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Paper Citation Record · LEDGER

What can CMB observations tell us about the neutrino distribution function?

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2111.12726.

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

pith.paper-citation-record.v1
2111.12726 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T11:36:50.296107Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-01T17:35:51.589817Z

Reference resolution

0 of 0 outbound references displayed

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External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 703ab5eb-717c-4358-8357-2e1f6ddcd3e5 · inbound

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics cites this paper.

Rapid and accurate numerical evolution of linear cosmological perturbations with non-cold relics What can CMB observations tell us about the neutrino distribution function?

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-07T11:36:50.296107Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T11:36:50.296107Z digest=sha256:3437f354619d073f557211543bb95f49215ef9a204cb6b0067758c682b988f08

Observation 479b0203-dd44-4202-afa7-5349d3afe4bb · 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 What can CMB observations tell us about the neutrino distribution function?

Reference 84

Resolution
verified exact
arxiv_id, observed 2026-05-13T05:37:19.351389Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-13T05:32:39.605539Z digest=sha256:b61c7aae65c17a32adeb89840b22b306dd6c997e4b781b5234f91b45f3feeca4

Observation cb848d06-587b-482f-9839-7c8e08a44799 · inbound

Probing the neutrino chemical potential with cosmological observations cites this paper.

Probing the neutrino chemical potential with cosmological observations What can CMB observations tell us about the neutrino distribution function?

Reference 6

Resolution
verified exact
arxiv_id, observed 2026-07-01T17:35:51.591442Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-06-29T03:34:41.413967Z digest=sha256:81de263dd201e82515192f8f8f71699bafcf3b9d76e78711b39a00836b963056