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Paper Citation Record · LEDGER

Cosmic implications of a low-scale solution to the axion domain wall problem

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1905.13116.

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

pith.paper-citation-record.v1
1905.13116 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 2026-08-14T06:32:32.682623+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T12:24:03.562047Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-18T14:56:31.172516Z

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 c533fc13-ced5-43c6-8f3e-5b9d4974e9b8 · inbound

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter cites this paper.

Using $\Delta N_{\rm eff}$ to constrain preferred axion model dark matter Cosmic implications of a low-scale solution to the axion domain wall problem

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-12T12:24:03.562047Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-12T12:24:03.562047Z digest=sha256:8306473e5f5b2016e954c0662d142cde815f39505a8db2fc0c25a9b079d41145

Observation b37b79a1-21b8-4abe-90e8-6c61c36db3b7 · inbound

Axions as Dark Matter, Dark Energy, and Dark Radiation cites this paper.

Axions as Dark Matter, Dark Energy, and Dark Radiation Cosmic implications of a low-scale solution to the axion domain wall problem

Reference 26

Resolution
verified exact
arxiv_id, observed 2026-05-18T14:56:31.174517Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-05-18T14:55:46.771551Z digest=sha256:ffec4f3b41d6587229dc0b1e3b8c278a0458f507c51c0868446a7a47201b7f36

Observation e810a967-972a-4ee7-934a-10760602af6c · inbound

How well can the QCD axion hide? cites this paper.

How well can the QCD axion hide? Cosmic implications of a low-scale solution to the axion domain wall problem

Reference 43

Resolution
verified exact
arxiv_id, observed 2026-05-11T07:41:00.700118Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-05-10T17:03:10.846811Z digest=sha256:81234c43084f66503adab8ff207fe00d7cedc5dcabcc03534262746139b9c286