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Paper Citation Record · LEDGER

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality

As of 13 August 2026, this Paper Citation Record lists 51 of 51 outbound references and 1 inbound Pith citation observation for arXiv:2501.00668.

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

pith.paper-citation-record.v1
2501.00668 v2

Coverage vector

measured 51 of 51 reference resolution

Typed states for the displayed outbound observations.

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measured 52 of 52 standing notices

One-hop event checks from named stored sources.

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measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T10:59:46.981799Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T10:59:57.954602Z

Reference resolution

51 of 51 outbound references displayed

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External citation measurements

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Outbound references

Observation 4ec34ca2-9519-4ec1-ad4c-2bee33d681be · outbound

This paper cites an unresolved cited work.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Unresolved cited work

Reference 1

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Observation 8e982339-003d-4434-8770-a10f178d8a74 · outbound

This paper cites an unresolved cited work.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Unresolved cited work

Reference 2

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This paper cites an unresolved cited work.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Unresolved cited work

Reference 3

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General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Unresolved cited work

Reference 4

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Observation c181d5db-8d4c-4f35-a293-a05574fa924f · outbound

This paper cites an unresolved cited work.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Unresolved cited work

Reference 5

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Observation c21f150f-2c90-4cd3-ac29-0fa9437d0348 · outbound

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General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Unresolved cited work

Reference 6

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Observation 90e05a55-a01e-4bb5-9954-3b118ad0aa46 · outbound

This paper cites Huth, et al., Constraining neutron-star matter with microscopic and macroscopic collisions, Nature 606 (2022) 276.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Huth, et al., Constraining neutron-star matter with microscopic and macroscopic collisions, Nature 606 (2022) 276

Reference 7

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Observation 8f6cc92e-09f8-4291-8a9b-3e480b933f83 · outbound

This paper cites an unresolved cited work.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Unresolved cited work

Reference 8

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Observation 55286c34-787d-4bff-b32e-81ae21b8e8da · outbound

This paper cites an unresolved cited work.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Unresolved cited work

Reference 9

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Observation 9cf1ca68-1d27-4d8a-b22f-33ec2396482f · outbound

This paper cites Klausner, G.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Klausner, G

Reference 10

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Observation 3614ac0b-940f-4d88-8b2e-8c6bc9d535a8 · outbound

This paper cites Sammarruca, The neutron skin of 48Ca and 208Pb: A critical analysis, Symmetry 16 (2024) 34.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Sammarruca, The neutron skin of 48Ca and 208Pb: A critical analysis, Symmetry 16 (2024) 34

Reference 11

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Observation 92b3b4bd-e74b-45c5-9fd9-d8e7a105b23e · outbound

This paper cites an unresolved cited work.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Unresolved cited work

Reference 12

Resolution
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Observation 4309c53a-adc6-4cf3-9355-787a0f74ae64 · outbound

This paper cites Potekhin, D.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Potekhin, D

Reference 13

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Observation 2d1fc3bf-e11b-42de-ad30-b0d93692f315 · outbound

This paper cites Sammarruca, R.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Sammarruca, R

Reference 14

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Observation 63618fad-e283-44b0-90c3-02e63a0edd13 · outbound

This paper cites Sammarruca, R.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Sammarruca, R

Reference 15

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Observation 4b6bc025-baf8-4519-8cc7-08f295afbc1e · outbound

This paper cites Sammarruca, R.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Sammarruca, R

Reference 16

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Observation b006caa3-c253-4f31-8407-cb9fe0ffc3da · outbound

This paper cites Machleidt, F.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Machleidt, F

Reference 17

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General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Unresolved cited work

Reference 18

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General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Unresolved cited work

Reference 19

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Observation ca52f4a6-e85a-4db3-a00c-50c9116ec3c1 · outbound

This paper cites Improved chiral nucleon-nucleon potential up to next-to-next-to-next-to-leading order.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Improved chiral nucleon-nucleon potential up to next-to-next-to-next-to-leading order

Reference 20

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General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Unresolved cited work

Reference 21

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Observation 3ffaea76-136a-41a1-a863-d21d9ac6a892 · outbound

This paper cites Epelbaum, H.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Epelbaum, H

Reference 22

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Observation 88abf122-db6a-42f7-9d74-482f9673c1a4 · outbound

This paper cites Epelbaum, H.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Epelbaum, H

Reference 23

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Observation 854ef757-96e7-40e2-94e1-349c0ad3f473 · outbound

This paper cites Bernard, E.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Bernard, E

Reference 24

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This paper cites Bernard, E.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Bernard, E

Reference 25

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Observation ae4c5e2f-c470-483d-b77b-8280d054b91f · outbound

This paper cites Towards consistent nuclear interactions from chiral Lagrangians I: The path-integral approach.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Towards consistent nuclear interactions from chiral Lagrangians I: The path-integral approach

