Pith. sign in

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 2026-08-15T06:32:42.880941+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

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:44.913910Z digest=sha256:4f7e74816495e1e1c7e7384a7d231d1c56f192994ca883711e61e598fdca3d05

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

This paper cites barotropic.

Rotating neutron stars with non-barotropic thermal profile barotropic

Reference 2

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:44.908933Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:44.908933Z digest=sha256:ee8848d76ce9c7eff0fc666f1fbc98b89d3fb4c8edd39a606ffd8fd5d3fe3ba0

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

Resolution
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=sha256:3bed58438ac0ce94801e95d4f4a0da4a4c4c4a87a8ab43c7620abed14159f4ed

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

Resolution
parse uncertain
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:f633f97840da0a3e6e54cfe65a8a99dbae467b3acb705b1388337f459280d09c

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
unresolved
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=sha256:2e50286fd3f2c1131c193d611b05e39c5667d9f5a02fe2775afe10ad99020ba2

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

Resolution
unresolved
no resolver link, observed 2026-08-14T10:30:44.928613Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:44.928613Z digest=sha256:2fa8af8f29215aac6c3bc3703d8fa0dfb483fc564d422da72be33b7aca43c29f

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:44.932394Z digest=sha256:5e5e660a1c1beda05de1f77b90e1b5b146a30a4c8c8442790577093b8eacdbd2

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

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:44.935665Z digest=sha256:b20221e1e2a3d9c16285e54ba60a75f35b7969e1b69b536767b0d294dfbab7b2

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:44.938751Z digest=sha256:c60d4d8eebe3213b2838d57bae468daaa9209ca7359acb9aaf04e2d4f6fa59b1

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:44.942740Z digest=sha256:35e978d12fe9e6cf9b542e40fc97b9a93e4123ddf7f977e40feb6a5a58db2d0d

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:44.946008Z digest=sha256:e411a78797fc31da306134fa39bc36079ca117964b9cf93f6c28f0cdf0b3cd88

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:44.949062Z digest=sha256:5637f9db3fedc74d8e0f49ba5c5080562ccfdafb0c75c5a637bbdf33cf54b4e9

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:44.952627Z digest=sha256:8f6eddf12c600dc8698335939333de19a5df3b3fb14cd62497b3162924e7c18d

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:44.955960Z digest=sha256:df91f7638d333fe2258374b36981bf8077925b8006a915e489623301b54f0799

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:44.959197Z digest=sha256:7c5915194b156d361c32430cbbd605e88468fd2614665027b627fbea4b54fbe1

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:ebdd98b210dc4a53a8b1ef54a9a546f3ee82a3090e91485fdfde7cdf5cc4054c

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:e5aabd72cc481ecf5013c5857ceebed0d53e0b63ef1b2ce471e4ad90581bba5d

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:bf9b27137f84ef9d49c39c2e2aaf9d4845402cba598e389bbd57dfe178fc9cb7

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

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T10:30:44.976404Z digest=sha256:49fe222fa44677f88ceb7a3bc097436db778de3a5c62e6299943638f3cd6d569

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

Resolution
unresolved
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=sha256:971e401a50b11844eddc1dd5adc7ea507836c257343f827f111e9a776d0031f8

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

Resolution
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=sha256:956c04c80dfb81e3254611da61e726f47e556b3e124e785d33c4fc598545cd71

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=sha256:04ebf72f55c6a46039dd2cd4232fa016ca1291c0db9e3dc3be76c9ea869068b0

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=sha256:18cb35708ff0ebcc632abc66cb338bd11093d7fbf2fd152ebf6040d8f610e9a8

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
unresolved
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=sha256:8fdf9af1037d46d1150bd34b06a2f586e7686a6720f30af2206614ffd34d0e11

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=sha256:7b4e1d8351ec2312a3073463005dc1447020b39a090927972a4f302d7679cd26

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.001540Z digest=sha256:f58a8c1863a9eda7ea0e56fb905ecea46de484fc23766102b5e80b99ca6004f3

