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Paper Citation Record · LEDGER

The equation of state for neutron stars

As of 21 August 2026, this Paper Citation Record lists 100 of 300 outbound references and 0 inbound Pith citation observations for arXiv:2607.17006.

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

pith.paper-citation-record.v1
2607.17006 v1

Coverage vector

measured 100 of 300 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-01T19:22:13.003054Z

measured 100 of 100 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-20T06:33:59.587034+00:00

measured 0 of 0 inbound itemization

Pith citing papers itemized under the disclosed page cap.

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measured 0 of 1 external citation measurements

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Source: cited_works

Reference resolution

100 of 300 outbound references displayed

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  • verified fuzzy0
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External citation measurements

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Outbound references

Observation ada19e82-f7b1-40fe-9894-4a1ab7280405 · outbound

This paper cites an unresolved cited work.

The equation of state for neutron stars Unresolved cited work

Reference 1

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Observation 680b4aec-6348-4937-b92f-dfd05cd93676 · outbound

This paper cites Experimental Tests of Asymptotic Freedom.

The equation of state for neutron stars Experimental Tests of Asymptotic Freedom

Reference 2

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Observation 9a7500e1-49d6-48df-a5c8-976581cf83c3 · outbound

This paper cites Effective Field Theory Approach to High-Temperature Thermodynamics.

The equation of state for neutron stars Effective Field Theory Approach to High-Temperature Thermodynamics

Reference 3

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Observation fd6f5cf3-8b2a-4117-bd29-3a7810a652da · outbound

This paper cites NNLO HTLpt predictions for the curvature of the QCD phase transition line.

The equation of state for neutron stars NNLO HTLpt predictions for the curvature of the QCD phase transition line

Reference 4

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source=arxiv_source observed=2026-08-01T19:22:02.211803Z digest=sha256:4c9fca9218501db9e006a0e9f461b984046d6110735e8d39de3f5994965b3e87

Observation 36756a75-2ce2-4678-bf87-39a29ae4d228 · outbound

This paper cites QCD Shear Viscosity at (almost) NLO.

The equation of state for neutron stars QCD Shear Viscosity at (almost) NLO

Reference 5

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source=arxiv_source observed=2026-08-01T19:22:02.327374Z digest=sha256:ad6e9e0dce6850b5250aba050a77d192a32e9ae23cb82c61085a6c7e2ad288ee

Observation 0d0e8f26-d054-43ca-8dfe-60e58f631ccc · outbound

This paper cites Transport coefficients in high temperature gauge theories: (I) Leading-log results.

The equation of state for neutron stars Transport coefficients in high temperature gauge theories: (I) Leading-log results

Reference 6

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Observation 48854988-4033-472b-b44e-3b5752136df0 · outbound

This paper cites Second-order Hydrodynamics in Next-to-Leading-Order QCD.

The equation of state for neutron stars Second-order Hydrodynamics in Next-to-Leading-Order QCD

Reference 7

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Observation 7c77f93a-b2db-4d98-9387-cd53a6ce7c6a · outbound

This paper cites Hot and Dense QCD Shear Viscosity at Leading Log.

The equation of state for neutron stars Hot and Dense QCD Shear Viscosity at Leading Log

Reference 8

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Observation 582420c3-db90-4629-aa27-2aac10b8ff66 · outbound

This paper cites The Bulk Viscosity of High-Temperature QCD.

The equation of state for neutron stars The Bulk Viscosity of High-Temperature QCD

Reference 9

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Observation 1ae5003c-2251-4b09-b323-d5ac353f0a91 · outbound

This paper cites Three-loop HTL QCD thermodynamics.

The equation of state for neutron stars Three-loop HTL QCD thermodynamics

Reference 10

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Observation 3f736fc5-7287-4b8a-a483-0ac91c11690a · outbound

This paper cites Anisotropy as a signature of transverse collective flow.

The equation of state for neutron stars Anisotropy as a signature of transverse collective flow

Reference 11

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Observation 38ddcd89-1ba7-43b0-a0ea-c950c6a57b8b · outbound

This paper cites Identified charged particle azimuthal anisotropy in PHENIX at RHIC.

The equation of state for neutron stars Identified charged particle azimuthal anisotropy in PHENIX at RHIC

Reference 12

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Observation ab8ba99e-6fad-495b-a628-3e9bc1faa7ad · outbound

This paper cites Azimuthal anisotropy of K0s and Lambda prduction at mid-rapidity from Au+Au collisions at root s = 130 GeV.

The equation of state for neutron stars Azimuthal anisotropy of K0s and Lambda prduction at mid-rapidity from Au+Au collisions at root s = 130 GeV

Reference 13

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Observation 7fc8493e-6706-4b9e-b015-20931e0c332d · outbound

This paper cites Quartic cumulant of baryon number in the presence of QCD critical point.

The equation of state for neutron stars Quartic cumulant of baryon number in the presence of QCD critical point

Reference 14

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Observation 25b4166d-a0ea-4487-b7e6-d2f7232250d3 · outbound

This paper cites Giant Monopole Resonances and nuclear incompressibilities studied for the zero-range and separable pairing interactions.

