Paper Citation Record · LEDGER

Dark Energy with Phantom Crossing and the $H_0$ tension

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 19 inbound Pith citation observations for arXiv:2005.12587.

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

pith.paper-citation-record.v1
2005.12587 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 19 of 19 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 19 of 19 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T01:13:35.444612Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T15:37:06.250072Z

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 e7737e35-564e-4da2-958c-c94df308f206 · 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 Dark Energy with Phantom Crossing and the $H_0$ tension

Reference 185

Resolution: verified exact; arxiv_id, observed 2026-05-15T11:50:21.428164Z

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 456f8525-cf27-4963-8de8-579f366bac47 · inbound

$\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity cites this paper.

$\Lambda_{\rm s}$CDM cosmology from a type-II minimally modified gravity Dark Energy with Phantom Crossing and the $H_0$ tension

Reference 123

Resolution: verified exact; arxiv_id, observed 2026-05-24T03:53:54.557384Z

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 276337c9-0acd-492b-8ce2-f04634ce9eb1 · inbound

Mapping the $\Lambda_{\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate cites this paper.

Mapping the $\Lambda_{\rm s}$CDM scenario to $f(T)$ modified gravity: Effects on structure growth rate Dark Energy with Phantom Crossing and the $H_0$ tension

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-10T01:13:35.444612Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7cb5e2e8-87cb-4690-bafb-9d3203097da0 · 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 Dark Energy with Phantom Crossing and the $H_0$ tension

Reference 176

Resolution: unresolved; no resolver link, observed 2026-08-07T18:51:43.921201Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 573c66f4-464c-4aef-87e2-ce968be0512e · inbound

Can the universe experience an AdS landscape since matter-radiation equality? cites this paper.

Can the universe experience an AdS landscape since matter-radiation equality? Dark Energy with Phantom Crossing and the $H_0$ tension

Reference 150

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:56.801122Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f375f5d6-f72f-4d8a-a156-07c8f5733a8d · inbound

Interacting Scalar Fields as Dark Energy and Dark Matter in Einstein scalar Gauss Bonnet Gravity cites this paper.

Interacting Scalar Fields as Dark Energy and Dark Matter in Einstein scalar Gauss Bonnet Gravity Dark Energy with Phantom Crossing and the $H_0$ tension

Reference 76

Resolution: verified exact; arxiv_id, observed 2026-05-19T05:57:09.070089Z

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 ecb57ee1-103b-4dbd-8902-8690ddcda273 · inbound

Dark energy era with a resolution of Hubble tension in generalized entropic cosmology cites this paper.

Dark energy era with a resolution of Hubble tension in generalized entropic cosmology Dark Energy with Phantom Crossing and the $H_0$ tension

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-06T15:45:30.333314Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7e8b6395-645a-45bd-9a12-40f9d746d825 · 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 Dark Energy with Phantom Crossing and the $H_0$ tension

Reference 280

Resolution: unresolved; no resolver link, observed 2026-08-04T12:53:56.453184Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e5c9f01e-fb7d-474e-98a3-b6258a9b6381 · 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 Dark Energy with Phantom Crossing and the $H_0$ tension

Reference 160

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:54.577828Z

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 89724670-9fb5-43bd-b6e4-be1655c85f73 · inbound

Is Phantom Divide Crossing in General Relativity Completely Impossible? Shortcomings in canonical and minimally coupled scalar field and Possible Solutions in $k$-essence Models cites this paper.

Is Phantom Divide Crossing in General Relativity Completely Impossible? Shortcomings in canonical and minimally coupled scalar field and Possible Solutions in $k$-essence Models Dark Energy with Phantom Crossing and the $H_0$ tension

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-03T07:07:23.950050Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation af272ead-85d7-4b20-8d7b-d655cf109b5e · 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 Dark Energy with Phantom Crossing and the $H_0$ tension

Reference 93

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:30:12.531228Z

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 299b3c01-30fa-4ba1-ae46-7f4b1e080f42 · 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 Dark Energy with Phantom Crossing and the $H_0$ tension

Reference 102

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 5a6afcd9-f789-49ab-ba99-322699e3383c · inbound

Negative neutrino mass or negative dark energy? cites this paper.

Negative neutrino mass or negative dark energy? Dark Energy with Phantom Crossing and the $H_0$ tension

Reference 36

Resolution: verified exact; arxiv_id, observed 2026-05-21T03:03:55.527309Z

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 5c185fcf-6a1c-41e6-8d68-3fafb6cfa5fc · inbound

Reconstructing dark energy with fewer assumptions cites this paper.

Reconstructing dark energy with fewer assumptions Dark Energy with Phantom Crossing and the $H_0$ tension

Reference 111

Resolution: verified exact; arxiv_id, observed 2026-07-02T14:57:04.235921Z

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 1cc824f0-eaab-467d-9161-11715855356f · inbound

What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2 cites this paper.

What it takes to solve the Hubble tension through Modifications of Cosmological Recombination II: in light of ACT DR6 and DESI DR2 Dark Energy with Phantom Crossing and the $H_0$ tension

Reference 37

Resolution: verified exact; arxiv_id, observed 2026-07-02T15:37:06.251576Z

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 4be031c4-b3ae-45b2-b61a-e36635f405f5 · inbound

Cosmological Viability of Exponential Infrared $f(T)$ Gravity cites this paper.

Cosmological Viability of Exponential Infrared $f(T)$ Gravity Dark Energy with Phantom Crossing and the $H_0$ tension

Reference 174

Resolution: verified exact; arxiv_id, observed 2026-07-01T11:15:42.507819Z

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 508f3a0f-cfc8-407e-a014-2b92bee5b00d · inbound

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

Hubble tension in k-essence: Evidence for robust tension alleviation Dark Energy with Phantom Crossing and the $H_0$ tension

Reference 44

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 cafca745-000c-4589-aed4-21f38048dcb9 · 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 Dark Energy with Phantom Crossing and the $H_0$ tension

Reference 82

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 15949ada-fdd7-43c8-af70-b6421e0e415f · inbound

Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide cites this paper.

Defocusing dark energy: Raychaudhuri diagnostics beyond $w<-1/3$ and the phantom divide Dark Energy with Phantom Crossing and the $H_0$ tension

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-01T16:29:59.600212Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.