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.004902Z digest=sha256:13da3a925cdb085c5c03784c01dc345f1a6eb753fa1e7d5ce5e3433813db73fa

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=sha256:7565c1bc255d3708c17b1c1fcf4267e76377d0c2de4bae42fbfc5eeac91db024

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=sha256:5b534a7474c60c23bb5f751ea2200ddb31c7a5dd7e6e1b130c8e66812d003789

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=sha256:534a256f87fa4c776a0ae4f6acb37201da8bf393f7cec1fc485a65a592887581

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.019516Z digest=sha256:ced28a14b928f86b8e3769d11ce98ad586f591f4143314a3a9ca66c7711a8a03

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.023217Z digest=sha256:9f104c7c3f51c5a50920c7a0ebf6d2b2c0b9bd5b66a8cb0ba1e097d077fed5b4

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.026577Z digest=sha256:40667ad2cc6a1e4e130ca2c2921a8191fbe0545998690fb0a216cd9a0872f4a5

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.030245Z digest=sha256:9022fa5f1475d1f1a40c9c532732b5b24a628502927912d11ac50543f8a6cc2b

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.033668Z digest=sha256:c38eb739d0275ad41cbe47ce18d663aa08f358a7757c59d17ef5188ce76e2ed6

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.036968Z digest=sha256:5c993ba60c43c2eff890791be6ed619f53f2e4eea8f29e4e4032a42d4238c7f2

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.040325Z digest=sha256:80e411f9a6c291b373bf896ba3865c454445fbf7cdcdaef0cb69e37a2489ec9b

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.043846Z digest=sha256:133ce69184a9fb05fded0eed04f7830f54842fa24b42a1afc36abd5646b263f3

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.047172Z digest=sha256:00326b253dd742384a3e706d35688943e2c09bf90ba4d2f403637456736ffd12

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.050621Z digest=sha256:13c1cc5acaa83e4deecbd6c195822291c6908748bd90cbd944e316508657c3e5

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.053829Z digest=sha256:07752a2e8b4ada814196242eaa85533c03eb2bb4e01ccf9b5b1d79f992e20195

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.057397Z digest=sha256:65246243a888fa183caf89320b2658d2bc404de04c4cd01ca6dc305cc3e08c8e

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.060605Z digest=sha256:e834fb53f1dff2a5b23e8cefef8b50ed5307c01f1e0cad77c563773578eec194

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.064301Z digest=sha256:3bc142366df5bfd72911fec44290f5fc2c3b2bb8357868ef24b398c91c197d6e

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.068042Z digest=sha256:02e9a7daca9add0173b8e1ff60d571de1a676cfa828b6dd79e1f02a0309c21b7

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:fa4417b22bf44c302f5d8c4d8586e45373b14c8e1548bcba904df032e3b93303

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=sha256:68316c95bd9c132c357f22b239e96fbf080c0002621483e3d414be09365b30bf

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.078373Z digest=sha256:02d426380426d72b77651bec092fa10b9049e6c9077a6692987f55d3e90b9732

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.081694Z digest=sha256:f65008845eb80824f9390f8c83e0e5041a03cec181f3ec703d826ce728662ff0

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=sha256:763af09d74b91f257e46d167153462c87e616a606988ad79b1da1a9d95ca7510

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=sha256:011f7d32b8094785af4e801f3eb254321a033201b0356b4fba64bfe6d6100550

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:c9e230c590077faebc7344a1e02e42b83690e1331061e4a40cc98a1bc4847205

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:ee3c0cb636be15de43ff926c4414e5b80a4e7899a4d9b53d0815832fe806d2a1

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=sha256:40c0ecdcea1ce418d7880662e8eed8beab6589860271f3917da789ac4f81920d

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=sha256:7f2706ea0d54ede10c48e3eed6d4f35c6232e8701b4b3b20a28077dae4e41f3d