The equation of state for neutron stars Giant Monopole Resonances and nuclear incompressibilities studied for the zero-range and separable pairing interactions

Reference 15

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Observation 56b10575-af0b-41b7-9ae2-96136bab88a9 · outbound

This paper cites Microscopic Study of the Isoscalar Giant Monopole Resonance in Cd, Sn and Pb Isotopes.

The equation of state for neutron stars Microscopic Study of the Isoscalar Giant Monopole Resonance in Cd, Sn and Pb Isotopes

Reference 16

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Observation ddc2d089-601e-4aa6-81fb-741d1ad1ac75 · outbound

This paper cites Nuclear matter incompressibility coefficient in relativistic and nonrelativistic microscopic models.

The equation of state for neutron stars Nuclear matter incompressibility coefficient in relativistic and nonrelativistic microscopic models

Reference 17

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Observation 3c24e0df-c4d9-43b7-aa16-f70bf4113b28 · outbound

This paper cites Microscopic determination of the nuclear incompressibility within the non-relativistic framework.

The equation of state for neutron stars Microscopic determination of the nuclear incompressibility within the non-relativistic framework

Reference 18

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Observation 3c0c611e-d47a-477a-a27d-d5afd4776d25 · outbound

This paper cites Symmetry energy from the nuclear collective motion: constraints from dipole, quadrupole, monopole and spin-dipole resonances.

The equation of state for neutron stars Symmetry energy from the nuclear collective motion: constraints from dipole, quadrupole, monopole and spin-dipole resonances

Reference 19

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Observation d984ca71-6186-447a-aa19-223da022c9c0 · outbound

This paper cites Neutron-Rich Nuclei in Heaven and Earth.

The equation of state for neutron stars Neutron-Rich Nuclei in Heaven and Earth

Reference 20

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Observation 21e2f7db-47af-449d-8e7f-9bf0ed1560f2 · outbound

This paper cites and Swiatecki, Wladyslaw J.

The equation of state for neutron stars and Swiatecki, Wladyslaw J

Reference 21

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Observation 54a06ae7-7b46-40f1-9732-83a0e6616a5e · outbound

This paper cites R and Shaw, G.

The equation of state for neutron stars R and Shaw, G

Reference 22

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Observation 2f49a675-8b19-4fb8-b2b1-ba96a69014d8 · outbound

This paper cites QCD equation of state matched to lattice data and exhibiting a critical point singularity.

The equation of state for neutron stars QCD equation of state matched to lattice data and exhibiting a critical point singularity

Reference 23

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Observation cf853ce4-a662-4817-9bd0-1de95d5d92fb · outbound

This paper cites an unresolved cited work.

The equation of state for neutron stars Unresolved cited work

Reference 24

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Observation b28126e5-bc59-435e-b2cc-005ac4e3db2b · outbound

This paper cites , year =.

The equation of state for neutron stars , year =

Reference 25

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Observation c6132f8e-baec-4e77-9eb0-4f290fedb00f · outbound

This paper cites The NANOGrav 15-year Data Set: Observations and Timing of 68 Millisecond Pulsars.

The equation of state for neutron stars The NANOGrav 15-year Data Set: Observations and Timing of 68 Millisecond Pulsars

Reference 26

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Observation c1871191-bc71-40f7-8a3a-667bb9980819 · outbound

This paper cites Constraining neutron star matter with QCD.

The equation of state for neutron stars Constraining neutron star matter with QCD

Reference 27

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Observation 442b276b-2641-4bc6-ae64-f9fdb9097dd2 · outbound

This paper cites A Novel Approach to Model Hybrid Stars.

The equation of state for neutron stars A Novel Approach to Model Hybrid Stars

Reference 28

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Observation 8a456cc3-cb80-4b74-9f99-75e959938ef0 · outbound

This paper cites A Lower Mass Estimate for PSR J0348+0432 Based on CHIME/Pulsar Precision Timing.

The equation of state for neutron stars A Lower Mass Estimate for PSR J0348+0432 Based on CHIME/Pulsar Precision Timing

Reference 29

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Observation eeebce35-a477-4432-b26e-89330f35f212 · outbound

This paper cites Gravitation and Relativity , editor =.

The equation of state for neutron stars Gravitation and Relativity , editor =

Reference 30

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Observation f2a62751-71ff-46ca-a761-648efb2f9e0d · outbound

This paper cites Kent and Thorne, Kip S.

The equation of state for neutron stars Kent and Thorne, Kip S

Reference 31

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Observation 640cc651-4f34-4942-8917-00f82b08cd8a · outbound

This paper cites The Radius of PSR J0437-4715 from NICER Data.

The equation of state for neutron stars The Radius of PSR J0437-4715 from NICER Data

Reference 32

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Observation e3690018-b5d7-4647-bd81-e0c4dac6c910 · outbound

This paper cites Dynamical response of twin stars to perturbations.

