Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Dark energy and matter interacting scenario to relieve $H_0$ and $S_8$ tensions
As of 15 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 9 inbound Pith citation observations for arXiv:2212.13146.
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 2026-08-14T06:32:32.682623+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-10T22:48:22.265346Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-04T02:19:23.749335Z
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 55076ec6-987e-4f1f-a7d8-02fc20051cd3 · inbound
Prospects for measuring neutrino mass with 21-cm forest cites this paper.
Prospects for measuring neutrino mass with 21-cm forest Dark energy and matter interacting scenario to relieve $H_0$ and $S_8$ tensions
Reference 120
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T22:48:22.265346Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 2607cb41-d1ce-42e1-bd8e-cbac49090f87 · 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 Dark energy and matter interacting scenario to relieve $H_0$ and $S_8$ tensions
Reference 80
- Resolution
- unresolved
- no resolver link, observed 2026-08-06T18:14:15.300064Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation b3fde515-ed86-4508-ada5-c01fa006b0d6 · 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 Dark energy and matter interacting scenario to relieve $H_0$ and $S_8$ tensions
Reference 235
- Resolution
- unresolved
- no resolver link, observed 2026-08-04T12:53:52.919293Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 94a6e458-c3c9-451b-8282-71c008c7370d · inbound
Robust Preference for Dark Sector Interactions cites this paper.
Robust Preference for Dark Sector Interactions Dark energy and matter interacting scenario to relieve $H_0$ and $S_8$ tensions
Reference 108
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T11:11:48.894279Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 56398904-7585-42ab-b4bf-fe5f929aa5ca · 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 Dark energy and matter interacting scenario to relieve $H_0$ and $S_8$ tensions
Reference 96
- Resolution
- verified exact
- arxiv_id, observed 2026-05-16T12:17:52.649626Z
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 1b4d9ad9-f248-40fa-a88f-34d97f88233e · inbound
Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions cites this paper.
Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions Dark energy and matter interacting scenario to relieve $H_0$ and $S_8$ tensions
Reference 186
- Resolution
- verified exact
- arxiv_id, observed 2026-07-01T16:35:50.543659Z
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 c392220d-cd66-4293-af7b-bbfa30b3fa9d · 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 Dark energy and matter interacting scenario to relieve $H_0$ and $S_8$ tensions
Reference 54
- Resolution
- verified exact
- arxiv_id, observed 2026-07-03T07:47:45.272753Z
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 a90305c2-d9f6-4f5e-b228-02efd200d2c6 · inbound
Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data cites this paper.
Resolving the Hubble Tension in the Early Dark Energy Framework with JWST and DESI Data Dark energy and matter interacting scenario to relieve $H_0$ and $S_8$ tensions
Reference 24
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T02:19:23.750929Z
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 24fd9841-4dbb-4524-9771-892855a1a52c · inbound
Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data cites this paper.
Neutrino mass constraints in the Schwarzschild-de Sitter black-hole dark energy model with ACT DR6 and DESI DR2 data Dark energy and matter interacting scenario to relieve $H_0$ and $S_8$ tensions
Reference 39
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T04:18:55.037825Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.