Paper Citation Record · LEDGER

Strong Dark Matter Self-interactions Diversify Halo Populations within and surrounding the Milky Way

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2211.13768.

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

pith.paper-citation-record.v1
2211.13768 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 9 of 9 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 9 of 9 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T23:34:34.803847Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T06:57:42.730197Z

Reference resolution

0 of 0 outbound references displayed

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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 de4b6585-5236-41e0-8cff-a4be082b08f0 · 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? Strong Dark Matter Self-interactions Diversify Halo Populations within and surrounding the Milky Way

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.803847Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8f2e3047-e3b7-46cf-9132-cbd8a0b587f8 · 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 Strong Dark Matter Self-interactions Diversify Halo Populations within and surrounding the Milky Way

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:20.207237Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 84d91abc-5a85-4cb6-ab11-72460f734b0e · inbound

Self-Interacting Dark Matter with Mass Segregation: A Unified Explanation of Dwarf Cores and Small-Scale Lenses cites this paper.

Self-Interacting Dark Matter with Mass Segregation: A Unified Explanation of Dwarf Cores and Small-Scale Lenses Strong Dark Matter Self-interactions Diversify Halo Populations within and surrounding the Milky Way

Reference 51

Resolution: verified exact; arxiv_id, observed 2026-05-19T08:47:13.052076Z

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.

Observation 233bd24e-60c0-4969-ac3d-235c4cb8c170 · inbound

Pion dark matter in a $\theta$ vacuum: a thermal relic with sharp velocity-dependent self-interactions cites this paper.

Pion dark matter in a $\theta$ vacuum: a thermal relic with sharp velocity-dependent self-interactions Strong Dark Matter Self-interactions Diversify Halo Populations within and surrounding the Milky Way

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-05T14:45:20.900968Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7d1696e2-9307-40b9-95dd-28734c4c04b0 · inbound

Strong-lensing Perturber Signatures in Self-interacting Dark Matter Simulations cites this paper.

Strong-lensing Perturber Signatures in Self-interacting Dark Matter Simulations Strong Dark Matter Self-interactions Diversify Halo Populations within and surrounding the Milky Way

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-04T12:56:23.715664Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 91abbf05-d222-4257-8450-c78b2aeedc18 · inbound

Bypassed Core Formation in Milky Way-Mass SIDM Halos: Implications for the Local Group Past-Pericenter Scenario cites this paper.

Bypassed Core Formation in Milky Way-Mass SIDM Halos: Implications for the Local Group Past-Pericenter Scenario Strong Dark Matter Self-interactions Diversify Halo Populations within and surrounding the Milky Way

Reference 30

Resolution: verified exact; arxiv_id, observed 2026-05-11T08:00:58.394632Z

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.

Observation 2491ee24-7d23-4994-97fd-8e4fbc0b0f22 · inbound

Probing Collapsed Dark Matter Halos with Fast Radio Bursts cites this paper.

Probing Collapsed Dark Matter Halos with Fast Radio Bursts Strong Dark Matter Self-interactions Diversify Halo Populations within and surrounding the Milky Way

Reference 55

Resolution: verified exact; arxiv_id, observed 2026-05-11T08:46:00.538732Z

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.

Observation e722b03a-041a-4ed4-b70b-d60ed717bfed · inbound

Gravothermal Collapse: Robust Against Baryonic Feedback cites this paper.

Gravothermal Collapse: Robust Against Baryonic Feedback Strong Dark Matter Self-interactions Diversify Halo Populations within and surrounding the Milky Way

Reference 52

Resolution: verified exact; arxiv_id, observed 2026-07-01T20:36:11.596417Z

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.

Observation 71d40746-649a-4c3a-89c9-f90eeb8b95c9 · 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 Strong Dark Matter Self-interactions Diversify Halo Populations within and surrounding the Milky Way

Reference 60

Resolution: verified exact; arxiv_id, observed 2026-07-03T06:57:42.731653Z

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.