The equation of state for neutron stars Dynamical response of twin stars to perturbations

Reference 33

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Observation 40f05e70-db5b-42fc-9e70-f91ccbc3fb4d · outbound

This paper cites The scenario of two families of compact stars 1. Equations of state, mass-radius relations and binary systems.

The equation of state for neutron stars The scenario of two families of compact stars 1. Equations of state, mass-radius relations and binary systems

Reference 34

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Observation de41b805-0093-43e8-80e5-b561176fc998 · outbound

This paper cites Quasi-Normal Modes of Stars and Black Holes.

The equation of state for neutron stars Quasi-Normal Modes of Stars and Black Holes

Reference 35

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Observation 1997df06-e225-4a85-9a4f-26992ea67fc1 · outbound

This paper cites an unresolved cited work.

The equation of state for neutron stars Unresolved cited work

Reference 36

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Observation 92e8a5cb-d498-4fb2-b4ed-ce1a7666645f · outbound

This paper cites Compact stars with sequential QCD phase transitions.

The equation of state for neutron stars Compact stars with sequential QCD phase transitions

Reference 37

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Observation 989a16a5-47a9-42ed-b263-e53fe74b39ca · outbound

This paper cites Equation of State at Supranuclear Densities and the Existence of a Third Family of Superdense Stars.

The equation of state for neutron stars Equation of State at Supranuclear Densities and the Existence of a Third Family of Superdense Stars

Reference 38

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Observation 80cae466-dc57-4233-8b27-a121a79a2781 · outbound

This paper cites Quark phases in neutron stars and a "third family" of compact stars as a signature for phase transitions.

The equation of state for neutron stars Quark phases in neutron stars and a "third family" of compact stars as a signature for phase transitions

Reference 39

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source=arxiv_source observed=2026-08-01T19:22:07.023636Z digest=sha256:7c7ed33ae1f9528700486e6822bc357422f29e717e5916a845b6ac46c8a4b715

Observation 9e799504-4053-4044-8711-d4db7453d517 · outbound

This paper cites ON COMPLEX PROBABILITIES.

The equation of state for neutron stars ON COMPLEX PROBABILITIES

Reference 40

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source=arxiv_source observed=2026-08-01T19:22:07.132876Z digest=sha256:413d4e4becadd95179cf5f6082de01c564b35e88447283711b72cff56d0a1fc9

Observation 545c290b-b967-45d9-8965-4cbcff88109f · outbound

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

The equation of state for neutron stars Reconciling GW170817 and GW190814 with a Nonmonotonic Sound-Speed Equation of State

Reference 41

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no resolver link, observed 2026-08-01T19:22:07.253487Z

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source=arxiv_source observed=2026-08-01T19:22:07.253487Z digest=sha256:ee141287e9814d689181fe58f9ae0690c819c012452fbea44abde06f8c09a434

Observation ddc8c6d6-914c-4038-95cf-eb36bf68f276 · outbound

This paper cites Necessary and sufficient conditions for correctness of complex Langevin.

The equation of state for neutron stars Necessary and sufficient conditions for correctness of complex Langevin

Reference 42

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no resolver link, observed 2026-08-01T19:22:07.369845Z

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source=arxiv_source observed=2026-08-01T19:22:07.369845Z digest=sha256:ac8eac5426d83b01c0f2ce260a98bffa91e5bc9775e582d83537eba8e697a503

Observation fed7156d-ed5e-434e-8ede-610e26f9573b · outbound

This paper cites Finite-density equation of state of hot QCD using the complex Langevin equation.

The equation of state for neutron stars Finite-density equation of state of hot QCD using the complex Langevin equation

Reference 43

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no resolver link, observed 2026-08-01T19:22:07.463533Z

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source=arxiv_source observed=2026-08-01T19:22:07.463533Z digest=sha256:c94d7b9924c7458bee586357f6ac1e769ea65444638d3f3d4d5962a19fe27f4c

Observation ddd7cd40-7db6-46d0-9e29-965af678b58d · outbound

This paper cites Lattice field theories with a sign problem.

The equation of state for neutron stars Lattice field theories with a sign problem

Reference 44

Resolution
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no resolver link, observed 2026-08-01T19:22:07.533337Z

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source=arxiv_source observed=2026-08-01T19:22:07.533337Z digest=sha256:df818e68cfde3a3f4f6ab97d674d04311c7eeacfc348d1f77393387b4c3b93cb

Observation 94a54f89-a0e6-4e68-984b-891659308e55 · outbound

This paper cites Introductory lectures on lattice QCD at nonzero baryon number.

The equation of state for neutron stars Introductory lectures on lattice QCD at nonzero baryon number

Reference 45

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no resolver link, observed 2026-08-01T19:22:07.658721Z

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source=arxiv_source observed=2026-08-01T19:22:07.658721Z digest=sha256:d4f909d66fd95de295c18308dec2d777113a745f6b94b9f781c5875b98e36848

Observation ff0ea24b-3221-4899-ac47-838480e67ca9 · outbound

This paper cites On the stability of strange dwarf hybrid stars.

