How neutron star properties disfavor a nuclear chiral density wave | Paper Citation Record

Observation 5b5e049a-5d03-4e32-916e-6da12cb0f67a · outbound

This paper cites an unresolved cited work.

How neutron star properties disfavor a nuclear chiral density wave Unresolved cited work

Reference 1

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Observation e6ff1c95-92bf-44a9-b84e-1cfb3b1dd6af · outbound

This paper cites (48) Using the numerical values of all fixed physical parameters, the relations (46) yield functions gω = gω(dω, M0) , g ρ = gρ(dω, dωρ, M0).

How neutron star properties disfavor a nuclear chiral density wave (48) Using the numerical values of all fixed physical parameters, the relations (46) yield functions gω = gω(dω, M0) , g ρ = gρ(dω, dωρ, M0)

Reference 2

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Observation d4d4ee36-2c41-4128-b058-1eddae04abc8 · outbound

This paper cites reasonable.

How neutron star properties disfavor a nuclear chiral density wave reasonable

Reference 3

Resolution: malformed identifier; raw_fallback, observed 2026-08-12T22:01:14.324448Z

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Observation 061b4ae4-9f6b-467e-8fca-0211a252abd8 · outbound

This paper cites Inhomogeneous chiral condensates.

How neutron star properties disfavor a nuclear chiral density wave Inhomogeneous chiral condensates

Reference 4

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Observation 9cf1b234-63f3-4ed5-8cc2-ea2b30c03dfa · outbound

This paper cites Dautry and E.

How neutron star properties disfavor a nuclear chiral density wave Dautry and E

Reference 5

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Observation 112ab610-c523-4368-a413-1dd63903e48a · outbound

This paper cites Takahashi and T.

How neutron star properties disfavor a nuclear chiral density wave Takahashi and T

Reference 6

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T22:01:14.277780Z

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Observation d4aa51e5-bf1d-406d-b92b-b3dbeb791367 · outbound

This paper cites Takahashi, Phys.

How neutron star properties disfavor a nuclear chiral density wave Takahashi, Phys

Reference 7

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T22:01:14.262154Z

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Observation 78958cdc-bdb6-4dd4-b8e4-924bd0eba3c8 · outbound

This paper cites Color superconductivity in dense quark matter.

How neutron star properties disfavor a nuclear chiral density wave Color superconductivity in dense quark matter

Reference 8

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Observation dda9d8b8-9f23-4b4c-92eb-f090eeb054ff · outbound

This paper cites Crystalline Color Superconductivity.

How neutron star properties disfavor a nuclear chiral density wave Crystalline Color Superconductivity

Reference 9

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Observation 558b5542-693a-4900-bb97-60b7b88dcc46 · outbound

This paper cites Therefore, a controlled approximation would require more sophisticated (strong-coupling) methods beyond our one-loop calculation of the pressure.

How neutron star properties disfavor a nuclear chiral density wave Therefore, a controlled approximation would require more sophisticated (strong-coupling) methods beyond our one-loop calculation of the pressure

Reference 10

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T22:01:14.308989Z

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Observation ea409658-1913-4274-b5cc-ca297064bfdd · outbound

This paper cites Meson Supercurrent State in High Density QCD.

How neutron star properties disfavor a nuclear chiral density wave Meson Supercurrent State in High Density QCD

Reference 11

Resolution: verified exact; local_arxiv, observed 2026-08-12T22:01:14.028332Z

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Observation 8bdbf003-2ae6-476f-bf5a-1dc2b160f9f0 · outbound

This paper cites Spontaneous Superfluid Current Generation in CFL at Nonzero Strange Quark Mass.

How neutron star properties disfavor a nuclear chiral density wave Spontaneous Superfluid Current Generation in CFL at Nonzero Strange Quark Mass

Reference 12

Resolution: verified exact; local_arxiv, observed 2026-08-12T22:01:14.007698Z

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Observation dc118d7e-db51-4ca5-9663-2f47f2bae719 · outbound

This paper cites Chiral crossover vs chiral density wave in dense nuclear matter.

