Paper Citation Record · LEDGER

A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension

As of 16 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 17 inbound Pith citation observations for arXiv:1906.08275.

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

pith.paper-citation-record.v1
1906.08275 v3

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measured 17 of 17 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-16T06:30:59.297886+00:00

measured 17 of 17 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-14T14:24:14.560148Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-21T13:30:12.379703Z

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Outbound references

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Pith citing papers

Observation 68fde0db-8b52-4483-8a75-a34af98be9a3 · inbound

Resolving Hubble Tension with Quintom Dark Energy Model cites this paper.

Resolving Hubble Tension with Quintom Dark Energy Model A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-14T14:24:14.560148Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 12633550-dc33-40b7-9326-ef2cbdf556de · inbound

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions cites this paper.

Interacting dark energy in the early 2020s: a promising solution to the $H_0$ and cosmic shear tensions A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-14T13:51:08.457564Z

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Unavailable: canonical work link unavailable.

Observation b21906fd-ff9e-4992-8599-588938e1d33c · inbound

Cosmology With Low-Redshift Observations: No Signal For New Physics cites this paper.

Cosmology With Low-Redshift Observations: No Signal For New Physics A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-14T12:25:23.802558Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4c19ddee-0776-47ac-a023-26350a32477d · inbound

In the Realm of the Hubble tension $-$ a Review of Solutions cites this paper.

In the Realm of the Hubble tension $-$ a Review of Solutions A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension

Reference 261

Resolution: verified exact; arxiv_id, observed 2026-05-15T11:50:32.928387Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 1656ea80-9779-4d67-8303-9d4acae232f0 · inbound

Extended Effective Field Theory of Dark Energy: Ghost Condensate Dark Energy with Sextic Dispersion Relation in de Sitter Spacetime cites this paper.

Extended Effective Field Theory of Dark Energy: Ghost Condensate Dark Energy with Sextic Dispersion Relation in de Sitter Spacetime A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-09T12:23:40.021131Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ac0623db-0ad3-421c-8880-85a4ea5cc9fe · inbound

An overview of what current data can (and cannot yet) say about evolving dark energy cites this paper.

An overview of what current data can (and cannot yet) say about evolving dark energy A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension

Reference 171

Resolution: unresolved; no resolver link, observed 2026-08-07T18:51:43.900647Z

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Unavailable: canonical work link unavailable.

Observation 35d0b324-b68b-4433-a18c-2d02a6c54d0f · inbound

Extended Dark Energy analysis using DESI DR2 BAO measurements cites this paper.

Extended Dark Energy analysis using DESI DR2 BAO measurements A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension

Reference 170

Resolution: verified exact; arxiv_id, observed 2026-05-14T21:04:04.021075Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 52c9384c-60b7-4b70-8d61-71bef803af52 · inbound

Revisiting $\Lambda$CDM extensions in light of re-analyzed CMB data cites this paper.

Revisiting $\Lambda$CDM extensions in light of re-analyzed CMB data A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension

Reference 61

Resolution: verified exact; arxiv_id, observed 2026-05-19T09:27:15.130297Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 4df514ab-45d8-426d-9550-d84b98413a31 · inbound

Hubble Tension and the G-step Model: Re-examination of Recent Constraints on Modified Local Physics cites this paper.

Hubble Tension and the G-step Model: Re-examination of Recent Constraints on Modified Local Physics A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-06T00:10:04.680583Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 59766eeb-55c0-435e-99fb-a05fa62de558 · 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 A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-04T09:59:15.383938Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8e5bec3e-7328-4389-bda8-370803037a30 · 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 A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension

Reference 154

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:55.168008Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 738c053e-9d9d-4885-a402-d446fa78e255 · 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 A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension

Reference 108

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:30:12.381565Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation b9e9ff62-d7d4-40c9-8b74-f7f5100ad0bb · 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 A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension

Reference 119

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7793104a-8427-4755-9a01-08afd469e31b · inbound

Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe? cites this paper.

Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe? A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension

Reference 47

Resolution: verified exact; arxiv_id, observed 2026-05-11T11:36:01.984462Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-16T06:30:59.297886+00:00.

Observation 7986744a-f329-4f7d-bcb0-b66ac015a8bc · inbound

Hubble tension in k-essence: Evidence for robust tension alleviation cites this paper.

Hubble tension in k-essence: Evidence for robust tension alleviation A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension

Reference 43

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 4c9eef64-2bb0-4497-b591-eff1a8c31aef · inbound

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus cites this paper.

Alleviating the Hubble Tension with Smooth Sign-Switching Dark Energy: Full CMB Constraints with DESI and PantheonPlus A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension

Reference 97

Resolution: unresolved; no resolver link, observed 2026-07-11T09:40:49.196932Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a6af1d4f-2641-4ff7-b873-d25290eefc59 · inbound

Hubble tension: a short review of theoretical explanations cites this paper.

Hubble tension: a short review of theoretical explanations A Simple Phenomenological Emergent Dark Energy Model can Resolve the Hubble Tension

Reference 223

Resolution: unresolved; no resolver link, observed 2026-08-01T07:20:08.212806Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.