Pith. sign in

Paper Citation Record · LEDGER

Anti-de Sitter $\to$ de Sitter transition driven by Casimir forces and mitigating tensions in cosmological parameters

As of 8 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 14 inbound Pith citation observations for arXiv:2312.12352.

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

pith.paper-citation-record.v1
2312.12352 v4

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 14 of 14 standing notices

One-hop event checks from named stored sources.

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

measured 14 of 14 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-07T01:08:41.653809Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-07-03T07:07:44.888177Z

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 d395a39b-9d66-4739-b81d-6a9f9f0c5774 · 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 Anti-de Sitter $\to$ de Sitter transition driven by Casimir forces and mitigating tensions in cosmological parameters

Reference 85

Resolution
verified exact
arxiv_id, observed 2026-05-24T03:53:54.697778Z

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.

source=pdf_text observed=2026-05-24T03:50:50.435997Z digest=sha256:66ec3e837c70b8048732175bc0281c30e099f261e65f713f10a9d4a167d89bff

Observation 312e0751-490d-492e-a4d2-7a620cfa437a · inbound

Cosmographic analysis of sign-switching dark energy cites this paper.

Cosmographic analysis of sign-switching dark energy Anti-de Sitter $\to$ de Sitter transition driven by Casimir forces and mitigating tensions in cosmological parameters

Reference 71

Resolution
unresolved
no resolver link, observed 2026-08-07T01:08:41.653809Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T01:08:41.653809Z digest=sha256:3cabc0e8f70bee1929fdfb388a7918bc8a7604a9633784d800e3c4f867951e04

Observation cd47559c-04b5-4663-886c-f4ad64c2eddc · 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 Anti-de Sitter $\to$ de Sitter transition driven by Casimir forces and mitigating tensions in cosmological parameters

Reference 189

Resolution
verified exact
arxiv_id, observed 2026-05-18T04:50:54.718323Z

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.

source=pdf_text observed=2026-05-18T04:46:14.832965Z digest=sha256:933b8a70356d30b21dd0cb82cd28d3efae372bbf354769b2a1c6a4799a2cc52a

Observation 75dbacd7-40bf-4e40-8378-e730fe8ed114 · inbound

Towards a unified quantum field theory of dark energy and inflation: unstable de Sitter vacuum and running vacuum cites this paper.

Towards a unified quantum field theory of dark energy and inflation: unstable de Sitter vacuum and running vacuum Anti-de Sitter $\to$ de Sitter transition driven by Casimir forces and mitigating tensions in cosmological parameters

Reference 64

Resolution
unresolved
no resolver link, observed 2026-08-03T11:53:06.038754Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-03T11:53:06.038754Z digest=sha256:bb6b85a00ce103e003948f3e317862e428472bb43083e8db728845d4a8eba652

Observation e7ee59e6-5fa8-4d1d-af1f-661f4887fddc · 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 Anti-de Sitter $\to$ de Sitter transition driven by Casimir forces and mitigating tensions in cosmological parameters

Reference 89

Resolution
verified exact
arxiv_id, observed 2026-05-21T13:30:12.573311Z

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.

source=pdf_text observed=2026-05-21T13:29:05.147292Z digest=sha256:0385c5566ca4cb440ff6177e7ab6be93e49315dd7a24e386440ad438eeda443d

Observation 43127ded-6e28-4068-bb9b-ebfca809fa20 · inbound

Sign-Switching Dark Energy: Smooth Transitions with Recent DESI DR2 Observations cites this paper.

Sign-Switching Dark Energy: Smooth Transitions with Recent DESI DR2 Observations Anti-de Sitter $\to$ de Sitter transition driven by Casimir forces and mitigating tensions in cosmological parameters

Reference 100

Resolution
verified exact
arxiv_id, observed 2026-05-16T05:20:39.634366Z

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.

source=pdf_text observed=2026-05-16T05:18:35.958352Z digest=sha256:fdf3b5d7b3b6ddbec23cd6d42c8508068509f63047494d2dbb4d9958e6dc1b13

Observation 08c4ccee-6c89-4aa2-99fb-854ff3641d38 · inbound

Statistical consistency of sign-switching vacuum energy with cosmological observations cites this paper.

