Paper Citation Record · LEDGER

Kick it like DESI: PNGB quintessence with a dynamically generated initial velocity

As of 17 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 12 inbound Pith citation observations for arXiv:2412.07418.

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

pith.paper-citation-record.v1
2412.07418 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 12 of 12 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-17T06:30:58.91139+00:00

measured 12 of 12 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T11:37:32.229123Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T03:07:35.366406Z

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 e7420bd8-62cd-45ad-8ad9-26f7c3e2110a · inbound

Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations? cites this paper.

Is excess smoothing of Planck CMB ansiotropy data partially responsible for evidence for dark energy dynamics in other $w(z)$CDM parametrizations? Kick it like DESI: PNGB quintessence with a dynamically generated initial velocity

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-10T22:00:59.898239Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4a17e97c-9150-4d11-9057-2fbdaf04488c · inbound

Robustness of dark energy phenomenology across different parameterizations cites this paper.

Robustness of dark energy phenomenology across different parameterizations Kick it like DESI: PNGB quintessence with a dynamically generated initial velocity

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-08T21:04:17.723679Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 482c75d8-d0a4-4fb5-a3a9-ff2633294218 · inbound

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background cites this paper.

Physical vs phantom dark energy after DESI: thawing quintessence in a curved background Kick it like DESI: PNGB quintessence with a dynamically generated initial velocity

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-16T11:37:32.229123Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a778d6b1-a552-4c72-b04b-609eb5d3d10b · inbound

Examining Quintessence Models with DESI Data cites this paper.

Examining Quintessence Models with DESI Data Kick it like DESI: PNGB quintessence with a dynamically generated initial velocity

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-07T14:30:35.180092Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0ee79c0e-0e0b-4b07-8441-fdadfdd5851d · inbound

About electroweak domain walls in Majoron models cites this paper.

About electroweak domain walls in Majoron models Kick it like DESI: PNGB quintessence with a dynamically generated initial velocity

Reference 159

Resolution: unresolved; no resolver link, observed 2026-08-07T11:21:38.669415Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fe57d556-8bbb-4e2d-86c6-4fd2892d7490 · inbound

Simple quintessence models in light of DESI-BAO observations cites this paper.

Simple quintessence models in light of DESI-BAO observations Kick it like DESI: PNGB quintessence with a dynamically generated initial velocity

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-07T00:43:07.361777Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 8a38e96f-0b99-4f08-b796-8f50f3148ecb · inbound

Beyond CPL: Evidence for dynamical dark energy in three-parameter models cites this paper.

Beyond CPL: Evidence for dynamical dark energy in three-parameter models Kick it like DESI: PNGB quintessence with a dynamically generated initial velocity

Reference 52

Resolution: verified exact; arxiv_id, observed 2026-05-18T10:46:16.273752Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 033e3486-2b2b-4a82-b369-435ab4ebcee0 · inbound

Cosmology of axion dark energy in supersymmetric models and constraints on high scale parameters cites this paper.

Cosmology of axion dark energy in supersymmetric models and constraints on high scale parameters Kick it like DESI: PNGB quintessence with a dynamically generated initial velocity

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-03T19:51:43.547033Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation eceb151e-90e8-402e-a600-987a3c46515f · inbound

Observational constraints on early time non-phantom behaviour of dynamical dark energy cites this paper.

Observational constraints on early time non-phantom behaviour of dynamical dark energy Kick it like DESI: PNGB quintessence with a dynamically generated initial velocity

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-03T14:40:55.442835Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e058a162-0a49-42ba-bff3-c0a55170ab07 · inbound

On the potential of pseudo-scalar dark energy cites this paper.

On the potential of pseudo-scalar dark energy Kick it like DESI: PNGB quintessence with a dynamically generated initial velocity

Reference 15

Resolution: verified exact; arxiv_id, observed 2026-07-03T03:07:35.367978Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation e24414b4-079a-4eb0-9f69-302f3df4d5e7 · inbound

Collider Probes of Dark Energy Microphysics cites this paper.

Collider Probes of Dark Energy Microphysics Kick it like DESI: PNGB quintessence with a dynamically generated initial velocity

Reference 108

Resolution: verified exact; arxiv_id, observed 2026-07-01T18:25:58.142662Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-17T06:30:58.91139+00:00.

Observation 4f415ca8-dd2a-4d77-9d8f-1e6a3690cdd8 · inbound

Collider Probes of Dark Energy Microphysics cites this paper.

Collider Probes of Dark Energy Microphysics Kick it like DESI: PNGB quintessence with a dynamically generated initial velocity

Reference 108

Resolution: unresolved; no resolver link, observed 2026-07-12T11:44:30.277942Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.