How neutron star properties disfavor a nuclear chiral density wave Chiral crossover vs chiral density wave in dense nuclear matter

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:12.851700Z

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Observation 02bc4a08-989a-4e24-a93b-d004e880f4e3 · outbound

This paper cites Inhomogeneous phases in the Nambu-Jona-Lasino and quark-meson model.

How neutron star properties disfavor a nuclear chiral density wave Inhomogeneous phases in the Nambu-Jona-Lasino and quark-meson model

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:12.856688Z

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Observation 74321a6b-4b8b-4a24-96cf-92971ac8c299 · outbound

This paper cites Boguta, Phys.

How neutron star properties disfavor a nuclear chiral density wave Boguta, Phys

Reference 15

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T22:01:14.245774Z

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Observation 0867892e-a9a5-4163-8639-de68e0849a08 · outbound

This paper cites Boguta and J.

How neutron star properties disfavor a nuclear chiral density wave Boguta and J

Reference 16

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T22:01:14.230425Z

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Observation 68093b25-aa81-4038-af91-1b8cd22322ea · outbound

This paper cites Chemical freeze-out in heavy ion collisions at large baryon densities.

How neutron star properties disfavor a nuclear chiral density wave Chemical freeze-out in heavy ion collisions at large baryon densities

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:12.870714Z

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Observation 335cc154-e066-4abe-96be-dd1cb8905437 · outbound

This paper cites Thermodynamic phases and mesonic fluctuations in a chiral nucleon-meson model.

How neutron star properties disfavor a nuclear chiral density wave Thermodynamic phases and mesonic fluctuations in a chiral nucleon-meson model

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:12.875471Z

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Observation ac9e4c3d-e064-4fd7-aea1-493c7dc961a1 · outbound

This paper cites From asymmetric nuclear matter to neutron stars: a functional renormalization group study.

How neutron star properties disfavor a nuclear chiral density wave From asymmetric nuclear matter to neutron stars: a functional renormalization group study

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:12.880190Z

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Observation cc0252ee-1233-43b6-a608-83211b4a6736 · outbound

This paper cites Surface tension of dense matter at the chiral phase transition.

How neutron star properties disfavor a nuclear chiral density wave Surface tension of dense matter at the chiral phase transition

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:12.884691Z

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Observation 572612bf-15de-4cd6-a34f-6e07514a30c8 · outbound

This paper cites Chiral pasta.

How neutron star properties disfavor a nuclear chiral density wave Chiral pasta

Reference 21

Resolution: verified exact; local_arxiv, observed 2026-08-12T22:01:13.885428Z

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Observation c6e84612-97ac-417f-8e4c-011107a5e8d7 · outbound

This paper cites Strange quark matter from a baryonic approach.

How neutron star properties disfavor a nuclear chiral density wave Strange quark matter from a baryonic approach

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:12.894061Z

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Observation 103a0a9c-727b-4c81-ac88-f7210af1d9a6 · outbound

This paper cites Chiral symmetry and density wave in quark matter.

How neutron star properties disfavor a nuclear chiral density wave Chiral symmetry and density wave in quark matter

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:12.898800Z

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Observation a6d7bd9f-e518-4068-8e2b-5f627f65920c · outbound

This paper cites Chiral density waves in quark matter within the Nambu--Jona-Lasinio model in an external magnetic field.

How neutron star properties disfavor a nuclear chiral density wave Chiral density waves in quark matter within the Nambu--Jona-Lasinio model in an external magnetic field

Reference 24

Resolution: verified exact; local_arxiv, observed 2026-08-12T22:01:13.835066Z

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Observation 9472cb21-8085-48f0-92d1-f12494ba3b38 · outbound

This paper cites Inhomogeneous islands and continents in the Nambu--Jona-Lasinio model.

How neutron star properties disfavor a nuclear chiral density wave Inhomogeneous islands and continents in the Nambu--Jona-Lasinio model

Reference 25

Resolution: verified exact; local_arxiv, observed 2026-08-12T22:01:13.814276Z

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Observation 1f3965be-f604-410f-9b5e-30a63c6303b0 · outbound

This paper cites Inhomogeneous phases in the quark-meson model with vacuum fluctuations.

