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Paper Citation Record · LEDGER

On the Energy Equation and Efficiency Parameter of the Common Envelope Evolution

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:astro-ph/0007034.

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

pith.paper-citation-record.v1
astro-ph/0007034 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-05T14:41:22.281287Z

measured 1 of 1 external citation measurements

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

Source: pith, observed 2026-08-05T02:28:24.338817Z

Reference resolution

0 of 0 outbound references displayed

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

External citation measurements

27
pith, observed 2026-08-05T02:28:24.338817Z

Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation 0630c501-7b90-4598-b8a3-54c78175fc1e · inbound

The power of binaries on stripped-envelope supernovae across metallicity: uniform progenitor parameter space and persistently low ejecta masses, but subtype diversity cites this paper.

The power of binaries on stripped-envelope supernovae across metallicity: uniform progenitor parameter space and persistently low ejecta masses, but subtype diversity On the Energy Equation and Efficiency Parameter of the Common Envelope Evolution

Reference 43

Resolution
unresolved
no resolver link, observed 2026-08-05T14:41:22.281287Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=arxiv_source observed=2026-08-05T14:41:22.281287Z digest=sha256:0fb36dff91221896bba6c1972632ecb2fd3eb946bec6e4ecdafc991b9edd830a

Observation 632f7f91-c587-40c1-ad6f-802a1e402911 · inbound

Formation of Extremely Low-mass White Dwarf Binaries Undergoing Enhanced Angular Momentum Loss cites this paper.

Formation of Extremely Low-mass White Dwarf Binaries Undergoing Enhanced Angular Momentum Loss On the Energy Equation and Efficiency Parameter of the Common Envelope Evolution

Reference 30

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:49:26.330658Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-05-21T02:48:26.950589Z digest=sha256:db4e25826b406775fbdd9e78c83a407e32d3306a4fcb1eead21703175aaffabd

Observation 0d9a3784-3e2f-43d5-af95-33dc2ebb4117 · inbound

Formation of Extremely Low-mass White Dwarf Binaries Undergoing Enhanced Angular Momentum Loss cites this paper.

Formation of Extremely Low-mass White Dwarf Binaries Undergoing Enhanced Angular Momentum Loss On the Energy Equation and Efficiency Parameter of the Common Envelope Evolution

Reference 30

Resolution
verified exact
local_arxiv, observed 2026-06-30T17:54:57.638037Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-06-30T17:45:09.334188Z digest=sha256:5d4cd714c6d7778470160e2b9505b53b99fceb6242f1176ab84f505814b92ed6

Observation 841f03c4-9675-415e-9133-87ba31485f00 · inbound

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models cites this paper.

Neutron star-companion interaction in core collapse supernovae. Population synthesis based on detailed binary evolution models On the Energy Equation and Efficiency Parameter of the Common Envelope Evolution

Reference 28

Resolution
verified exact
local_arxiv, observed 2026-05-21T02:13:54.974190Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-05-21T02:13:20.739968Z digest=sha256:743ae8f16efcc4ac136f45b6f72a773a912904be589632cc7901fb222a5a38f1

Observation a3939c09-1d3b-437f-b167-4c283cbb56e2 · inbound

Comparative Study of Two Luminous Red Novae I. Progenitor Modeling and Dust Formation cites this paper.

Comparative Study of Two Luminous Red Novae I. Progenitor Modeling and Dust Formation On the Energy Equation and Efficiency Parameter of the Common Envelope Evolution

Reference 166

Resolution
verified exact
local_arxiv, observed 2026-06-26T09:59:18.125747Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-06-26T09:40:03.967210Z digest=sha256:31d39d44d6dbc086d7c8cf1c20bdafdadb48d35ffd775487de63e703c0ab3b6e

Observation 494b34fd-4402-4b10-ac47-8f42847ca52a · inbound

The Best Guess: Testing new and old formalisms for the common envelope against observations cites this paper.

The Best Guess: Testing new and old formalisms for the common envelope against observations On the Energy Equation and Efficiency Parameter of the Common Envelope Evolution

Reference 30

Resolution
verified exact
local_arxiv, observed 2026-07-08T09:44:48.866427Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=arxiv_source observed=2026-07-08T09:38:52.637692Z digest=sha256:3139830671529404512b03a247e2d20f3c1f08022303627e039ebe3cb990ff2d