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Paper Citation Record · LEDGER

Dissipative $\Lambda$CDM model with causal sign-switching bulk viscous pressure

As of 21 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:2409.10919.

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

pith.paper-citation-record.v1
2409.10919 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 5 of 5 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-21T06:32:19.484+00:00

measured 5 of 5 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-16T05:58:50.798315Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-21T13:30:12.601830Z

Reference resolution

0 of 0 outbound references displayed

  • verified exact0
  • verified fuzzy0
  • unresolved0
  • parse uncertain0
  • malformed identifier0
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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 e8991389-b379-45bc-82bf-8cc0c4306707 · inbound

Observational constraints in late time for an axially symmetric transitioning model with bulk viscous fluid cites this paper.

Observational constraints in late time for an axially symmetric transitioning model with bulk viscous fluid Dissipative $\Lambda$CDM model with causal sign-switching bulk viscous pressure

Reference 44

Resolution
unresolved
no resolver link, observed 2026-08-16T05:58:50.798315Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-16T05:58:50.798315Z digest=sha256:95736cf5112d166e36ebfb2ebfed206c597e15f93290be0626502107c678e79f

Observation 3ab95a55-ef53-42cf-8493-7cdb6cfc570b · 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 Dissipative $\Lambda$CDM model with causal sign-switching bulk viscous pressure

Reference 208

Resolution
verified exact
arxiv_id, observed 2026-05-18T04:50:54.856284Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-05-18T04:46:14.832965Z digest=sha256:c32fe5eb819b5d76ea3d543d836c860c7fbdee6953cf704c6eb2b56bd8e8187f

Observation 0f34b6bc-0ace-4388-8d9c-e5d2c1998b8f · 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 Dissipative $\Lambda$CDM model with causal sign-switching bulk viscous pressure

Reference 152

Resolution
verified exact
arxiv_id, observed 2026-05-21T13:30:12.603790Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-21T06:32:19.484+00:00.

source=pdf_text observed=2026-05-21T13:29:05.147292Z digest=sha256:08dd6bcd1edaa4e61c26aeacf17acb75ade312c6e806a8439ded3552b4698cde

Observation 5e8762b0-5e09-4863-a40a-70ba30c14c0e · 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 Dissipative $\Lambda$CDM model with causal sign-switching bulk viscous pressure

Reference 161

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:de281ea84a7c25424946118a805096b70c01f2c91dc7d32cff40b1011d38b65e

Observation ec033137-5022-4931-bac8-39426fa09ecc · 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 Dissipative $\Lambda$CDM model with causal sign-switching bulk viscous pressure

Reference 138

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=sha256:2f9a83ebd8fd6007c96933bd85a87fe635a22bc3d339b7087863a1b71dd30ed9