Paper Citation Record · LEDGER

Cosmological viable models in $f(T,B)$ gravity as solutions to the $H_0$ tension

As of 22 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:1909.10328.

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

pith.paper-citation-record.v1
1909.10328 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-22T06:32:14.747728+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-12T18:51:10.289908Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-06-30T20:15:03.817453Z

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 ab804a17-2111-4e9c-8168-6a6e18dfdbac · inbound

Late Time Phenomena in $f(T,\mathcal{T})$ Gravity Framework: Role of $H_0$ Priors cites this paper.

Late Time Phenomena in $f(T,\mathcal{T})$ Gravity Framework: Role of $H_0$ Priors Cosmological viable models in $f(T,B)$ gravity as solutions to the $H_0$ tension

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-12T18:51:10.289908Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ae43290a-fed6-4ad1-a9e9-810dfc68fc6b · inbound

Cosmological solutions in teleparallel $F(T,B)$ gravity cites this paper.

Cosmological solutions in teleparallel $F(T,B)$ gravity Cosmological viable models in $f(T,B)$ gravity as solutions to the $H_0$ tension

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-12T11:23:17.448823Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2f0db4bf-9749-4f7e-81e4-e3c5d3056af0 · inbound

Charged black hole solutions in $f(R,T)$ gravity coupled to nonlinear electrodynamics cites this paper.

Charged black hole solutions in $f(R,T)$ gravity coupled to nonlinear electrodynamics Cosmological viable models in $f(T,B)$ gravity as solutions to the $H_0$ tension

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-12T05:23:30.459329Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

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 2026-08-22T06:32:14.747728+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.