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Paper Citation Record · LEDGER

The impact of inelastic self-interacting dark matter on the dark matter structure of a Milky Way halo

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2010.08562.

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

pith.paper-citation-record.v1
2010.08562 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-09T06:31:02.800959+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T10:52:20.324228Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-10T10:09:06.637899Z

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 8cfd616e-a8f7-45cc-a175-6308c05931ec · inbound

Numerical evolution of self-gravitating halos of self-interacting dark matter cites this paper.

Numerical evolution of self-gravitating halos of self-interacting dark matter The impact of inelastic self-interacting dark matter on the dark matter structure of a Milky Way halo

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-07T10:52:20.324228Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T10:52:20.324228Z digest=sha256:f0318612fd80dc0600f293770768e4f666b5133892aa96bb10cc35a046d1ac6d

Observation 02bccd22-a19c-458f-8969-513e255ab1b8 · inbound

Cosmology of Inelastic Self-Interacting Dark Matter: Linear Evolution and Observational Constraints cites this paper.

Cosmology of Inelastic Self-Interacting Dark Matter: Linear Evolution and Observational Constraints The impact of inelastic self-interacting dark matter on the dark matter structure of a Milky Way halo

Reference 47

Resolution
verified exact
arxiv_id, observed 2026-05-10T10:09:06.640225Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-05-10T10:08:33.578196Z digest=sha256:dcd6859aa762f7fa170bd3341b8b01257131b2b4c22769f83959b66e9068ab14