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Paper Citation Record · LEDGER

Rotating neutron stars with non-barotropic thermal profile

As of 15 August 2026, this Paper Citation Record lists 86 of 86 outbound references and 1 inbound Pith citation observation for arXiv:1908.11258.

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

pith.paper-citation-record.v1
1908.11258 v2

Coverage vector

measured 86 of 86 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-14T10:30:45.219142Z

measured 87 of 87 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 1 of 1 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-06-26T23:50:12.361235Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T22:08:58.814793Z

Reference resolution

86 of 86 outbound references displayed

  • verified exact10
  • verified fuzzy14
  • unresolved59
  • parse uncertain2
  • malformed identifier1
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 4095b468-239c-43b9-924f-320a781f8bb8 · outbound

This paper cites Otherwise, determine Ω from Eq.

Rotating neutron stars with non-barotropic thermal profile Otherwise, determine Ω from Eq

Reference 1

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no resolver link, observed 2026-08-14T10:30:44.913910Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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Observation 8a4dacfc-886a-49e3-bc72-8e639ba14fcb · outbound

This paper cites barotropic.

Rotating neutron stars with non-barotropic thermal profile barotropic

Reference 2

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Observation c1d4e5af-33e7-4e99-ad90-2ac1a73caefa · outbound

This paper cites an unresolved cited work.

Rotating neutron stars with non-barotropic thermal profile Unresolved cited work

Reference 3

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parse uncertain
no resolver link, observed 2026-08-14T10:30:44.917213Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:44.917213Z digest=sha256:5a8a6fc9b0d68f4484458f61481a6e1798dfd95f29f80f8ee00783c5c58b7e28

Observation 2f8ffda1-3190-4bc0-ad19-42533f2d3c57 · outbound

This paper cites an unresolved cited work.

Rotating neutron stars with non-barotropic thermal profile Unresolved cited work

Reference 4

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no resolver link, observed 2026-08-14T10:30:44.920749Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:44.920749Z digest=sha256:72a98d72f48bf5f7cbacb089697a71026293689e93fb8351274923fb0ed6c0eb

Observation de01c013-30b2-455e-8124-d6208aec82d1 · outbound

This paper cites an unresolved cited work.

Rotating neutron stars with non-barotropic thermal profile Unresolved cited work

Reference 5

Resolution
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no resolver link, observed 2026-08-14T10:30:44.924935Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:44.924935Z digest=sha256:4a40d924513c93ea2c04724d368f83fda3987be8317b08d46b9220d3f0842bd7

Observation a5495391-ed50-4bae-8d95-16c3cb786ef3 · outbound

This paper cites an unresolved cited work.

Rotating neutron stars with non-barotropic thermal profile Unresolved cited work

Reference 6

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Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:44.928613Z digest=sha256:44b81ef1c5ef39dadf7a1fff0bbf528a69100911c0903fa71548f9f61fcd5216

Observation b92dc603-1d6f-41db-bbd9-49c3632179fd · outbound

This paper cites Solve the EOS from p (if barotropic) or p, h (if non barotropic).

Rotating neutron stars with non-barotropic thermal profile Solve the EOS from p (if barotropic) or p, h (if non barotropic)

Reference 7

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T10:30:46.330494Z

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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Observation 5f571048-e059-4400-a1db-cc4bc3f6204e · outbound

This paper cites an unresolved cited work.

Rotating neutron stars with non-barotropic thermal profile Unresolved cited work

Reference 8

Resolution
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raw_fallback, observed 2026-08-14T10:30:46.320117Z

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

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Observation ff42131b-7d29-44a8-8e10-054d8c301a12 · outbound

This paper cites same as above.

Rotating neutron stars with non-barotropic thermal profile same as above

Reference 9

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T10:30:46.309074Z

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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Observation 5dff556a-fd16-47c8-81c6-7c5d5e663bc9 · outbound

This paper cites The vice versa is also true.

Rotating neutron stars with non-barotropic thermal profile The vice versa is also true

Reference 10

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T10:30:46.296504Z

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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Observation 701280f6-a96e-43b6-a896-e494937b0fec · outbound

This paper cites an unresolved cited work.

Rotating neutron stars with non-barotropic thermal profile Unresolved cited work

Reference 11

Resolution
unresolved
raw_fallback, observed 2026-08-14T10:30:46.285855Z

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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Observation b1bd78cb-44d2-40da-9847-319248228ed3 · outbound

This paper cites However, this is not true in general for a non-barotropic star (but it is for the non-barotropic cases considered in this work) [18, 19, 21, 23, 24, 26].

Rotating neutron stars with non-barotropic thermal profile However, this is not true in general for a non-barotropic star (but it is for the non-barotropic cases considered in this work) [18, 19, 21, 23, 24, 26]

Reference 12

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T10:30:46.274880Z

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.

source=pdf_text observed=2026-08-14T10:30:44.949062Z digest=sha256:5e107059dabfc643499178a1219d56e813cdf1e5d34f8b2f960d19e710507280

Observation 0e9b0379-0154-402a-8809-d0bda66e5b2e · outbound

This paper cites III is that there are only two EOS quantities that can be directly determined from the Euler equation with- out solving the EOS, namely p and h.

