Paper Citation Record · LEDGER

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars

As of 19 August 2026, this Paper Citation Record lists 43 of 43 outbound references and 1 inbound Pith citation observation for arXiv:2505.14921.

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

pith.paper-citation-record.v1
2505.14921 v1

Coverage vector

measured 43 of 43 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-07T15:31:32.716643Z

measured 44 of 44 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-19T06:32:44.657259+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-06-26T00:47:21.247516Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T16:19:57.436349Z

Reference resolution

43 of 43 outbound references displayed

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External citation measurements

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Outbound references

Observation 6e8cb820-f37f-4198-8f70-11d8697ac094 · outbound

This paper cites From hadrons to quarks in neutron stars: a review.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars From hadrons to quarks in neutron stars: a review

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-07T15:31:32.509252Z

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Observation 9d093b45-9274-4c21-9f60-d2cd2f593867 · outbound

This paper cites Theoretical and Experimental Constraints for the Equation of State of Dense and Hot Matter.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Theoretical and Experimental Constraints for the Equation of State of Dense and Hot Matter

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-07T15:31:32.514949Z

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Observation f1419f82-fc3a-4533-a4a0-25b3c1d4d2a5 · outbound

This paper cites an unresolved cited work.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Unresolved cited work

Reference 3

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Observation 667db487-b389-4a7f-996f-f153c46c29b1 · outbound

This paper cites Hot and Dense Homogeneous Nucleonic Matter Constrained by Observations, Experiment, and Theory.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Hot and Dense Homogeneous Nucleonic Matter Constrained by Observations, Experiment, and Theory

Reference 4

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Observation 7d9aec86-7819-43a0-ac87-4345732c13e7 · outbound

This paper cites Hot and Dense Matter Equation of State Probability Distributions for Astrophysical Simulations.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Hot and Dense Matter Equation of State Probability Distributions for Astrophysical Simulations

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-07T15:31:32.529764Z

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Observation 6eaf6bca-58e9-461a-80bc-a9d5bdc925d2 · outbound

This paper cites Steiner and S.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Steiner and S

Reference 6

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Observation 8e972136-626a-4bb5-ba7b-56f9880bf4f0 · outbound

This paper cites Chiral effective field theory and nuclear forces.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Chiral effective field theory and nuclear forces

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-07T15:31:32.540456Z

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Observation d558c782-4bb1-4aac-b8db-b6698391e5d2 · outbound

This paper cites Chiral Effective Field Theory and the High-Density Nuclear Equation of State.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Chiral Effective Field Theory and the High-Density Nuclear Equation of State

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-07T15:31:32.545672Z

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Observation c2e68cbd-2c9b-45c3-98e5-9ce113d56477 · outbound

This paper cites Friedenberg and J.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Friedenberg and J

Reference 9

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Observation 4f709645-1e60-49d2-8d05-537d7c202da1 · outbound

This paper cites Proto-Neutron and Neutron Stars in a Chiral SU(3) Model.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Proto-Neutron and Neutron Stars in a Chiral SU(3) Model

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-07T15:31:32.554423Z

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Observation 847eb139-7184-47a7-8f2c-780206020507 · outbound

This paper cites A Novel Approach to Model Hybrid Stars.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars A Novel Approach to Model Hybrid Stars

Reference 11

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Source-reported events for the cited work

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Observation ab4ab60b-da18-4e9f-8468-8ab614d39000 · outbound

This paper cites Phase Stability in the 3-Dimensional Open-source Code for the Chiral mean-field Model.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Phase Stability in the 3-Dimensional Open-source Code for the Chiral mean-field Model

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-07T15:31:32.564223Z

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Observation 3f5ec24c-ec4b-48fb-ac96-0e92aa7ab5f0 · outbound

This paper cites an unresolved cited work.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Unresolved cited work

Reference 13

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Observation d03e153d-e2bb-4f0a-8dc5-9c0577037f75 · outbound

This paper cites an unresolved cited work.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Unresolved cited work

Reference 14

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Observation 2a44c6ac-806e-41ce-bd8d-2784aaf7180a · outbound

