Paper Citation Record · LEDGER

Negative cosmological constant in the dark sector?

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 10 inbound Pith citation observations for arXiv:2008.10237.

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

pith.paper-citation-record.v1
2008.10237 v3

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 10 of 10 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 10 of 10 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T10:52:56.805805Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T15:37:06.432646Z

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 7c9c08c3-2908-4f84-8ff3-845253b9f003 · 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 Negative cosmological constant in the dark sector?

Reference 122

Resolution: verified exact; arxiv_id, observed 2026-05-15T11:50:21.182219Z

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 9ec5ab48-d90d-4b5f-b4d9-8e73f9cff157 · 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 Negative cosmological constant in the dark sector?

Reference 105

Resolution: verified exact; arxiv_id, observed 2026-05-24T03:53:54.920749Z

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 3e0d7c4f-8c41-4b31-a553-3ddb2b7a4a81 · 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? Negative cosmological constant in the dark sector?

Reference 151

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:56.805805Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4c0e09e9-983c-4759-8085-4843a5ba9551 · inbound

The Lifespan of our Universe cites this paper.

The Lifespan of our Universe Negative cosmological constant in the dark sector?

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-06T21:35:00.788264Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a262a527-9ea8-4279-8266-ca3f516ea696 · 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 Negative cosmological constant in the dark sector?

Reference 161

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:54.898042Z

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 5e2793c0-b70f-40f8-b625-82c592c2780d · 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 Negative cosmological constant in the dark sector?

Reference 114

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:30:12.114255Z

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 cb86257b-c01f-4488-8113-176f885e4033 · 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 Negative cosmological constant in the dark sector?

Reference 125

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 9c5ab49d-251c-4fa3-8c8e-406f458e03eb · 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 Negative cosmological constant in the dark sector?

Reference 38

Resolution: verified exact; arxiv_id, observed 2026-07-02T15:37:06.433958Z

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 4463f0b3-c3c7-4d4a-b6b3-b19854360092 · 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 Negative cosmological constant in the dark sector?

Reference 103

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 daad98d9-8355-473a-b6c8-107f438f839e · 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 Negative cosmological constant in the dark sector?

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-01T16:29:57.794865Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.