Pith. sign in

Paper Citation Record · LEDGER

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation

As of 18 August 2026, this Paper Citation Record lists 69 of 69 outbound references and 2 inbound Pith citation observations for arXiv:2505.19400.

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

pith.paper-citation-record.v1
2505.19400 v1

Coverage vector

measured 69 of 69 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links, observed 2026-08-07T14:21:15.040363Z

measured 71 of 71 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-18T06:34:40.430872+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T05:44:22.117557Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-06-29T20:33:58.096508Z

Reference resolution

69 of 69 outbound references displayed

  • verified exact10
  • verified fuzzy13
  • unresolved46
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

Observation 65ad0e5c-ab0a-44c2-a46f-e8cf66f6a151 · outbound

This paper cites an unresolved cited work.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Unresolved cited work

Reference 1

Resolution
unresolved
raw_fallback, observed 2026-08-07T14:21:19.110577Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:12.329461Z digest=sha256:d2dc9b1fd9314cefba932521f952f36f83d012326ca32d0078900d73639fead8

Observation 7695ae67-01d4-4db9-8213-b3464541b3c5 · outbound

This paper cites III B, the metric perturbations describing the mass monopole corrections of the star (ℓ = 0 and s being even) are described by the functions m(s) 0 , h(s) 0 , and ξ(s) 0.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation III B, the metric perturbations describing the mass monopole corrections of the star (ℓ = 0 and s being even) are described by the functions m(s) 0 , h(s) 0 , and ξ(s) 0

Reference 2

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T14:21:19.053255Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:12.441368Z digest=sha256:a7704e61011501ff19922331c9a38402f87790f67fa8917fe08c54825495d362

Observation ba5648ee-20d3-45b3-b535-c7ae989ad782 · outbound

This paper cites an unresolved cited work.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Unresolved cited work

Reference 3

Resolution
unresolved
raw_fallback, observed 2026-08-07T14:21:18.999127Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:12.579894Z digest=sha256:8bf62c65d40c63f8a1ee690ba08dc50ed6750c7b917d7f0f9d329083168b31c1

Observation 2be05ac4-cda6-43fa-8e6f-5add125a9f1f · outbound

This paper cites quark stars) The previously discussed matching procedure relied on imposing continuity at R = R∗.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation quark stars) The previously discussed matching procedure relied on imposing continuity at R = R∗

Reference 4

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T14:21:18.927315Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:12.610267Z digest=sha256:02227f036120bb82fb905893b0fb4c630fa946f3d8f6bf7d6152b47216444a2e

Observation d2f14fe7-3116-4eb0-8b25-4981342fdfce · outbound

This paper cites an unresolved cited work.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Unresolved cited work

Reference 5

Resolution
unresolved
raw_fallback, observed 2026-08-07T14:21:18.795269Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:12.695536Z digest=sha256:6a216e5f4f6049756aeb30ab015998d0c1b7e6e5b9ae1311c19009a62126d348

Observation 686987a9-982d-48f7-a619-d40c5247d98c · outbound

This paper cites LOFT: Large Observatory For X-ray Timing.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation LOFT: Large Observatory For X-ray Timing

Reference 6

Resolution
verified exact
local_arxiv, observed 2026-08-07T14:21:16.295074Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:12.698695Z digest=sha256:3c794ac61a57497d6c7e7396b8f9354aac76cfcb87ad9e23274f544210abe850

Observation 8b0371c1-dc09-41da-abde-7511b4cda474 · outbound

This paper cites LIGO: The Laser Interferometer Gravitational-Wave Observatory.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation LIGO: The Laser Interferometer Gravitational-Wave Observatory

Reference 7

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:12.702071Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:12.702071Z digest=sha256:3743b23076cf9b40014a1f4a3b0a00cd377fca63924413059551189ad9d6bf54

Observation 679955f5-1738-481a-b7ab-945a9a8745ff · outbound

This paper cites Advanced LIGO.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Advanced LIGO