Rotating neutron stars with non-barotropic thermal profile III is that there are only two EOS quantities that can be directly determined from the Euler equation with- out solving the EOS, namely p and h

Reference 13

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T10:30:46.264050Z

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.

source=pdf_text observed=2026-08-14T10:30:44.952627Z digest=sha256:bb90ab7d79ce33285042ffebfeb8c5ae98070e4ab5f37edad0305764dba4564a

Observation 7464859a-5112-4abf-9b19-9f8158fcc0ea · outbound

This paper cites an unresolved cited work.

Rotating neutron stars with non-barotropic thermal profile Unresolved cited work

Reference 14

Resolution
unresolved
raw_fallback, observed 2026-08-14T10:30:46.252687Z

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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Observation 24b40de2-e18a-4005-98a7-d00fd66fc89a · outbound

This paper cites including viscosity [24].

Rotating neutron stars with non-barotropic thermal profile including viscosity [24]

Reference 15

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T10:30:46.242347Z

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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Observation 19196ca8-b022-4f3f-b2c4-b79d9fb047e7 · outbound

This paper cites The Nuclear Equation of State and Neutron Star Masses.

Rotating neutron stars with non-barotropic thermal profile The Nuclear Equation of State and Neutron Star Masses

Reference 16

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:44.964501Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:44.964501Z digest=sha256:3033aff036e54ae174c637858bd2d20ed0b65db7c94f8259f27e41a71fe2781e

Observation 1b08d1a5-f7c9-414a-b46a-60b4af13e310 · outbound

This paper cites The Equation of State of Hot, Dense Matter and Neutron Stars.

Rotating neutron stars with non-barotropic thermal profile The Equation of State of Hot, Dense Matter and Neutron Stars

Reference 17

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:44.968450Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:44.968450Z digest=sha256:5de489283a1d1327f0be2ef080cdbd6731f475eaf351d44cf1a3af779bf3a36b

Observation f7a068bf-9608-4da5-a0fe-9bd63483bdda · outbound

This paper cites GW170817: Measurements of Neutron Star Radii and Equation of State.

Rotating neutron stars with non-barotropic thermal profile GW170817: Measurements of Neutron Star Radii and Equation of State

Reference 18

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:44.972295Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:44.972295Z digest=sha256:90a889bee78a32af5e56d08a9bd0a814d9a4642d9e8616bdd85d3a0f80f78e89

Observation 14c69457-7939-4e94-b02e-dfecb1240f84 · outbound

This paper cites Thermodynamics conditions of matter in neutron star mergers.

Rotating neutron stars with non-barotropic thermal profile Thermodynamics conditions of matter in neutron star mergers

Reference 19

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no resolver link, observed 2026-08-14T10:30:44.976404Z

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Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:44.976404Z digest=sha256:fcaf3e3fd00829be11ed59937933cedb89f33305ed2c2ba029903d52c9bda5ff

Observation 8eb30560-2448-401e-a304-5d4388291ffc · outbound

This paper cites Core-collapse supernova explosions triggered by a quark-hadron phase transition during the early post-bounce phase.

Rotating neutron stars with non-barotropic thermal profile Core-collapse supernova explosions triggered by a quark-hadron phase transition during the early post-bounce phase

Reference 20

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no resolver link, observed 2026-08-14T10:30:44.980232Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:44.980232Z digest=sha256:9caeee620a865386e8126794000654314c62ac9c3c33408208806e1306a991f1

Observation 9ea5f1f4-2e4c-4732-bf8f-8bce0a8f1411 · outbound

This paper cites Punturo et al., Class.

Rotating neutron stars with non-barotropic thermal profile Punturo et al., Class

Reference 21

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unresolved
no resolver link, observed 2026-08-14T10:30:44.984139Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:44.984139Z digest=sha256:ef19f452cc1025e08ed5f5acb9dd4404d9a51ecc85ede4bf4dcd488007c80597

Observation 3a8d4ca7-e2f6-4c1b-bba1-1d877743ed06 · outbound

This paper cites an unresolved cited work.

Rotating neutron stars with non-barotropic thermal profile Unresolved cited work

Reference 22

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:44.987196Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:44.987196Z digest=sha256:a743495b81751028b18858ba8cca77e3246d91a878eb544a719c3efc0737b582

Observation 642bb8fe-dce6-4ae6-a4e8-705d7db07688 · outbound

This paper cites GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral.

Rotating neutron stars with non-barotropic thermal profile GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral

Reference 23

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:44.990546Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:44.990546Z digest=sha256:c3cf860c69940a36a7d51797df4e35ee2257b78fd0179a12aeb9f871379c07f4

Observation 3405f6d0-b347-40dc-a495-d00ec9117705 · outbound

This paper cites Multi-messenger Observations of a Binary Neutron Star Merger.

