Pith. sign in

Paper Citation Record · LEDGER

Impact of chiral hyperonic three-body forces on neutron stars

As of 13 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1906.11722.

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

pith.paper-citation-record.v1
1906.11722 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T13:53:44.107321Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T07:49:39.984176Z

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 174b0e49-1767-444d-b997-5a52089933a2 · inbound

Neutron Star Properties and Femtoscopic Constraints cites this paper.

Neutron Star Properties and Femtoscopic Constraints Impact of chiral hyperonic three-body forces on neutron stars

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-11T13:53:44.107321Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T13:53:44.107321Z digest=sha256:a7960fae0bbb8effc46a594c3cd055f6045cdeb46bde256d167050013d065255

Observation bcad680b-cc8b-4894-9256-64183a90db0f · inbound

In-medium $\Lambda N$ interactions with leading order covariant chiral hyperon/nucleon-nucleon forces cites this paper.

In-medium $\Lambda N$ interactions with leading order covariant chiral hyperon/nucleon-nucleon forces Impact of chiral hyperonic three-body forces on neutron stars

Reference 59

Resolution
unresolved
no resolver link, observed 2026-08-10T22:08:32.190994Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T22:08:32.190994Z digest=sha256:38221867a044f48f6822a3fc83f991a2e04065b99324168284686c2b20158cc5

Observation 7e684907-4f1a-4696-b025-6b325f5070c1 · inbound

The impact of hyperons on neutron star mergers: gravitational waves, mass ejection and black hole formation cites this paper.

The impact of hyperons on neutron star mergers: gravitational waves, mass ejection and black hole formation Impact of chiral hyperonic three-body forces on neutron stars

Reference 50

Resolution
unresolved
no resolver link, observed 2026-08-10T16:45:20.301326Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T16:45:20.301326Z digest=sha256:989fcb23842b0559eee59ba4b38cfc5db66074e0387d606a4b54275bfbc18669

Observation c1b3695e-469c-4392-99ab-085645754bae · 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 Impact of chiral hyperonic three-body forces on neutron stars

Reference 31

Resolution
verified exact
arxiv_id, observed 2026-07-04T07:49:39.109578Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-06-26T12:50:53.032717Z digest=sha256:4fbe0530e68dfdbb57c6b8fc3bd02d2360f2a661967164502dc4e5605609fbac

Observation 79c28abc-2992-41e9-befd-a143cacce0bd · inbound

Hyperonic equation of state for neutron stars: A systematic Bayesian comparison of density-dependent and non-linear relativistic mean-field models cites this paper.

Hyperonic equation of state for neutron stars: A systematic Bayesian comparison of density-dependent and non-linear relativistic mean-field models Impact of chiral hyperonic three-body forces on neutron stars

Reference 16

Resolution
verified exact
arxiv_id, observed 2026-07-04T07:49:39.985438Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

source=pdf_text observed=2026-06-26T12:34:28.137843Z digest=sha256:db4cacee25812f2af6daf1b018843ddf5157000d4d1970f9a3894f833a079874