Pith. sign in

Paper Citation Record · LEDGER

Determination of the Equation of State of Dense Matter

As of 12 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 18 inbound Pith citation observations for arXiv:nucl-th/0208016.

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

pith.paper-citation-record.v1
nucl-th/0208016 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 18 of 18 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-12T06:34:41.77262+00:00

measured 18 of 18 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T17:11:13.081926Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-10T07:56:57.934194Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
  • metadata mismatch0

External citation measurements

No source-named external measurement is stored.

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation bd10a3e9-ae0b-4d5b-94de-bb485c8e78db · inbound

Extended Skyrme effective interactions with higher-order momentum-dependence for transport models and neutron stars cites this paper.

Extended Skyrme effective interactions with higher-order momentum-dependence for transport models and neutron stars Determination of the Equation of State of Dense Matter

Reference 5

Resolution
unresolved
no resolver link, observed 2026-08-11T17:11:13.081926Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T17:11:13.081926Z digest=sha256:9e9f1fee455d7b745a4ddb4b75d540297b59a06ae16ebb7f93788bcad52cd761

Observation a4e4bbac-0a12-4e6d-9088-00a419343f10 · inbound

Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis cites this paper.

Towards constraining QCD phase transitions in neutron star interiors: Bayesian Inference with TOV linear response analysis Determination of the Equation of State of Dense Matter

Reference 112

Resolution
unresolved
no resolver link, observed 2026-08-10T14:01:09.058956Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T14:01:09.058956Z digest=sha256:b7db27bbf3b52f96998fcfe4f3623cfcc71d91872736d7c63578fc16036c0567

Observation 51f40ef5-387d-4a7f-a157-1537d1d7a353 · inbound

Novel Scalings of Neutron Star Properties from Analyzing Dimensionless Tolman--Oppenheimer--Volkoff Equations cites this paper.

Novel Scalings of Neutron Star Properties from Analyzing Dimensionless Tolman--Oppenheimer--Volkoff Equations Determination of the Equation of State of Dense Matter

Reference 1596

Resolution
unresolved
no resolver link, observed 2026-08-09T23:06:17.535286Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-09T23:06:17.535286Z digest=sha256:79149eb7c13547ca11ec9319512e143ec8ee351e12d2b8b23ba2566cbf226dca

Observation 8b5e1d83-e8a6-4b88-a7da-736d3eddb4a4 · inbound

Symmetry Energy Expansion with Strange Dense Matter cites this paper.

Symmetry Energy Expansion with Strange Dense Matter Determination of the Equation of State of Dense Matter

Reference 10

Resolution
verified exact
local_arxiv, observed 2026-05-22T18:21:55.380146Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-05-22T18:20:24.680116Z digest=sha256:2c8faec06906dd5ea84899f0072f505a13232ba91bae8112bf854edf93dc0080

Observation fcd53419-1198-4187-95a9-0b19256880c2 · inbound

Study on the equation-of-state with light clusters and hypernuclei cites this paper.

Study on the equation-of-state with light clusters and hypernuclei Determination of the Equation of State of Dense Matter

Reference 80

Resolution
unresolved
no resolver link, observed 2026-08-04T19:51:05.718684Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T19:51:05.718684Z digest=sha256:91248f06a6a5cc01d48aefd673545e12ebb8a6e3a672d0b55b16052346e156b2

Observation 816ff124-323d-4697-80ff-fadcce836ae2 · inbound

Toward a Unified Understanding of the Dense Matter Equation of State cites this paper.

Toward a Unified Understanding of the Dense Matter Equation of State Determination of the Equation of State of Dense Matter

Reference 62

Resolution
unresolved
no resolver link, observed 2026-08-03T20:20:19.329175Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T20:20:19.329175Z digest=sha256:cfb1413ff42087cdf7229a6789e758d77b30bff0f9090121b73ae91a2a21afc8

Observation 976ccac6-2236-4a01-9978-57930cf13c1f · inbound

Quarkyonic Quark-Meson Coupling Model for Nuclear and Neutron Matter cites this paper.

Quarkyonic Quark-Meson Coupling Model for Nuclear and Neutron Matter Determination of the Equation of State of Dense Matter

Reference 79

Resolution
unresolved
no resolver link, observed 2026-08-03T18:37:52.052150Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T18:37:52.052150Z digest=sha256:669a4222f1e4d64d32eafc8243785717a7ae250758630ce5babfe136352ae511

Observation c1f63be8-2a24-4223-8156-637f6cfea65e · inbound

Space-time regions of high baryon density and baryon stopping in heavy-ion collisions cites this paper.

Space-time regions of high baryon density and baryon stopping in heavy-ion collisions Determination of the Equation of State of Dense Matter

Reference 55

Resolution
unresolved
no resolver link, observed 2026-08-02T20:41:22.363019Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T20:41:22.363019Z digest=sha256:0b2b3b3019a80e829adcd6fce4c20b5cd1295681bfff3ec33d96c00ae0084591

Observation b0ac0614-5d1f-4efe-bf98-d49258924b53 · inbound

Isentropic thermodynamics across the hadron-quark mixed phase in a two-phase model with a PNJL quark description cites this paper.

Isentropic thermodynamics across the hadron-quark mixed phase in a two-phase model with a PNJL quark description Determination of the Equation of State of Dense Matter

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-02T18:31:48.559345Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T18:31:48.559345Z digest=sha256:1f0c71bd3b7b64104f8a05702fec16251ff289af54c91042f974f0bf7afff156

Observation 0810d5b9-c104-4703-bce9-9bc7dea3c758 · inbound

Nuclear matter and proton parton distributions in a light-front Hamiltonian framework cites this paper.