Reference 8

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:12.730175Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:12.730175Z digest=sha256:061f3118d32634a66eb985ea364c0a927a1bc07c4e95a72dfe488f9d8ff46158

Observation e42656c2-c363-471d-bc14-af4a1d8a183b · outbound

This paper cites Accadia et al.(VIRGO), Virgo: a laser interferometer to detect gravitational waves, JINST 7, P03012.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Accadia et al.(VIRGO), Virgo: a laser interferometer to detect gravitational waves, JINST 7, P03012

Reference 9

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T14:21:18.736131Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:12.776363Z digest=sha256:627c0c3f3584f569f22d7cc8a1af341d3abd7a6a9f0ceb9d488db552a642a24b

Observation f5000c7a-9790-4346-884b-90c9f4c8b520 · outbound

This paper cites Interferometer design of the KAGRA gravitational wave detector.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Interferometer design of the KAGRA gravitational wave detector

Reference 10

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:12.857965Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:12.857965Z digest=sha256:71319c9c7ee083770d98b2e5c63574e007a5b9c819ec2c301d20370da2edf7b2

Observation 1866e445-1292-453c-a93a-b7aa3fc5bae3 · outbound

This paper cites Observation of Gravitational Waves from a Binary Black Hole Merger.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Observation of Gravitational Waves from a Binary Black Hole Merger

Reference 11

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:12.902834Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:12.902834Z digest=sha256:84dfd22618ec63328f58ef7fd579280e36d4fcb3e8ac0b7df039070557b88afd

Observation e4e962b8-7b00-4c7b-8903-b16d1a45a2f2 · outbound

This paper cites an unresolved cited work.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Unresolved cited work

Reference 12

Resolution
unresolved
raw_fallback, observed 2026-08-07T14:21:18.637553Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:12.937922Z digest=sha256:f49bd93a4a97d91a3b5cc4e5cd2d7c49606b1226c41035dc5a668a857062f45b

Observation b94d306a-08e2-4388-8e4d-c5055c4eacb3 · outbound

This paper cites an unresolved cited work.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Unresolved cited work

Reference 13

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:13.010654Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:13.010654Z digest=sha256:4d4c515336060d6755db9158830ae0b652669b57a584d1e65b045d51b9722edf

Observation 1d2411a0-8068-48eb-9286-f4fe61f26efd · outbound

This paper cites an unresolved cited work.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Unresolved cited work

Reference 14

Resolution
unresolved
raw_fallback, observed 2026-08-07T14:21:18.561697Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:13.076355Z digest=sha256:3b232684f8ec875bc72bf5021eb5fa36425374b31082c97ce50e1a15ee70ff2a

Observation 9672460b-a488-4408-b0f8-bc88a92e7cc0 · outbound

This paper cites an unresolved cited work.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Unresolved cited work

Reference 15

Resolution
unresolved
raw_fallback, observed 2026-08-07T14:21:18.523305Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:13.120305Z digest=sha256:557e97b508ba3dc71fb286d76046fff445b8db1532b5f1626cf654e35a0ac373

Observation 1638eb90-963f-49ed-8812-5a834c74ba72 · outbound

This paper cites an unresolved cited work.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Unresolved cited work

Reference 16

Resolution
unresolved
raw_fallback, observed 2026-08-07T14:21:18.481704Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:13.183582Z digest=sha256:e6bf52462b11073c87f7a6916f7d6f83bdc9376e408fca4240fa398825b3e970

Observation 0361bcae-b8a7-4e2c-82a7-1026d74f7505 · outbound

This paper cites an unresolved cited work.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Unresolved cited work

Reference 17

Resolution
unresolved
raw_fallback, observed 2026-08-07T14:21:18.314430Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:13.202094Z digest=sha256:99be31f4bdcfa0eaa7afe2fb4587fe3417689527c1d5c544997103b487895cbc

