Paper Citation Record · LEDGER

Can Non-standard Recombination Resolve the Hubble Tension?

As of 3 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1912.00190.

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

pith.paper-citation-record.v1
1912.00190 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-03T06:30:56.289259+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-01T02:46:22.675752Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T05:19:36.141481Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

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 99861f72-1f5b-49a1-b26e-5d0d472953e1 · inbound

Unified dark sector and Hubble-tension alleviation in scalar-vector-tensor gravity cites this paper.

Unified dark sector and Hubble-tension alleviation in scalar-vector-tensor gravity Can Non-standard Recombination Resolve the Hubble Tension?

Reference 30

Resolution: verified exact; arxiv_id, observed 2026-06-30T20:15:05.467395Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

Observation b7ed072c-ea58-47c3-bebc-fda8f1d9e871 · inbound

Early- and Late-Time Modifications to $\Lambda$CDM: Implications for the Hubble Tension cites this paper.

Early- and Late-Time Modifications to $\Lambda$CDM: Implications for the Hubble Tension Can Non-standard Recombination Resolve the Hubble Tension?

Reference 30

Resolution: verified exact; arxiv_id, observed 2026-06-30T00:14:05.084224Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

Observation 9a737372-bf16-409a-81f9-5297ec84f298 · inbound

The Hubble tension: A decade review cites this paper.

The Hubble tension: A decade review Can Non-standard Recombination Resolve the Hubble Tension?

Reference 225

Resolution: verified exact; arxiv_id, observed 2026-07-04T05:19:36.142895Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-03T06:30:56.289259+00:00.

Observation e8b781ec-06fc-4ade-9cab-09671fd32825 · inbound

The Hubble tension: A decade review cites this paper.

The Hubble tension: A decade review Can Non-standard Recombination Resolve the Hubble Tension?

Reference 225

Resolution: unresolved; no resolver link, observed 2026-07-15T10:41:50.733215Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 28411046-8a5b-4730-9c0d-a62ce4f557e9 · inbound

Early- and late-time constraints on Wald-Gauss-Bonnet topological dark energy and implications for the $H_0$ and $S_8$ tensions cites this paper.

Early- and late-time constraints on Wald-Gauss-Bonnet topological dark energy and implications for the $H_0$ and $S_8$ tensions Can Non-standard Recombination Resolve the Hubble Tension?

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-01T02:46:22.675752Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.