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Paper Citation Record · LEDGER

Stable and unstable cosmological models in bimetric massive gravity

As of 7 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1407.4331.

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

pith.paper-citation-record.v1
1407.4331 v3

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 2026-08-06T21:35:36.956100Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-06T20:45:32.873970Z

Reference resolution

0 of 0 outbound references displayed

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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 ef399e62-c076-4320-97e9-ec157a95c6b3 · inbound

Line-of-sight acceleration as a test of the Galactic Yukawa potential cites this paper.

Line-of-sight acceleration as a test of the Galactic Yukawa potential Stable and unstable cosmological models in bimetric massive gravity

Reference 16

Resolution
unresolved
no resolver link, observed 2026-08-06T21:35:36.956100Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T21:35:36.956100Z digest=sha256:16d12786ef691c64723e939f5de15c2732e9be5eb032f6cfae49c6039c83c2a6

Observation 793d079e-11a2-4462-8ee0-067d3099f494 · inbound

Do Pulsar Timing Datasets Favor Massive Gravity? cites this paper.

Do Pulsar Timing Datasets Favor Massive Gravity? Stable and unstable cosmological models in bimetric massive gravity

Reference 43

Resolution
verified exact
local_arxiv, observed 2026-08-06T20:45:32.877365Z

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=2026-08-06T20:45:31.980384Z digest=sha256:dd9334a0643a555241178f06c13e8254d6e459bd4280bae2f589d4affe458153