Paper Citation Record · LEDGER

What will it take to measure individual neutrino mass states using cosmology?

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2003.03354.

A citation records a reference. It does not transfer a finding from one paper to another.

pith.paper-citation-record.v1
2003.03354 v3

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measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T01:04:42.925818Z

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A source-named dated measurement, never combined with another source.

Source: arxiv_reference, observed 2026-05-17T04:19:00.888525Z

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Outbound references

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Pith citing papers

Observation 3d63bb67-0f74-4fc2-b0a7-3f7951c3a121 · 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 What will it take to measure individual neutrino mass states using cosmology?

Reference 170

Resolution: verified exact; arxiv_id, observed 2026-05-16T17:46:23.305028Z

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Observation e148f259-ae71-4419-b792-1665f1a2b3d0 · inbound

Bayesian and frequentist perspectives agree on dynamical dark energy cites this paper.

Bayesian and frequentist perspectives agree on dynamical dark energy What will it take to measure individual neutrino mass states using cosmology?

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-07T01:04:42.925818Z

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Observation cd09cc23-9845-4a20-b607-b0b1148219e7 · inbound

Cosmological neutrino mass: a frequentist overview in light of DESI cites this paper.

Cosmological neutrino mass: a frequentist overview in light of DESI What will it take to measure individual neutrino mass states using cosmology?

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-06T16:55:41.754249Z

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Observation f64332d7-8229-492e-a584-acad7d51a00c · inbound

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses cites this paper.

Reanalyzing DESI DR1: 2. Constraints on Dark Energy, Spatial Curvature, and Neutrino Masses What will it take to measure individual neutrino mass states using cosmology?

Reference 59

Resolution: verified exact; arxiv_id, observed 2026-05-17T04:19:00.890574Z

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Observation 60e993f8-6acd-4d8b-b383-82700b3f6baf · 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 What will it take to measure individual neutrino mass states using cosmology?

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-03T08:41:48.197029Z

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Observation 627cea36-0395-4c28-bb5d-befb9187a387 · inbound

The $H_0$ world cup. II. A comprehensive competition between proposed Hubble tension solutions cites this paper.

The $H_0$ world cup. II. A comprehensive competition between proposed Hubble tension solutions What will it take to measure individual neutrino mass states using cosmology?

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-02T05:48:05.781107Z

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Unavailable: canonical work link unavailable.