Paper Citation Record · LEDGER

Strongly interacting matter exhibits deconfined behavior in massive neutron stars

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 17 inbound Pith citation observations for arXiv:2303.11356.

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

pith.paper-citation-record.v1
2303.11356 v2

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

measured 17 of 17 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T04:40:52.840607Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T19:00:04.458864Z

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Outbound references

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Pith citing papers

Observation 2655e816-6b50-4ac6-8a7b-0fcce41a8e70 · inbound

Locating the QCD critical point with neutron-star observations cites this paper.

Locating the QCD critical point with neutron-star observations Strongly interacting matter exhibits deconfined behavior in massive neutron stars

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-07T04:40:52.840607Z

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Observation 1794d3e3-fc96-4b08-a0ec-62bc8160e3ff · inbound

Density dependent speed of sound and its consequences in neutron stars cites this paper.

Density dependent speed of sound and its consequences in neutron stars Strongly interacting matter exhibits deconfined behavior in massive neutron stars

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-06T20:31:47.217644Z

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Observation b9f79722-90e2-4c96-83d2-1b9f6a9258dc · inbound

Tracing the Trace Anomaly of Dense Matter inside Neutron Stars cites this paper.

Tracing the Trace Anomaly of Dense Matter inside Neutron Stars Strongly interacting matter exhibits deconfined behavior in massive neutron stars

Reference 12

Resolution: verified exact; arxiv_id, observed 2026-05-17T06:24:09.923884Z

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Observation 7dde4629-4f24-4c85-95b2-be2df089a71c · inbound

Toward a Unified Understanding of the Dense Matter Equation of State cites this paper.

Toward a Unified Understanding of the Dense Matter Equation of State Strongly interacting matter exhibits deconfined behavior in massive neutron stars

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-03T20:20:19.088682Z

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Observation 19155787-2ca9-4244-9b1c-fc19e781035c · inbound

Properties of Stable Massive Quark Stars in Holography cites this paper.

Properties of Stable Massive Quark Stars in Holography Strongly interacting matter exhibits deconfined behavior in massive neutron stars

Reference 8

Resolution: verified exact; arxiv_id, observed 2026-05-17T03:08:56.887346Z

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Observation cbaf0882-9d2a-41fd-998f-7c133fc9d26f · inbound

Isentropic thermodynamics across the hadron-quark mixed phase in a two-phase model with a PNJL quark description cites this paper.

Isentropic thermodynamics across the hadron-quark mixed phase in a two-phase model with a PNJL quark description Strongly interacting matter exhibits deconfined behavior in massive neutron stars

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-02T18:31:51.202326Z

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Observation 43a51cc2-9024-43f0-8ed4-5e1f08fef8c8 · inbound

Sensitivity of Neutron Star Observables to Transition Density in Hybrid Equation-of-State Models cites this paper.

Sensitivity of Neutron Star Observables to Transition Density in Hybrid Equation-of-State Models Strongly interacting matter exhibits deconfined behavior in massive neutron stars

Reference 48

Resolution: verified exact; arxiv_id, observed 2026-05-11T08:30:57.835107Z

Source-reported events for the cited work

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Observation a6d6f6be-1981-4b80-a5a2-55fca0ac3faf · inbound

The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover cites this paper.

The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover Strongly interacting matter exhibits deconfined behavior in massive neutron stars

Reference 26

Resolution: verified exact; arxiv_id, observed 2026-05-12T08:21:25.902408Z

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Observation 35aed5f8-a425-4696-872d-8fdab50b2848 · inbound

The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover cites this paper.

The Non-parametric Equation of State Realizes a Generalized Quark-Hadron Crossover Strongly interacting matter exhibits deconfined behavior in massive neutron stars

Reference 32

Resolution: verified exact; arxiv_id, observed 2026-07-01T13:15:46.540126Z

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.

Observation 0baf9295-fb51-47eb-ba52-553f62d935bc · inbound

Sensitivity of the Neutron Star Equation of State Inferences to Mass and Radius Measurements cites this paper.

Sensitivity of the Neutron Star Equation of State Inferences to Mass and Radius Measurements Strongly interacting matter exhibits deconfined behavior in massive neutron stars

Reference 15

Resolution: verified exact; arxiv_id, observed 2026-07-02T04:06:35.479603Z

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.

Observation 9e4c26e5-5e74-4f3e-9b13-af7e9dae4e95 · 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? Strongly interacting matter exhibits deconfined behavior in massive neutron stars

Reference 19

Resolution: verified exact; arxiv_id, observed 2026-07-03T19:08:50.134128Z

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

Observation 04b1144c-43c8-49d4-88e5-5bb43fed16f4 · inbound

Is the coexistence of strange quark stars and hadronic stars favored by astrophysical data? A Bayesian analysis cites this paper.

Is the coexistence of strange quark stars and hadronic stars favored by astrophysical data? A Bayesian analysis Strongly interacting matter exhibits deconfined behavior in massive neutron stars

Reference 91

Resolution: verified exact; arxiv_id, observed 2026-07-04T07:49:38.833933Z

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.

Observation 5237077a-e86d-4f34-b30b-2159c0da8d65 · inbound

Observables and conformal properties of dark matter admixed isentropic neutron stars cites this paper.

Observables and conformal properties of dark matter admixed isentropic neutron stars Strongly interacting matter exhibits deconfined behavior in massive neutron stars

Reference 65

Resolution: metadata mismatch; arxiv_id, observed 2026-07-04T11:19:50.482552Z

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.

Observation 452ad6b5-6deb-4f12-974b-299cdcaef5ac · inbound

Causality alone bounds the maximum radius difference between different-mass neutron stars cites this paper.

Causality alone bounds the maximum radius difference between different-mass neutron stars Strongly interacting matter exhibits deconfined behavior in massive neutron stars

Reference 19

Resolution: verified exact; arxiv_id, observed 2026-07-04T19:00:04.460185Z

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.

Observation c6cc9cc8-e13a-417e-a05e-10cceadd9b63 · inbound

Quark and hybrid stars with renormalization group improvement of NNLO perturbative QCD cites this paper.

Quark and hybrid stars with renormalization group improvement of NNLO perturbative QCD Strongly interacting matter exhibits deconfined behavior in massive neutron stars

Reference 12

Resolution: verified exact; arxiv_id, observed 2026-06-30T03:04:15.009737Z

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.

Observation b96f4ec3-e489-474d-8d6b-d7d21e09868d · 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? Strongly interacting matter exhibits deconfined behavior in massive neutron stars

Reference 11

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

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Observation 71ad5e24-dd3a-446f-9bb8-f44a4024c27e · inbound

Quarkyonic Stars with Strangeness cites this paper.

Quarkyonic Stars with Strangeness Strongly interacting matter exhibits deconfined behavior in massive neutron stars

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-01T13:16:52.121125Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.