The equation of state for neutron stars On the stability of strange dwarf hybrid stars

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:07.791956Z

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source=arxiv_source observed=2026-08-01T19:22:07.791956Z digest=sha256:c8d62c5d4f9c102f92583d79ab90605ee52f4ad2d95a0f08b7ef331ca99b3614

Observation 7835e491-20b7-4f96-acfe-d480b973ac51 · outbound

This paper cites Non-Identical Neutron Star Twins.

The equation of state for neutron stars Non-Identical Neutron Star Twins

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:07.865744Z

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source=arxiv_source observed=2026-08-01T19:22:07.865744Z digest=sha256:d7ac5591780cbd6731c443d1121407425d83228052f22f1c9ad1b6abf6529b6d

Observation e8276008-c029-4f50-913e-b4389356fc90 · outbound

This paper cites Approximate Universal Relations for Neutron Stars and Quark Stars.

The equation of state for neutron stars Approximate Universal Relations for Neutron Stars and Quark Stars

Reference 48

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:07.959991Z

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source=arxiv_source observed=2026-08-01T19:22:07.959991Z digest=sha256:ff44346ecd463880cdafb08e53f26357272ffb27b6120930589d2a27ff9c252c

Observation de067e8b-b73d-4a87-abdf-085728873c87 · outbound

This paper cites Composition and Structure of Protoneutron Stars.

The equation of state for neutron stars Composition and Structure of Protoneutron Stars

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:08.086399Z

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source=arxiv_source observed=2026-08-01T19:22:08.086399Z digest=sha256:8bfec947f73d1ca361a67492bbe704b7b56364850d2c0dcc527f4c0748f3835d

Observation 9bea3b3d-0aca-48b9-bdbf-3b7f4d99a5ec · outbound

This paper cites an unresolved cited work.

The equation of state for neutron stars Unresolved cited work

Reference 50

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unresolved
no resolver link, observed 2026-08-01T19:22:08.180399Z

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source=arxiv_source observed=2026-08-01T19:22:08.180399Z digest=sha256:8443ca3a12bfaedbfa6f72aba276b5d530a4c7ac784ed6e6ac5bb41abe2119db

Observation 6e2bd803-ed86-4141-9330-62e88fd4b4c2 · outbound

This paper cites and Satz, H.

The equation of state for neutron stars and Satz, H

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:08.274159Z

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source=arxiv_source observed=2026-08-01T19:22:08.274159Z digest=sha256:6b67ff003e089745b578283b295acf8bfdda5f8742a100b9c050c1c341785fa7

Observation 7814630c-e223-4be3-b287-ef34cb994dc0 · outbound

This paper cites Effects of the QCD phase transition on hadronic observables in relativistic hydrodynamic simulations of heavy-ion reactions in the FAIR/NICA energy regime.

The equation of state for neutron stars Effects of the QCD phase transition on hadronic observables in relativistic hydrodynamic simulations of heavy-ion reactions in the FAIR/NICA energy regime

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:08.362751Z

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source=arxiv_source observed=2026-08-01T19:22:08.362751Z digest=sha256:3e2faa1bedfb2f136704281fb1c3f7ceb12a21e3c5876c615b53adb7fcd42ee6

Observation 03066613-98d4-4242-94b3-7960a0eae62c · outbound

This paper cites Non-Gaussian fluctuations near the QCD critical point.

The equation of state for neutron stars Non-Gaussian fluctuations near the QCD critical point

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:08.429616Z

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source=arxiv_source observed=2026-08-01T19:22:08.429616Z digest=sha256:b9478b986b804b32f61cdb1d13dc90fe0d4009892b396d9a5a6c962b5959d0fe

Observation 10999ff1-fdff-410b-835c-04f719993ba1 · outbound

This paper cites Determination of the Equation of State of Dense Matter.

The equation of state for neutron stars Determination of the Equation of State of Dense Matter

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:08.523264Z

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source=arxiv_source observed=2026-08-01T19:22:08.523264Z digest=sha256:b8741695bd721adef9e468277eccba77b7a7acea13b9dbceef7e89f4207ede14

Observation 52036a62-41da-4919-a696-c31a48c9afc4 · outbound

This paper cites Evolution of Protoneutron Stars.

The equation of state for neutron stars Evolution of Protoneutron Stars

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:08.629517Z

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source=arxiv_source observed=2026-08-01T19:22:08.629517Z digest=sha256:4c7cbafb02d0b95068eec3f76bdade8835cda79ac51373d4ff0bbb71c2867366

Observation e250c034-f6cf-49f4-8bc2-a2cbf43decdf · outbound

This paper cites Astrophysics with the Laser Interferometer Space Antenna.

The equation of state for neutron stars Astrophysics with the Laser Interferometer Space Antenna

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:08.715426Z

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source=arxiv_source observed=2026-08-01T19:22:08.715426Z digest=sha256:25e4f793787f7cfbbdb259825fc65a32a1f25610bc99877d847ce909aeaf9845

Observation 946609a5-a97b-42ee-86f7-11821a0ca75f · outbound

This paper cites Free Energy of QCD at High Temperature.

