Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-10T22:51:08.798386Z
Paper Citation Record · LEDGER
General features of the stellar matter equation of state from microscopic theory, new maximum-mass constraints, and causality
As of 14 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.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-05T10:59:46.981799Z
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
- verified exact0
- verified fuzzy21
- unresolved30
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
No source-named external measurement is stored.
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T22:51:08.606945Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
- Resolution
- unresolved
- raw_fallback, observed 2026-08-10T22:51:09.361361Z
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 ab373b07-0cd1-43b4-bfd4-f4b602744574 · 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 3
- Resolution
- unresolved
- raw_fallback, observed 2026-08-10T22:51:09.349261Z
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 1cc107c6-8ca5-4f82-bea1-ca4507f160d2 · 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 4
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T22:51:08.619306Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T22:51:08.623521Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation c21f150f-2c90-4cd3-ac29-0fa9437d0348 · 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 6
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T22:51:08.627451Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-10T22:51:09.313889Z
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 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
- Resolution
- unresolved
- raw_fallback, observed 2026-08-10T22:51:09.301628Z
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 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
- Resolution
- unresolved
- raw_fallback, observed 2026-08-10T22:51:09.289859Z
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 9cf1ca68-1d27-4d8a-b22f-33ec2396482f · outbound
This paper cites Klausner, G.
Reference 10
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-10T22:51:09.277500Z
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 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
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T22:51:08.646593Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
- unresolved
- raw_fallback, observed 2026-08-10T22:51:09.257883Z
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 4309c53a-adc6-4cf3-9355-787a0f74ae64 · outbound
This paper cites Potekhin, D.
Reference 13
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-10T22:51:09.245247Z
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 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
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-10T22:51:09.233140Z
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 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
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-10T22:51:09.221055Z
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 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
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-10T22:51:09.209396Z
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 b006caa3-c253-4f31-8407-cb9fe0ffc3da · outbound
This paper cites Machleidt, F.
Reference 17
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-10T22:51:09.197720Z
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 897001e7-60af-4f6b-a913-35337c743769 · 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 18
- Resolution
- unresolved
- raw_fallback, observed 2026-08-10T22:51:09.185980Z
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 5f152a3d-f14d-43b1-a353-9057991ae28c · 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 19
- Resolution
- unresolved
- raw_fallback, observed 2026-08-10T22:51:09.173703Z
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 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
- Resolution
- unresolved
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ea4072ef-06a1-4e16-bc82-83aa73c5b016 · 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 21
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T22:51:08.684126Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3ffaea76-136a-41a1-a863-d21d9ac6a892 · outbound
This paper cites Epelbaum, H.
Reference 22
- Resolution
- unresolved
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 88abf122-db6a-42f7-9d74-482f9673c1a4 · outbound
This paper cites Epelbaum, H.
Reference 23
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-10T22:51:09.144412Z
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 854ef757-96e7-40e2-94e1-349c0ad3f473 · outbound
This paper cites Bernard, E.
Reference 24
- Resolution
- unresolved
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 70f474c1-0d9c-4220-9817-c5a0785bc66b · outbound
This paper cites Bernard, E.
Reference 25
- Resolution
- unresolved
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T22:51:08.705014Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T22:51:08.709354Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bf02d52f-4452-4548-8e2b-15460038016b · 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 28
- Resolution
- unresolved
- raw_fallback, observed 2026-08-10T22:51:09.117882Z
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 0d4b972f-7136-4d07-905c-72531fe082db · outbound
This paper cites Linares, S.
Reference 29
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-10T22:51:09.105636Z
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 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
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T22:51:08.721057Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T22:51:08.725099Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
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
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-10T22:51:09.092857Z
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 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
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T22:51:08.733215Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a2e44a00-b9ff-4b3a-8ea8-406023f8346c · outbound
This paper cites Fonseca, H.
Reference 34
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-10T22:51:09.073823Z
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 31c940c9-073b-4a44-86b1-519f0500ccc0 · outbound
This paper cites 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 2026-08-14T06:32:32.682623+00:00.
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 2026-08-14T06:32:32.682623+00:00.
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 2026-08-14T06:32:32.682623+00:00.
Observation 3e33e729-ad63-44a9-8528-209d21b2d8e1 · outbound
This paper cites 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 2026-08-14T06:32:32.682623+00:00.
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 2026-08-14T06:32:32.682623+00:00.
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 2026-08-14T06:32:32.682623+00:00.
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 2026-08-14T06:32:32.682623+00:00.
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 2026-08-14T06:32:32.682623+00:00.
Observation 46014d07-ea64-4e8e-a142-1519a67f36fa · outbound
This paper cites 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 2026-08-14T06:32:32.682623+00:00.
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 2026-08-14T06:32:32.682623+00:00.
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 2026-08-14T06:32:32.682623+00:00.
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 2026-08-14T06:32:32.682623+00:00.
Observation 5c51ee6b-26bb-4043-b7d3-16e8fc5113a1 · outbound
This paper cites 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 2026-08-14T06:32:32.682623+00:00.
Observation 42a4aa3e-eccf-4870-8d56-9b697e815825 · outbound
This paper cites 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 2026-08-14T06:32:32.682623+00:00.
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 2026-08-14T06:32:32.682623+00:00.
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 2026-08-14T06:32:32.682623+00:00.
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.
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 2026-08-14T06:32:32.682623+00:00.