Reference 26

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Observation c0bcfc5c-4a0a-4add-8da7-79f0e2074a47 · outbound

This paper cites Towards consistent nuclear interactions from chiral Lagrangians II: Symmetry preserving regularization.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Towards consistent nuclear interactions from chiral Lagrangians II: Symmetry preserving regularization

Reference 27

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General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Unresolved cited work

Reference 28

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Observation 0d4b972f-7136-4d07-905c-72531fe082db · outbound

This paper cites Linares, S.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Linares, S

Reference 29

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Observation 5256f981-c425-48bb-9101-6a1bacee334b · outbound

This paper cites The Intrabinary Shock and Companion Star of Redback Pulsar J2215+5135.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality The Intrabinary Shock and Companion Star of Redback Pulsar J2215+5135

Reference 30

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unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 37bcc566-225c-4ac7-a6c0-1e85b7f807e4 · outbound

This paper cites Maximum gravitational mass $M_{\rm TOV}=2.25^{+0.08}_{-0.07}M_\odot$ inferred at about $3\%$ precision with multimessenger data of neutron stars.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Maximum gravitational mass $M_{\rm TOV}=2.25^{+0.08}_{-0.07}M_\odot$ inferred at about $3\%$ precision with multimessenger data of neutron stars

Reference 31

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unresolved
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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 21c070d6-864f-4381-a53d-cb4638e1723d · outbound

This paper cites Kanakis-Pegios, P.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Kanakis-Pegios, P

Reference 32

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verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

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Observation a9f47240-64ab-42ae-bb7c-9e3e52582eb1 · outbound

This paper cites an unresolved cited work.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Unresolved cited work

Reference 33

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unresolved
no resolver link, observed 2026-08-10T22:51:08.733215Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T22:51:08.733215Z digest=sha256:489a79c19dcaee17edef7c1d518489e492489e6f34419c32ee7bbde3807887ef

Observation a2e44a00-b9ff-4b3a-8ea8-406023f8346c · outbound

This paper cites Fonseca, H.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Fonseca, H

Reference 34

Resolution
verified fuzzy
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Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-08-10T22:51:08.736660Z digest=sha256:f30e770b526a23bb886baae95eedff38223ab31d438dd0ab0a765dd73367b9ae

Observation 31c940c9-073b-4a44-86b1-519f0500ccc0 · outbound

This paper cites Kumar, S.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Kumar, S

Reference 35

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T22:51:09.063132Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-08-10T22:51:08.740218Z digest=sha256:a1e2fa8acc4d9dfce2c6eec5eebdefc50690f2be20c09e4aa179d42c8587f820

Observation 697a3229-465b-48dd-9137-ffa01c090fda · outbound

This paper cites Sammarruca, Contribution of isovector mesons to the symmetry energy in a microscopic model, Phys.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Sammarruca, Contribution of isovector mesons to the symmetry energy in a microscopic model, Phys

Reference 36

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T22:51:09.052578Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-08-10T22:51:08.743763Z digest=sha256:45e6e56b0038e89c41db874e8fe41be4b2fff0a16f33d58c8d083ca7ff52e8cf

Observation 1ea52a4f-3b6a-47f4-8d86-4ac0b22e2156 · outbound

This paper cites Grasso, Effective density functional beyond mean field, PPNP 106 (2019) 256.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Grasso, Effective density functional beyond mean field, PPNP 106 (2019) 256

Reference 37

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T22:51:09.041143Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-08-10T22:51:08.747488Z digest=sha256:13934b0aa3c6587a832122e5079fc49b812012253034c8e9910e436e2828820e

Observation 3e33e729-ad63-44a9-8528-209d21b2d8e1 · outbound

This paper cites Burrello, M.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Burrello, M

Reference 38

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T22:51:09.029642Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-08-10T22:51:08.751033Z digest=sha256:f926d5acdc9236f7b27ea5431f2d46e7cd5761aea25dcc901abff8d61c954237

Observation 4fc3ba70-ba5f-4c77-8e9b-6b263e175f90 · outbound

This paper cites an unresolved cited work.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Unresolved cited work

Reference 39

Resolution
unresolved
raw_fallback, observed 2026-08-10T22:51:09.018920Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

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Observation 55303445-3244-4034-8b49-f9ac7a4d7de2 · outbound

This paper cites an unresolved cited work.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Unresolved cited work

Reference 40

Resolution
unresolved
raw_fallback, observed 2026-08-10T22:51:09.007499Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-08-10T22:51:08.757784Z digest=sha256:3e4d78d53c31f0f06a6511856ac0f19c7e049c369daf95f0d3e7ff2fe0e4ba62

