Paper Citation Record · LEDGER

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

As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 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 10 of 10 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-23T06:30:58.430688+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-15T19:14:09.983920Z

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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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 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 2026-08-23T06:30:58.430688+00:00.

Observation eaf323c3-d726-4826-8b2e-68987019819e · inbound

Dark Bondi Accretion Aided by Baryons and the Origin of JWST Little Red Dots cites this paper.

Dark Bondi Accretion Aided by Baryons and the Origin of JWST Little Red Dots Strong Dark Matter Self-interactions Diversify Halo Populations within and surrounding the Milky Way

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-15T19:14:09.983920Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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 2026-08-23T06:30:58.430688+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 2026-08-23T06:30:58.430688+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 2026-08-23T06:30:58.430688+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 2026-08-23T06:30:58.430688+00:00.