Observation adfc6957-0a6e-45d9-9690-6698c4617bd6 · outbound

This paper cites an unresolved cited work.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Unresolved cited work

Reference 18

Resolution
unresolved
raw_fallback, observed 2026-08-07T14:21:18.156965Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:13.218227Z digest=sha256:964181df45362148eb73d8aaed75d35b6e029e82b9fcb8d05934de7283a75c16

Observation 1fc7fa40-73b7-405f-a5d6-3c070a954f12 · outbound

This paper cites Benhar, V.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Benhar, V

Reference 19

Resolution
verified exact
raw_fallback, observed 2026-08-07T14:21:16.167521Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:13.221185Z digest=sha256:d53dd99cf79aaae4e8fff15442a19cc76c453b75f8fbe74d69205019894fe053

Observation dd0e3a0f-0040-4206-a912-0d1042eaee34 · outbound

This paper cites Effective No-Hair Relations for Neutron Stars and Quark Stars: Relativistic Results.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Effective No-Hair Relations for Neutron Stars and Quark Stars: Relativistic Results

Reference 20

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:13.223862Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:13.223862Z digest=sha256:532fd72cad9233a6f7fba231325d880cac15354c7997b66a72a0f38e843dda00

Observation 94e5c386-56f9-4200-b2b2-7ac3091ced48 · outbound

This paper cites Rotating Stars in Relativity.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Rotating Stars in Relativity

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:13.226298Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:13.226298Z digest=sha256:c8799ca77315c0e1cdee5331d418532ccbfa715b143de6de67f6f2b33d4dedf1

Observation f5bef584-0219-48a1-b43e-61cfa396cda2 · outbound

This paper cites an unresolved cited work.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Unresolved cited work

Reference 22

Resolution
unresolved
raw_fallback, observed 2026-08-07T14:21:18.082010Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:13.229332Z digest=sha256:723603b8810e990a43a7aeef61f1efb33dfd358107809b2999ccbf792b70df44

Observation fc7a3407-de7d-401f-934b-60b2e72986dc · outbound

This paper cites Bonazzola, E.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Bonazzola, E

Reference 23

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T14:21:17.938811Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:13.255330Z digest=sha256:70723b539ecdb37389eac2256909665d28206443fe14cc5d856d06e55660dae6

Observation cb086b75-cdb2-43c5-85b7-e4870f3d0e5c · outbound

This paper cites Bonazzola, E.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Bonazzola, E

Reference 24

Resolution
verified exact
raw_fallback, observed 2026-08-07T14:21:16.003036Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:13.334891Z digest=sha256:11d163d8f54988425c502bd1d40297a3948d182cbcfa92b19cd3c807d11ea48a

Observation 32c8f3d7-ed97-4e60-bdab-4236ef6a0848 · outbound

This paper cites Komatsu, Y.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Komatsu, Y

Reference 25

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T14:21:17.864278Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:13.378444Z digest=sha256:101b22eaf23ec457e96e9fbfb6dc28be9e942ccd096cfdc006e864616176c339

Observation 0b5728cb-0c59-40d9-8d8e-37da5f3e0c5b · outbound

This paper cites an unresolved cited work.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Unresolved cited work

Reference 26

Resolution
unresolved
raw_fallback, observed 2026-08-07T14:21:17.734860Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:13.413894Z digest=sha256:2ad341dd81800fcc4a92761ec7d12523a498a6f77e69a17293404d1025b4cdac

Observation 4013ece6-9d24-44f3-b64c-bfdc80b570db · outbound

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

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Comparing Models of Rapidly Rotating Relativistic Stars Constructed by Two Numerical Methods

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:13.459138Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:13.459138Z digest=sha256:6d697ef1929f82cbb6ff5b49e85f0685a2f2aa03ed982d39d03cd4340a9364fc