Observation 76a8cc5f-8c3d-4347-b925-99a6b712cc97 · outbound

This paper cites an unresolved cited work.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Unresolved cited work

Reference 41

Resolution
unresolved
raw_fallback, observed 2026-08-10T22:51:08.996823Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-08-10T22:51:08.761424Z digest=sha256:f11cca335645efce25f136866d2b9cf1669cef4cc3e6a588f34a61171e9a070e

Observation 614cb958-8d13-453f-b117-5380758d134a · outbound

This paper cites an unresolved cited work.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Unresolved cited work

Reference 42

Resolution
unresolved
raw_fallback, observed 2026-08-10T22:51:08.984489Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-08-10T22:51:08.764852Z digest=sha256:2a5d7b8335e6ac78952f8eaf998b293d17883031b20b33eb49cddbac6eae572a

Observation 46014d07-ea64-4e8e-a142-1519a67f36fa · outbound

This paper cites Das, J.-B.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Das, J.-B

Reference 43

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T22:51:08.973467Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-08-10T22:51:08.768818Z digest=sha256:e788e7e2e3bb4d25e134eea254adba12f06756b2923b0fe3d71e82565fb63ea0

Observation c38b4f7f-aae3-4bcf-a566-fa9a3f768589 · outbound

This paper cites Gonzalez-Jimenez, C.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Gonzalez-Jimenez, C

Reference 44

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T22:51:08.962674Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-08-10T22:51:08.772560Z digest=sha256:eb92a724055b0a179d2dd809d953435e4cc592e4519dd288f7b277394e939a02

Observation 5fe75719-d459-4ac5-bc4f-f2ec9e7253ca · outbound

This paper cites Gonzalez-Caniulef, S.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Gonzalez-Caniulef, S

Reference 45

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T22:51:08.951064Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-08-10T22:51:08.776485Z digest=sha256:98a39fb2e802aedcc895bb3c44f33e4e92bcd2c4093608f282a0ffcd8f93657e

Observation f5eab67c-a07b-4625-8e35-961e39576dbd · outbound

This paper cites an unresolved cited work.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Unresolved cited work

Reference 46

Resolution
unresolved
raw_fallback, observed 2026-08-10T22:51:08.938954Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-08-10T22:51:08.780243Z digest=sha256:a0758c661f16b14e2fef1703038839458f9cebeba864d0747df50f2ade274c32

Observation 5c51ee6b-26bb-4043-b7d3-16e8fc5113a1 · outbound

This paper cites Potekhin, G.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Potekhin, G

Reference 47

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T22:51:08.927806Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-08-10T22:51:08.783882Z digest=sha256:5a7687902d0c7efe0aef226e4f088ea352098ee03adb8635f3dc7de375634bd5

Observation 42a4aa3e-eccf-4870-8d56-9b697e815825 · outbound

This paper cites Nomoto, S.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Nomoto, S

Reference 48

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T22:51:08.916773Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-08-10T22:51:08.787625Z digest=sha256:38ed03d8214a1cf627638bf4cf2c830df2ab37149f39094e1b3d5ce249ba6810

Observation 97360bc8-a0ca-47d3-b328-4d5437db16a5 · outbound

This paper cites Krotscheck, P.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Krotscheck, P

Reference 49

Resolution
verified fuzzy
raw_fallback, observed 2026-08-10T22:51:08.905365Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-08-10T22:51:08.791133Z digest=sha256:ced0270d491d7407b13fd9af08b716bee2fa54eb4f43f815936d502e5dec4dff

Observation f0e4a0b5-3d47-47f8-af9b-362e834dddd0 · outbound

This paper cites an unresolved cited work.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Unresolved cited work

Reference 50

Resolution
unresolved
raw_fallback, observed 2026-08-10T22:51:08.892778Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-08-10T22:51:08.794739Z digest=sha256:f22c5f1cb894711b2b0ff1f541a41da37364b4ff9981417545b45ace4678eb9c

Observation d6f9045d-05ec-4776-b530-4d761d87db5e · outbound

This paper cites an unresolved cited work.

General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality Unresolved cited work

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-10T22:51:08.798386Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T22:51:08.798386Z digest=sha256:37a66f8f62ab54e9e71d64062a25d3bbb60061b175c6bfa75ad533fab1f9d748

Pith citing papers

Observation 2da7da03-d248-46a6-88e8-b6f92baf81b4 · inbound

Bayesian analysis of properties of nuclear matter with the FOPI experimental data cites this paper.

Bayesian analysis of properties of nuclear matter with the FOPI experimental data General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality

Reference 25

Resolution
verified exact
local_arxiv, observed 2026-08-05T10:59:58.028055Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-08-05T10:59:46.981799Z digest=sha256:c37819b8fcd2f34c1190793277aa25727c1d32b3c98c78d8c98d301faa3d9f04