Rotating neutron stars with non-barotropic thermal profile Multi-messenger Observations of a Binary Neutron Star Merger

Reference 24

Resolution
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no resolver link, observed 2026-08-14T10:30:44.994149Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:44.994149Z digest=sha256:412f25caffcea42691a7d6820d804acc4ae99ae0fef0909b7d022e221984657e

Observation c256200c-4f4d-41b6-ab87-c85f7bfcda6a · outbound

This paper cites Swope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source.

Rotating neutron stars with non-barotropic thermal profile Swope Supernova Survey 2017a (SSS17a), the Optical Counterpart to a Gravitational Wave Source

Reference 25

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:44.997608Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:44.997608Z digest=sha256:e9cc0b4b8ce0ce04dce6577f1216a8c2d4716f8c0a6fb3a5e5946e9e0f6e06ac

Observation 5551ecf6-27fd-4e4f-86d2-869d586a2086 · outbound

This paper cites Burrows, Astrophys.

Rotating neutron stars with non-barotropic thermal profile Burrows, Astrophys

Reference 26

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T10:30:46.226522Z

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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Observation 132498b2-8708-4b88-93d8-fa73454efcc1 · outbound

This paper cites Bonazzola, E.

Rotating neutron stars with non-barotropic thermal profile Bonazzola, E

Reference 27

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T10:30:46.216107Z

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.

source=pdf_text observed=2026-08-14T10:30:45.004902Z digest=sha256:1e4c96227811894e14735244923792efabca08fcf919f1618cd6f582afabdea6

Observation 27b83a46-5cc0-4d2e-b30a-6a4abda491e2 · outbound

This paper cites Rapid uniform rotation of protoneutron stars.

Rotating neutron stars with non-barotropic thermal profile Rapid uniform rotation of protoneutron stars

Reference 28

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.008379Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.008379Z digest=sha256:3a012f9521410399eda3561f86ce245001b8d11de3d09b4a7653738ceef720a5

Observation fb683243-1a72-44e6-baea-dc1bd8913bf5 · outbound

This paper cites GRMHD in axisymmetric dynamical spacetimes: the X-ECHO code.

Rotating neutron stars with non-barotropic thermal profile GRMHD in axisymmetric dynamical spacetimes: the X-ECHO code

Reference 29

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.012212Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.012212Z digest=sha256:d5798fadfdd963abcc739a7774b2d35f36a00c2d7f66d014b97a81f7a2f84a55

Observation 71281088-bbba-4557-86ea-2629d7f4d2fd · outbound

This paper cites Axisymmetric equilibrium models for magnetized neutron stars in General Relativity under the Conformally Flat Condition.

Rotating neutron stars with non-barotropic thermal profile Axisymmetric equilibrium models for magnetized neutron stars in General Relativity under the Conformally Flat Condition

Reference 30

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.015921Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.015921Z digest=sha256:c4f130f06383dc1b8126cbd30a9d84b1ae1b7008623370e81f6258dbab7bcbb9

Observation 56264f38-8cf9-4775-bdb3-214c2792e2a1 · outbound

This paper cites Disk formation in the collapse of supramassive neutron stars.

Rotating neutron stars with non-barotropic thermal profile Disk formation in the collapse of supramassive neutron stars

Reference 31

Resolution
verified exact
local_arxiv, observed 2026-08-14T10:30:45.862980Z

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.

source=pdf_text observed=2026-08-14T10:30:45.019516Z digest=sha256:55d27c5b3fdf2a8399528e72d6bc2b497909497a1224e58e1b746825449e225a

Observation 968f5b6f-1147-4eb5-a501-59fcea34758e · outbound

This paper cites an unresolved cited work.

Rotating neutron stars with non-barotropic thermal profile Unresolved cited work

Reference 32

Resolution
unresolved
raw_fallback, observed 2026-08-14T10:30:46.206119Z

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.

source=pdf_text observed=2026-08-14T10:30:45.023217Z digest=sha256:1093b385b9dd1c83cd06d3d33484d28bbb28b89313ef216ec4aab10ba6990410

Observation d121dd7d-2212-45b5-af56-9b1f4f57c9e3 · outbound

This paper cites an unresolved cited work.

Rotating neutron stars with non-barotropic thermal profile Unresolved cited work

Reference 33

Resolution
unresolved
raw_fallback, observed 2026-08-14T10:30:46.195942Z

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.

source=pdf_text observed=2026-08-14T10:30:45.026577Z digest=sha256:6338f6e0035710bcb72ab8a072d940fef5b354a901f75a2769a0e1270cdd0201

Observation 72038974-e73f-48e9-8f1b-d963371e4f68 · outbound

This paper cites an unresolved cited work.

Rotating neutron stars with non-barotropic thermal profile Unresolved cited work

Reference 34

Resolution
unresolved
raw_fallback, observed 2026-08-14T10:30:46.186030Z

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.

source=pdf_text observed=2026-08-14T10:30:45.030245Z digest=sha256:e2470e1d6b49c240cd587c40dd96b02f2373e01e8b9e903e23dae519fee80398

Observation 3190285c-5a09-4b08-abfd-d29bae22267f · outbound

This paper cites an unresolved cited work.