Observation bc3476ad-3b31-4803-b012-75f34ed7efda · outbound

This paper cites Pulse Profiles from Spinning Neutron Stars in the Hartle-Thorne Approximation.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Pulse Profiles from Spinning Neutron Stars in the Hartle-Thorne Approximation

Reference 28

Resolution
verified exact
local_arxiv, observed 2026-08-07T14:21:15.874533Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:13.526190Z digest=sha256:281aed29ea6d60e392fd898b6f0b7571b6a63de660d19a75959b86a51faa699c

Observation 3330200d-5b14-4da9-95dd-7a9a4365ebba · outbound

This paper cites What can quasi-periodic oscillations tell us about the structure of the corresponding compact objects?.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation What can quasi-periodic oscillations tell us about the structure of the corresponding compact objects?

Reference 29

Resolution
verified exact
local_arxiv, observed 2026-08-07T14:21:15.738260Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:13.566620Z digest=sha256:8a98578917d2279f99628c278a5024d27b88f6be36a513a06ce4ec29cc6d9960

Observation 5cf2cbb0-433a-4ec3-b8e9-a7d121cddf71 · outbound

This paper cites an unresolved cited work.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Unresolved cited work

Reference 30

Resolution
unresolved
raw_fallback, observed 2026-08-07T14:21:17.722403Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:13.599477Z digest=sha256:c213e5b26d2d6a6a2368182320e561531f708891e697cca89ac29023c059eee4

Observation b537f4ed-c246-4788-8541-9da693d73bb8 · outbound

This paper cites Rotating neutron stars: an invariant comparison of approximate and numerical spacetime models.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Rotating neutron stars: an invariant comparison of approximate and numerical spacetime models

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:13.645287Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:13.645287Z digest=sha256:2687ac03f041144014ae4cd42042b51332bba6773682d39368f94122c45edd72

Observation 4e9e98b8-7e8e-4723-8812-1ff846a1e293 · outbound

This paper cites an unresolved cited work.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Unresolved cited work

Reference 32

Resolution
unresolved
raw_fallback, observed 2026-08-07T14:21:17.679227Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:13.721062Z digest=sha256:1ff6c26951d81d717ed06ed50c992d10fa31125a7d590d56debd788a520099da

Observation c36b7840-880a-4655-b3d0-9973e2d83351 · outbound

This paper cites Approximate Matching of Analytic and Numerical Solutions for Rapidly Rotating Neutron Stars.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Approximate Matching of Analytic and Numerical Solutions for Rapidly Rotating Neutron Stars

Reference 33

Resolution
verified exact
local_arxiv, observed 2026-08-07T14:21:15.674862Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:13.726071Z digest=sha256:aaecf1bf3bb808cb44b7178cba017057658fb71813ba5c950d9a519b43b64d4c

Observation da1799c8-a557-480a-a999-4edacf978f66 · outbound

This paper cites Akmal, V.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Akmal, V

Reference 34

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:13.734271Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:13.734271Z digest=sha256:ce836dddee7d93a52197d024e4175a54babfee2d177bc5e9356d995be048af6c

Observation 148034df-6302-4f6e-889a-4e2e2173e6c1 · outbound

This paper cites Chandrasekhar, Ellipsoidal figures of equilibrium, New York: Dover (1987).

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Chandrasekhar, Ellipsoidal figures of equilibrium, New York: Dover (1987)

Reference 35

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T14:21:17.579578Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:13.738610Z digest=sha256:80eea1ea006ff0ed069b10699d564648323423b70358bd2599664ad5ac440b04

Observation be065e45-115d-4e64-88ba-996ba3406ac2 · outbound

This paper cites an unresolved cited work.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Unresolved cited work

Reference 36

Resolution
unresolved
raw_fallback, observed 2026-08-07T14:21:17.489290Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:13.763716Z digest=sha256:5c39a0afe8e609d4b3a2ff5564807ff87cef6120e539714c843ae97efbb9fdc2

Observation db2a28bf-d536-4a94-b79f-0f1e03bfdbe2 · outbound

This paper cites Boshkayev, H.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Boshkayev, H