Statistical consistency of sign-switching vacuum energy with cosmological observations Anti-de Sitter $\to$ de Sitter transition driven by Casimir forces and mitigating tensions in cosmological parameters

Reference 56

Resolution
unresolved
no resolver link, observed 2026-08-02T18:35:52.277354Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-02T18:35:52.277354Z digest=sha256:84623a754d2f39782005c7da01284319a32fd138d3c7e7e06b71504f9398dcd3

Observation 465952fe-c213-4c43-b465-2444071b20c0 · 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 Anti-de Sitter $\to$ de Sitter transition driven by Casimir forces and mitigating tensions in cosmological parameters

Reference 98

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-15T12:01:04.317365Z digest=sha256:0f47a54cc7528be68e7bcb21d5dbbcd4b2dd3e61edd708014d7ddf588ab00f68

Observation 67d29d32-5120-482a-b3fb-19d4a6d87238 · inbound

Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe? cites this paper.

Do equation of state parametrizations of dark energy faithfully capture the dynamics of the late universe? Anti-de Sitter $\to$ de Sitter transition driven by Casimir forces and mitigating tensions in cosmological parameters

Reference 50

Resolution
verified exact
arxiv_id, observed 2026-05-10T14:15:30.030201Z

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.

source=pdf_text observed=2026-05-10T14:10:57.749079Z digest=sha256:026381f2a13527a4655d92c7064334ac7475a4ff87569887da5d26261b7fbfd6

Observation 9d4d4374-58ed-44e5-8825-000539f15a68 · inbound

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

Negative neutrino mass or negative dark energy? Anti-de Sitter $\to$ de Sitter transition driven by Casimir forces and mitigating tensions in cosmological parameters

Reference 84

Resolution
verified exact
arxiv_id, observed 2026-05-21T03:03:55.821011Z

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.

source=pdf_text observed=2026-05-21T03:03:07.191130Z digest=sha256:a70e523e6e19c3b1ffac0273307597f4b3fa969076d36c82dbfdbdd238c69407

Observation a4a724f2-b3d8-4b78-b88b-bd6688716875 · 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 Anti-de Sitter $\to$ de Sitter transition driven by Casimir forces and mitigating tensions in cosmological parameters

Reference 85

Resolution
verified exact
arxiv_id, observed 2026-07-02T15:37:06.386989Z

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.

source=pdf_text observed=2026-06-27T23:47:15.644279Z digest=sha256:65d6c90c5ad3822fa8aa6dec2662388efdecb7ae43e1cefc4d659555ef94f8ff

Observation b404f501-31ca-49b1-9b16-87dd0904d646 · inbound

Endpoint Logarithms in the NLO Mueller-Navelet Jet Vertex: Threshold Matching and BLM/MOM Prescription Sensitivity cites this paper.

Endpoint Logarithms in the NLO Mueller-Navelet Jet Vertex: Threshold Matching and BLM/MOM Prescription Sensitivity Anti-de Sitter $\to$ de Sitter transition driven by Casimir forces and mitigating tensions in cosmological parameters

Reference 22

Resolution
unresolved
no resolver link, observed 2026-07-12T14:25:03.782538Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-12T14:25:03.782538Z digest=sha256:12c2bbd02cd689ca4b7e1fd3842c2df0dbc583f904ce3933627bd57b2dca7669

Observation 3cc2a7e1-f644-4c90-92d3-766389998afe · inbound

A Friendly Phantom: Late-time AdS-to-dS transition and cosmological tensions cites this paper.

A Friendly Phantom: Late-time AdS-to-dS transition and cosmological tensions Anti-de Sitter $\to$ de Sitter transition driven by Casimir forces and mitigating tensions in cosmological parameters

Reference 22

Resolution
verified exact
arxiv_id, observed 2026-07-03T07:07:44.889699Z

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.

source=pdf_text observed=2026-06-27T12:16:15.909335Z digest=sha256:b34b2cb9e46ac4d9167c1baa9744c5d504f4f66649614cfac95dfcbf89b90ecf

Observation 00f16fda-b4b3-4312-94b4-21f3673b043e · 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 Anti-de Sitter $\to$ de Sitter transition driven by Casimir forces and mitigating tensions in cosmological parameters

Reference 77

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

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-07-11T09:40:49.196932Z digest=sha256:0074210ff2ba711d94a266b15ba75567875af321dba9078eef98dd3531e066c7