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Paper Citation Record · LEDGER

Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of $^{208}$Pb with Minimal Modeling Assumptions

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2102.10074.

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pith.paper-citation-record.v1
2102.10074 v2

Coverage vector

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Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 7 of 7 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 7 of 7 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T00:43:19.671183Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T19:10:05.577637Z

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External citation measurements

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Outbound references

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Pith citing papers

Observation 0f6ed6d5-4fe5-4be3-9cc9-14a1f8a68879 · inbound

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring cites this paper.

Designing Singing Syllabi with Virtual Avatars: AI-Assisted Syllabus Reauthoring Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of $^{208}$Pb with Minimal Modeling Assumptions

Reference 44

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unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 1f9f8a6e-514d-43b8-ad96-86d2c5236a30 · 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 Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of $^{208}$Pb with Minimal Modeling Assumptions

Reference 245

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Unavailable: canonical work link unavailable.

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Observation e3e3378e-7a08-42f8-afe2-e221d9941629 · inbound

Constraining Hamiltonians from chiral effective field theory with neutron-star data cites this paper.

Constraining Hamiltonians from chiral effective field theory with neutron-star data Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of $^{208}$Pb with Minimal Modeling Assumptions

Reference 84

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Observation 766144df-cabc-4541-8c71-e53edb1f1dca · inbound

Ab initio calculations of parity-violating electron scattering off $^{48}$Ca and $^{208}$Pb cites this paper.

Ab initio calculations of parity-violating electron scattering off $^{48}$Ca and $^{208}$Pb Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of $^{208}$Pb with Minimal Modeling Assumptions

Reference 5

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verified exact
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Observation 63f110b4-ccca-4091-9006-2dfa28d2e722 · inbound

The petit four of color-superconducting phases in proto-neutron star evolution cites this paper.

The petit four of color-superconducting phases in proto-neutron star evolution Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of $^{208}$Pb with Minimal Modeling Assumptions

Reference 72

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 0364c8f4-2f04-4362-8597-7a710f8e64b6 · inbound

Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures cites this paper.

Black hole-neutron star binaries with high spins and large mass asymmetries: III. Properties of the ejected material and its electromagnetic signatures Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of $^{208}$Pb with Minimal Modeling Assumptions

Reference 24

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unresolved
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Unavailable: canonical work link unavailable.

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Observation 19e3a646-646c-449d-85e8-d3608dd17ec1 · inbound

From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State cites this paper.

From Multimessenger Inference to Simulations: A Ranked Ensemble of Finite-Temperature Equations of State Astrophysical Constraints on the Symmetry Energy and the Neutron Skin of $^{208}$Pb with Minimal Modeling Assumptions

Reference 100

Resolution
unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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