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Paper Citation Record · LEDGER

Higher Spin Dark Matter

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2010.15125.

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

pith.paper-citation-record.v1
2010.15125 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T12:23:11.626390Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-01T12:35:44.472914Z

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 ffdc9ca8-170b-47b2-a0a9-097ff579fad5 · inbound

Superheavy Dark Matter from the String Theory Axiverse cites this paper.

Superheavy Dark Matter from the String Theory Axiverse Higher Spin Dark Matter

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-16T12:23:11.626390Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T12:23:11.626390Z digest=sha256:0bc01ccf8c4ea9b353d8c10d3fe828f56466f2815967e68eea87cf0172569a0c

Observation 54804ea2-6a30-462a-b49f-d34ed0e41a07 · inbound

The effects of non Bunch-Davies initial conditions on gravitationally produced relics cites this paper.

The effects of non Bunch-Davies initial conditions on gravitationally produced relics Higher Spin Dark Matter

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-02T19:15:18.135841Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T19:15:18.135841Z digest=sha256:5db3e8556e95a5cd5e7374df7535a9f19427ea358fd1d1358c8508b5c61cdd9e

Observation 06554391-10d6-4210-aab1-608fc368f397 · inbound

Numerical polology: towards next-generation model-building for cosmology cites this paper.

Numerical polology: towards next-generation model-building for cosmology Higher Spin Dark Matter

Reference 35

Resolution
verified exact
arxiv_id, observed 2026-07-01T12:35:44.474653Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-07-01T01:53:27.058990Z digest=sha256:16e1e9c125488ae3560966308cb2b7206219c83bf2691f647593db1aa6a11dba

Observation 553a3abc-8f9d-4508-8688-5b9949464918 · inbound

Numerical polology: towards next-generation model-building for cosmology cites this paper.

Numerical polology: towards next-generation model-building for cosmology Higher Spin Dark Matter

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-02T09:32:00.022985Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T09:32:00.022985Z digest=sha256:86ff3ca05dd63923c1132bc8c63f09d4d7ff71fe16609d970a5e55b3f6dd4096