Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Hawking Radiation Spectra for Scalar Fields by a Higher-Dimensional Schwarzschild-de-Sitter Black Hole
As of 19 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 5 inbound Pith citation observations for arXiv:1604.08617.
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 2026-08-19T06:32:44.657259+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-14T14:46:37.931640Z
A source-named dated measurement, never combined with another source.
Source: pith, observed 2026-06-30T00:04:06.102492Z
Reference resolution
0 of 0 outbound references displayed
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- 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 b8d6f035-3972-451f-b2a6-9a080eeaabcf · inbound
Black Hole and Cosmological Particle Production in Schwarzschild de Sitter cites this paper.
Black Hole and Cosmological Particle Production in Schwarzschild de Sitter Hawking Radiation Spectra for Scalar Fields by a Higher-Dimensional Schwarzschild-de-Sitter Black Hole
Reference 57
- Resolution
- unresolved
- no resolver link, observed 2026-08-14T14:46:37.931640Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 9e48ed91-5621-4d81-8b1a-234dc6a72b41 · inbound
Correspondence between quasinormal modes and grey-body factors for massive fields in Schwarzschild-de Sitter spacetime cites this paper.
Correspondence between quasinormal modes and grey-body factors for massive fields in Schwarzschild-de Sitter spacetime Hawking Radiation Spectra for Scalar Fields by a Higher-Dimensional Schwarzschild-de-Sitter Black Hole
Reference 30
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T00:40:59.383241Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 3616138d-51c1-4bf7-aa90-9149bd0c957c · inbound
Charged black holes in Kalb-Ramond gravity: Weak Deflection Angle, Shadow cast, Quasinormal Modes and Neutrino annihilation cites this paper.
Charged black holes in Kalb-Ramond gravity: Weak Deflection Angle, Shadow cast, Quasinormal Modes and Neutrino annihilation Hawking Radiation Spectra for Scalar Fields by a Higher-Dimensional Schwarzschild-de-Sitter Black Hole
Reference 58
- Resolution
- unresolved
- no resolver link, observed 2026-08-07T14:46:36.874782Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation a02c13ec-e88b-4782-919d-ce27743dc271 · inbound
Grey-Body Factors and Thermodynamics of Asymptotically de Sitter Black Holes in Generalized Proca Theory cites this paper.
Grey-Body Factors and Thermodynamics of Asymptotically de Sitter Black Holes in Generalized Proca Theory Hawking Radiation Spectra for Scalar Fields by a Higher-Dimensional Schwarzschild-de-Sitter Black Hole
Reference 107
- Resolution
- verified exact
- local_arxiv, observed 2026-06-30T00:04:06.104468Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-19T06:32:44.657259+00:00.
Observation b1507b05-4cb4-49a2-b8eb-2e973f4830fd · inbound
Quasinormal modes of a quantum inspired black hole in four dimensions with cosmological constant cites this paper.
Quasinormal modes of a quantum inspired black hole in four dimensions with cosmological constant Hawking Radiation Spectra for Scalar Fields by a Higher-Dimensional Schwarzschild-de-Sitter Black Hole
Reference 33
- Resolution
- unresolved
- no resolver link, observed 2026-08-01T04:06:28.605837Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.