The equation of state for neutron stars Free Energy of QCD at High Temperature

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:08.809084Z

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source=arxiv_source observed=2026-08-01T19:22:08.809084Z digest=sha256:c794cb2cebe05cde885037d090c6da8012ea5fdfee9dc5382f201054e2bd1350

Observation 6c9f5b05-bf9f-4fc9-bd0f-fb8535e1a607 · outbound

This paper cites The equation of state in lattice QCD: with physical quark masses towards the continuum limit.

The equation of state for neutron stars The equation of state in lattice QCD: with physical quark masses towards the continuum limit

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:08.889981Z

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source=arxiv_source observed=2026-08-01T19:22:08.889981Z digest=sha256:89fecb77973a0f9bb956451218f7010d09e6763553e72cd7bdcd3436415bdd50

Observation 30fca1f2-b0a4-4fa6-83a5-f616edb0be31 · outbound

This paper cites THERMUS -- A Thermal Model Package for ROOT.

The equation of state for neutron stars THERMUS -- A Thermal Model Package for ROOT

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:08.984996Z

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source=arxiv_source observed=2026-08-01T19:22:08.984996Z digest=sha256:7bbd8dd7075ea7f69e683c7dfbc60cb19912d01970f3d98efd226256f2853f9c

Observation 6873d5ca-50a4-4c80-bfab-467a937b0eb9 · outbound

This paper cites Measuring the speed of sound using cumulants of baryon number.

The equation of state for neutron stars Measuring the speed of sound using cumulants of baryon number

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:09.067358Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:22:09.067358Z digest=sha256:291643fd6f73bdda3307a32985878594872d91d4861ebb6febf1ac1035aabd35

Observation 16cef3b2-9adc-4231-908b-f6876d41906d · outbound

This paper cites Deconfining Phase Transition on Lattices with Boundaries at Low Temperature.

The equation of state for neutron stars Deconfining Phase Transition on Lattices with Boundaries at Low Temperature

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:09.131880Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:22:09.131880Z digest=sha256:e7476408feb3387aae41824c0f7751a86701d82a87150085d864fcbd73d77adc

Observation d3f65fae-646a-4c0d-b4ad-bb56f504b320 · outbound

This paper cites Finite-size effects and the search for the critical endpoint of QCD.

The equation of state for neutron stars Finite-size effects and the search for the critical endpoint of QCD

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:09.224949Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:22:09.224949Z digest=sha256:09b337cc5caac8d96e4bc44419eea9bc19d5b68b49fed6c7be09f6994351c28c

Observation 1b5f7696-9656-4989-a0a4-002d5abc3e75 · outbound

This paper cites (Non)Thermal Aspects of Charmonium Production and a New Look at J/$\psi$ Suppression.

The equation of state for neutron stars (Non)Thermal Aspects of Charmonium Production and a New Look at J/$\psi$ Suppression

Reference 63

Resolution
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no resolver link, observed 2026-08-01T19:22:09.341414Z

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source=arxiv_source observed=2026-08-01T19:22:09.341414Z digest=sha256:2004402ddaee903fef4a79b73be6a464e369fb99a661eb372a84b7a06068b483

Observation 22307e04-1085-47e9-9eca-19ddf9669d19 · outbound

This paper cites Quarkonium Feed-Down and Sequential Suppression.

The equation of state for neutron stars Quarkonium Feed-Down and Sequential Suppression

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:09.463024Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:22:09.463024Z digest=sha256:61c6e21f34ed83ab2a54143f7a63297f9078cb0a795bc6e9b5210865c44b6f67

Observation 33c07971-8e3c-458a-9760-98cb455a2f34 · outbound

This paper cites Jet Quenching in Dense Matter.

The equation of state for neutron stars Jet Quenching in Dense Matter

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:09.557548Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:22:09.557548Z digest=sha256:7a1c4065a2491723474650e2bd5f37510406b73aa154844243896bbfcd234349

Observation dd89de56-585b-4bce-8a7a-cedbb3f7b58d · outbound

This paper cites Femtoscopy in relativistic heavy ion collisions.

The equation of state for neutron stars Femtoscopy in relativistic heavy ion collisions

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:09.658741Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:22:09.658741Z digest=sha256:ebba681d1e16fbbcb112b571b76f6e928e25505997e6656d32ac79d2ac56793b

Observation 2b233201-985a-4de7-a24f-2ca4f1f3b714 · outbound

This paper cites Particle Interferometry for Relativistic Heavy-Ion Collisions.

The equation of state for neutron stars Particle Interferometry for Relativistic Heavy-Ion Collisions

Reference 67

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unresolved
no resolver link, observed 2026-08-01T19:22:09.750153Z

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source=arxiv_source observed=2026-08-01T19:22:09.750153Z digest=sha256:ce1a1624f82e446c6c498f3cfe62573f65826a5a7cec10d1500a0a0022206061

Observation 40d27bda-bb05-478d-9cd7-3c514c77fced · outbound

This paper cites Two-Particle Correlations in Relativistic Heavy-Ion Collisions.

