Paper Citation Record · LEDGER

Phase space analysis of sign-shifting interacting dark energy models

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2403.01397.

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

pith.paper-citation-record.v1
2403.01397 v1

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 10 of 10 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 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T11:29:07.795348Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T07:47:45.300198Z

Reference resolution

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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 7d6790d8-67c5-4c40-a355-9dc0cc8c3384 · inbound

Interacting phantom dark energy: new accelerating scaling attractors cites this paper.

Interacting phantom dark energy: new accelerating scaling attractors Phase space analysis of sign-shifting interacting dark energy models

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-12T11:29:07.795348Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3c5ebfa2-53de-4852-aacc-14c64e8d3c9e · inbound

Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions cites this paper.

Sign Switching in Dark Sector Coupling Interactions as a Candidate for Resolving Cosmological Tensions Phase space analysis of sign-shifting interacting dark energy models

Reference 111

Resolution: unresolved; no resolver link, observed 2026-08-10T19:20:17.002376Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 42c3c189-f80c-4b3f-87df-a011e0a6c29b · inbound

An overview of what current data can (and cannot yet) say about evolving dark energy cites this paper.

An overview of what current data can (and cannot yet) say about evolving dark energy Phase space analysis of sign-shifting interacting dark energy models

Reference 113

Resolution: unresolved; no resolver link, observed 2026-08-07T18:51:43.677089Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7230138f-bddb-4f8a-a616-49b05e54d931 · inbound

Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints cites this paper.

Solving an Interacting Quintessence Model with a Sound Horizon Initial Condition and its Observational Constraints Phase space analysis of sign-shifting interacting dark energy models

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-06T18:14:15.972826Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 017caabc-ac7b-4c39-9268-c0e46941aefc · inbound

Robust Preference for Dark Sector Interactions cites this paper.

Robust Preference for Dark Sector Interactions Phase space analysis of sign-shifting interacting dark energy models

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.839182Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 49ee83aa-0e05-48a7-8eb5-e9eba3e99cec · inbound

Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension cites this paper.

Revisiting the Matter Creation Process: Observational Constraints on Gravitationally Induced Dark Energy and the Hubble Tension Phase space analysis of sign-shifting interacting dark energy models

Reference 107

Resolution: verified exact; arxiv_id, observed 2026-05-16T12:17:52.424074Z

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.

Observation b3d1fbee-8c67-40a4-958d-424cac75f3c4 · inbound

Accelerating scaling solutions from dark matter particle creation cites this paper.

Accelerating scaling solutions from dark matter particle creation Phase space analysis of sign-shifting interacting dark energy models

Reference 99

Resolution: unresolved; no resolver link, observed 2026-07-12T18:37:05.978670Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5c5131db-7ad7-420f-b151-83485b50c143 · inbound

What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2 cites this paper.

What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2 Phase space analysis of sign-shifting interacting dark energy models

Reference 94

Resolution: verified exact; arxiv_id, observed 2026-07-02T15:37:06.436998Z

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.

Observation 114155da-0b9c-40cd-b3d6-176fa07ef982 · inbound

Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies cites this paper.

Non-linear Structure Formation in Planck+DESI Favoured Interacting Dark Energy Cosmologies Phase space analysis of sign-shifting interacting dark energy models

Reference 69

Resolution: verified exact; arxiv_id, observed 2026-07-03T07:47:45.301503Z

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.

Observation a66e797f-2ac6-4e07-81b3-b7c653f6ca9c · inbound

Cosmological Viability of Exponential Infrared $f(T)$ Gravity cites this paper.

Cosmological Viability of Exponential Infrared $f(T)$ Gravity Phase space analysis of sign-shifting interacting dark energy models

Reference 171

Resolution: verified exact; arxiv_id, observed 2026-07-01T11:15:42.561009Z

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.