How neutron star properties disfavor a nuclear chiral density wave Inhomogeneous phases in the quark-meson model with vacuum fluctuations

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:12.913524Z

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Observation f926aa54-31bf-4d09-b745-d36988dae4e4 · outbound

This paper cites Inhomogeneous chiral symmetry breaking in dense neutron-star matter.

How neutron star properties disfavor a nuclear chiral density wave Inhomogeneous chiral symmetry breaking in dense neutron-star matter

Reference 27

Resolution: verified exact; local_arxiv, observed 2026-08-12T22:01:13.777949Z

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Observation 4e6c0c07-9a4b-4529-b772-f1b15aedf92e · outbound

This paper cites Inhomogeneous chiral condensate in the quark-meson model.

How neutron star properties disfavor a nuclear chiral density wave Inhomogeneous chiral condensate in the quark-meson model

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:12.923359Z

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Observation 1c6e3bf0-5974-4474-a746-06f6f1a652ea · outbound

This paper cites Chiral density wave versus pion condensation at finite density.

How neutron star properties disfavor a nuclear chiral density wave Chiral density wave versus pion condensation at finite density

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:12.928103Z

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Observation 72b1cbbe-9387-49bb-af2e-384847af98c2 · outbound

This paper cites Absence of Landau-Peierls Instability in the Magnetic Dual Chiral Density Wave Phase of Dense QCD.

How neutron star properties disfavor a nuclear chiral density wave Absence of Landau-Peierls Instability in the Magnetic Dual Chiral Density Wave Phase of Dense QCD

Reference 30

Resolution: verified exact; local_arxiv, observed 2026-08-12T22:01:13.728222Z

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No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation bba199cb-4769-47c0-b5e2-3bba7110caab · outbound

This paper cites Inhomogeneous chiral condensates in three-flavor quark matter.

How neutron star properties disfavor a nuclear chiral density wave Inhomogeneous chiral condensates in three-flavor quark matter

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:12.938004Z

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Observation c7e31a8d-4e2c-4d32-bdaf-1b249f13ae29 · outbound

This paper cites Competition of inhomogeneous chiral phases and two-flavor color superconductivity in the NJL model.

How neutron star properties disfavor a nuclear chiral density wave Competition of inhomogeneous chiral phases and two-flavor color superconductivity in the NJL model

Reference 32

Resolution: verified exact; local_arxiv, observed 2026-08-12T22:01:13.693154Z

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Observation 70546367-29fa-49a2-9937-3f503ebd9dbd · outbound

This paper cites Inhomogeneous phases in the quark-meson model with explicit chiral-symmetry breaking.

How neutron star properties disfavor a nuclear chiral density wave Inhomogeneous phases in the quark-meson model with explicit chiral-symmetry breaking

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:12.948155Z

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Observation 069e3c51-5115-4983-b289-1a67d7bac726 · outbound

This paper cites Chiral density wave in nuclear matter.

How neutron star properties disfavor a nuclear chiral density wave Chiral density wave in nuclear matter

Reference 34

Resolution: verified exact; local_arxiv, observed 2026-08-12T22:01:13.657978Z

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No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation f7b1eb96-f749-4e15-9fbd-743f90909daf · outbound

This paper cites A novel Dual Chiral Density Wave in nuclear matter based on a parity doublet structure.

How neutron star properties disfavor a nuclear chiral density wave A novel Dual Chiral Density Wave in nuclear matter based on a parity doublet structure

Reference 35

Resolution: verified exact; local_arxiv, observed 2026-08-12T22:01:13.638148Z

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No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 8f6c5713-a00a-4fc8-baf0-0942c2620ca7 · outbound

This paper cites Crystalline chiral condensates off the tricritical point in a generalized Ginzburg-Landau approach.

How neutron star properties disfavor a nuclear chiral density wave Crystalline chiral condensates off the tricritical point in a generalized Ginzburg-Landau approach

Reference 36

Resolution: verified exact; local_arxiv, observed 2026-08-12T22:01:13.617782Z

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Observation 29c8508c-1840-43bf-a2c8-0e30c7eab238 · outbound

This paper cites Two-dimensional chiral crystals in the NJL model.