Reference 37

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T14:21:17.423991Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:13.836605Z digest=sha256:9103ef6fbde1975b0d04de3116df5d252f56a83639d94b8d5f106e245bb0b761

Observation f7c8c070-7d7e-46dd-9e21-7f357337ab8f · outbound

This paper cites an unresolved cited work.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Unresolved cited work

Reference 38

Resolution
unresolved
raw_fallback, observed 2026-08-07T14:21:17.294669Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:13.863039Z digest=sha256:7370565826184f0f8774a0be8ad9ca9b1db1a3791f3e79f06f8e20b83c943792

Observation c5d7e1e1-b5d9-4e69-bba2-39b3c6ef7eb1 · outbound

This paper cites Slowly rotating neutron stars with small differential rotation: equilibrium models and oscillations in the Cowling approximation.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Slowly rotating neutron stars with small differential rotation: equilibrium models and oscillations in the Cowling approximation

Reference 39

Resolution
verified exact
local_arxiv, observed 2026-08-07T14:21:15.486515Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:13.895824Z digest=sha256:3d39db5fd11522c0f95175fef0adc8ef6c7dccdcd82d1224109e94924ca6eae3

Observation b388f059-ba37-4725-8763-f266911b0eb1 · outbound

This paper cites Evolution of magnetized, differentially rotating neutron stars: Simulations in full general relativity.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Evolution of magnetized, differentially rotating neutron stars: Simulations in full general relativity

Reference 40

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:13.974194Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:13.974194Z digest=sha256:e2a3e2943555ceb1b1a430266dcfaab8c84acfc9ca6ffb86cd5dbbc3c2f9a60b

Observation 4d589a3e-f450-40bc-9245-15adfd67347f · outbound

This paper cites Self-gravitating anisotropic fluid. III: Relativistic theory.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Self-gravitating anisotropic fluid. III: Relativistic theory

Reference 41

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:14.028339Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:14.028339Z digest=sha256:0c1f66de36c78de4d48a7d3ce815c3af0b907a13566c9e3b37dc4e8c06a1208d

Observation 2015e000-35a3-4eae-8e46-bbcbb1e6ca3c · outbound

This paper cites I-Love-Q anisotropically: Universal relations for compact stars with scalar pressure anisotropy.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation I-Love-Q anisotropically: Universal relations for compact stars with scalar pressure anisotropy

Reference 42

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:14.064073Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:14.064073Z digest=sha256:01f4cd47f1e6eab110d394b8e1c87899629a4dd138cbe199350246fc96720338

Observation c70a9641-6231-4379-98ff-6f72d5d28236 · outbound

This paper cites Slowly rotating anisotropic relativistic stars.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Slowly rotating anisotropic relativistic stars

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:14.109855Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:14.109855Z digest=sha256:ae47b2ce6b6f0308469dbe18d80ddadcbce10febddbb3b930ecc304058919c1e

Observation 3bce86ee-1f12-4681-8561-1072b2958757 · outbound

This paper cites Gravitational perturbations of the Schwarzschild spacetime: A practical covariant and gauge-invariant formalism.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Gravitational perturbations of the Schwarzschild spacetime: A practical covariant and gauge-invariant formalism

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:14.189198Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:14.189198Z digest=sha256:653f19624367f6b384c1ee0f5f8d8643731adea89d0e08b7ba06f606dc254052

Observation 3cbfd22a-a545-43f3-9aef-cdb4420028a0 · outbound

This paper cites Regge and J.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Regge and J

Reference 45

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T14:21:17.177507Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:14.231196Z digest=sha256:30d05e93d083962ef0892fa66be0a44e38dcca9b4bb7ddb6c3f14fef9032e37b

Observation 40a9a9c9-96b5-4381-bcbc-e1cc9b9b6ef4 · outbound

This paper cites Conde, Hartle-thorne project, https://gitlab.com/ carlosc7/hartle-thorne-project (2025).

