Paper Citation Record · LEDGER

Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 13 inbound Pith citation observations for arXiv:2012.11830.

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

pith.paper-citation-record.v1
2012.11830 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 13 of 13 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 13 of 13 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T21:12:37.534138Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T18:30:01.045360Z

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External citation measurements

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 23224b62-b657-4ba2-b64b-98e4328094da · inbound

Neutrino masses from large-scale structures: future sensitivity and theory dependence cites this paper.

Neutrino masses from large-scale structures: future sensitivity and theory dependence Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-11T21:12:37.534138Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 550aa6d8-cb33-449d-aed2-85c3fb16aa2b · inbound

Probing Long-Range Forces Between Neutrinos with Cosmic Structures cites this paper.

Probing Long-Range Forces Between Neutrinos with Cosmic Structures Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-10T23:18:06.572869Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 057a899c-aa65-4239-a17f-a0b40860fb63 · inbound

Enabling Strong Neutrino Self-interaction with an Unparticle Mediator cites this paper.

Enabling Strong Neutrino Self-interaction with an Unparticle Mediator Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-10T22:28:51.328453Z

Source-reported events for the cited work

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Observation 6a61cc26-16c4-4fa6-abe1-70bf5bd42973 · inbound

New Constraints on Neutrino-Dark Matter Interactions: A Comprehensive Analysis cites this paper.

New Constraints on Neutrino-Dark Matter Interactions: A Comprehensive Analysis Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background

Reference 156

Resolution: unresolved; no resolver link, observed 2026-08-06T21:08:55.300324Z

Source-reported events for the cited work

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Observation e7154d95-dc05-47e2-92e2-28c9d365420b · inbound

Towards a complete scheme of cosmological neutrino self-interactions: Collision term for a wide range of mediator masses cites this paper.

Towards a complete scheme of cosmological neutrino self-interactions: Collision term for a wide range of mediator masses Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background

Reference 20

Resolution: verified exact; arxiv_id, observed 2026-05-16T02:00:29.493418Z

Source-reported events for the cited work

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Observation c7511ed5-d0fa-4cfc-9cdc-0c5e6ae053a5 · inbound

Double the axions, half the tension: multi-field early dark energy eases the Hubble tension cites this paper.

Double the axions, half the tension: multi-field early dark energy eases the Hubble tension Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background

Reference 42

Resolution: verified exact; arxiv_id, observed 2026-05-11T11:41:01.583783Z

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Observation ef760282-c3ad-4a81-a948-ca74f726269c · inbound

Neutrino self-interactions in post-reionization era: Lyman-$\alpha$, 21-cm and cross-spectra cites this paper.

Neutrino self-interactions in post-reionization era: Lyman-$\alpha$, 21-cm and cross-spectra Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background

Reference 20

Resolution: verified exact; arxiv_id, observed 2026-05-10T09:48:47.428016Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation fe66ba58-1f0c-4e89-8c8e-55c2faf90855 · inbound

Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension cites this paper.

Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background

Reference 28

Resolution: verified exact; arxiv_id, observed 2026-05-12T00:36:16.308349Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 81e8d402-3e52-404d-a619-0b65f41ec0c8 · inbound

Recoupled Dark Radiation reconciling CMB and DESI BAO measurements cites this paper.

Recoupled Dark Radiation reconciling CMB and DESI BAO measurements Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background

Reference 29

Resolution: verified exact; arxiv_id, observed 2026-05-20T09:03:09.981468Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 9b534de1-c54f-4278-b05d-0a0cb7ded9d5 · inbound

Reconstructing dark energy with fewer assumptions cites this paper.

Reconstructing dark energy with fewer assumptions Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background

Reference 138

Resolution: verified exact; arxiv_id, observed 2026-07-02T14:57:04.114436Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation c3f0c51c-5f9f-4f3c-8661-45ede6b90ad8 · inbound

Probing Scalar Non-Standard Neutrino Interactions using High-Energy Astrophysical Neutrinos cites this paper.

Probing Scalar Non-Standard Neutrino Interactions using High-Energy Astrophysical Neutrinos Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background

Reference 92

Resolution: verified exact; arxiv_id, observed 2026-07-04T18:30:01.049607Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation 90ad25b1-1c12-41da-b570-1acb23059e41 · inbound

Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension cites this paper.

Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background

Reference 185

Resolution: verified exact; arxiv_id, observed 2026-07-01T11:25:45.243602Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

Observation c00ca14b-29d8-4c6f-87f0-6c93ad675b65 · inbound

Hubble tension: the shape wall cites this paper.

Hubble tension: the shape wall Self-interacting neutrinos, the Hubble parameter tension, and the Cosmic Microwave Background

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-01T08:08:40.666459Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.