Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Late time interacting cosmologies and the Hubble constant tension
As of 9 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2111.03152.
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 2026-08-09T06:31:02.800959+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-06T18:14:14.850785Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-02T15:37:06.406918Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
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 48e0a603-34a2-4df1-b0c4-3a1878c2ed87 · 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 Late time interacting cosmologies and the Hubble constant tension
Reference 75
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T18:14:14.850785Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b7992508-e649-43f5-95ad-1a9c25bb5495 · inbound
Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime cites this paper.
Averaging Dynamics of Scalar Field-Matter Interacting Models in Anisotropic Universes: The Locally Rotationally Symmetric Bianchi I Spacetime Late time interacting cosmologies and the Hubble constant tension
Reference 69
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T05:29:00.993497Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 4dc5ca7a-0f08-4b60-ad88-ab9d714c13fc · inbound
Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO cites this paper.
Dark Energy Is Not That Into You: Variable Couplings after DESI DR2 BAO Late time interacting cosmologies and the Hubble constant tension
Reference 87
- Resolution
- unresolved
- no resolver link, observed 2026-08-05T16:03:01.348252Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d9bf3025-3518-42e4-abef-921065d41352 · inbound
BAO miscalibration cannot rescue late-time solutions to the Hubble tension cites this paper.
BAO miscalibration cannot rescue late-time solutions to the Hubble tension Late time interacting cosmologies and the Hubble constant tension
Reference 230
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T12:53:52.581568Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 07f1d444-6615-44f4-b78b-da0884c2f33d · inbound
A microphysically inspired approach to dark matter-dark energy interactions: first bounds on dark-sector scattering cross sections cites this paper.
A microphysically inspired approach to dark matter-dark energy interactions: first bounds on dark-sector scattering cross sections Late time interacting cosmologies and the Hubble constant tension
Reference 26
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T11:41:15.305897Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 7080e133-6953-46e0-8a0b-17766c0b1795 · 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 Late time interacting cosmologies and the Hubble constant tension
Reference 50
- Resolution
- verified exact
- arxiv_id, observed 2026-07-02T15:37:06.408249Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-09T06:31:02.800959+00:00.