How neutron star properties disfavor a nuclear chiral density wave Two-dimensional chiral crystals in the NJL model

Reference 37

Resolution: verified exact; local_arxiv, observed 2026-08-12T22:01:13.596482Z

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No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation de4a136b-7d40-4787-a56b-9d6e93dc8053 · outbound

This paper cites How transverse thermal fluctuations disorder a condensate of chiral spirals into a quantum spin liquid.

How neutron star properties disfavor a nuclear chiral density wave How transverse thermal fluctuations disorder a condensate of chiral spirals into a quantum spin liquid

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:12.972886Z

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Observation 25786b87-60a3-4fb0-bdfc-b421555985cc · outbound

This paper cites Lattice study of disordering of inhomogeneous condensates and the Quantum Pion Liquid in effective $O(N)$ model.

How neutron star properties disfavor a nuclear chiral density wave Lattice study of disordering of inhomogeneous condensates and the Quantum Pion Liquid in effective $O(N)$ model

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:12.977745Z

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Observation eef89f60-6a6c-4aa7-8331-62a990bbf0f5 · outbound

This paper cites an unresolved cited work.

How neutron star properties disfavor a nuclear chiral density wave Unresolved cited work

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:12.983024Z

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Observation 90452c11-20ed-45fb-aca9-fc2b407fc5b5 · outbound

This paper cites Heiselberg, C.

How neutron star properties disfavor a nuclear chiral density wave Heiselberg, C

Reference 41

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T22:01:14.205727Z

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Observation 7a12b478-ddc5-4dd8-ba26-30d9189e4a46 · outbound

This paper cites Crystalline chiral condensates as a component of compact stars.

How neutron star properties disfavor a nuclear chiral density wave Crystalline chiral condensates as a component of compact stars

Reference 42

Resolution: verified exact; local_arxiv, observed 2026-08-12T22:01:13.545830Z

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No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 57bbd09f-2b3d-45dd-af45-ac7f0fd62bea · outbound

This paper cites Magnetic Dual Chiral Density Wave: A Candidate Quark Matter Phase for the Interior of Neutron Stars.

How neutron star properties disfavor a nuclear chiral density wave Magnetic Dual Chiral Density Wave: A Candidate Quark Matter Phase for the Interior of Neutron Stars

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:12.997901Z

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Observation 74d812d6-8b05-417b-98c3-fca0a73bec33 · outbound

This paper cites Quark beta decay in the inhomogeneous chiral phase and cooling of compact stars.

How neutron star properties disfavor a nuclear chiral density wave Quark beta decay in the inhomogeneous chiral phase and cooling of compact stars

Reference 44

Resolution: verified exact; local_arxiv, observed 2026-08-12T22:01:13.509673Z

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No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation afccc97c-7982-4367-9d5a-6aa1a2ee1664 · outbound

This paper cites Constraining the speed of sound inside neutron stars with chiral effective field theory interactions and observations.

How neutron star properties disfavor a nuclear chiral density wave Constraining the speed of sound inside neutron stars with chiral effective field theory interactions and observations

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:13.007330Z

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Observation 4e1f0027-277c-42b8-9699-7db0d7d8b8f0 · outbound

This paper cites Relativistic mean-field theories for neutron-star physics based on chiral effective field theory.

How neutron star properties disfavor a nuclear chiral density wave Relativistic mean-field theories for neutron-star physics based on chiral effective field theory

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:13.012097Z

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Observation d16b0192-02ed-4d18-8588-8a713edbdf15 · outbound

This paper cites an unresolved cited work.

How neutron star properties disfavor a nuclear chiral density wave Unresolved cited work

Reference 47

Resolution: unresolved; raw_fallback, observed 2026-08-12T22:01:14.191982Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 1b4ed410-07a1-43ee-8106-f06576de7d3e · outbound

This paper cites Isospin Asymmetry in Nuclei and Neutron Stars.

