Paper Citation Record · LEDGER

A Quantitative Study of Interacting Dark Matter in Halos

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 8 inbound Pith citation observations for arXiv:astro-ph/0003483.

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

pith.paper-citation-record.v1
astro-ph/0003483 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 8 of 8 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 8 of 8 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T23:34:34.723998Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

External citation measurements

131
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 8c8a0c94-c9c2-40cd-8c0a-f2d1111e775d · 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? A Quantitative Study of Interacting Dark Matter in Halos

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-08T23:34:34.723998Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 689e5434-3743-4038-8e86-732678a05ec6 · inbound

Calibrating the SIDM Gravothermal Catastrophe with N-body Simulations cites this paper.

Calibrating the SIDM Gravothermal Catastrophe with N-body Simulations A Quantitative Study of Interacting Dark Matter in Halos

Reference 46

Resolution: verified exact; local_arxiv, observed 2026-05-22T19:32:00.782580Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 6ac4efa8-f459-4148-b2ee-7fec42a552fb · 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 A Quantitative Study of Interacting Dark Matter in Halos

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:20.217739Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c6749b1c-f8fc-45e5-963d-775f09801e80 · inbound

MARVELously Dark: the density profile evolution of dwarf halos in velocity-dependent SIDM cites this paper.

MARVELously Dark: the density profile evolution of dwarf halos in velocity-dependent SIDM A Quantitative Study of Interacting Dark Matter in Halos

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-03T06:13:36.312586Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4908cc70-8fc4-4fba-a5f9-3fa296497dff · inbound

The Sensitivity of Substructure Lensing to SIDM Core-collapse Model Variation cites this paper.

The Sensitivity of Substructure Lensing to SIDM Core-collapse Model Variation A Quantitative Study of Interacting Dark Matter in Halos

Reference 8

Resolution: verified exact; local_arxiv, observed 2026-06-30T14:14:45.687076Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 52724751-3d67-41a4-b841-25b4d5d003cb · inbound

Cooling, conduction, compact objects: Gravothermal evolution of dissipative self-interacting dark matter halos cites this paper.

Cooling, conduction, compact objects: Gravothermal evolution of dissipative self-interacting dark matter halos A Quantitative Study of Interacting Dark Matter in Halos

Reference 61

Resolution: metadata mismatch; local_arxiv, observed 2026-07-04T02:39:24.257226Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 6a3eeb5c-379b-4b81-adef-7cc1028082ce · inbound

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

Self-interacting dark matter promotes bar formation in disk galaxies A Quantitative Study of Interacting Dark Matter in Halos

Reference 8

Resolution: verified exact; local_arxiv, observed 2026-06-29T01:32:58.915999Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation d16af5a1-88e4-4f90-8e64-163443b70452 · inbound

A Novel Implementation of Self-Interacting Dark Matter in AREPO cites this paper.

A Novel Implementation of Self-Interacting Dark Matter in AREPO A Quantitative Study of Interacting Dark Matter in Halos

Reference 101

Resolution: unresolved; no resolver link, observed 2026-07-11T06:38:02.275303Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.