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Paper Citation Record · LEDGER

Do Neutrinos Become Flavor Unstable Due to Collisions with Matter in the Supernova Decoupling Region?

As of 10 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 6 inbound Pith citation observations for arXiv:2307.10366.

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

pith.paper-citation-record.v1
2307.10366 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 6 of 6 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-10T06:31:04.303077+00:00

measured 6 of 6 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-10T15:26:59.483200Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-11T00:20:53.302343Z

Reference resolution

0 of 0 outbound references displayed

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  • verified fuzzy0
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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 70de5762-9e1a-4bd6-b5c8-9982ced20fe8 · inbound

Resolution requirements for numerical modeling of neutrino quantum kinetics cites this paper.

Resolution requirements for numerical modeling of neutrino quantum kinetics Do Neutrinos Become Flavor Unstable Due to Collisions with Matter in the Supernova Decoupling Region?

Reference 35

Resolution
unresolved
no resolver link, observed 2026-08-10T15:26:59.483200Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T15:26:59.483200Z digest=sha256:04a83791cf8a42bfc5a98fd862bf65aa0402f66edb5b138ef6de66539eb16f07

Observation 5356f35d-7100-4d2f-a9e6-2d04f9973f6c · inbound

Predicting the outcome of collisional neutrino flavor conversion cites this paper.

Predicting the outcome of collisional neutrino flavor conversion Do Neutrinos Become Flavor Unstable Due to Collisions with Matter in the Supernova Decoupling Region?

Reference 58

Resolution
unresolved
no resolver link, observed 2026-08-07T14:59:00.241458Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:59:00.241458Z digest=sha256:91f5c38023edbc021f0c8e84d0c526d2cb8521baaf00ae67fd062e5373e0c64c

Observation ded915fc-4628-4de9-8e37-a48f1bf5fa3f · inbound

Electron-neutrino lepton number crossings: Variations with the supernova core physics cites this paper.

Electron-neutrino lepton number crossings: Variations with the supernova core physics Do Neutrinos Become Flavor Unstable Due to Collisions with Matter in the Supernova Decoupling Region?

Reference 38

Resolution
unresolved
no resolver link, observed 2026-08-06T16:29:14.997843Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T16:29:14.997843Z digest=sha256:7a3574c6e7653c25c3ec5282d0959f6b024943ac9515839e3f476a3f1048a288

Observation a2665aea-7572-45b8-b8b4-1fe45ab14983 · inbound

Neutrino transport and flavor instabilities in a post-merger disk cites this paper.

Neutrino transport and flavor instabilities in a post-merger disk Do Neutrinos Become Flavor Unstable Due to Collisions with Matter in the Supernova Decoupling Region?

Reference 59

Resolution
verified exact
arxiv_id, observed 2026-05-11T00:20:53.307731Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-10T06:31:04.303077+00:00.

source=pdf_text observed=2026-05-10T18:35:42.044621Z digest=sha256:fe23ea24b45b55d0f15db0266db0ea53d4ebc96fa451e94e7c838c02195137ef

Observation 75b5ca3a-3ed4-4e08-9f89-0995577b1dd6 · inbound

Neutrino flavor-wave transport: Numerical tests and theoretical challenges cites this paper.

Neutrino flavor-wave transport: Numerical tests and theoretical challenges Do Neutrinos Become Flavor Unstable Due to Collisions with Matter in the Supernova Decoupling Region?

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-08T04:27:02.023018Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T04:27:02.023018Z digest=sha256:b36fb4600482c94c0cd0b3ca8b8b68b9eb4e4e2a9bd200d0d570f62535853c1e

Observation d19d6ed2-e1c0-49aa-84a8-5ba9baa24298 · inbound

Neutrino flavor-wave transport: Numerical tests and theoretical challenges cites this paper.

Neutrino flavor-wave transport: Numerical tests and theoretical challenges Do Neutrinos Become Flavor Unstable Due to Collisions with Matter in the Supernova Decoupling Region?

Reference 46

Resolution
unresolved
no resolver link, observed 2026-08-10T04:32:48.735974Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T04:32:48.735974Z digest=sha256:51b43fc15721b63bd838c06ecb64ebacbe90b091285b0384165f81770ae4cbce