The equation of state for neutron stars Two-Particle Correlations in Relativistic Heavy-Ion Collisions

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:09.823317Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:22:09.823317Z digest=sha256:62758f18c91506d0eca793b738c8b9d2d82071e70b4ae160f6e35923623c0d07

Observation 12af60d5-4c38-4c9b-b05c-ed3ed06aa4da · outbound

This paper cites 2011 , url=.

The equation of state for neutron stars 2011 , url=

Reference 69

Resolution
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no resolver link, observed 2026-08-01T19:22:09.918768Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:22:09.918768Z digest=sha256:18cc382c9772813259111d229c5b57e1df942ac56d923cefa4520fa1fe041404

Observation 4d999b84-d14c-4bf0-9c56-1a089c97afe9 · outbound

This paper cites Experimental and Theoretical Challenges in the Search for the Quark Gluon Plasma: The STAR Collaboration's Critical Assessment of the Evidence from RHIC Collisions.

The equation of state for neutron stars Experimental and Theoretical Challenges in the Search for the Quark Gluon Plasma: The STAR Collaboration's Critical Assessment of the Evidence from RHIC Collisions

Reference 70

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:09.980288Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:22:09.980288Z digest=sha256:f288637b494f75addcd193f281a687f69dae8bc661ffeac6950d47f29fa7cd45

Observation 5d51b791-4837-497f-b5ce-b6c70e3c529c · outbound

This paper cites The PHOBOS Perspective on Discoveries at RHIC.

The equation of state for neutron stars The PHOBOS Perspective on Discoveries at RHIC

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:10.061198Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:22:10.061198Z digest=sha256:24a6c0c871bceb6c8b6ed2f82b14b45cbd931206296475c1bc73ec876d8baeb3

Observation ec2be748-1153-4c46-84fa-5b7ab73ce150 · outbound

This paper cites Formation of dense partonic matter in relativistic nucleus-nucleus collisions at RHIC: Experimental evaluation by the PHENIX collaboration.

The equation of state for neutron stars Formation of dense partonic matter in relativistic nucleus-nucleus collisions at RHIC: Experimental evaluation by the PHENIX collaboration

Reference 72

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:10.195607Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:22:10.195607Z digest=sha256:a08cd3b0ec8d18110d223f188e02e271bd2f110c956269b06e3339ae0671e849

Observation e293e6a6-16cb-44ba-b42a-7f69adefc58a · outbound

This paper cites Enhanced strange baryon production in Au+Au collisions compared to p+p at sqrts = 200 GeV.

The equation of state for neutron stars Enhanced strange baryon production in Au+Au collisions compared to p+p at sqrts = 200 GeV

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:10.257250Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:22:10.257250Z digest=sha256:59073cd570574045346d386760d7386f1ba018132a01bc944c2cdfc7d248295b

Observation d77a3134-fb15-49ab-9882-57effc37e5f0 · outbound

This paper cites Multi-strange baryon production at mid-rapidity in Pb-Pb collisions at $\sqrt{s_{\rm NN}}$ = 2.76 TeV.

The equation of state for neutron stars Multi-strange baryon production at mid-rapidity in Pb-Pb collisions at $\sqrt{s_{\rm NN}}$ = 2.76 TeV

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:10.326931Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:22:10.326931Z digest=sha256:cbb77d5b4e05670a2d03ba114a92a082702599138b961b88347d881367f40293

Observation 20076ab7-9c0c-4aa3-af96-455fd31caa4e · outbound

This paper cites Production and Elliptic Flow of Dileptons and Photons in the semi-Quark Gluon Plasma.

The equation of state for neutron stars Production and Elliptic Flow of Dileptons and Photons in the semi-Quark Gluon Plasma

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:10.418116Z

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Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:22:10.418116Z digest=sha256:20abcac32c632d3bfe3cd2a225d6bb11313f1f01daeeaf32057c3bef05888ef6

Observation fb2c49f9-b0cb-4330-a4d7-9e82c7d1ea36 · outbound

This paper cites an unresolved cited work.

The equation of state for neutron stars Unresolved cited work

Reference 76

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:10.473806Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:22:10.473806Z digest=sha256:4d160b7db9a69f4416e570d9cf7de0c90e838c5f882b28910400fafb971a1f45

Observation 24ff7549-a64a-4e77-80e5-973c5fb16a95 · outbound

This paper cites Statistical thermodynamics of strong interactions at high-energies.

The equation of state for neutron stars Statistical thermodynamics of strong interactions at high-energies

Reference 77

Resolution
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no resolver link, observed 2026-08-01T19:22:10.562661Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:22:10.562661Z digest=sha256:88b1156c5e0fc17eeed3641dbf0bedc719c21a9ddf91d5fd17cdbb5659ba7b62

Observation 875abacf-10bb-4be4-a513-bce2b5e5f32c · outbound

This paper cites The influence of strong magnetic fields on proto-quark stars.

