arxiv_id, observed 2026-05-13T05:37:19.526809Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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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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verified exact
arxiv_id, observed 2026-05-21T03:03:55.567199Z

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No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation 75ab4cb2-ce72-4c8d-b79f-293124015d5c · inbound

Minimal dark $SU(2)$ origin of a massless Dirac neutrino cites this paper.

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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verified exact
arxiv_id, observed 2026-06-29T11:23:21.510948Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation 06009409-5ad5-413f-bea7-f793fd5d3b69 · inbound

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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arxiv_id, observed 2026-07-02T10:56:52.430308Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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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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arxiv_id, observed 2026-07-02T09:36:50.082466Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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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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arxiv_id, observed 2026-07-02T20:07:22.286284Z

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No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation d6b47165-af37-45a3-a2fb-10e81ee3dbc9 · inbound

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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verified exact
arxiv_id, observed 2026-07-04T07:09:38.617946Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation 70f75d80-9cf7-453b-90a1-b85ac51a1f3e · inbound

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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arxiv_id, observed 2026-06-26T01:38:51.865721Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation 41297c95-2464-4fbe-a0e9-bae998302249 · inbound

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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verified exact
arxiv_id, observed 2026-07-02T06:16:43.500184Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

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Observation ad4223e4-3353-4403-a432-36edf5910c95 · inbound

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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no resolver link, observed 2026-07-12T04:18:55.037825Z

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Observation e1413bc5-8047-41a3-8f5d-700028913fad · inbound

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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verified exact
local_arxiv, observed 2026-07-08T15:55:04.920210Z

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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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no resolver link, observed 2026-07-14T16:44:02.461654Z

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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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no resolver link, observed 2026-08-01T08:09:01.467153Z

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