How neutron star properties disfavor a nuclear chiral density wave Isospin Asymmetry in Nuclei and Neutron Stars

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:13.021490Z

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Observation 5c860be7-02c3-4167-a4fb-64da051c6945 · outbound

This paper cites Kapusta and C.

How neutron star properties disfavor a nuclear chiral density wave Kapusta and C

Reference 49

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T22:01:14.177058Z

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No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation f5c53f80-acc4-41e4-82f7-1b91e94ccd61 · outbound

This paper cites Cold Quark Matter.

How neutron star properties disfavor a nuclear chiral density wave Cold Quark Matter

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:13.031273Z

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Observation 622e5a0d-c19b-46af-b5d7-56d5d5756440 · outbound

This paper cites Hot perturbative QCD in a very strong magnetic background.

How neutron star properties disfavor a nuclear chiral density wave Hot perturbative QCD in a very strong magnetic background

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:13.036314Z

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Observation 565e54ed-fb73-4e3f-9f8b-08ab03ea6394 · outbound

This paper cites Dense matter in compact stars - A pedagogical introduction.

How neutron star properties disfavor a nuclear chiral density wave Dense matter in compact stars - A pedagogical introduction

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:13.041255Z

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Observation 81f2104a-ad67-4fc6-afd0-6152f4010254 · outbound

This paper cites an unresolved cited work.

How neutron star properties disfavor a nuclear chiral density wave Unresolved cited work

Reference 53

Resolution: unresolved; raw_fallback, observed 2026-08-12T22:01:14.160882Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation d0a864a2-d2f9-45b6-a0a7-f69e5bd72f87 · outbound

This paper cites A microscopic estimate of the nuclear matter compressibility and symmetry energy in relativistic mean-field models.

How neutron star properties disfavor a nuclear chiral density wave A microscopic estimate of the nuclear matter compressibility and symmetry energy in relativistic mean-field models

Reference 54

Resolution: verified exact; local_arxiv, observed 2026-08-12T22:01:13.401173Z

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No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 8955a64c-2290-4ab9-813f-946fb14370a9 · outbound

This paper cites an unresolved cited work.

How neutron star properties disfavor a nuclear chiral density wave Unresolved cited work

Reference 55

Resolution: unresolved; raw_fallback, observed 2026-08-12T22:01:14.146602Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation df170901-a6ee-46cd-b6ea-f4a79f3b0b21 · outbound

This paper cites Shlomo, V.

How neutron star properties disfavor a nuclear chiral density wave Shlomo, V

Reference 56

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T22:01:14.132111Z

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No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 62737647-3647-404e-94df-9c45fd13ecec · outbound

This paper cites Liu, J.-D.

How neutron star properties disfavor a nuclear chiral density wave Liu, J.-D

Reference 57

Resolution: verified fuzzy; raw_fallback, observed 2026-08-12T22:01:14.117300Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation e06be52d-1c26-426d-82d2-425a43af3ad4 · outbound

This paper cites Vacuum fluctuations and the thermodynamics of chiral models.

How neutron star properties disfavor a nuclear chiral density wave Vacuum fluctuations and the thermodynamics of chiral models

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:13.068916Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 71d24700-9236-438c-a3d4-9d0b5bda8e35 · outbound

This paper cites Accurate Determination of the Neutron Skin Thickness of $^{208}$Pb through Parity-Violation in Electron Scattering.

How neutron star properties disfavor a nuclear chiral density wave Accurate Determination of the Neutron Skin Thickness of $^{208}$Pb through Parity-Violation in Electron Scattering

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:13.073686Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 764b6e31-e59f-4239-a28b-0911617b1420 · outbound

This paper cites Ab initio predictions link the neutron skin of ${}^{208}$Pb to nuclear forces.

How neutron star properties disfavor a nuclear chiral density wave Ab initio predictions link the neutron skin of ${}^{208}$Pb to nuclear forces

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:13.078813Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c176f4d3-6c5c-460c-b571-2cfec3ff8bac · outbound

This paper cites New constraints on the neutron-star mass and radius relation from terrestrial nuclear experiments.