The equation of state for neutron stars The influence of strong magnetic fields on proto-quark stars

Reference 78

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:10.625176Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:22:10.625176Z digest=sha256:d811c98b4839fd99cb3354f13b3f0a277b954355531b9959db55dc3d701a011f

Observation 40909c3c-9823-4c8e-bdcf-6ad308c862c3 · outbound

This paper cites Hyperon-nucleon interaction within chiral effective field theory revisited.

The equation of state for neutron stars Hyperon-nucleon interaction within chiral effective field theory revisited

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:10.709972Z

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source=arxiv_source observed=2026-08-01T19:22:10.709972Z digest=sha256:2d5d932afbe0209ff15db69c473ca256788a3288347fdc33ed3c3a591802b350

Observation 24e5d098-fcf1-4d1d-8524-688070c217fb · outbound

This paper cites QCD at finite isospin density.

The equation of state for neutron stars QCD at finite isospin density

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:10.804009Z

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Observation d91c09d1-8a5d-4e46-b490-0b420a3fca46 · outbound

This paper cites Nuclear thermodynamics from chiral low-momentum interactions.

The equation of state for neutron stars Nuclear thermodynamics from chiral low-momentum interactions

Reference 81

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source=arxiv_source observed=2026-08-01T19:22:10.865389Z digest=sha256:753993c4340d514b8f4e140113bd624186b8fa633e5ff0eba4cdd4d4d8c831a8

Observation bfc79848-76e4-4ce2-bef2-2124e40a2a49 · outbound

This paper cites Equation of state of nuclear and neutron matter at third-order in perturbation theory from chiral EFT.

The equation of state for neutron stars Equation of state of nuclear and neutron matter at third-order in perturbation theory from chiral EFT

Reference 82

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source=arxiv_source observed=2026-08-01T19:22:10.940216Z digest=sha256:17d6246a31caf75688afd6e87e1de244b1e7e1f16ca7a70cdde2979f4f2c20c5

Observation bba75d49-04b0-4cc5-a5a7-ad70770a4448 · outbound

This paper cites Nuclear matter properties from local chiral interactions with $\Delta$ isobar intermediate states.

The equation of state for neutron stars Nuclear matter properties from local chiral interactions with $\Delta$ isobar intermediate states

Reference 83

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source=arxiv_source observed=2026-08-01T19:22:11.010982Z digest=sha256:185c131ce766d51046330f33bf34b37273a100e0e90f1d0e89061c6f3e59560c

Observation 125bb474-9e7e-4925-8f52-d85851c9df56 · outbound

This paper cites Nuclear matter saturation with chiral three-nucleon interactions fitted to light nuclei properties.

The equation of state for neutron stars Nuclear matter saturation with chiral three-nucleon interactions fitted to light nuclei properties

Reference 84

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source=arxiv_source observed=2026-08-01T19:22:11.128154Z digest=sha256:fcb8ce4f34dfdef6c5d4e87fcc3756be949d47bf5ebd5eefb078b5b37c57f8f4

Observation cb6fa8b5-37ca-4c0e-809f-864a07ab6230 · outbound

This paper cites Cool quark matter.

The equation of state for neutron stars Cool quark matter

Reference 85

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source=arxiv_source observed=2026-08-01T19:22:11.211425Z digest=sha256:4d1d0a7996dff48857ee03cb567200a7c395138d7516a7156a162f90a0c2e91b

Observation 133c150e-1cce-4a52-bc29-c25b1c5e2e68 · outbound

This paper cites Cold quark matter at N3LO: soft contributions.

The equation of state for neutron stars Cold quark matter at N3LO: soft contributions

Reference 86

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source=arxiv_source observed=2026-08-01T19:22:11.267875Z digest=sha256:cdf9daf56f94b4ef86191776da41bdbbb0c1ae4771b1be532cf3af1801e2c086

Observation f5ae1e40-4411-4d08-97c6-3a5d56b127cc · outbound

This paper cites Soft interactions in cold quark matter.

The equation of state for neutron stars Soft interactions in cold quark matter

Reference 87

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source=arxiv_source observed=2026-08-01T19:22:11.361398Z digest=sha256:af974f8d401043bf5e5e822ec1a1ae5f2a193da20f8b59bba32fc28b9a6c1cf7

Observation 9ed3c1ab-1697-47e3-b3e2-9011a86b391d · outbound

This paper cites NNNLO pressure of cold quark matter: leading logarithm.

The equation of state for neutron stars NNNLO pressure of cold quark matter: leading logarithm

Reference 88

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source=arxiv_source observed=2026-08-01T19:22:11.491098Z digest=sha256:7b854fadb44d03c804d4395c48890a2e2022f86d6583ed6121e0cb063229b987

Observation fb053186-74d5-4cac-8aff-6aaee81c5580 · outbound

This paper cites and McLerran, Larry D.

