Typed states for the displayed outbound observations.
Source: paper_references, paper_reference_links
Paper Citation Record · LEDGER
Flavor Triangle of the Diffuse Supernova Neutrino Background
As of 23 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 7 inbound Pith citation observations for arXiv:2011.10933.
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 2026-08-23T06:30:58.430688+00:00
Pith citing papers itemized under the disclosed page cap.
Source: paper_references, paper_reference_links, observed 2026-08-11T12:06:20.438959Z
A source-named dated measurement, never combined with another source.
Source: arxiv_reference, observed 2026-07-04T10:49:46.036736Z
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 e71805a6-9852-4368-a32d-1d13b3890152 · inbound
Diffuse Supernova Neutrino Background and Neutrino Non-Radiative Decay: a Bayesian Perspective cites this paper.
Diffuse Supernova Neutrino Background and Neutrino Non-Radiative Decay: a Bayesian Perspective Flavor Triangle of the Diffuse Supernova Neutrino Background
Reference 26
- Resolution
- unresolved
- no resolver link, observed 2026-08-11T12:06:20.438959Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation d7563d4d-f4ed-423e-8ff9-b2640c26faa0 · inbound
Dynamic Neutrino Mass Ordering and Its Imprint on the Diffuse Supernova Neutrino Background cites this paper.
Dynamic Neutrino Mass Ordering and Its Imprint on the Diffuse Supernova Neutrino Background Flavor Triangle of the Diffuse Supernova Neutrino Background
Reference 45
- Resolution
- unresolved
- no resolver link, observed 2026-08-10T13:30:00.619415Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 08c832b4-29b0-4384-85c7-2fcd41e5aab4 · inbound
Prospects for Neutrino Observation and Mass Measurement from Binary Neutron Star Mergers cites this paper.
Prospects for Neutrino Observation and Mass Measurement from Binary Neutron Star Mergers Flavor Triangle of the Diffuse Supernova Neutrino Background
Reference 74
- Resolution
- unresolved
- no resolver link, observed 2026-08-03T21:17:45.203674Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.
Observation 31595aa1-dd05-4757-bd8b-9da962321281 · inbound
Dark Matter Interpretation of the Super-Kamiokande Antineutrino Excess and Predictions for JUNO cites this paper.
Dark Matter Interpretation of the Super-Kamiokande Antineutrino Excess and Predictions for JUNO Flavor Triangle of the Diffuse Supernova Neutrino Background
Reference 26
- Resolution
- verified exact
- arxiv_id, observed 2026-05-20T04:08:03.034465Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.
Observation 0528abd1-381d-4872-a0f1-5932b04e3403 · inbound
Dark Matter Interpretation of the Super-Kamiokande Antineutrino Excess in $\mathrm{U}(1)_{L_\mu-L_\tau}$ model cites this paper.
Dark Matter Interpretation of the Super-Kamiokande Antineutrino Excess in $\mathrm{U}(1)_{L_\mu-L_\tau}$ model Flavor Triangle of the Diffuse Supernova Neutrino Background
Reference 5
- Resolution
- metadata mismatch
- arxiv_id, observed 2026-06-29T12:03:24.268533Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.
Observation 154899dd-5d6c-4e94-80c2-e36fe824329f · inbound
Diffuse Supernova Neutrinos with Secret Neutrino Interactions cites this paper.
Diffuse Supernova Neutrinos with Secret Neutrino Interactions Flavor Triangle of the Diffuse Supernova Neutrino Background
Reference 20
- Resolution
- verified exact
- arxiv_id, observed 2026-07-04T10:49:46.038084Z
Source-reported events for the cited work
No event found in the named queried sources as of 2026-08-23T06:30:58.430688+00:00.
Observation 36570163-4fcb-4892-aebe-d04d340c1f59 · inbound
A Unified Dark Matter Explanation for $\boldsymbol{B^+ \!\to K^+\nu\bar{\nu}}$ and the Super-Kamiokande Antineutrino Excess cites this paper.
A Unified Dark Matter Explanation for $\boldsymbol{B^+ \!\to K^+\nu\bar{\nu}}$ and the Super-Kamiokande Antineutrino Excess Flavor Triangle of the Diffuse Supernova Neutrino Background
Reference 22
- Resolution
- unresolved
- no resolver link, observed 2026-07-12T04:08:44.112644Z
Source-reported events for the cited work
Unavailable: canonical work link unavailable.