This paper cites Moments of inertia for neutron and strange stars: limits derived for the Crab pulsar.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Moments of inertia for neutron and strange stars: limits derived for the Crab pulsar

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-07T15:31:32.577824Z

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Observation 9b356ddf-65ba-413f-9099-fe9583c04402 · outbound

This paper cites Why I-Love-Q.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Why I-Love-Q

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-07T15:31:32.582332Z

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Observation 0995517c-ee47-4ee4-a242-ab7178ffab23 · outbound

This paper cites an unresolved cited work.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Unresolved cited work

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-07T15:31:32.587575Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c4ac166c-e850-480c-8b5d-9a95267b4e30 · outbound

This paper cites Isospin Equilibration in Neutron Star Mergers.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Isospin Equilibration in Neutron Star Mergers

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-07T15:31:32.591640Z

Source-reported events for the cited work

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Observation b0d1bec3-b832-4557-8eec-73fb886bbab8 · outbound

This paper cites Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Beyond modified Urca: the nucleon width approximation for flavor-changing processes in dense matter

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-07T15:31:32.597991Z

Source-reported events for the cited work

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Observation ea6cc625-42bd-40b0-b79a-ab2513409216 · outbound

This paper cites Alford and Z.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Alford and Z

Reference 20

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Observation bc31f5f9-cfa7-487d-88b3-f24961c47ade · outbound

This paper cites Building Neutron Stars with the MUSES Calculation Engine.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Building Neutron Stars with the MUSES Calculation Engine

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-07T15:31:32.607156Z

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Observation 8456e11b-c412-443e-aa9f-f58fb8df801e · outbound

This paper cites Equation of state for neutron star matter with NJL model and Dirac-Brueckner-Hartree-Fock approximation.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Equation of state for neutron star matter with NJL model and Dirac-Brueckner-Hartree-Fock approximation

Reference 22

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Observation e10ce630-8fc2-4b0f-89eb-1c28470da66e · outbound

This paper cites Exploring hybrid equation of state with constraints from tidal deformability of GW170817.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Exploring hybrid equation of state with constraints from tidal deformability of GW170817

Reference 23

Resolution: verified exact; local_arxiv, observed 2026-08-07T15:31:33.056267Z

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Observation 1acbde54-5884-4945-8400-34ca4645e5a7 · outbound

This paper cites Baryon Number Fluctuations from a Crossover Equation of State Compared to Heavy-Ion Collision Measurements in the Beam Energy Range $\sqrt{s_{NN}}$ = 7.7 to 200 GeV.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Baryon Number Fluctuations from a Crossover Equation of State Compared to Heavy-Ion Collision Measurements in the Beam Energy Range $\sqrt{s_{NN}}$ = 7.7 to 200 GeV

Reference 24

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Observation 27c2040d-aadd-4af0-be9f-16a94dcf482e · outbound

This paper cites an unresolved cited work.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Unresolved cited work

Reference 25

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Observation c3d0dfac-4030-4df2-92df-9c644dfbf490 · outbound

This paper cites Neutron Star Equation of State in light of GW190814.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Neutron Star Equation of State in light of GW190814

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-07T15:31:32.630621Z

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Observation 7c380675-3678-4561-91f3-0e49f0d7d87b · outbound

This paper cites Extreme Matter meets Extreme Gravity: Ultra-heavy neutron stars with crossovers and first-order phase transitions.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Extreme Matter meets Extreme Gravity: Ultra-heavy neutron stars with crossovers and first-order phase transitions

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-07T15:31:32.636100Z

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Observation ddd76856-4f8f-4ac3-9d6b-2cb3110c6267 · outbound

This paper cites The slope, the hill, the drop, and the swoosh: Learning about the nuclear matter equation of state from the binary Love relations.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars The slope, the hill, the drop, and the swoosh: Learning about the nuclear matter equation of state from the binary Love relations

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-07T15:31:32.640727Z

Source-reported events for the cited work

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Observation 007bcd57-8f4b-4f97-a661-871414df23cf · outbound

This paper cites Enhanced production of multi-strange hadrons in high-multiplicity proton-proton collisions.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Enhanced production of multi-strange hadrons in high-multiplicity proton-proton collisions

