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Paper Citation Record · LEDGER

Halo Properties in Cosmological Simulations of Self-Interacting Cold Dark Matter

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:astro-ph/0006218.

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

pith.paper-citation-record.v1
astro-ph/0006218 v1

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 2026-08-09T06:31:02.800959+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T23:34:34.772352Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-04T02:39:24.153207Z

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 71f98f64-54ad-424e-aa16-b46fe76ce28f · 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? Halo Properties in Cosmological Simulations of Self-Interacting Cold Dark Matter

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-08T23:34:34.772352Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T23:34:34.772352Z digest=sha256:564f5c0a2c944a3351a0e625f45be1556b088121ff22e8cdae211742f6f8b6a2

Observation 6597db9a-a6c9-4758-80da-949d9c699bee · 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 Halo Properties in Cosmological Simulations of Self-Interacting Cold Dark Matter

Reference 15

Resolution
unresolved
no resolver link, observed 2026-08-07T10:52:20.227534Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T10:52:20.227534Z digest=sha256:4dd1efc5c49116eac83ba9ae05d08315b6c07dea0cec3c43281a2f561e560351

Observation 1de440bb-ec61-46fc-a2c1-66ec8c9c872f · 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 Halo Properties in Cosmological Simulations of Self-Interacting Cold Dark Matter

Reference 81

Resolution
unresolved
no resolver link, observed 2026-08-05T14:45:20.820889Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T14:45:20.820889Z digest=sha256:3c36cb082e3f54c1f75de7ecee4f9f3438726987806c9fe237beda3b4d792b3f

Observation 0c6393ae-dc56-41a7-9f5d-f3f7f39645f2 · inbound

Nearly Degenerate Majorana Dark Matter and Its Self-Interactions in a Gauged $U(1)_{L_\mu - L_\tau}$ Model cites this paper.

Nearly Degenerate Majorana Dark Matter and Its Self-Interactions in a Gauged $U(1)_{L_\mu - L_\tau}$ Model Halo Properties in Cosmological Simulations of Self-Interacting Cold Dark Matter

Reference 106

Resolution
verified exact
local_arxiv, observed 2026-05-17T01:23:48.887117Z

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.

source=pdf_text observed=2026-05-17T01:22:56.006007Z digest=sha256:19c809215303a7fe3da49508e69bec10d850c9d3b6eb950a560aeb1b4c0d1c65

Observation f34623cc-fa0b-4b8f-beac-25dfdb143773 · 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 Halo Properties in Cosmological Simulations of Self-Interacting Cold Dark Matter

Reference 33

Resolution
unresolved
no resolver link, observed 2026-08-03T06:13:32.210977Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T06:13:32.210977Z digest=sha256:e5166bf913a90432670a3bcd19d3151068188a6a973b6c3206609ab2a7ddaf4d

Observation 364b9300-6557-4271-afad-7eb253b075e7 · inbound

Axion-Like Electrophilic Portal for Pion Dark Matter cites this paper.

Axion-Like Electrophilic Portal for Pion Dark Matter Halo Properties in Cosmological Simulations of Self-Interacting Cold Dark Matter

Reference 39

Resolution
verified exact
local_arxiv, observed 2026-05-16T08:02:33.835741Z

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.

source=pdf_text observed=2026-05-16T08:02:11.945688Z digest=sha256:e8a3c620e0057062e87327ca7d13993b5499f48263b9939873e604747faecefe

Observation 26ec9623-4eea-4cd2-a27c-019779b6fda5 · inbound

It's Not Just Star Formation: A trend of low dark matter densities in the Andromeda dwarf galaxy system cites this paper.

It's Not Just Star Formation: A trend of low dark matter densities in the Andromeda dwarf galaxy system Halo Properties in Cosmological Simulations of Self-Interacting Cold Dark Matter

Reference 182

Resolution
verified exact
local_arxiv, observed 2026-06-28T21:32:38.557027Z

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.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:0c46860209ed1fe48430bedc698fa1ecd623c3c2e09c9799919fcef83912a355

Observation 03ac8e99-d8f4-4186-9389-dfd51ff9c1cc · 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 Halo Properties in Cosmological Simulations of Self-Interacting Cold Dark Matter

Reference 60

Resolution
metadata mismatch
local_arxiv, observed 2026-07-04T02:39:24.155909Z

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.

source=arxiv_source observed=2026-06-26T19:37:26.893514Z digest=sha256:83385f6eeb2d6821d7fe79ee7fb79949a89d3e2f24bb48bedbffcb40dc35e690

Observation a63e25f1-ea32-4efb-9e99-2a92a739a2c0 · inbound

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

A Novel Implementation of Self-Interacting Dark Matter in AREPO Halo Properties in Cosmological Simulations of Self-Interacting Cold Dark Matter

Reference 44

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-07-11T06:38:02.275303Z digest=sha256:1f60b8c2da974c65726981887fa83b243262ed92186ccf3c4a87d238fd5d6908

Observation c02d29e7-7fad-438f-a9f1-b0b008e7dd76 · inbound

High resolution Lyman-{\alpha} forest constraints on dark matter-neutrino scattering cites this paper.

High resolution Lyman-{\alpha} forest constraints on dark matter-neutrino scattering Halo Properties in Cosmological Simulations of Self-Interacting Cold Dark Matter

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-02T00:29:45.298335Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T00:29:45.298335Z digest=sha256:10741b092bccbc40e39309a53650400df6c3bd7c737b0edae417c8557df65afa