Rotating neutron stars with non-barotropic thermal profile Unresolved cited work

Reference 35

Resolution
unresolved
raw_fallback, observed 2026-08-14T10:30:46.176089Z

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.

source=pdf_text observed=2026-08-14T10:30:45.033668Z digest=sha256:60c7d17e26244cc0dc063ebaa8c7b55fa2f49148e5c1d91bacf76708123e72a2

Observation 43c2bb56-f257-49ae-a919-2ae25afd85b9 · outbound

This paper cites Uryu and Y.

Rotating neutron stars with non-barotropic thermal profile Uryu and Y

Reference 36

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T10:30:46.166160Z

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.

source=pdf_text observed=2026-08-14T10:30:45.036968Z digest=sha256:a0e4acc81f05d8006121122e994fc64cda7537f6a79672722db63a26f68487bb

Observation 000fb4c2-c9d7-4479-9dc0-7fb9773f1d18 · outbound

This paper cites an unresolved cited work.

Rotating neutron stars with non-barotropic thermal profile Unresolved cited work

Reference 37

Resolution
unresolved
raw_fallback, observed 2026-08-14T10:30:46.154960Z

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.

source=pdf_text observed=2026-08-14T10:30:45.040325Z digest=sha256:3018eab1ed1890140c989cad9a8cba983888a81a0bf6a8122547fbe157309f83

Observation 0134004a-3a63-4b5f-a54b-a6c4ec8ac0fb · outbound

This paper cites Espinosa Lara and M.

Rotating neutron stars with non-barotropic thermal profile Espinosa Lara and M

Reference 38

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T10:30:46.144186Z

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.

source=pdf_text observed=2026-08-14T10:30:45.043846Z digest=sha256:2f0dae8da46b8218f093e75a575a2abcbb1e8d91630be62130063803b9e9eecb

Observation c5a9b6e4-92ef-4fe3-9bfe-935a690ce3cd · outbound

This paper cites Self-consistent 2D models of fast rotating early-type star.

Rotating neutron stars with non-barotropic thermal profile Self-consistent 2D models of fast rotating early-type star

Reference 39

Resolution
verified exact
local_arxiv, observed 2026-08-14T10:30:45.848779Z

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.

source=pdf_text observed=2026-08-14T10:30:45.047172Z digest=sha256:d0654ca0223a6664d0dbb293aa1b4ed4f8e8c3ff20c79da8cf26d056e88fcc69

Observation 324873a3-bd0d-4fbe-be21-2df75bd51b61 · outbound

This paper cites A Novel Formulation by Lagrangian Variational Principle for Rotational Equilibria: Toward Multi-Dimensional Stellar Evolutions.

Rotating neutron stars with non-barotropic thermal profile A Novel Formulation by Lagrangian Variational Principle for Rotational Equilibria: Toward Multi-Dimensional Stellar Evolutions

Reference 40

Resolution
verified exact
local_arxiv, observed 2026-08-14T10:30:45.834995Z

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.

source=pdf_text observed=2026-08-14T10:30:45.050621Z digest=sha256:2df9bd9cc526503928a8c4eaf566890cc27660bfe6279c7e6ebb75667db35dd2

Observation 00676bac-d21d-428b-b92a-784f4a0dd034 · outbound

This paper cites A versatile numerical method for obtaining structures of rapidly rotating baroclinic stars: self-consistent and systematic solutions with shellular-type rotation.

Rotating neutron stars with non-barotropic thermal profile A versatile numerical method for obtaining structures of rapidly rotating baroclinic stars: self-consistent and systematic solutions with shellular-type rotation

Reference 41

Resolution
verified exact
local_arxiv, observed 2026-08-14T10:30:45.820730Z

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.

source=pdf_text observed=2026-08-14T10:30:45.053829Z digest=sha256:b091473628f11b2cad317c348152f650c18db7b8c7e493495f445a333dbf31a5

Observation 5ea8bb21-b324-42fb-a77c-26ea8f90091f · outbound

This paper cites Amendt, A.

Rotating neutron stars with non-barotropic thermal profile Amendt, A

Reference 42

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T10:30:46.134064Z

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.

source=pdf_text observed=2026-08-14T10:30:45.057397Z digest=sha256:ccb68d9185b48c4fad9b62197108961feaac1b1e9d07bd60bf5fa39f39ecdfc5

Observation f5765c82-eb1a-411a-b0bf-6153a36a3ecb · outbound

This paper cites Analytic construction of baroclinic tori by non-linear summation.

Rotating neutron stars with non-barotropic thermal profile Analytic construction of baroclinic tori by non-linear summation

Reference 43

Resolution
verified exact
local_arxiv, observed 2026-08-14T10:30:45.806036Z

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.

source=pdf_text observed=2026-08-14T10:30:45.060605Z digest=sha256:5c584ace9ae318758f6ea7f0130d2f0c16fc32506455a2343779a2643ac3c41c

Observation 7251dd1f-d100-487e-86dc-7e756d9dedaf · outbound

This paper cites an unresolved cited work.

