Pith. sign in

Paper Citation Record · LEDGER

Collisional versus Collisionless Dark Matter

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:astro-ph/0002308.

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

pith.paper-citation-record.v1
astro-ph/0002308 v2

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 2026-08-10T06:31:04.303077+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T23:34:34.741239Z

measured 0 of 1 external citation measurements

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

Source: cited_works

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 f1de08ec-bb70-4042-ac23-b9e2587b4894 · inbound

Can a secluded self-interacting dark sector generate detectable gravitational waves? cites this paper.

Can a secluded self-interacting dark sector generate detectable gravitational waves? Collisional versus Collisionless Dark Matter

Reference 18

Resolution
unresolved
no resolver link, observed 2026-08-08T23:34:34.741239Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T23:34:34.741239Z digest=sha256:c4dd306df0a5f80d280a8371d1df7f7896a2781a21020e2e00ad400a62bae41c

Observation 578d5b3e-113a-47ab-84d2-bf92ec14994c · inbound

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps cites this paper.

Cosmological simulations of the same spiral galaxy: satellite properties, the role of baryonic physics and star formation history in shaping dark matter cores/cusps Collisional versus Collisionless Dark Matter

Reference 4

Resolution
unresolved
no resolver link, observed 2026-08-04T22:14:21.701783Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T22:14:21.701783Z digest=sha256:69c4e835e9f07b27fd9736d6046538f3bf00703434865d4cf6ed339a99ce6b05