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Conde, Hartle-thorne project, https://gitlab.com/ carlosc7/hartle-thorne-project (2025)

Reference 46

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T14:21:17.062571Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:14.240009Z digest=sha256:96d72e0386b6d38bb0f9ff7dad5c5974648b454742f40f171aada800c1d66ef1

Observation b09d1c91-4bfa-4e84-bdcd-8a0b8736883e · outbound

This paper cites Isolated and Binary Neutron Stars in Dynamical Chern-Simons Gravity.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Isolated and Binary Neutron Stars in Dynamical Chern-Simons Gravity

Reference 47

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:14.242446Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:14.242446Z digest=sha256:fb391e1849b153c05995fc63e0d48e398dd766c66a9b84ddfcc7236a1e5a8480

Observation e222c563-1c54-42a7-9b55-8b6d9346851e · outbound

This paper cites an unresolved cited work.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Unresolved cited work

Reference 48

Resolution
unresolved
raw_fallback, observed 2026-08-07T14:21:16.981477Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:14.245586Z digest=sha256:bbe97f4e9d571ad39c7cd9f0e932708be638388aeb887d8ec5555fc66fe6e0cf

Observation 26a2bb13-e58d-4110-89f4-294defc9151d · outbound

This paper cites xPert: Computer algebra for metric perturbation theory.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation xPert: Computer algebra for metric perturbation theory

Reference 49

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:14.248522Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:14.248522Z digest=sha256:a854ac26fb0a3c61d18761b92521ebf867be0cfe4b76e252db247a5fa016615e

Observation c8eb98ab-fea9-4265-b6aa-2f0cde15eb3f · outbound

This paper cites Abramowitz and I.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Abramowitz and I

Reference 50

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T14:21:16.954771Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:14.270632Z digest=sha256:e464c996bff3165a492ba3674d03be010a5eee00b4f41bd82463c1bb89e9df42

Observation e6cf1216-0edb-4fdc-88b5-23c28bb87e5d · outbound

This paper cites I-Love-Q Relations in Neutron Stars and their Applications to Astrophysics, Gravitational Waves and Fundamental Physics.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation I-Love-Q Relations in Neutron Stars and their Applications to Astrophysics, Gravitational Waves and Fundamental Physics

Reference 51

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:14.344223Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:14.344223Z digest=sha256:97ae48f0c01416ce5e1ad415b8d65df849361f0e097c489d1faff32df73e56e4

Observation f288d7d0-f5ef-4ad3-a31d-435ad8beffb5 · outbound

This paper cites Revisiting Hartle's model using perturbed matching theory to second order: amending the change in mass.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Revisiting Hartle's model using perturbed matching theory to second order: amending the change in mass

Reference 52

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:14.393831Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:14.393831Z digest=sha256:a9b622b4a700108405ad43ce4e5b16224a7f636661b22832b5221ec184e79eda

Observation fbc44e30-5217-45e7-9687-4872157bae5e · outbound

This paper cites Completion of the universal I-Love-Q relations in compact stars including the mass.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Completion of the universal I-Love-Q relations in compact stars including the mass

Reference 53

Resolution
verified exact
local_arxiv, observed 2026-08-07T14:21:15.345798Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:14.445271Z digest=sha256:ff9df2e1c121d5c9fd10b47756863d488b3ba0ce5e69d8b4165b03ba4380fc29

Observation f5f77a21-cef8-4fbb-b1d7-1604a6d0f644 · outbound

This paper cites Quasi-universal relations for generalized Skyrme stars.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Quasi-universal relations for generalized Skyrme stars

Reference 54

Resolution
verified exact
local_arxiv, observed 2026-08-07T14:21:15.327670Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:14.498092Z digest=sha256:5dda1f84e9e82d2220950c20fa65ca96275ec314a3663765fe0f9fb14c5e4d7b

Observation 0e8e0717-8534-4509-8705-0063f9a702c3 · outbound

This paper cites an unresolved cited work.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Unresolved cited work

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:14.553352Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:14.553352Z digest=sha256:f20da033bc20d6005684efad6b18e02df100d46a78e5b45ea0db45de5a8537cc

Observation 875d8bfe-3b6e-409c-b354-f6de4976c31e · outbound

This paper cites G¨ ursel, Multipole moments for stationary systems: The equivalence of the geroch-hansen formulation and the thorne formulation, General relativity and gravita- tion 15, 737 (1983).