Nuclear matter and proton parton distributions in a light-front Hamiltonian framework Determination of the Equation of State of Dense Matter

Reference 38

Resolution
malformed identifier
local_arxiv, observed 2026-07-01T19:36:09.484917Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-06-28T22:10:16.997484Z digest=sha256:6e277b4c60e330c3413c16a4a4a9c7ced8ef6a8d1f23b99cdd266435056f9439

Observation 7ced91eb-5822-442b-9865-701330056455 · inbound

Hybrid stars among mass gap objects are excluded by twin stars at $1.4\,M_\odot$ cites this paper.

Hybrid stars among mass gap objects are excluded by twin stars at $1.4\,M_\odot$ Determination of the Equation of State of Dense Matter

Reference 92

Resolution
verified exact
local_arxiv, observed 2026-06-30T16:04:52.392337Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=arxiv_source observed=2026-07-11T11:50:26.030339Z digest=sha256:808fdb76862813465d8fc76822c7aa8544f84c01c9968397e26b2b113ea4a677

Observation cf175bd9-91da-47ae-b13b-3586badf74a1 · inbound

Is the coexistence of strange quark stars and hadronic stars favored by astrophysical data? A Bayesian analysis cites this paper.

Is the coexistence of strange quark stars and hadronic stars favored by astrophysical data? A Bayesian analysis Determination of the Equation of State of Dense Matter

Reference 11

Resolution
verified exact
local_arxiv, observed 2026-07-04T07:49:39.160889Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-06-26T12:50:53.032717Z digest=sha256:e0ff77b264750b126e8ef6f5b4c05da4437ce51b1545e3ab4c20533e773db255

Observation af48e357-b2ac-4333-b1ad-ad3a564bf516 · inbound

Machine learning the impact parameter in heavy-ion collisions at $\sqrt{s_{\rm NN}}$ = 4 and 11 GeV: a cross-check study with UrQMD, AMPT, and JAM cites this paper.

Machine learning the impact parameter in heavy-ion collisions at $\sqrt{s_{\rm NN}}$ = 4 and 11 GeV: a cross-check study with UrQMD, AMPT, and JAM Determination of the Equation of State of Dense Matter

Reference 2

Resolution
verified exact
local_arxiv, observed 2026-07-09T23:36:37.185626Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-07-09T23:32:28.932487Z digest=sha256:e148cf4c9e8bf55d693de5eefb0e50180cfd53bbba835331eb0d2a14043d580c

Observation cdca8ece-4572-48dd-b91b-62648a969013 · inbound

Relativistic Mean Field Approach with Chiral Symmetry Breaking and Quark Confinement in the light of Astrophysical Observations cites this paper.

Relativistic Mean Field Approach with Chiral Symmetry Breaking and Quark Confinement in the light of Astrophysical Observations Determination of the Equation of State of Dense Matter

Reference 4

Resolution
verified exact
local_arxiv, observed 2026-07-10T07:56:57.935738Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-12T06:34:41.77262+00:00.

source=pdf_text observed=2026-07-10T07:51:26.601892Z digest=sha256:8a572784a0647d37fc4e6ffc97d17bb79a19f4bb8cbbd2d2b46438034754c8ce

Observation 2c345067-fd96-4b99-82ba-8778065709b6 · 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 Determination of the Equation of State of Dense Matter

Reference 11

Resolution
unresolved
no resolver link, observed 2026-08-02T05:44:16.255488Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T05:44:16.255488Z digest=sha256:d61e610accc949037d78182c4800ad9f493160d8327fdea2643d09fd6b099372

Observation 10999ff1-fdff-410b-835c-04f719993ba1 · inbound

The equation of state for neutron stars cites this paper.

The equation of state for neutron stars Determination of the Equation of State of Dense Matter

Reference 54

Resolution
unresolved
no resolver link, observed 2026-08-01T19:22:08.523264Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-01T19:22:08.523264Z digest=sha256:a42e54f118efc87f559a2cfc906df5f511f45ac4ba171c6fd08d446f28d50e35

Observation c927a3e1-ee84-49ec-b776-db1ea5e1f737 · inbound

Effects of light-cluster degrees of freedom on collective flows in heavy-ion collisions at FOPI energies cites this paper.

Effects of light-cluster degrees of freedom on collective flows in heavy-ion collisions at FOPI energies Determination of the Equation of State of Dense Matter

Reference 2

Resolution
unresolved
no resolver link, observed 2026-08-04T08:20:36.725051Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-04T08:20:36.725051Z digest=sha256:4c08c572c522e6e980aafd5ed14e57683d4ad1130b832fc722e30be1734d2579

Observation a566dafa-a032-48f6-abd0-4d557ed2b2f0 · inbound

Fast and Accurate Prediction of Neutron Star Structure with Deep Neural Networks cites this paper.

Fast and Accurate Prediction of Neutron Star Structure with Deep Neural Networks Determination of the Equation of State of Dense Matter

Reference 9

Resolution
unresolved
no resolver link, observed 2026-08-11T00:26:46.196492Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T00:26:46.196492Z digest=sha256:79f8ef4e762f41ff3aea2c2431cb26ce1e93798dc9cc8c96914b6153dcf19096