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Paper Citation Record · LEDGER

Constraints on strong phase transitions in neutron stars

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2212.10576.

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

pith.paper-citation-record.v1
2212.10576 v2

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 2026-08-22T06:32:14.747728+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T00:09:04.281990Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-06T17:18:13.178545Z

Reference resolution

0 of 0 outbound references displayed

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation b0ead121-133a-4c46-bdf8-4216611e0791 · inbound

X-ray pulsed light curves of highly compact neutron stars as probes of scalar-tensor theories of gravity cites this paper.

X-ray pulsed light curves of highly compact neutron stars as probes of scalar-tensor theories of gravity Constraints on strong phase transitions in neutron stars

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-11T12:49:06.113346Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T12:49:06.113346Z digest=sha256:432fafbc5552f7257c902b0cfb19f5f69ddc99e3c8f6aac30142618f6f8a3fdc

Observation 35735da9-7ff6-44dd-89de-6a938cedffb0 · inbound

Coherent State Path Integral Reveals Unexpected Vacuum Structure in Thermal Field Theory cites this paper.

Coherent State Path Integral Reveals Unexpected Vacuum Structure in Thermal Field Theory Constraints on strong phase transitions in neutron stars

Reference 57

Resolution
verified exact
local_arxiv, observed 2026-08-06T17:18:13.210327Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-22T06:32:14.747728+00:00.

source=pdf_text observed=2026-08-06T17:18:07.384763Z digest=sha256:db6b3eb47e1143b0fc28897df3007385deeeb919395e136ab5e4e4d6cefc2037

Observation d7155f7c-8bf2-4265-805a-68bd93c17ce7 · inbound

Can average speed of sound and thermodynamic response functions signal the exotic phases in neutron star cores? cites this paper.

Can average speed of sound and thermodynamic response functions signal the exotic phases in neutron star cores? Constraints on strong phase transitions in neutron stars

Reference 33

Resolution
unresolved
no resolver link, observed 2026-07-11T05:52:28.674753Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-11T05:52:28.674753Z digest=sha256:85b6d2930f4994e0c61b6d4a86cd826956aa3028ee50332bcc184a77997843c2

Observation 7a191ac3-6e1c-4efc-884e-8ccb5650283e · inbound

Quantifying the Information Gain from Future High-Precision Radius Measurements for Identifying Twin Neutron Stars cites this paper.

Quantifying the Information Gain from Future High-Precision Radius Measurements for Identifying Twin Neutron Stars Constraints on strong phase transitions in neutron stars

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-01T16:06:33.632182Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T16:06:33.632182Z digest=sha256:64f0deb6ee73fd2fbdfb4ba0667fb3ae631f7eea8de869386d804551df242ed4

Observation a4f80822-aca1-4cca-b891-df827f6a0165 · inbound

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition cites this paper.

How Neutron Star Radii Encode the Dense-Matter Equation of State and Hadron-Quark Transition Constraints on strong phase transitions in neutron stars

Reference 20

Resolution
unresolved
no resolver link, observed 2026-08-16T00:09:04.281990Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-16T00:09:04.281990Z digest=sha256:afde274e4b2fbfb761ee95ac17aeb40128ee3c02e4d9a090b74ed2d628c82c73