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Paper Citation Record · LEDGER

Supercool Composite Dark Matter Beyond 100 TeV

As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2110.13926.

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

pith.paper-citation-record.v1
2110.13926 v3

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 2026-08-15T06:32:42.880941+00:00

measured 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T20:39:36.032587Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T06:59:38.389925Z

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 44b30500-96b0-4ec2-8fe3-b54c8acf4f55 · inbound

Populating dark sectors with relativistic bubble walls cites this paper.

Populating dark sectors with relativistic bubble walls Supercool Composite Dark Matter Beyond 100 TeV

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-11T20:39:36.032587Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T20:39:36.032587Z digest=sha256:24eff5a535e6703c44d3bddfe00923e4e4e95a81b8f567499f9cfa8011e4c9e8

Observation b77abf3e-7cf9-423e-a2dc-4cf02363f4f6 · inbound

Acoustically driven dark matter freeze-out cites this paper.

Acoustically driven dark matter freeze-out Supercool Composite Dark Matter Beyond 100 TeV

Reference 20

Resolution
unresolved
no resolver link, observed 2026-08-07T01:20:45.659665Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T01:20:45.659665Z digest=sha256:e729a6632e4890cd15036e7e22366bcc70a50476e1d610766c45b556b28291c8

Observation 3309441e-e029-40b5-940e-2259fc88bc41 · inbound

Uncool soft-wall transitions and gravitational waves cites this paper.

Uncool soft-wall transitions and gravitational waves Supercool Composite Dark Matter Beyond 100 TeV

Reference 18

Resolution
verified exact
arxiv_id, observed 2026-05-10T23:20:52.005248Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-05-10T19:12:50.767365Z digest=sha256:2a1ebb26f47dad8cd55b85c0f146d0f1358cbbf44d8b1622ee8ef2b30731e9e1

Observation 2938b534-85f1-4ea6-a004-b4647e305539 · inbound

Theoretical consistency and phenomenology of supercooled cosmological phase transitions cites this paper.

Theoretical consistency and phenomenology of supercooled cosmological phase transitions Supercool Composite Dark Matter Beyond 100 TeV

Reference 22

Resolution
metadata mismatch
arxiv_id, observed 2026-07-04T06:59:38.391684Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-06-26T13:53:10.056352Z digest=sha256:8237786c146d760e79ac22faca1d308e48bc86e2666e218f7c0eaca906d088fb

Observation 09439044-b3dd-4266-a610-35049cc3d75a · inbound

Rich Phenomenology from Simple Ingredients: A Review of Confining Dark Sectors cites this paper.

Rich Phenomenology from Simple Ingredients: A Review of Confining Dark Sectors Supercool Composite Dark Matter Beyond 100 TeV

Reference 206

Resolution
metadata mismatch
arxiv_id, observed 2026-07-01T12:45:43.928026Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-07-01T01:53:12.193904Z digest=sha256:6afbae4e79cbc3c0d0648e30c6ca8b4fe24b6b21872535d18dda18245895d749

Observation 19b97731-8645-4c6d-8a04-9fd8a67c5131 · inbound

Dark matter in composite Higgs models with a scotogenic EFT cites this paper.

Dark matter in composite Higgs models with a scotogenic EFT Supercool Composite Dark Matter Beyond 100 TeV

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-02T02:51:18.798358Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T02:51:18.798358Z digest=sha256:bc519fd0ac4989da7eb88839498ad4ff5e87d16eb2f8cc3b9167b4edd02a7292

Observation 85a533c3-a09e-45e7-b8fe-dcc270255755 · inbound

Particle productions during collisions of highly boosted bubble walls cites this paper.

Particle productions during collisions of highly boosted bubble walls Supercool Composite Dark Matter Beyond 100 TeV

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-01T21:10:05.607318Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T21:10:05.607318Z digest=sha256:7b71f43b98d7bbe23e57b3c3b6fb285df09b1b60dec8668b7dee837d4d8cf9b1

Observation b87b05a2-aea6-4539-a148-f521c7e95383 · inbound

Theoretical uncertainties in reconstructing model parameters with gravitational waves from supercooled phase transitions cites this paper.

Theoretical uncertainties in reconstructing model parameters with gravitational waves from supercooled phase transitions Supercool Composite Dark Matter Beyond 100 TeV

Reference 45

Resolution
unresolved
no resolver link, observed 2026-08-01T15:42:14.778988Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T15:42:14.778988Z digest=sha256:566f1db518feb10098dbfeb9ebb6c43abd08649a9fc553ef10bd609a569053db

Observation 40c5a446-652e-4cb2-835b-8b8067dca450 · inbound

Can the universe be matter-dominated after a supercooled first-order phase transition? cites this paper.

Can the universe be matter-dominated after a supercooled first-order phase transition? Supercool Composite Dark Matter Beyond 100 TeV

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-01T12:45:38.668598Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T12:45:38.668598Z digest=sha256:95fc2cf1038a566134206fadb0022d117d323234a599bfd8c77c621d5aca5cd8

Observation aeedfc3b-1951-4eee-a3ed-d8a7e3896ed3 · inbound

Particle Production via Rippled Bubble Walls cites this paper.

Particle Production via Rippled Bubble Walls Supercool Composite Dark Matter Beyond 100 TeV

Reference 11

Resolution
unresolved
no resolver link, observed 2026-08-01T13:14:49.749538Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T13:14:49.749538Z digest=sha256:21ea77fc29a238050730caa2fb4413837b68107db00de8282e91ad65efc2ef0a