Paper Citation Record · LEDGER

Revisiting a negative cosmological constant from low-redshift data

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 16 inbound Pith citation observations for arXiv:1907.07953.

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

pith.paper-citation-record.v1
1907.07953 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 16 of 16 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-07T06:34:17.273281+00:00

measured 16 of 16 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T10:52:56.792036Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T15:37:06.517892Z

Reference resolution

0 of 0 outbound references displayed

verified exact0
verified fuzzy0
unresolved0
parse uncertain0
malformed identifier0
metadata mismatch0

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 aa893091-fbee-45a0-b689-38fc477994d4 · 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 Revisiting a negative cosmological constant from low-redshift data

Reference 121

Resolution: verified exact; arxiv_id, observed 2026-05-15T11:50:21.178695Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 4fe32fc4-4cc4-44a0-a6fd-16cb04211492 · 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 Revisiting a negative cosmological constant from low-redshift data

Reference 101

Resolution: verified exact; arxiv_id, observed 2026-05-24T03:53:54.777050Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 70838edf-6051-401d-87d8-967bae176cbf · inbound

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

Extended Dark Energy analysis using DESI DR2 BAO measurements Revisiting a negative cosmological constant from low-redshift data

Reference 114

Resolution: verified exact; arxiv_id, observed 2026-05-14T21:04:03.806560Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 1a09ee75-cf9b-4e0a-abe3-3e8069e76ed4 · inbound

Cosmic Strings as Dynamical Dark Energy: Novel Constraints cites this paper.

Cosmic Strings as Dynamical Dark Energy: Novel Constraints Revisiting a negative cosmological constant from low-redshift data

Reference 39

Resolution: verified exact; arxiv_id, observed 2026-05-19T14:22:24.221297Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 70a1bf97-f1cf-4191-892f-c7e8f57f059b · 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? Revisiting a negative cosmological constant from low-redshift data

Reference 148

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:56.792036Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 860327d7-4970-4b04-96fd-00c73ad42edb · inbound

The Lifespan of our Universe cites this paper.

The Lifespan of our Universe Revisiting a negative cosmological constant from low-redshift data

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-06T21:35:00.396513Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 09fb897f-3d7f-4f78-a9e2-627cc0b689bf · 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 Revisiting a negative cosmological constant from low-redshift data

Reference 155

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:55.190234Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation b85c6d95-b040-4daa-8847-80fae95663e7 · inbound

Dark Matter from Holography cites this paper.

Dark Matter from Holography Revisiting a negative cosmological constant from low-redshift data

Reference 43

Resolution: verified exact; arxiv_id, observed 2026-05-17T22:12:09.077109Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation a01891b1-447d-4b5e-ac45-4c09d398b941 · 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 Revisiting a negative cosmological constant from low-redshift data

Reference 110

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:30:11.872821Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 7a0f4513-ec09-4de1-8bf7-b83e20202da4 · 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 Revisiting a negative cosmological constant from low-redshift data

Reference 120

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 0ff88e4a-3460-4617-9ceb-8411405acb0a · 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 Revisiting a negative cosmological constant from low-redshift data

Reference 34

Resolution: verified exact; arxiv_id, observed 2026-05-10T13:00:24.856159Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation a71dfec6-7b33-43da-9598-b32c6e941c0c · 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 Revisiting a negative cosmological constant from low-redshift data

Reference 20

Resolution: verified exact; arxiv_id, observed 2026-07-02T15:37:06.519126Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation e49b5c6e-e8eb-4678-804a-bceebeb19a2b · 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 Revisiting a negative cosmological constant from low-redshift data

Reference 176

Resolution: verified exact; arxiv_id, observed 2026-07-01T11:25:45.563071Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-07T06:34:17.273281+00:00.

Observation 7c28979d-9082-4e20-b120-a782c3237bd7 · 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 Revisiting a negative cosmological constant from low-redshift data

Reference 98

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 c679fa51-8ec3-4016-82d7-a138f61089d7 · 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 Revisiting a negative cosmological constant from low-redshift data

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-01T16:29:57.656786Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3c3fc4b7-fb93-4fdf-8c89-5b3650d58190 · inbound

Hubble tension: the shape wall cites this paper.

Hubble tension: the shape wall Revisiting a negative cosmological constant from low-redshift data

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-01T08:08:36.364103Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.