Rotating neutron stars with non-barotropic thermal profile Unresolved cited work

Reference 44

Resolution
unresolved
raw_fallback, observed 2026-08-14T10:30:46.122637Z

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.

source=pdf_text observed=2026-08-14T10:30:45.064301Z digest=sha256:1731df95936c4ad21c818302ff61b5c8daeb4c57b7cd7d7953ac4da241319664

Observation 3f66aa9f-bca3-4ce1-972e-c8edca2b17cd · outbound

This paper cites Stergioulas, Living Reviews in Relativity 6, 3 (2003), ISSN 1433-8351, URL https://doi.org/10.

Rotating neutron stars with non-barotropic thermal profile Stergioulas, Living Reviews in Relativity 6, 3 (2003), ISSN 1433-8351, URL https://doi.org/10

Reference 45

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T10:30:46.111685Z

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.

source=pdf_text observed=2026-08-14T10:30:45.068042Z digest=sha256:9502bc7b8db50cd66f6616568f2f477adb3522a7e140f18c34075a656fa26794

Observation 0b3b869a-1e61-4d28-8ea7-aee6a2c025dd · outbound

This paper cites Komatsu, Y.

Rotating neutron stars with non-barotropic thermal profile Komatsu, Y

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.071493Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.071493Z digest=sha256:2626dc0bef478c4aee4ca7f3685521925f54ca316442c28b8a4a7850c43b2d5a

Observation 82021f0b-21ad-4780-8031-927d700893a4 · outbound

This paper cites Modeling differential rotations of compact stars in equilibriums.

Rotating neutron stars with non-barotropic thermal profile Modeling differential rotations of compact stars in equilibriums

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.074876Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.074876Z digest=sha256:c4481112f89cef444f2efc4a6daeaf1f6f647f7bc05ce6541ffd65e7719874ab

Observation 6813f9b2-6976-4f30-adbf-e648e0c8f74b · outbound

This paper cites Witzany and P.

Rotating neutron stars with non-barotropic thermal profile Witzany and P

Reference 48

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T10:30:46.094616Z

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.

source=pdf_text observed=2026-08-14T10:30:45.078373Z digest=sha256:2f43121eb736d4e95aeec7584dc823b5bc47d6d6484827f3d77bc26c23f88b43

Observation 6864e208-7b1e-47d9-b4e2-3baaff97b07d · outbound

This paper cites Villain, J.

Rotating neutron stars with non-barotropic thermal profile Villain, J

Reference 49

Resolution
verified exact
raw_fallback, observed 2026-08-14T10:30:45.780797Z

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.

source=pdf_text observed=2026-08-14T10:30:45.081694Z digest=sha256:7b39cdae00a8cd54c077b845819aa9a94cb878570d7d4dfb206f48e7adfa94c5

Observation 875b2437-7c4e-417f-98a5-cbbbcece5052 · outbound

This paper cites Improved constrained scheme for the Einstein equations: An approach to the uniqueness issue.

Rotating neutron stars with non-barotropic thermal profile Improved constrained scheme for the Einstein equations: An approach to the uniqueness issue

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.085451Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.085451Z digest=sha256:fb65bebc668aa78ba2b8743876dd57a78e729910f4c17e0f286b25fd114c8ea2

Observation 7f57ebd2-79ad-457e-9422-e5dc435cdadf · outbound

This paper cites An introduction to the theory of rotating relativistic stars.

Rotating neutron stars with non-barotropic thermal profile An introduction to the theory of rotating relativistic stars

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.089039Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.089039Z digest=sha256:e8864882a3ba2276c3d583d33ee9d0295512b21a49a29a2bcdf33cc20e9b52da

Observation 975e878d-c6f1-47ae-9009-19b4db048cd6 · outbound

This paper cites On the accuracy of the IWM-CFC approximation in differentially rotating relativistic stars.

Rotating neutron stars with non-barotropic thermal profile On the accuracy of the IWM-CFC approximation in differentially rotating relativistic stars

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.092726Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.092726Z digest=sha256:c8fcb95d6890cc5da0fd7b95f6ec5514aa4182803cab6375c376cbf5c8437f25

Observation 7f67dc93-caac-4f69-a388-e4d4496cd6ce · outbound

This paper cites Comparing Models of Rapidly Rotating Relativistic Stars Constructed by Two Numerical Methods.

Rotating neutron stars with non-barotropic thermal profile Comparing Models of Rapidly Rotating Relativistic Stars Constructed by Two Numerical Methods

Reference 53

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.096445Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.096445Z digest=sha256:2d1c9f0e34bf7c7da527fa8a0805d4399a9c106ad59df541b8a18970292f7d34

Observation b8d83319-4d57-4f58-b12b-bf8759c6c0cb · outbound

This paper cites Numerical simulation of orbiting black holes.

Rotating neutron stars with non-barotropic thermal profile Numerical simulation of orbiting black holes

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.100259Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.100259Z digest=sha256:7390e754f4947d72c41f4244fe7b12789a728e21632f7511f1c4f9eea2079ccd

Observation 31e14b21-645b-43d7-aa54-054057b78680 · outbound

This paper cites Br¨ ugmann, J.