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation G¨ ursel, Multipole moments for stationary systems: The equivalence of the geroch-hansen formulation and the thorne formulation, General relativity and gravita- tion 15, 737 (1983)

Reference 56

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T14:21:16.896873Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:14.586040Z digest=sha256:f7e87e0a86490fa719b95e878f9a1eeb62c1a08f39595557492fa4551ecc6d7a

Observation cc3d0a7d-53cb-49e5-b679-c0dc6373e25a · outbound

This paper cites Gravitational Multipoles in General Stationary Spacetimes.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Gravitational Multipoles in General Stationary Spacetimes

Reference 57

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:14.614921Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:14.614921Z digest=sha256:fea344e6fa676d0bad0e1a05019415f169f500f162afd3e29ddbf2965a38f753

Observation d80c587e-f51c-4af2-9704-ff5518903694 · outbound

This paper cites Testing the black hole "no-hair" hypothesis.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Testing the black hole "no-hair" hypothesis

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:14.658030Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:14.658030Z digest=sha256:25d9e57331fc8e2f2b11e1197347efea7b25ebc8e17e4084003d7c0ae2431f40

Observation 5bfccbe7-58fc-4043-8b41-edb47f7239c2 · outbound

This paper cites an unresolved cited work.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Unresolved cited work

Reference 59

Resolution
unresolved
raw_fallback, observed 2026-08-07T14:21:16.842487Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:14.705550Z digest=sha256:1d4f18bc9f8c209dcee583f30e0f119ea5d63ca4f7309a49dce0515ef2e91cb5

Observation 9bc6283c-ee7e-4286-bbe4-ca8d133df017 · outbound

This paper cites an unresolved cited work.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Unresolved cited work

Reference 60

Resolution
unresolved
raw_fallback, observed 2026-08-07T14:21:16.744413Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:14.772677Z digest=sha256:e1b78aa5021dc78209baa69d7898f1c83966debebb28dc4afa9ff8bb8e52bea1

Observation ab1581d1-be97-4704-b95b-c372879c4fb4 · outbound

This paper cites Poisson and C.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Poisson and C

Reference 61

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:14.785492Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:14.785492Z digest=sha256:b049f244de98db35c6cd93b397144d9d7542b4cc1c0f5eb8ff77fcbb55f623b3

Observation 4a1cdc75-b99e-43ea-9f2c-7acbdb0c2467 · outbound

This paper cites an unresolved cited work.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Unresolved cited work

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:14.788559Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:14.788559Z digest=sha256:20749c5992f5c5aea12fad549d16285125f1ce0299a466228f4a266e1db98f1b

Observation 3e6e4e08-4e47-40e4-9794-4bf0f2b0a137 · outbound

This paper cites Fodor, C.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Fodor, C

Reference 63

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T14:21:16.616969Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:14.791289Z digest=sha256:17c2136111d810923d1e08feb44d8d848dcee273c1917d35af902f6f4406f626

Observation e679db30-eb8a-4f4b-8276-f0ee48874308 · outbound

This paper cites Calculation of multipole moments of axistationary electrovacuum spacetimes.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Calculation of multipole moments of axistationary electrovacuum spacetimes

Reference 64

Resolution
verified exact
local_arxiv, observed 2026-08-07T14:21:15.180032Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:14.795342Z digest=sha256:80d592961f95c640f762ca4af53dc68e8e0af0cf55c6ee7c3e1cc437a2fc8490