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-07T15:31:32.645330Z

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Observation a977cd91-3f0f-4465-b3c5-b8fde3477437 · outbound

This paper cites BSQ Conserved Charges in Relativistic Viscous Hydrodynamics solved with Smoothed Particle Hydrodynamics.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars BSQ Conserved Charges in Relativistic Viscous Hydrodynamics solved with Smoothed Particle Hydrodynamics

Reference 30

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Observation 4a59f46e-6b27-427d-90b3-e919ad93fae8 · outbound

This paper cites Lattice-based equation of state at finite baryon number, electric charge and strangeness chemical potentials.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Lattice-based equation of state at finite baryon number, electric charge and strangeness chemical potentials

Reference 31

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Observation 73a7571f-9749-4784-9c13-d850302bc61e · outbound

This paper cites Jahan, H.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Jahan, H

Reference 32

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Observation 9155665a-1592-450c-a844-272bfc456a4c · outbound

This paper cites Lattice QCD equation of state at finite chemical potential from an alternative expansion scheme.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Lattice QCD equation of state at finite chemical potential from an alternative expansion scheme

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-07T15:31:32.665279Z

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Observation 125efcc2-dc64-47fd-afea-b83ad5668dd4 · outbound

This paper cites Finite density QCD equation of state: critical point and lattice-based $T'$-expansion.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Finite density QCD equation of state: critical point and lattice-based $T'$-expansion

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-07T15:31:32.669868Z

Source-reported events for the cited work

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Observation fdc03c40-de55-4e77-80da-bcbab394ea35 · outbound

This paper cites Kahangirwe, J.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Kahangirwe, J

Reference 35

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T15:31:33.362257Z

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Observation 95d7a03e-f27d-4aa6-8d8e-648374a327cb · outbound

This paper cites Critical point in the phase diagram of primordial quark-gluon matter from black hole physics.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Critical point in the phase diagram of primordial quark-gluon matter from black hole physics

Reference 36

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Observation 70e32178-aff0-437a-a0ed-104505804615 · outbound

This paper cites Hot QCD Phase Diagram From Holographic Einstein-Maxwell-Dilaton Models.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Hot QCD Phase Diagram From Holographic Einstein-Maxwell-Dilaton Models

Reference 37

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Observation 448f2a31-8cd7-41e6-a170-b6473eec34c9 · outbound

This paper cites Hot and dense quark-gluon plasma thermodynamics from holographic black holes.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Hot and dense quark-gluon plasma thermodynamics from holographic black holes

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-07T15:31:32.690874Z

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This paper cites Bayesian location of the QCD critical point from a holographic perspective.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Bayesian location of the QCD critical point from a holographic perspective

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-07T15:31:32.696247Z

Source-reported events for the cited work

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Observation fef02521-59f1-4cc7-8e75-991a49ca9ba1 · outbound

This paper cites Yang and M.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Yang and M

Reference 40

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T15:31:33.346868Z

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This paper cites Hippert, J.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Hippert, J

Reference 41

Resolution: verified fuzzy; raw_fallback, observed 2026-08-07T15:31:33.330801Z

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No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Observation 8d91deab-4d2b-4825-bd7d-62550236ea86 · outbound

This paper cites an unresolved cited work.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Unresolved cited work

Reference 42

Resolution: unresolved; raw_fallback, observed 2026-08-07T15:31:33.314590Z

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No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

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This paper cites an unresolved cited work.

An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars Unresolved cited work

Reference 43

Resolution: unresolved; raw_fallback, observed 2026-08-07T15:31:33.297946Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.

Pith citing papers

Observation 5fa114a7-1978-47df-84b5-70f6743dc2d9 · inbound

Studying the QCD Matter produced in Heavy-Ion Collisions using the MUSES Calculation Engine cites this paper.

Studying the QCD Matter produced in Heavy-Ion Collisions using the MUSES Calculation Engine An Overview of the MUSES Calculation Engine and How It Can Be Used to Describe Neutron Stars

Reference 170

Resolution: verified exact; arxiv_id, observed 2026-07-04T16:19:57.438106Z

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No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.