Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links, observed 2026-08-16T00:21:02.272576Z
Paper Citation Record · LEDGER
Why There is No Memory Burden in Holographic Space-time Models of Black Hole Formation and Evaporation
As of 19 August 2026, this Paper Citation Record lists 14 of 14 outbound references and 0 inbound Pith citation observations for arXiv:2608.12139.
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 2026-08-18T06:34:40.430872+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links
A source-named dated measurement, never combined with another source.
Source: cited_works
Reference resolution
14 of 14 outbound references displayed
- verified exact3
- verified fuzzy1
- unresolved9
- parse uncertain0
- malformed identifier1
- metadata mismatch0
External citation measurements
No source-named external measurement is stored.
Outbound references
Observation 3bdfefc0-5af1-4d3c-bf92-b8164ac97bf8 · outbound
This paper cites Black Hole Memory Burden and its Signatures in Gravitational Waves from Mergers.
Why There is No Memory Burden in Holographic Space-time Models of Black Hole Formation and Evaporation Black Hole Memory Burden and its Signatures in Gravitational Waves from Mergers
Reference 1
- Resolution
- verified exact
- local_arxiv, observed 2026-08-16T00:21:02.657006Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation e8e63fc6-f773-4600-a988-c19b46947253 · outbound
This paper cites Holographic Space-time, Newton`s Law, and the Dynamics of Horizons.
Why There is No Memory Burden in Holographic Space-time Models of Black Hole Formation and Evaporation Holographic Space-time, Newton`s Law, and the Dynamics of Horizons
Reference 2
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T00:21:02.210024Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation f81c87b4-5f71-4463-a691-cf309623b9e7 · outbound
This paper cites Noncommutative geometry,.
Why There is No Memory Burden in Holographic Space-time Models of Black Hole Formation and Evaporation Noncommutative geometry,
Reference 3
- Resolution
- verified fuzzy
- raw_fallback, observed 2026-08-16T00:21:02.673358Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation 0dc9259c-7d49-4468-ade6-dbb9d10e64bb · outbound
This paper cites Black Hole Entropy from Conformal Field Theory in Any Dimension.
Why There is No Memory Burden in Holographic Space-time Models of Black Hole Formation and Evaporation Black Hole Entropy from Conformal Field Theory in Any Dimension
Reference 4
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T00:21:02.220864Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 07d87f50-2d42-42b6-91e2-29276fa6b7fc · outbound
This paper cites Conformal Description of Near-Horizon Vacuum States.
Why There is No Memory Burden in Holographic Space-time Models of Black Hole Formation and Evaporation Conformal Description of Near-Horizon Vacuum States
Reference 5
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T00:21:02.226806Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ac1ba7e3-cda5-4148-9ef9-d60fe9ff579e · outbound
This paper cites Microscopic quantum mechanics of the p = rho universe,.
Why There is No Memory Burden in Holographic Space-time Models of Black Hole Formation and Evaporation Microscopic quantum mechanics of the p = rho universe,
Reference 6
- Resolution
- verified exact
- raw_fallback, observed 2026-08-16T00:21:02.591531Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation bf31c07c-da03-41a3-904a-290f9933b8e0 · outbound
This paper cites Hilbert Bundles and Holographic Space-time: the Hydrodynamic Approach to Gravity.
Why There is No Memory Burden in Holographic Space-time Models of Black Hole Formation and Evaporation Hilbert Bundles and Holographic Space-time: the Hydrodynamic Approach to Gravity
Reference 7
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T00:21:02.237544Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation cd8370bf-d95f-4abc-96f7-4cb0eb39cc81 · outbound
This paper cites CONFORMAL SUPERGRAV- ITY, TWISTORS AND THE SUPER BMS GROUP,.
Why There is No Memory Burden in Holographic Space-time Models of Black Hole Formation and Evaporation CONFORMAL SUPERGRAV- ITY, TWISTORS AND THE SUPER BMS GROUP,
Reference 8
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T00:21:02.243099Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 479a477c-8cb9-4975-b78b-7eb531c00a98 · outbound
This paper cites Holography and Cosmology.
Why There is No Memory Burden in Holographic Space-time Models of Black Hole Formation and Evaporation Holography and Cosmology
Reference 9
- Resolution
- malformed identifier
- no resolver link, observed 2026-08-16T00:21:02.249404Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a01e79b5-b216-4ffb-9691-89c7a3274600 · outbound
This paper cites AdS3 Black Holes and a Stringy Exclusion Principle.
Why There is No Memory Burden in Holographic Space-time Models of Black Hole Formation and Evaporation AdS3 Black Holes and a Stringy Exclusion Principle
Reference 10
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T00:21:02.254669Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3dc77ef0-5750-42c5-92e4-aa7a627cbeb5 · outbound
This paper cites Effective Field Theory, Black Holes, and the Cosmological Constant.
Why There is No Memory Burden in Holographic Space-time Models of Black Hole Formation and Evaporation Effective Field Theory, Black Holes, and the Cosmological Constant
Reference 11
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T00:21:02.259470Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation ee37d696-7915-48f3-b0c8-85fd54a57be6 · outbound
This paper cites On the Quantum Structure of a Black Hole,.
Why There is No Memory Burden in Holographic Space-time Models of Black Hole Formation and Evaporation On the Quantum Structure of a Black Hole,
Reference 12
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T00:21:02.263833Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a92d3daf-7041-4dd0-956f-2464c0266172 · outbound
This paper cites Divergences problem in black hole brick-wall model.
Why There is No Memory Burden in Holographic Space-time Models of Black Hole Formation and Evaporation Divergences problem in black hole brick-wall model
Reference 13
- Resolution
- verified exact
- local_arxiv, observed 2026-08-16T00:21:02.353679Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-18T06:34:40.430872+00:00.
Observation a5a8ebd4-199d-4a2f-8bb8-bb852ad734c4 · outbound
This paper cites Black Holes: Complementarity or Firewalls?.
Why There is No Memory Burden in Holographic Space-time Models of Black Hole Formation and Evaporation Black Holes: Complementarity or Firewalls?
Reference 14
- Resolution
- unresolved
- no resolver link, observed 2026-08-16T00:21:02.272576Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Pith citing papers
No inbound Pith citation observations are available.