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Paper Citation Record · LEDGER

Which first order phase transitions to quark matter are possible in neutron stars?

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 4 inbound Pith citation observations for arXiv:2312.10148.

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pith.paper-citation-record.v1
2312.10148 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 4 of 4 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T19:05:26.130057Z

measured 0 of 1 external citation measurements

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Source: arxiv_reference, observed 2026-07-03T22:08:58.784723Z

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0 of 0 outbound references displayed

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Pith citing papers

Observation de0bafae-d6ad-45bb-bf5c-6eccb637a560 · inbound

Strongly Interacting Dark Matter admixed Neutron Stars cites this paper.

Strongly Interacting Dark Matter admixed Neutron Stars Which first order phase transitions to quark matter are possible in neutron stars?

Reference 79

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verified exact
arxiv_id, observed 2026-05-22T22:47:13.444630Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-22T22:45:48.648963Z digest=sha256:f9b1b8f8dddd8063f4201ae6154c01be36ecdc6a3c1e2bf9d9663166da3c8056

Observation bd6a2b5b-c705-4de4-aad2-d41d9a65597f · inbound

Ferromagnetic instabilities in quarkyonic matter cites this paper.

Ferromagnetic instabilities in quarkyonic matter Which first order phase transitions to quark matter are possible in neutron stars?

Reference 16

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unresolved
no resolver link, observed 2026-08-06T19:05:26.130057Z

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T19:05:26.130057Z digest=sha256:3d75d542b4c818e47cc8e2301b14d4535ced8f0d94adb62290961b3c3eaffc2f

Observation 81c8a1f1-61c4-4acc-b3ca-cbf99dd56cf1 · inbound

Subsurface Vacancy Engineering Enables Atomically Clean and Oxidation-Resistant Copper Interfaces for Anode-Free Lithium Metal Batteries cites this paper.

Subsurface Vacancy Engineering Enables Atomically Clean and Oxidation-Resistant Copper Interfaces for Anode-Free Lithium Metal Batteries Which first order phase transitions to quark matter are possible in neutron stars?

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-06T10:19:17.940444Z

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T10:19:17.940444Z digest=sha256:b66bceca1077e1446ebaf31b7d89d177b74d70ecbac11844e8bf4bce2e5a174b

Observation 71de0316-eec2-4998-9e57-6785fc4b629e · inbound

Hybrid Stars with Post-Merger Rotation Profiles cites this paper.

Hybrid Stars with Post-Merger Rotation Profiles Which first order phase transitions to quark matter are possible in neutron stars?

Reference 32

Resolution
verified exact
arxiv_id, observed 2026-07-03T22:08:58.786060Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-06-26T23:50:12.361235Z digest=sha256:a1e237696e38098228cd593fcd72c9c68101aa218a4a688163369d0e69b67267