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=sha256:05a7f2a85cda9363b17e8d05a3cc60256c863975acd0fdd9845e5c146ddd7cad

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:b3f69e984aab8f919d3b3e34a574373da80d198cdf5067b6015a487bc8657c19

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:c064f6177843d7f31f0f3ca21dacc8175a6ea8725d374b0beb7a1a2c24266971

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:aee6d73d5bbce8d0f98b2d33ac03992f79e346b57db574b6fab08a35a524e44c

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=sha256:3cde5db608f5aecfcf0c7cc505e7fde5b3cd7feb5de1ad0fe2b578c467a06e1b

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=sha256:71defdf1a60bcc29fea18d1da59bc37da6cc64b058244677f222ed34f0f04e87

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=sha256:6c631e948ab12ce6ee0ec553911211b28085dc75e3af3fbf37972329156afbbb

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:d0bda4a69d3709d257c6f4359081f2418b82b56a48be23dc355eecb674f5bf9a

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:a11088faa0451795c537778c7e93ef61a9dbd9e04d0410ebf0d0eb3604a0862f

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:bf4e83b99b0c3a2b8203ffaf7ea6d9ab340b0fb0ee4100f9d62df908b5078613

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:fd6680aa9f4beb45131536b50af0c154f9bec66c0810909d4a7c89789ae3a560

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:ba82580bacb70b7aa99e1220fedca67555d10e93e3aa0332b8ebb1f53da60efc

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:f0ec79f3e83cac1418c8cfd4933626f24ab30bb141f2e82663d00a43e6d01813

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:bf56ef638f845b185f6978d1e544af9536740eb144e2d70bac9e6a17bbc67f29

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.159506Z digest=sha256:a70881f09a59d76c42ab502a2b9d7806184574ae72b223e67d78030af3ea26f7

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=sha256:1a01d9562bf5c165b25476af17c225246cd0f96d58cbe03eb4397f8cceb88393

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.167178Z digest=sha256:a891bbc5790783d91e08babd763e21d5ca1b13dae130a96c1a343fbf5aa96b43

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:d9b123d3a9fbe40644aea4b30e11f73e28e255fc31782bde9d5f896df717639b

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=sha256:86d9a07f657ac6ffe8e0d8acde3be4455df98147d782f948844f69e03a4af812

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:a3b1b7f1afbab167f89ed96c593544234e0fb94077cc730b1a25685a4a5a6308

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.182219Z digest=sha256:1d08366c86cee580014fdbc5a1d7ca2b505765539c0d66681c071e4487eb9178

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.185882Z digest=sha256:8676a189146f4847f264353472bc748868977dd91be52317b2b098c95c7a2368

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.189640Z digest=sha256:01dfb13f040dadaba63f87e685b04225e695eaf89a3b8810215874d06b1b7cb3

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:faa90ad4e2326de65cd66c8946b3ebcdf1840f8893f7784caf5d2a091d477fc8

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=sha256:0b52609b2013306e366e17b131762952a4080ce7b8ac430e81ba94ef0557c990

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.200678Z digest=sha256:529a9bfd7993f11f44abe6a116351a93d390690ad91e222b3a78e1d812fc931f

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:e01b7ffa74abf7e6cfdf209abc4d1eaa8d5c694718ff59106d1ba0d5e65552e0

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=sha256:7a5f2703ad8a04028536b5b27414cf39347a03a8e4bb14081a4f49ee842e24f3

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:b53642db8262fbc9d78ba7f17b617a7424b06a5210865664b366c8ffd2dd765b

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-08-14T10:30:45.215508Z digest=sha256:f595d258fc433ff981a7e5deb8a08a4f5179591075e15a0090df86b404606659

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=sha256:47c1f23282eb4ccd618d058f615c003d8bf372038d8104d1697662227035ea4f

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 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-06-26T23:50:12.361235Z digest=sha256:400dc06658f5ed6c639f0a28b1676034ba170d56c05044c27c2838aaaee31688