Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 23 inbound Pith citation observations for arXiv:hep-th/9408025.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-08T21:22:06.668052Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-07-04T05:09:35.605699Z
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 0c8b96b0-a38b-4515-a756-3e5cdf3a6596 · inbound
Assessing observational constraints on dark energy cites this paper.
Assessing observational constraints on dark energy The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
Reference 18
- Resolution
- verified exact
- local_arxiv, observed 2026-05-24T01:18:42.317953Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 4052ee37-abfb-467f-94ab-1857bbcd3434 · inbound
Deviations from the von Laue condition: Implications for the on-shell Lagrangian of particles and fluids cites this paper.
Deviations from the von Laue condition: Implications for the on-shell Lagrangian of particles and fluids The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
Reference 11
- Resolution
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d2abd99e-06ad-42d5-a27b-266e5d080241 · inbound
Geometric formulation of $k$-essence and late-time acceleration cites this paper.
Geometric formulation of $k$-essence and late-time acceleration The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
Reference 12
- Resolution
- unresolved
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 5456ef1f-424b-4a95-a721-05cdc2294222 · inbound
Discretely Evanescent Dark Energy cites this paper.
Discretely Evanescent Dark Energy The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
Reference 4
- Resolution
- unresolved
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Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 17e5846d-e218-4f14-b2ed-90e597d188f8 · inbound
Barrow holographic dark energy interacting model in the presence of radiation and matter cites this paper.
Barrow holographic dark energy interacting model in the presence of radiation and matter The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
Reference 66
- Resolution
- verified exact
- local_arxiv, observed 2026-05-19T07:07:07.746886Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 7709f418-94e9-4a9f-bb29-bd9fa8db81d8 · inbound
Weyl-invariant Einstein-Cartan gravity with a heavy ALP: Higgs Inflation and $\alpha$-attractors cites this paper.
Weyl-invariant Einstein-Cartan gravity with a heavy ALP: Higgs Inflation and $\alpha$-attractors The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
Reference 14
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T15:32:57.062210Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 41c798c6-dae3-482c-94d5-27625855d7e4 · inbound
Resolving the Planck-DESI tension by nonminimally coupled quintessence cites this paper.
Resolving the Planck-DESI tension by nonminimally coupled quintessence The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
Reference 60
- Resolution
- verified exact
- local_arxiv, observed 2026-05-19T01:36:57.968981Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 0ec36284-d0a6-4966-93f1-604a898d396c · inbound
Probing Dark Energy Microphysics with kSZ Tomography cites this paper.
Probing Dark Energy Microphysics with kSZ Tomography The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
Reference 32
- Resolution
- verified exact
- local_arxiv, observed 2026-05-21T19:34:20.332961Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation c4635c28-9fcd-4eea-b30c-267f9d93ecd1 · inbound
Constraining interacting dark energy models with black hole superradiance cites this paper.
Constraining interacting dark energy models with black hole superradiance The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
Reference 82
- Resolution
- verified exact
- local_arxiv, observed 2026-05-17T21:10:16.770050Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation e7cde08c-7d10-40ce-93d9-a5395ec65a87 · inbound
Robust Preference for Dark Sector Interactions cites this paper.
Robust Preference for Dark Sector Interactions The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
Reference 112
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T11:11:48.904613Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 25fcde23-440e-4e25-9944-500f631ba774 · inbound
Tachyonic gravitational dark matter production after inflation cites this paper.
Tachyonic gravitational dark matter production after inflation The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
Reference 96
- Resolution
- verified exact
- local_arxiv, observed 2026-05-16T15:01:03.758721Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation b9a11213-4890-44f4-bb69-d1952b362421 · inbound
Scaling solutions in three-form cosmology cites this paper.
Scaling solutions in three-form cosmology The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
Reference 17
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T23:00:23.232532Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a275235b-6657-457a-9074-9a432606aa97 · inbound
Dark energy from string theory: an introductory review cites this paper.
Dark energy from string theory: an introductory review The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
Reference 3
- Resolution
- verified exact
- local_arxiv, observed 2026-05-15T00:18:22.711760Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 5db454cd-028c-4544-937c-c7df09171400 · inbound
Non-minimally coupled quintessence with sign-switching interaction cites this paper.
Non-minimally coupled quintessence with sign-switching interaction The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
Reference 36
- Resolution
- verified exact
- arxiv_id, observed 2026-05-13T20:48:15.401053Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation a723b3d0-5a19-48d1-aaf5-3f07e4bd7638 · inbound
Accelerating scaling solutions from dark matter particle creation cites this paper.
Accelerating scaling solutions from dark matter particle creation The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
Reference 75
- 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 6281305c-113c-4f16-81b3-e5430c84dd5d · inbound
Breaking Free from the Swampland of Impossible Universes through the DESI Portal cites this paper.
Breaking Free from the Swampland of Impossible Universes through the DESI Portal The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
Reference 11
- Resolution
- verified exact
- arxiv_id, observed 2026-05-12T06:21:27.437270Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 422104f0-aa0b-47a1-bf58-b15d89aada1f · inbound
Breaking Free from the Swampland of Impossible Universes through the DESI Portal cites this paper.
Breaking Free from the Swampland of Impossible Universes through the DESI Portal The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
Reference 14
- Resolution
- verified exact
- local_arxiv, observed 2026-07-01T13:55:45.779533Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation d838a630-1b58-49a1-b645-e4678bf266e9 · inbound
Breaking Free from the Swampland of Impossible Universes through the DESI Portal cites this paper.
Breaking Free from the Swampland of Impossible Universes through the DESI Portal The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
Reference 14
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T14:29:15.778269Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 85214786-19e1-4134-89ef-8b309d0fcc12 · 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 The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
Reference 22
- Resolution
- verified exact
- local_arxiv, observed 2026-07-03T07:57:44.194692Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 324a3c98-da25-4869-ada3-283abb6994cc · inbound
Evolving Dark Energy Is Vacuum Energy After All cites this paper.
Evolving Dark Energy Is Vacuum Energy After All The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
Reference 64
- Resolution
- verified exact
- local_arxiv, observed 2026-07-04T05:09:35.607338Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 97c73b3a-aaca-437e-99a9-b01f7590ca48 · inbound
Evolving Dark Energy Is Vacuum Energy After All cites this paper.
Evolving Dark Energy Is Vacuum Energy After All The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
Reference 321
- Resolution
- unresolved
- no resolver link, observed 2026-08-02T10:56:49.061598Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation bbc8eff7-0bd3-4405-a132-838b1a26cb4c · inbound
The cosmology of long range Yukawa interactions in general backgrounds cites this paper.
The cosmology of long range Yukawa interactions in general backgrounds The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
Reference 62
- Resolution
- verified exact
- local_arxiv, observed 2026-07-01T17:45:52.424423Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.
Observation 271a7e72-91d3-4216-930a-299a932cbaf8 · inbound
The Goldstone Awakens: Unimodular dark energy in scale-invariant $R^2$ gravity cites this paper.
The Goldstone Awakens: Unimodular dark energy in scale-invariant $R^2$ gravity The cosmon model for an asymptotically vanishing time-dependent cosmological ``constant''
Reference 131
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T21:08:51.651208Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.