Rotating neutron stars with non-barotropic thermal profile Br¨ ugmann, J

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.104103Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.104103Z digest=sha256:50a0dd0126e0ecb99d6fc5ec7047cfa80f2fc56c0f6c58860aaf700ca3da27e9

Observation 3a6b5ee4-8827-48d2-9114-454ada80d986 · outbound

This paper cites Numerical relativity simulations of binary neutron stars.

Rotating neutron stars with non-barotropic thermal profile Numerical relativity simulations of binary neutron stars

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.107746Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.107746Z digest=sha256:6182b59f8ae093b9d528e1bbc3a5455247b670695f99763ce1258dfcb1062286

Observation a4ed2abf-1f86-4431-8c71-75a2f04963ff · outbound

This paper cites Numerical relativity simulations of neutron star merger remnants using conservative mesh refinement.

Rotating neutron stars with non-barotropic thermal profile Numerical relativity simulations of neutron star merger remnants using conservative mesh refinement

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.111585Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.111585Z digest=sha256:86542652b4e091fe2d29ae30811eec4836bf4f1e2dcd48d60c759d5aab7b0599

Observation b1b8e46e-baa4-43c7-b3ea-6e04d26212f3 · outbound

This paper cites Gravitational waveforms from binary neutron star mergers with high-order WENO schemes in numerical relativity.

Rotating neutron stars with non-barotropic thermal profile Gravitational waveforms from binary neutron star mergers with high-order WENO schemes in numerical relativity

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.115845Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.115845Z digest=sha256:bbcbf1d884ee2836e72e91cf92d286606bc85b2868236867c52ba5abb2576ef2

Observation 1a3b2abd-8476-4922-8f72-3bde5047a0d1 · outbound

This paper cites Full 3D Numerical Relativity Simulations of Neutron Star -- Boson Star Collisions with BAM.

Rotating neutron stars with non-barotropic thermal profile Full 3D Numerical Relativity Simulations of Neutron Star -- Boson Star Collisions with BAM

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.119466Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.119466Z digest=sha256:c76292c362d1f301de93b72e69bf367a91b23dddd90cf9cdc78b99eb45268099

Observation 27a6a7d1-ccd2-418d-ad98-f892bd0b6c53 · outbound

This paper cites Constraint violation in free evolution schemes: comparing BSSNOK with a conformal decomposition of Z4.

Rotating neutron stars with non-barotropic thermal profile Constraint violation in free evolution schemes: comparing BSSNOK with a conformal decomposition of Z4

Reference 60

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.122955Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.122955Z digest=sha256:8b57ed40463b00dd5abda9aed9295f93af9114cf8ed9482aa1ce47760c4371f9

Observation b784072d-528c-460a-b61d-2d6f88f6e516 · outbound

This paper cites Constraint damping for the Z4c formulation of general relativity.

Rotating neutron stars with non-barotropic thermal profile Constraint damping for the Z4c formulation of general relativity

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.126580Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.126580Z digest=sha256:0b1d012ecc604c9da011a16e9eed60c6914c4e1fba369f20ebbbf7d9c64e31d5

Observation 48820c0d-fdb1-486a-926f-47907d886635 · outbound

This paper cites Compact binary evolutions with the Z4c formulation.

Rotating neutron stars with non-barotropic thermal profile Compact binary evolutions with the Z4c formulation

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.130453Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.130453Z digest=sha256:c131c506a5a0498540de7558791f7c4bb900179e74ac106c84be10757714c545

Observation 368d7803-4d3f-4317-9b80-a61ac3c64ad9 · outbound

This paper cites Borges, M.

Rotating neutron stars with non-barotropic thermal profile Borges, M

Reference 63

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.134273Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.134273Z digest=sha256:06ed02db0e8c862f0c9ebec7c22ee1102bd079437804c1b156a7917bc4afd5d5

Observation d28d7580-d89e-4c23-991f-c3299e6e3e31 · outbound

This paper cites Accuracy of numerical relativity waveforms from binary neutron star mergers and their comparison with post-Newtonian waveforms.

Rotating neutron stars with non-barotropic thermal profile Accuracy of numerical relativity waveforms from binary neutron star mergers and their comparison with post-Newtonian waveforms

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.137929Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.137929Z digest=sha256:d180e6efee751b5f6d055112017428247289e523be4cc601c140c71dd4b6a2a3

Observation b88f1592-33d3-4ae9-83c3-c9a3c7a31c36 · outbound

This paper cites High-resolution numerical relativity simulations of spinning binary neutron star mergers.

Rotating neutron stars with non-barotropic thermal profile High-resolution numerical relativity simulations of spinning binary neutron star mergers

Reference 65

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.141690Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.141690Z digest=sha256:6f7f71b325746bf076a26aa713807a1baade84de3fbbe6883dddf242724d0139

Observation 76506d96-1c33-458e-8b5c-138a7dd5cfe8 · outbound

This paper cites CoRe database of binary neutron star merger waveforms and its application in waveform development.

