Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Cosmological viable models in $f(T,B)$ gravity as solutions to the $H_0$ tension
As of 6 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 3 inbound Pith citation observations for arXiv:1909.10328.
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 2026-08-05T06:32:48.257954+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-01T02:46:22.927493Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-06-30T20:15:03.817453Z
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 6312e842-18a3-472c-8607-e60e2392a95f · inbound
Unified dark sector and Hubble-tension alleviation in scalar-vector-tensor gravity cites this paper.
Unified dark sector and Hubble-tension alleviation in scalar-vector-tensor gravity Cosmological viable models in $f(T,B)$ gravity as solutions to the $H_0$ tension
Reference 52
- Resolution
- verified exact
- arxiv_id, observed 2026-06-30T20:15:03.819040Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-05T06:32:48.257954+00:00.
Observation dbf031e8-4938-42a4-934f-d901a93860a8 · inbound
Hubble tension in k-essence: Evidence for robust tension alleviation cites this paper.
Hubble tension in k-essence: Evidence for robust tension alleviation Cosmological viable models in $f(T,B)$ gravity as solutions to the $H_0$ tension
Reference 34
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T01:30:43.080456Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ed5fbb09-f461-45bc-90c7-6a39aac8c5bc · inbound
Early- and late-time constraints on Wald-Gauss-Bonnet topological dark energy and implications for the $H_0$ and $S_8$ tensions cites this paper.
Early- and late-time constraints on Wald-Gauss-Bonnet topological dark energy and implications for the $H_0$ and $S_8$ tensions Cosmological viable models in $f(T,B)$ gravity as solutions to the $H_0$ tension
Reference 56
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T02:46:22.927493Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.