Paper Citation Record · LEDGER

Do cosmological observations allow a negative $\Lambda$?

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 11 inbound Pith citation observations for arXiv:2112.10641.

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

pith.paper-citation-record.v1
2112.10641 v2

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measured 0 of 0 reference resolution

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measured 11 of 11 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-08T06:32:00.761636+00:00

measured 11 of 11 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T10:52:56.810513Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-02T15:37:06.475545Z

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Outbound references

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Pith citing papers

Observation 6f946c57-3046-495e-9ef9-8aa38f6ee7b7 · 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? Do cosmological observations allow a negative $\Lambda$?

Reference 152

Resolution: unresolved; no resolver link, observed 2026-08-07T10:52:56.810513Z

Source-reported events for the cited work

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Observation 01d2b014-aeb6-40dd-81f9-5de155317a2c · inbound

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

Simple quintessence models in light of DESI-BAO observations Do cosmological observations allow a negative $\Lambda$?

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-07T00:43:08.090774Z

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Observation de425178-ab5c-44f6-bf5a-1257aaeb431e · inbound

The Lifespan of our Universe cites this paper.

The Lifespan of our Universe Do cosmological observations allow a negative $\Lambda$?

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-06T21:35:00.583205Z

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Observation 184b917a-b05d-41e2-ade5-8044e059d4d0 · 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 Do cosmological observations allow a negative $\Lambda$?

Reference 170

Resolution: verified exact; arxiv_id, observed 2026-05-18T04:50:55.301506Z

Source-reported events for the cited work

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Observation f216d52b-f036-4a35-92bf-87157b1759e3 · 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 Do cosmological observations allow a negative $\Lambda$?

Reference 122

Resolution: verified exact; arxiv_id, observed 2026-05-21T13:30:11.894138Z

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Observation 38f8b6b3-15ac-4015-9176-e36a7a92275e · 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 Do cosmological observations allow a negative $\Lambda$?

Reference 133

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

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Observation 6601e9b4-0fa3-4c8e-b130-ebe4398e8475 · inbound

Early- and Late-Time Modifications to $\Lambda$CDM: Implications for the Hubble Tension cites this paper.

Early- and Late-Time Modifications to $\Lambda$CDM: Implications for the Hubble Tension Do cosmological observations allow a negative $\Lambda$?

Reference 54

Resolution: verified exact; arxiv_id, observed 2026-06-30T00:14:05.024296Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation c2defe48-5cc8-492b-b7bc-738628aa76d1 · 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 Do cosmological observations allow a negative $\Lambda$?

Reference 52

Resolution: verified exact; arxiv_id, observed 2026-07-02T15:37:06.477442Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-08T06:32:00.761636+00:00.

Observation da4b6a06-a531-4ddb-8e94-08160097f432 · 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 Do cosmological observations allow a negative $\Lambda$?

Reference 111

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

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Unavailable: canonical work link unavailable.

Observation 3b12916f-7ea0-4f97-8689-0ede07d21654 · 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 Do cosmological observations allow a negative $\Lambda$?

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-01T16:29:57.879187Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 66011e77-a55d-4f82-94e5-1e4789fe04b8 · inbound

Revisiting Metastable Dark Energy in Light of DESI DR2 BAO and DESI DR1 Full-Shape Measurements cites this paper.

Revisiting Metastable Dark Energy in Light of DESI DR2 BAO and DESI DR1 Full-Shape Measurements Do cosmological observations allow a negative $\Lambda$?

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-04T19:55:29.288416Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.