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Paper Citation Record · LEDGER

The role of the tachyonic instability in Horndeski gravity

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 2 inbound Pith citation observations for arXiv:1810.03461.

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

pith.paper-citation-record.v1
1810.03461 v2

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 2026-08-15T06:32:42.880941+00:00

measured 2 of 2 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T14:35:13.355393Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-05-16T16:08:04.759015Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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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 dfb40108-0221-4c9a-b298-4ed0cc21ce06 · inbound

Cosmological Instabilities and the Role of Matter Interactions in Dynamical Dark Energy Models cites this paper.

Cosmological Instabilities and the Role of Matter Interactions in Dynamical Dark Energy Models The role of the tachyonic instability in Horndeski gravity

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-14T14:35:13.355393Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-14T14:35:13.355393Z digest=sha256:0cb3322a811c9ebf9e86741359ad0207e0e2672d7a6818ec7ca364586d432dc5

Observation 0b1e1fe4-367c-4ea7-8cb6-a603c2c36fbd · inbound

How deep can a cosmic void be? Voids-informed theoretical bounds in Galileon gravity cites this paper.

How deep can a cosmic void be? Voids-informed theoretical bounds in Galileon gravity The role of the tachyonic instability in Horndeski gravity

Reference 26

Resolution
verified exact
local_arxiv, observed 2026-05-16T16:08:04.760542Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-15T06:32:42.880941+00:00.

source=pdf_text observed=2026-05-16T16:04:11.710388Z digest=sha256:46dce09fbeb48c74c4de13709f06468d4d7320912c05f01f7e941d8bed4eef31