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Paper Citation Record · LEDGER

Proto-neutron stars with heavy baryons and universal relations

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:2008.00213.

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

pith.paper-citation-record.v1
2008.00213 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 2 of 2 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T17:02:27.084458Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-17T23:12:12.049112Z

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 835c5ff6-9fa1-4cc9-a472-9e1a5df87268 · inbound

Investigating Universal Relations in Compact Stars featuring $\Delta-$Admixed Exotic Dense Matter cites this paper.

Investigating Universal Relations in Compact Stars featuring $\Delta-$Admixed Exotic Dense Matter Proto-neutron stars with heavy baryons and universal relations

Reference 37

Resolution
unresolved
no resolver link, observed 2026-08-06T17:02:27.084458Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T17:02:27.084458Z digest=sha256:1a0b9a3802f5dab3885bdf3980a7b8b8df26b61b4be501b1bbc64e3b7da4ec95

Observation f86ee13f-36ec-4077-a9c8-b6c1af40c2e2 · inbound

Dark Matter Heating in Evolving Proto-Neutron Stars: A Two-Fluid Approach cites this paper.

Dark Matter Heating in Evolving Proto-Neutron Stars: A Two-Fluid Approach Proto-neutron stars with heavy baryons and universal relations

Reference 89

Resolution
verified exact
arxiv_id, observed 2026-05-17T23:12:12.050721Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

source=pdf_text observed=2026-05-17T23:10:30.793407Z digest=sha256:cb801ce751bb6fe86deea91c5eaaf97d3faf78acc168dceaaec1484d2a14ac10