The equation of state for neutron stars and McLerran, Larry D

Reference 89

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source=arxiv_source observed=2026-08-01T19:22:11.575637Z digest=sha256:922813d0a88a52261670ce400a1397e47298459ffb8bb3538e491f8801ec681e

Observation a3d6abf6-046a-40dc-ab5e-1af5f469a0a8 · outbound

This paper cites and McLerran, Larry D.

The equation of state for neutron stars and McLerran, Larry D

Reference 90

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source=arxiv_source observed=2026-08-01T19:22:11.728707Z digest=sha256:04627a326135610e62f587a632763cc384ffb3acea50d3563896662de65870a3

Observation aed713b6-906c-49d3-be42-983dae6b5e42 · outbound

This paper cites and McLerran, Larry D.

The equation of state for neutron stars and McLerran, Larry D

Reference 91

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source=arxiv_source observed=2026-08-01T19:22:11.827645Z digest=sha256:2185ecd7e1fc2622a5d1525f9ac122f40575b08ab0f44a6b765d3eec9c15d651

Observation 970003f8-3d14-40cc-a004-16676c10be92 · outbound

This paper cites Two-loop HTL Thermodynamics with Quarks.

The equation of state for neutron stars Two-loop HTL Thermodynamics with Quarks

Reference 92

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source=arxiv_source observed=2026-08-01T19:22:11.964267Z digest=sha256:c04e6d785c2b4d0dfff84e942e9d844c3afd9238f8918263d2f2f1322f25002f

Observation 6071f14c-cc86-420f-9dd0-0e4808a7cc62 · outbound

This paper cites HTL Perturbation Theory to Two Loops.

The equation of state for neutron stars HTL Perturbation Theory to Two Loops

Reference 93

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source=arxiv_source observed=2026-08-01T19:22:12.123066Z digest=sha256:a11ce0fed11587fd6cfdc122705d1f2ebc46251f064c6169c6e08b8ef0ac0f67

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

This paper cites How perturbative QCD constrains the Equation of State at Neutron-Star densities.

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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source=arxiv_source observed=2026-08-01T19:22:12.243560Z digest=sha256:13fc10f4efb16ef414de529d6a9b19c400745e8b3ad08e08f9641228e4f6ca29

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This paper cites Second order hydrodynamic coefficients from kinetic theory.

The equation of state for neutron stars Second order hydrodynamic coefficients from kinetic theory

Reference 95

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source=arxiv_source observed=2026-08-01T19:22:12.368859Z digest=sha256:6838f8f46ca4ca9d5662d432a975051eac5f99b9a05a362600c7bc19d6dd8e5e

Observation e776b2d5-0541-440e-bfcd-d23b3251fa51 · outbound

This paper cites Three-loop HTLpt thermodynamics at finite temperature and chemical potential.

The equation of state for neutron stars Three-loop HTLpt thermodynamics at finite temperature and chemical potential

Reference 96

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source=arxiv_source observed=2026-08-01T19:22:12.508942Z digest=sha256:5baea46e211d22b4334a269694aff664213bac0e8dd1951146a79f2d17d2c390

Observation bcd78d4c-8d1d-4318-b1f9-ebc18d3bf6c3 · outbound

This paper cites Perturbative Thermal QCD: Formalism and Applications.

The equation of state for neutron stars Perturbative Thermal QCD: Formalism and Applications

Reference 97

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source=arxiv_source observed=2026-08-01T19:22:12.666646Z digest=sha256:1f9712019ae62313fefa7eddce10c38f6c141d3e37ef25ec25d8f86bfd6cb588

Observation e49d6982-de91-4f64-809c-83f2b7fb7309 · outbound

This paper cites Phenomenological Lagrangians.

The equation of state for neutron stars Phenomenological Lagrangians

Reference 98

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source=arxiv_source observed=2026-08-01T19:22:12.790037Z digest=sha256:924792d621bad95374555f9230468843a38b978457bc1f2154b360d7ccbbf0d7

Observation e03bb967-e9b7-4b43-ac97-7a937d3b1bfc · outbound

This paper cites Constraints on neutron star radii based on chiral effective field theory interactions.

The equation of state for neutron stars Constraints on neutron star radii based on chiral effective field theory interactions

Reference 99

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source=arxiv_source observed=2026-08-01T19:22:12.909953Z digest=sha256:3f4e36ae603c2b213332165c13489a78030f81231020f0c29407a0f95cae32ba

Observation 5b622d84-bd0c-4b13-b4aa-3ea1c125ef19 · outbound

This paper cites How well do we know the neutron-matter equation of state at the densities inside neutron stars? A Bayesian approach with correlated uncertainties.

The equation of state for neutron stars How well do we know the neutron-matter equation of state at the densities inside neutron stars? A Bayesian approach with correlated uncertainties

Reference 100

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source=arxiv_source observed=2026-08-01T19:22:13.003054Z digest=sha256:b7d8d0c72717731493a4e74e5476ce51ff2b8b89fe2d219dc85b3254a00f2e09

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