Observation 7aaa8951-a406-40e4-bba0-6382fc8bbf6f · outbound

This paper cites Dietz, NEW EXACT SOLUTIONS OF EINSTEIN’S FIELD EQUATIONS: GRA VITATIONAL FORCE CAN ALSO BE REPULSIVE!, Found.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Dietz, NEW EXACT SOLUTIONS OF EINSTEIN’S FIELD EQUATIONS: GRA VITATIONAL FORCE CAN ALSO BE REPULSIVE!, Found

Reference 65

Resolution
verified fuzzy
raw_fallback, observed 2026-08-07T14:21:16.447164Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:14.846975Z digest=sha256:3bb8a557f13045477453df7117bfff3bb4c4136183456275dbda12abba3f2741

Observation 4914cf19-9973-4ba2-be61-bf1e22831284 · outbound

This paper cites an unresolved cited work.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Unresolved cited work

Reference 66

Resolution
unresolved
raw_fallback, observed 2026-08-07T14:21:16.419063Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:14.914022Z digest=sha256:a7262463647d5dfe70c4f6423df646255b4ce960f80324017b0585d1c9fa02b5

Observation 27f53119-d009-4668-b935-95395b2db195 · outbound

This paper cites Building Neutron Stars with the MUSES Calculation Engine.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Building Neutron Stars with the MUSES Calculation Engine

Reference 67

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:14.947288Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:14.947288Z digest=sha256:c27d44cd44b7ea0afa1a7831f678c16e1825270f8ee8407dd6c1a70f9e6a058c

Observation 1194f709-addd-4f06-b76a-fc16be48b4f9 · outbound

This paper cites an unresolved cited work.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Unresolved cited work

Reference 68

Resolution
unresolved
raw_fallback, observed 2026-08-07T14:21:16.407094Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-08-07T14:21:14.984296Z digest=sha256:72a628c6194b3e362d7d4943193e049a279cd74b087055b6aa8c69ae8278ae99

Observation 66df1bf2-8b90-4e16-a8ca-9ade43507dc8 · outbound

This paper cites Theoretical and Experimental Constraints for the Equation of State of Dense and Hot Matter.

Highly-accurate neutron star modeling in the Hartle-Thorne Approximation Theoretical and Experimental Constraints for the Equation of State of Dense and Hot Matter

Reference 69

Resolution
unresolved
no resolver link, observed 2026-08-07T14:21:15.040363Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:21:15.040363Z digest=sha256:18619b3b9ae8f21766e1825b9592774b1c55963bb7221c7c1a3492895a55204c

Pith citing papers

Observation f55f5da1-481c-487c-8864-6e442809c69c · inbound

Donutization Inside Neutron Stars: Shell-Localized Scalar Fields cites this paper.

Donutization Inside Neutron Stars: Shell-Localized Scalar Fields Highly-accurate neutron star modeling in the Hartle-Thorne Approximation

Reference 111

Resolution
verified exact
arxiv_id, observed 2026-06-29T20:33:58.097797Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.

source=pdf_text observed=2026-06-29T20:33:28.058638Z digest=sha256:efd71575704f7ca60fd5c47146a73e23da94ab4879da6d1b95df49f035c5529f

Observation 243d0f2c-24fb-4292-b9ac-083e3ee9bfa8 · inbound

Neural-Accelerated Bayesian Calibration of Chiral Mean-Field Models to Nuclear Saturation and Vacuum Properties cites this paper.

Neural-Accelerated Bayesian Calibration of Chiral Mean-Field Models to Nuclear Saturation and Vacuum Properties Highly-accurate neutron star modeling in the Hartle-Thorne Approximation

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-02T05:44:22.117557Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T05:44:22.117557Z digest=sha256:740440309ffac308682a0e72d82259c80f0fbff6a88ac1aa99bbac6dd5ce9e66