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Paper Citation Record · LEDGER

Cosmic bubble and domain wall instabilities I: parametric amplification of linear fluctuations

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1412.5591.

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

pith.paper-citation-record.v1
1412.5591 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T21:24:36.640182Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T21:24:36.818643Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

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 5bafa7cf-944b-462b-874c-73231883cf04 · inbound

Thin and thick bubble walls III: wall energy cites this paper.

Thin and thick bubble walls III: wall energy Cosmic bubble and domain wall instabilities I: parametric amplification of linear fluctuations

Reference 14

Resolution
verified exact
local_arxiv, observed 2026-08-10T21:24:36.822739Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-10T21:24:36.640182Z digest=sha256:e063950f82ed17c3f4d00484130c0fdb05deab47bae1086580b8c976dda8b7f2

Observation e2a2c4b6-cff9-4c2b-a588-fc7cfbe98776 · 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? Cosmic bubble and domain wall instabilities I: parametric amplification of linear fluctuations

Reference 181

Resolution
unresolved
no resolver link, observed 2026-08-01T12:45:39.355506Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T12:45:39.355506Z digest=sha256:ac1d7f9623a3853402e894ded5ee160562ab5df52f06de3507a0e686ffada13a