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Paper Citation Record · LEDGER

How perturbative QCD constrains the Equation of State at Neutron-Star densities

As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 20 inbound Pith citation observations for arXiv:2111.05350.

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pith.paper-citation-record.v1
2111.05350 v2

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Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-08T00:43:19.060431Z

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

Source: arxiv_reference, observed 2026-07-04T19:00:04.473647Z

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Pith citing papers

Observation 0770718e-5118-4a8a-8eb4-430595c52cbf · inbound

Constraints on the strength of first-order phase transition and its relation to nucleon mass cites this paper.

Constraints on the strength of first-order phase transition and its relation to nucleon mass How perturbative QCD constrains the Equation of State at Neutron-Star densities

Reference 44

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Observation 45bf6613-c402-40a2-a0a9-2938da17ece7 · inbound

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

Locating the QCD critical point with neutron-star observations How perturbative QCD constrains the Equation of State at Neutron-Star densities

Reference 88

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Observation 1af1904c-02d6-43f1-a2b3-495b2bcbf5f5 · 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 How perturbative QCD constrains the Equation of State at Neutron-Star densities

Reference 25

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Observation feda8830-a6a6-41cd-87aa-52f8c9999748 · 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 How perturbative QCD constrains the Equation of State at Neutron-Star densities

Reference 66

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Observation 44c41083-09c9-4704-ad81-7507e2e86fdd · inbound

Renormalization group analysis of color superconductivity revisited cites this paper.

Renormalization group analysis of color superconductivity revisited How perturbative QCD constrains the Equation of State at Neutron-Star densities

Reference 42

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Observation 2ea5d41d-fba8-4ab6-927e-e20c3d345611 · inbound

Updated Astrophysical Equation-of-State Constraints on the Color-Superconducting Gap cites this paper.

Updated Astrophysical Equation-of-State Constraints on the Color-Superconducting Gap How perturbative QCD constrains the Equation of State at Neutron-Star densities

Reference 5

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Observation 44adbfcc-da70-49b8-a5ed-ab4b2cfbe001 · inbound

Equation of State Extrapolation Systematics: Parametric vs. Nonparametric Inference of Neutron Star Structure cites this paper.

Equation of State Extrapolation Systematics: Parametric vs. Nonparametric Inference of Neutron Star Structure How perturbative QCD constrains the Equation of State at Neutron-Star densities

Reference 22

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arxiv_id, observed 2026-05-21T23:00:43.742613Z

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Observation 905a9278-308e-4ac1-96e8-9066abe2a846 · inbound

General gravitational properties of neutron stars: curvature invariants, binding energy, and trace anomaly cites this paper.

General gravitational properties of neutron stars: curvature invariants, binding energy, and trace anomaly How perturbative QCD constrains the Equation of State at Neutron-Star densities

Reference 5

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arxiv_id, observed 2026-05-16T14:48:00.646890Z

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Observation 485a9ed7-9b8d-4d73-bb1d-c34797093d3c · inbound

A Physics Informed Bayesian Neural Network for the Neutron Star Equation of State cites this paper.

A Physics Informed Bayesian Neural Network for the Neutron Star Equation of State How perturbative QCD constrains the Equation of State at Neutron-Star densities

Reference 48

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Observation b96f21ae-a74b-4608-bc63-4658f8df7203 · 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 How perturbative QCD constrains the Equation of State at Neutron-Star densities

Reference 23

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arxiv_id, observed 2026-05-12T08:21:25.672656Z

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Observation 00506412-6b97-4363-a50a-7252efe0839d · 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 How perturbative QCD constrains the Equation of State at Neutron-Star densities

Reference 19

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Observation 70ccd823-bd7b-410d-adb6-0eb1a86908fc · inbound

Reconciling GW170817 and GW190814 with a Nonmonotonic Sound-Speed Equation of State cites this paper.

Reconciling GW170817 and GW190814 with a Nonmonotonic Sound-Speed Equation of State How perturbative QCD constrains the Equation of State at Neutron-Star densities

Reference 36

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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 How perturbative QCD constrains the Equation of State at Neutron-Star densities

Reference 31

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Observation d42fb7bf-b284-40aa-866b-6d1b8c700ad2 · 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 How perturbative QCD constrains the Equation of State at Neutron-Star densities

Reference 6

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Observation aa7df289-bb28-4fa6-aeb0-ff83479467e1 · inbound

Hyperonic equation of state for neutron stars: A systematic Bayesian comparison of density-dependent and non-linear relativistic mean-field models cites this paper.

Hyperonic equation of state for neutron stars: A systematic Bayesian comparison of density-dependent and non-linear relativistic mean-field models How perturbative QCD constrains the Equation of State at Neutron-Star densities

Reference 38

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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 How perturbative QCD constrains the Equation of State at Neutron-Star densities

Reference 25

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Observation 16a36f0c-8a92-4b4e-9a06-46618bd53531 · 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 How perturbative QCD constrains the Equation of State at Neutron-Star densities

Reference 38

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Observation 29c33303-a39b-47bc-aa4f-0945cff95c1e · inbound

The equation of state for neutron stars cites this paper.

The equation of state for neutron stars How perturbative QCD constrains the Equation of State at Neutron-Star densities

Reference 94

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Observation 323e7882-a42a-4bde-8dd2-b7f566a0a2ca · inbound

Nuclear matter equation of state and astrophysics cites this paper.

Nuclear matter equation of state and astrophysics How perturbative QCD constrains the Equation of State at Neutron-Star densities

Reference 11

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Observation 7d6d9ecb-4c02-4a4d-8e62-79071d36bc4b · 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 How perturbative QCD constrains the Equation of State at Neutron-Star densities

Reference 24

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