Rotating neutron stars with non-barotropic thermal profile CoRe database of binary neutron star merger waveforms and its application in waveform development

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.145383Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.145383Z digest=sha256:3b80a3fea25dc3c263ab796b1460b07eb0c9d32096c109edd43bb2e4272b4d6f

Observation 844b8dc8-53e3-48dc-8bcb-29b817faae97 · outbound

This paper cites Improving the NRTidal model for binary neutron star systems.

Rotating neutron stars with non-barotropic thermal profile Improving the NRTidal model for binary neutron star systems

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.148836Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.148836Z digest=sha256:976b5c16fffbe7d477b6d8dba63062a6d7111109b399e625f14eb3b578b80f00

Observation be452ef9-9cb2-4390-b85c-c6983f8dccdb · outbound

This paper cites Sub-radian-accuracy gravitational waveforms of coalescing binary neutron stars in numerical relativity.

Rotating neutron stars with non-barotropic thermal profile Sub-radian-accuracy gravitational waveforms of coalescing binary neutron stars in numerical relativity

Reference 68

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.152433Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.152433Z digest=sha256:0e0ea3ef1e5cfaf0e42babac55994d8658713f66c34c0a453b3c9d13a5af8de9

Observation a7c9ea48-2600-46c5-b16d-4d95423a4c37 · outbound

This paper cites Entropy-limited hydrodynamics: a novel approach to relativistic hydrodynamics.

Rotating neutron stars with non-barotropic thermal profile Entropy-limited hydrodynamics: a novel approach to relativistic hydrodynamics

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.155985Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.155985Z digest=sha256:998386e15cd86db06aa8f6b8d678db322666abc0968559e690b9ee570af4f359

Observation 39b019a6-7aec-4867-93fc-cb584c4b6c2e · outbound

This paper cites Stationary, Axisymmetric Neutron Stars with Meridional Circulation in General Relativity.

Rotating neutron stars with non-barotropic thermal profile Stationary, Axisymmetric Neutron Stars with Meridional Circulation in General Relativity

Reference 70

Resolution
verified exact
local_arxiv, observed 2026-08-14T10:30:45.493851Z

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.

source=pdf_text observed=2026-08-14T10:30:45.159506Z digest=sha256:0176fbf18290ff6600ca91cf74b8a60499e4e5cd12eccd2555d7bb9d07ed964a

Observation 314eb06b-0848-459d-9376-68754acf4860 · outbound

This paper cites an unresolved cited work.

Rotating neutron stars with non-barotropic thermal profile Unresolved cited work

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.163367Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.163367Z digest=sha256:e911cd15d8a748937a167ee7361bd903a8514c2fb518951097cc789c2e352e71

Observation 0d813f76-4437-4b50-9dcd-917cef2fa97f · outbound

This paper cites an unresolved cited work.

Rotating neutron stars with non-barotropic thermal profile Unresolved cited work

Reference 72

Resolution
unresolved
raw_fallback, observed 2026-08-14T10:30:46.078204Z

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.

source=pdf_text observed=2026-08-14T10:30:45.167178Z digest=sha256:bfda9bdd893ea1792a942c8e22a57139843c68dd7a702aa35c95f793898ffe23

Observation 48e31f26-9c42-4ea5-be19-b7cf84bb95b7 · outbound

This paper cites Burrows and J.

Rotating neutron stars with non-barotropic thermal profile Burrows and J

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.170988Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.170988Z digest=sha256:302c78c363e3abeea4e674d2d64663f919f7a274e68d795f3632d293c82b0455

Observation b4f0ed72-1abb-4f82-a8ce-9c1273e44a9b · outbound

This paper cites Keil and H.

Rotating neutron stars with non-barotropic thermal profile Keil and H

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.174871Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.174871Z digest=sha256:0fd4c9edc1fa11cf159fe97da6d1b01d85d95bbb523f7c20fdf5d1af0b020abe

Observation b1af2844-7eb9-4b84-96cf-78165798f19c · outbound

This paper cites an unresolved cited work.

Rotating neutron stars with non-barotropic thermal profile Unresolved cited work

Reference 75

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.178650Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.178650Z digest=sha256:354f84f042e85ccf5758493f458481302d8980d35f7200698f015ce221492e3e

Observation b570b36a-a7da-48b7-b4fe-826213b13dc5 · outbound

This paper cites an unresolved cited work.

Rotating neutron stars with non-barotropic thermal profile Unresolved cited work

Reference 76

Resolution
malformed identifier
raw_fallback, observed 2026-08-14T10:30:46.054721Z

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.

source=pdf_text observed=2026-08-14T10:30:45.182219Z digest=sha256:bb06b8485a9ba46789ce9671f6427d3d1675e7f19c1eed8d27cbe9c11f78cf88

Observation 78305be9-74f6-4e26-86df-a0293187914e · outbound

This paper cites Spin evolution of a proto-neutron star.

