Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Can vacuum decay in our Universe?
As of 20 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:astro-ph/0408495.
A citation records a reference. It does not transfer a finding from one paper to another.
Coverage vector
One-hop event checks from named stored sources.
Source: scholarly_work_events, retraction_status_cache, observed 2026-08-20T06:33:59.587034+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-15T21:30:02.916187Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-08-05T02:28:24.338817Z
Reference resolution
0 of 0 outbound references displayed
- verified exact0
- verified fuzzy0
- unresolved0
- parse uncertain0
- malformed identifier0
- metadata mismatch0
External citation measurements
215
pith, observed 2026-08-05T02:28:24.338817Z
Outbound references
No outbound reference observations are available for this paper version.
Pith citing papers
Observation 8996c7ac-c604-420e-ad51-e02c887dbbf7 · inbound
New cosmological constraints on the evolution of dark matter energy density cites this paper.
New cosmological constraints on the evolution of dark matter energy density Can vacuum decay in our Universe?
Reference 36
- Resolution
- unresolved
- no resolver link, observed 2026-08-15T21:30:02.916187Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9f38b7b6-6817-43c2-b21d-5024f4a3fb61 · inbound
Generalizing the CPL Parametrization through Dark Sector Interaction cites this paper.
Generalizing the CPL Parametrization through Dark Sector Interaction Can vacuum decay in our Universe?
Reference 38
- Resolution
- verified exact
- arxiv_id, observed 2026-05-12T00:31:16.421559Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.
Observation 7360054a-eff4-4bb8-8d41-60509329f6a2 · inbound
Generalizing the CPL Parametrization through Dark Sector Interaction cites this paper.
Generalizing the CPL Parametrization through Dark Sector Interaction Can vacuum decay in our Universe?
Reference 38
- Resolution
- verified exact
- local_arxiv, observed 2026-05-21T08:34:05.832359Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.
Observation 5e21eaa6-c125-446f-94d0-a06fc5a0f9cf · inbound
Effective Phantom Dark Energy: What Cosmological Reconstruction Does and Does Not Imply cites this paper.
Effective Phantom Dark Energy: What Cosmological Reconstruction Does and Does Not Imply Can vacuum decay in our Universe?
Reference 140
- Resolution
- verified exact
- local_arxiv, observed 2026-06-29T15:33:32.428549Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.
Observation ff99fe3e-6039-4945-bb49-3b5eccc4eb98 · inbound
Running Vacuum in the expanding Universe: a unified QFT paradigm for Inflation and Dark Energy cites this paper.
Running Vacuum in the expanding Universe: a unified QFT paradigm for Inflation and Dark Energy Can vacuum decay in our Universe?
Reference 241
- Resolution
- verified exact
- local_arxiv, observed 2026-07-02T10:36:52.600101Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-20T06:33:59.587034+00:00.
Observation 9058507e-8880-413d-8837-f64b46ddf795 · inbound
Running Vacuum in the expanding Universe: a unified QFT paradigm for Inflation and Dark Energy cites this paper.
Running Vacuum in the expanding Universe: a unified QFT paradigm for Inflation and Dark Energy Can vacuum decay in our Universe?
Reference 241
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T15:09:17.581029Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.