Pith. sign in

Paper Citation Record · LEDGER

Dark Energy and Dark Matter from an additional adiabatic fluid

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1604.06908.

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

pith.paper-citation-record.v1
1604.06908 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 2026-08-06T12:47:16.774638Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-06T12:47:16.872844Z

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 28ce2887-85bb-4448-b97d-b759c07175d3 · inbound

Bondi accretion disk luminosity around neutral and charged Simpson-Visser spacetimes cites this paper.

Bondi accretion disk luminosity around neutral and charged Simpson-Visser spacetimes Dark Energy and Dark Matter from an additional adiabatic fluid

Reference 78

Resolution
verified exact
local_arxiv, observed 2026-08-06T12:47:16.875668Z

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=2026-08-06T12:47:16.774638Z digest=sha256:0421141cac5bfe0a4167296e17c9972e7d7588742727bf93f0a5450a72ceaf56

Observation 80709519-026f-4bde-9584-93f0596fe290 · inbound

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? cites this paper.

Do we really need alternatives to the $\omega_0\omega_a$CDM parameterization after the DESI DR2? Dark Energy and Dark Matter from an additional adiabatic fluid

Reference 27

Resolution
unresolved
no resolver link, observed 2026-08-06T00:32:10.409143Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T00:32:10.409143Z digest=sha256:87ab249347dbb0050672b1f12b59e1fa07399a771a2e1029cf9d97dd947c4ea0