Rotating neutron stars with non-barotropic thermal profile Spin evolution of a proto-neutron star

Reference 77

Resolution
verified exact
local_arxiv, observed 2026-08-14T10:30:45.421004Z

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.

source=pdf_text observed=2026-08-14T10:30:45.185882Z digest=sha256:83201a2b75423d62545497e75f998f8fccd9c2513bc78c5eb54b51742598d3ff

Observation b0714e12-f1e7-4f4d-9822-5566a6b894c0 · outbound

This paper cites Ferrari, G.

Rotating neutron stars with non-barotropic thermal profile Ferrari, G

Reference 78

Resolution
verified exact
arxiv_id_nonexistent, observed 2026-08-14T10:30:45.404655Z

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.

source=pdf_text observed=2026-08-14T10:30:45.189640Z digest=sha256:bc7dc7fb598c818de9072d27cc155eeba34058e19675fa3d78249ed3f0da22b4

Observation 5fc21d87-e3e7-4934-9412-e26ec0bbdf2a · outbound

This paper cites Evolution of a proto-neutron star with a nuclear many-body equation of state: Neutrino luminosity and gravitational wave frequencies.

Rotating neutron stars with non-barotropic thermal profile Evolution of a proto-neutron star with a nuclear many-body equation of state: Neutrino luminosity and gravitational wave frequencies

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.192945Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.192945Z digest=sha256:5ec0ad0581b8838fff919262583884d579caa8d98e5e13409986b0fd345fc70d

Observation 48850e41-92e8-4bae-8c86-67c840195641 · outbound

This paper cites Chatterjee, T.

Rotating neutron stars with non-barotropic thermal profile Chatterjee, T

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.196827Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.196827Z digest=sha256:22ebacf492168f024ba01186fd051ab4314d37746e66f160b5048c8703496f88

Observation e20b609f-64c0-401e-8a31-6eeb84c5a0c5 · outbound

This paper cites Rosswog and M.

Rotating neutron stars with non-barotropic thermal profile Rosswog and M

Reference 81

Resolution
verified exact
raw_fallback, observed 2026-08-14T10:30:45.360108Z

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.

source=pdf_text observed=2026-08-14T10:30:45.200678Z digest=sha256:ab8c41bc3fdbb0646e9e115a8cd983a7a045355d37db361f0ee7c0613a604da2

Observation ed22a475-a397-4c26-8a2d-db954b0f33ce · outbound

This paper cites Bauswein, H.-T.

Rotating neutron stars with non-barotropic thermal profile Bauswein, H.-T

Reference 82

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.204388Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.204388Z digest=sha256:b9d595f4ae1c8b17423b2cb6106ec23d9dc8bc50e96ac59f4adae77e34af8cc4

Observation db76c4a1-a4bd-44ea-8d02-9e7ad79b88e0 · outbound

This paper cites Equation of state effects in core-collapse supernovae.

Rotating neutron stars with non-barotropic thermal profile Equation of state effects in core-collapse supernovae

Reference 83

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.208015Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.208015Z digest=sha256:03525c006bcf8cb6f85a1a6aed45ab58fbce352966adb2d6f8df93f8966316c9

Observation 198cd6c3-d236-4798-abd4-0c7a0d4e717d · outbound

This paper cites an unresolved cited work.

Rotating neutron stars with non-barotropic thermal profile Unresolved cited work

Reference 84

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.211772Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.211772Z digest=sha256:37823b6ab9e88709ad93c2551cb47b6428771a02d2a1f8b6cb30c3b74cbc3fec

Observation 1fa08e41-9e77-46a3-a47f-9a26421f51fc · outbound

This paper cites De Pietri, A.

Rotating neutron stars with non-barotropic thermal profile De Pietri, A

Reference 85

Resolution
verified fuzzy
raw_fallback, observed 2026-08-14T10:30:46.037880Z

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.

source=pdf_text observed=2026-08-14T10:30:45.215508Z digest=sha256:d68b45b02e6e0847e2deb4ecd6aa9a24594c6791269193c0a181cb5e39450b13

Observation 45abae36-3911-493a-a11a-ee2e4844f7ef · outbound

This paper cites Numerical-relativity simulations of long-lived remnants of binary neutron star mergers.

Rotating neutron stars with non-barotropic thermal profile Numerical-relativity simulations of long-lived remnants of binary neutron star mergers

Reference 86

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:45.219142Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:45.219142Z digest=sha256:679ee3d94e70e23a74b41ae0e0aff635f4402a39dcf7bed11cfaa8e6b2423aef

Pith citing papers

Observation 7cd5b759-9ec1-410d-8597-d4d41eebeae7 · inbound

Hybrid Stars with Post-Merger Rotation Profiles cites this paper.

Hybrid Stars with Post-Merger Rotation Profiles Rotating neutron stars with non-barotropic thermal profile

Reference 16

Resolution
verified exact
arxiv_id, observed 2026-07-03T22:08:58.816648Z

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.

source=pdf_text observed=2026-06-26T23:50:12.361235Z digest=sha256:fce3815c4661b0f9a14997af46759a682e47cb08914c754397bbe2cf970eefea