Paper Citation Record · LEDGER

How the Self-Interacting Dark Matter Model Explains the Diverse Galactic Rotation Curves

As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:1611.02716.

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

pith.paper-citation-record.v1
1611.02716 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 7 of 7 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-06T06:34:29.942622+00:00

measured 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-03T19:01:06.129005Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-03T06:57:42.802281Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
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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 f791fb38-b302-42d5-98d0-d4e529ef2f0e · inbound

Modeling dark matter halos with self-interacting fermions: A polytropic approach cites this paper.

Modeling dark matter halos with self-interacting fermions: A polytropic approach How the Self-Interacting Dark Matter Model Explains the Diverse Galactic Rotation Curves

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-03T19:01:06.129005Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d9c1a7b5-6809-476b-a407-4d445789878a · inbound

Scalar-Mediated Inelastic Dark Matter as a Solution to Small-Scale Structure Anomalies cites this paper.

Scalar-Mediated Inelastic Dark Matter as a Solution to Small-Scale Structure Anomalies How the Self-Interacting Dark Matter Model Explains the Diverse Galactic Rotation Curves

Reference 28

Resolution: verified exact; local_arxiv, observed 2026-05-16T21:13:32.464401Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 821e4285-03ea-4e66-8be8-e13f0479540e · inbound

Reionization Topology as a Probe of Self-Interacting Dark Matter cites this paper.

Reionization Topology as a Probe of Self-Interacting Dark Matter How the Self-Interacting Dark Matter Model Explains the Diverse Galactic Rotation Curves

Reference 7

Resolution: verified exact; arxiv_id, observed 2026-05-11T10:41:01.946939Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 2d352650-ebe6-479e-befa-51aabd9b2a0f · inbound

Breaking the UV Luminosity Function Degeneracy:Self-Interacting Dark Matter Constraints from Reionization Topology cites this paper.

Breaking the UV Luminosity Function Degeneracy:Self-Interacting Dark Matter Constraints from Reionization Topology How the Self-Interacting Dark Matter Model Explains the Diverse Galactic Rotation Curves

Reference 13

Resolution: verified exact; arxiv_id, observed 2026-05-11T13:31:05.035563Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation 764b4fe1-ff5d-4c91-bbf2-c2633640a1cf · inbound

Steep Redshift Evolution of the Ionizing Escape Fraction at $z = 5$--$12$: Empirical Constraints and Comparison with Simulations cites this paper.

Steep Redshift Evolution of the Ionizing Escape Fraction at $z = 5$--$12$: Empirical Constraints and Comparison with Simulations How the Self-Interacting Dark Matter Model Explains the Diverse Galactic Rotation Curves

Reference 17

Resolution: verified exact; local_arxiv, observed 2026-06-28T05:21:41.050280Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation dc96efcc-dbf8-4299-bf5c-5278454562eb · inbound

Self-interacting dark matter promotes bar formation in disk galaxies cites this paper.

Self-interacting dark matter promotes bar formation in disk galaxies How the Self-Interacting Dark Matter Model Explains the Diverse Galactic Rotation Curves

Reference 56

Resolution: verified exact; local_arxiv, observed 2026-06-29T01:32:58.888487Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.

Observation d9e2a868-f132-4b30-bc26-6dba03aaf922 · inbound

Spherically Symmetric Fluid Simulations of Black Hole Accretion in Self-Interacting Dark Matter Halos cites this paper.

Spherically Symmetric Fluid Simulations of Black Hole Accretion in Self-Interacting Dark Matter Halos How the Self-Interacting Dark Matter Model Explains the Diverse Galactic Rotation Curves

Reference 22

Resolution: verified exact; local_arxiv, observed 2026-07-03T06:57:42.803682Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-06T06:34:29.942622+00:00.