How neutron star properties disfavor a nuclear chiral density wave New constraints on the neutron-star mass and radius relation from terrestrial nuclear experiments

Reference 61

Resolution: verified exact; local_arxiv, observed 2026-08-12T22:01:13.333261Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 4f7691e1-5162-438d-b371-a96533b863c7 · outbound

This paper cites Precision Determination of the Neutral Weak Form Factor of $^{48}$Ca.

How neutron star properties disfavor a nuclear chiral density wave Precision Determination of the Neutral Weak Form Factor of $^{48}$Ca

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:13.088171Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e73b6d56-9f2c-4373-a41a-eab7d1e0e0f7 · outbound

This paper cites Constraints on Nuclear Symmetry Energy Parameters.

How neutron star properties disfavor a nuclear chiral density wave Constraints on Nuclear Symmetry Energy Parameters

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:13.093131Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7d506ba2-430b-44ee-82ea-c618c0c6815c · outbound

This paper cites Determination of the neutron skin of $^{208}$Pb from ultrarelativistic nuclear collisions.

How neutron star properties disfavor a nuclear chiral density wave Determination of the neutron skin of $^{208}$Pb from ultrarelativistic nuclear collisions

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:13.097839Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 80bc88dc-5967-42c6-b5e7-44205d68a7df · outbound

This paper cites an unresolved cited work.

How neutron star properties disfavor a nuclear chiral density wave Unresolved cited work

Reference 65

Resolution: unresolved; raw_fallback, observed 2026-08-12T22:01:14.101940Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

Observation 70021135-215f-436c-8dae-de386c7a950f · outbound

This paper cites an unresolved cited work.

How neutron star properties disfavor a nuclear chiral density wave Unresolved cited work

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:13.107350Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2510b0f8-1f94-437d-8510-aad22df5088d · outbound

This paper cites an unresolved cited work.

How neutron star properties disfavor a nuclear chiral density wave Unresolved cited work

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:13.112086Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f8170ada-4dac-45f9-a04a-e86158465cd9 · outbound

This paper cites Building a realistic neutron star from holography.

How neutron star properties disfavor a nuclear chiral density wave Building a realistic neutron star from holography

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:13.116710Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 08debcee-dec4-43f5-bcf3-7b967eec2e18 · outbound

This paper cites an unresolved cited work.

How neutron star properties disfavor a nuclear chiral density wave Unresolved cited work

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:13.121569Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 95e360e3-5dd4-483f-a4f9-4a0a5d6ec251 · outbound

This paper cites Refined Mass and Geometric Measurements of the High-Mass PSR J0740+6620.

How neutron star properties disfavor a nuclear chiral density wave Refined Mass and Geometric Measurements of the High-Mass PSR J0740+6620

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:13.126491Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e2265913-c573-48c8-b1e6-027930519619 · outbound

This paper cites PSR J0952-0607: The Fastest and Heaviest Known Galactic Neutron Star.

How neutron star properties disfavor a nuclear chiral density wave PSR J0952-0607: The Fastest and Heaviest Known Galactic Neutron Star

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:13.131529Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9728c631-ab20-48b6-aa1a-1af92802de90 · outbound

This paper cites Classifications of Twin Star Solutions for a Constant Speed of Sound Parameterized Equation of State.

How neutron star properties disfavor a nuclear chiral density wave Classifications of Twin Star Solutions for a Constant Speed of Sound Parameterized Equation of State

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:13.136140Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a03bb68d-1f84-43ed-bb26-0dd97683917a · outbound

This paper cites Isospin asymmetry in holographic baryonic matter.

How neutron star properties disfavor a nuclear chiral density wave Isospin asymmetry in holographic baryonic matter

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-12T22:01:13.141231Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cc1792c2-3aaa-4ae8-beb0-f5e5054557e6 · outbound

This paper cites Phases of cold holographic QCD: baryons, pions and rho mesons.

How neutron star properties disfavor a nuclear chiral density wave Phases of cold holographic QCD: baryons, pions and rho mesons

Reference 74

Resolution: verified exact; local_arxiv, observed 2026-08-12T22:01:13.192989Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

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