Paper Citation Record · LEDGER

Relieving the $H_0$ tension with a new interacting dark energy model

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 22 inbound Pith citation observations for arXiv:2101.10714.

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

pith.paper-citation-record.v1
2101.10714 v2

Coverage vector

measured 0 of 0 reference resolution

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measured 22 of 22 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 22 of 22 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-06T18:14:14.946578Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-04T02:19:23.584092Z

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External citation measurements

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Outbound references

No outbound reference observations are available for this paper version.

Pith citing papers

Observation ba57314c-ade2-40da-8aed-2fc3c763d497 · 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 Relieving the $H_0$ tension with a new interacting dark energy model

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-06T18:14:14.946578Z

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Unavailable: canonical work link unavailable.

Observation 45c7aab6-34b4-40f6-97d9-9e8bfe4edd28 · 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 Relieving the $H_0$ tension with a new interacting dark energy model

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-06T05:29:00.615033Z

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Observation 7588f95b-1d24-47d6-85c4-7a759a68c032 · 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 Relieving the $H_0$ tension with a new interacting dark energy model

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-05T16:03:01.360730Z

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Unavailable: canonical work link unavailable.

Observation 231ebba1-2879-4770-9881-93d5e6118e81 · 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 Relieving the $H_0$ tension with a new interacting dark energy model

Reference 224

Resolution: unresolved; no resolver link, observed 2026-08-04T12:53:52.113802Z

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Observation f392e5ad-35e9-4dd2-90d6-80e2624affb1 · inbound

Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2 cites this paper.

Alleviating the $H_0$ tension through the interacting dark energy model from quantum gravitational field theory in light of DESI DR2 Relieving the $H_0$ tension with a new interacting dark energy model

Reference 110

Resolution: unresolved; no resolver link, observed 2026-08-04T09:59:20.892287Z

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Observation 142ea9d9-b536-4506-8ec3-2188e635acbc · inbound

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM cites this paper.

Nonlinear Matter Power Spectrum from relativistic $N$-body Simulations: $\Lambda_{\rm s}$CDM versus $\Lambda$CDM Relieving the $H_0$ tension with a new interacting dark energy model

Reference 94

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:55.594558Z

Source-reported events for the cited work

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Observation dabffe47-f2b1-4fff-abb9-cbf89841b7a2 · inbound

Robust Preference for Dark Sector Interactions cites this paper.

Robust Preference for Dark Sector Interactions Relieving the $H_0$ tension with a new interacting dark energy model

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-03T11:11:48.805079Z

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Unavailable: canonical work link unavailable.

Observation cf1b423c-f10f-4d93-93af-c017fca81b51 · 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 Relieving the $H_0$ tension with a new interacting dark energy model

Reference 84

Resolution: verified exact; arxiv_id, observed 2026-05-16T12:17:52.520189Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 5fed99bc-f52b-4060-bc72-f63ce837ddd2 · inbound

Evidence for deviation in gravitational light deflection from general relativity at cosmological scales with KiDS-Legacy and CMB lensing cites this paper.

Evidence for deviation in gravitational light deflection from general relativity at cosmological scales with KiDS-Legacy and CMB lensing Relieving the $H_0$ tension with a new interacting dark energy model

Reference 25

Resolution: verified exact; arxiv_id, observed 2026-05-16T08:17:35.875696Z

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No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 1026c9c4-a250-42b4-a84b-41bff312151a · inbound

Probing Dynamical Dark Energy with Late-Time Data: Evidence, Tensions, and the Limits of the $w_0w_a$CDM Framework cites this paper.

Probing Dynamical Dark Energy with Late-Time Data: Evidence, Tensions, and the Limits of the $w_0w_a$CDM Framework Relieving the $H_0$ tension with a new interacting dark energy model

Reference 60

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:30:12.330785Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 26ab0f92-d2ab-4bd7-adeb-b24469cf02fb · inbound

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families cites this paper.

Background-level reconstruction of scalar-field potentials from dark-energy histories and comparison with analytic potential families Relieving the $H_0$ tension with a new interacting dark energy model

Reference 69

Resolution: unresolved; no resolver link, observed 2026-07-15T12:01:04.317365Z

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Unavailable: canonical work link unavailable.

Observation 96fb6d3a-c8c8-4651-8cbd-bbec96c3fc75 · inbound

Double the axions, half the tension: multi-field early dark energy eases the Hubble tension cites this paper.

Double the axions, half the tension: multi-field early dark energy eases the Hubble tension Relieving the $H_0$ tension with a new interacting dark energy model

Reference 43

Resolution: verified exact; arxiv_id, observed 2026-05-11T11:41:02.205341Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation a50d4a0f-3054-4223-9799-22783bf2fcc0 · inbound

Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension cites this paper.

Geometric Constraints on the Pre-Recombination Expansion History from the Hubble Tension Relieving the $H_0$ tension with a new interacting dark energy model

Reference 29

Resolution: verified exact; arxiv_id, observed 2026-05-12T00:36:16.652832Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 96500ec3-a68e-4c43-9d7c-aad783101dbf · 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 Relieving the $H_0$ tension with a new interacting dark energy model

Reference 27

Resolution: verified exact; arxiv_id, observed 2026-06-30T20:15:05.531249Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 4ce11883-beb3-4320-b309-a9d271102ade · inbound

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions cites this paper.

Unifying Early and Late Dark Energy: Dynamical Requirements and Obstructions Relieving the $H_0$ tension with a new interacting dark energy model

Reference 175

Resolution: verified exact; arxiv_id, observed 2026-07-01T16:45:50.871264Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 6e0537c5-32f6-49eb-985f-4d62e2dec04c · inbound

Neutrino mass constraints in interacting dark energy models after DESI DR2 cites this paper.

Neutrino mass constraints in interacting dark energy models after DESI DR2 Relieving the $H_0$ tension with a new interacting dark energy model

Reference 149

Resolution: verified exact; arxiv_id, observed 2026-07-02T10:56:52.532017Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation bbec1621-cb34-4099-bf98-ab5a6862ee37 · 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 Relieving the $H_0$ tension with a new interacting dark energy model

Reference 39

Resolution: verified exact; arxiv_id, observed 2026-07-03T07:47:45.322017Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 42ff3cfd-7bf0-40da-8d59-25c4903c6a56 · 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 Relieving the $H_0$ tension with a new interacting dark energy model

Reference 12

Resolution: verified exact; arxiv_id, observed 2026-07-04T02:19:23.585674Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 3d1e35a6-aca6-44e2-a8b4-3d804e940f06 · inbound

Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension cites this paper.

Running into tension: primordial black holes from ultra-slow-roll inflation, spectral running, and the Hubble tension Relieving the $H_0$ tension with a new interacting dark energy model

Reference 186

Resolution: verified exact; arxiv_id, observed 2026-07-01T11:25:45.207935Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

Observation 034d45da-9a2f-4c27-81fa-7e039b467514 · 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 Relieving the $H_0$ tension with a new interacting dark energy model

Reference 32

Resolution: unresolved; no resolver link, observed 2026-07-12T04:18:55.037825Z

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Unavailable: canonical work link unavailable.

Observation 79dd7aaf-d238-4431-812f-aeb0243299d1 · inbound

Hubble tension: the shape wall cites this paper.

Hubble tension: the shape wall Relieving the $H_0$ tension with a new interacting dark energy model

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-01T08:08:40.787937Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0120f800-773f-4936-bca2-2d580294dcff · 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 Relieving the $H_0$ tension with a new interacting dark energy model

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-01T02:46:22.863457Z

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Unavailable: canonical work link unavailable.