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Paper Citation Record · LEDGER

Interface modes in inspiralling neutron stars: A gravitational-wave probe of first-order phase transitions

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2504.06181.

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

pith.paper-citation-record.v1
2504.06181 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T15:35:19.053519Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T19:08:50.085109Z

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 6b0b2f73-9d0e-422f-a31b-597e0f168658 · inbound

Model-Independent Determination of the Tidal Deformability of a 1.4 $M_{\odot}$ Neutron Star from Gravitational-Wave Measurements cites this paper.

Model-Independent Determination of the Tidal Deformability of a 1.4 $M_{\odot}$ Neutron Star from Gravitational-Wave Measurements Interface modes in inspiralling neutron stars: A gravitational-wave probe of first-order phase transitions

Reference 14

Resolution
unresolved
no resolver link, observed 2026-08-07T15:35:19.053519Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T15:35:19.053519Z digest=sha256:395ee475d03b7a91e3efcd76d79775846fff4236fc33cc33a3bd9a1581ac8570

Observation bf8d7133-d179-4aa5-8b8f-037e37fa115e · inbound

Dynamical neutron-star tides: The signature of a mode resonance cites this paper.

Dynamical neutron-star tides: The signature of a mode resonance Interface modes in inspiralling neutron stars: A gravitational-wave probe of first-order phase transitions

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-05T22:52:12.781475Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T22:52:12.781475Z digest=sha256:332bab7d9274d5a0035d425f3854708b4f4863cfea2d16abf3f3ec8d19427bec

Observation b66b24b4-ab59-4916-8ec1-a892ceecce9d · inbound

Universal Relations with Dynamical Tides cites this paper.

Universal Relations with Dynamical Tides Interface modes in inspiralling neutron stars: A gravitational-wave probe of first-order phase transitions

Reference 56

Resolution
verified exact
arxiv_id, observed 2026-05-17T05:54:08.485040Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-05-17T05:53:11.977211Z digest=sha256:4a0fa5086225191895010d7f4503c8500460aae43777d30eca8e66bd59ea9b2b

Observation 621f37f8-8e03-4fb7-8aad-345aaac6cd87 · inbound

TTE-CAM: Self-Explainable Class Activation Maps for Pretrained Black-Box CNNs cites this paper.

TTE-CAM: Self-Explainable Class Activation Maps for Pretrained Black-Box CNNs Interface modes in inspiralling neutron stars: A gravitational-wave probe of first-order phase transitions

Reference 21

Resolution
unresolved
no resolver link, observed 2026-07-13T17:23:25.842886Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-13T17:23:25.842886Z digest=sha256:357b25bb9e616855a0e6e4635b8ffa454c6d199fa967c297f602d30f741dfa27

Observation bfaebac6-1240-42d3-af21-bb02e8bd71ac · inbound

Can a Slow and Strong Phase Transition in Neutron Stars Relieve Major Compact-Star Observation Tensions? cites this paper.

Can a Slow and Strong Phase Transition in Neutron Stars Relieve Major Compact-Star Observation Tensions? Interface modes in inspiralling neutron stars: A gravitational-wave probe of first-order phase transitions

Reference 94

Resolution
verified exact
arxiv_id, observed 2026-07-03T19:08:50.086571Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

source=pdf_text observed=2026-06-27T02:06:36.071557Z digest=sha256:76512cf8fa30d3625cbc5298d01b6982f4db8060b2160b3080031a05ec3d5780