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Paper Citation Record · LEDGER

Alleviating the $H_0$ and $\sigma_8$ tensions in the interacting cubic covariant Galileon model

As of 11 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:2405.20240.

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

pith.paper-citation-record.v1
2405.20240 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 3 of 3 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-11T06:34:44.6726+00:00

measured 3 of 3 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T13:41:23.832056Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-08-10T20:19:25.020701Z

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 0de474c3-58c2-446d-91a7-c5d32a580edb · inbound

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? cites this paper.

DESI and SNe: Dynamical Dark Energy, $\Omega_m$ Tension or Systematics? Alleviating the $H_0$ and $\sigma_8$ tensions in the interacting cubic covariant Galileon model

Reference 73

Resolution
unresolved
no resolver link, observed 2026-08-11T13:41:23.832056Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T13:41:23.832056Z digest=sha256:7237923a0c1be4d48d7cdae20bd24da24c92bc3164faf153b3670106623d1c9b

Observation 7b570abe-e1f4-4d14-9110-9cf13ad281e4 · inbound

The case for a low dark matter density in dynamical dark energy model from local probes cites this paper.

The case for a low dark matter density in dynamical dark energy model from local probes Alleviating the $H_0$ and $\sigma_8$ tensions in the interacting cubic covariant Galileon model

Reference 16

Resolution
verified exact
local_arxiv, observed 2026-08-10T20:19:25.026733Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-11T06:34:44.6726+00:00.

source=pdf_text observed=2026-08-10T20:19:23.817684Z digest=sha256:b5a5de8b7b2b9f51cfbad716d0a62d3c835e58fe53e86a8188772c366defd44f

Observation 9e2e7f3c-7b2a-43f4-88f4-5a9616cbd127 · inbound

Scalar-Tensor Gravity and DESI 2024 BAO data cites this paper.

Scalar-Tensor Gravity and DESI 2024 BAO data Alleviating the $H_0$ and $\sigma_8$ tensions in the interacting cubic covariant Galileon model

Reference 31

Resolution
unresolved
no resolver link, observed 2026-08-10T14:29:27.485881Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T14:29:27.485881Z digest=sha256:0c3856c5e09512b6d7b122b4e2c10fc05b475413ae1937137d4b069de788166b