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Paper Citation Record · LEDGER

Relativistic mean-field predictions for dense matter equation of state and application to neutron stars

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2503.23028.

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

pith.paper-citation-record.v1
2503.23028 v1

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 2026-08-09T06:31:02.800959+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T16:49:31.555882Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T07:56:57.845097Z

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 d01933d7-0b97-4c25-9c76-57cf4be4a116 · inbound

Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State cites this paper.

Systematics from NICER Pulse Profiles Drive Uncertainty in Multi-Messenger Inference of the Neutron Star Equation of State Relativistic mean-field predictions for dense matter equation of state and application to neutron stars

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-06T16:49:31.555882Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 38610576-08f5-48af-b2b4-62dd92eaaa08 · inbound

The equation of state for neutron stars with speed of sound constraints via Bayesian inference cites this paper.

The equation of state for neutron stars with speed of sound constraints via Bayesian inference Relativistic mean-field predictions for dense matter equation of state and application to neutron stars

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-05T11:14:11.711821Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-05T11:14:11.711821Z digest=sha256:5dba7418e30f8b286a0bfd0cc732da55f55b5f201f660b043d79a9a89dd7c723

Observation ad39d0fa-5088-4304-81c1-f4343f2fbe02 · 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 Relativistic mean-field predictions for dense matter equation of state and application to neutron stars

Reference 73

Resolution
verified exact
arxiv_id, observed 2026-07-04T07:49:39.121611Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-06-26T12:50:53.032717Z digest=sha256:d089baf97fa444ed7e388c50b0a9b6beb4b886cef60164e20cc158dd95d442a9

Observation 246fb29f-fbf4-46c6-acbd-6786fa0800ad · inbound

Relativistic Mean Field Approach with Chiral Symmetry Breaking and Quark Confinement in the light of Astrophysical Observations cites this paper.

Relativistic Mean Field Approach with Chiral Symmetry Breaking and Quark Confinement in the light of Astrophysical Observations Relativistic mean-field predictions for dense matter equation of state and application to neutron stars

Reference 131

Resolution
verified exact
local_arxiv, observed 2026-07-10T07:56:57.847030Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.

source=pdf_text observed=2026-07-10T07:51:26.601892Z digest=sha256:aefc2eb1d8c8c587bd154e6bb615352182de8272ef32073ff2b42708bc62d7d5

Observation bda7010c-3be7-42cf-9e25-637c537e3516 · inbound

Effects of dark matter and magnetic field on neutron star properties in relativistic mean-field theory: A single-fluid approach cites this paper.

Effects of dark matter and magnetic field on neutron star properties in relativistic mean-field theory: A single-fluid approach Relativistic mean-field predictions for dense matter equation of state and application to neutron stars

Reference 47

Resolution
unresolved
no resolver link, observed 2026-07-13T05:17:12.889672Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-13T05:17:12.889672Z digest=sha256:b8e5edbfb64070ec601702f990628ce9afa5150593ae4aad4590226e449488e5