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Paper Citation Record · LEDGER

Fast Neutrino Flavor Conversions can Help and Hinder Neutrino-Driven Explosions

As of 14 August 2026, this Paper Citation Record lists 0 of 0 outbound references and 14 inbound Pith citation observations for arXiv:2305.11207.

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

pith.paper-citation-record.v1
2305.11207 v2

Coverage vector

measured 0 of 0 reference resolution

Typed states for the displayed outbound observations.

Source: paper_references, paper_reference_links

measured 14 of 14 standing notices

One-hop event checks from named stored sources.

Source: scholarly_work_events, retraction_status_cache, observed 2026-08-14T06:32:32.682623+00:00

measured 14 of 14 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-11T16:53:00.363856Z

measured 0 of 1 external citation measurements

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

Source: arxiv_reference, observed 2026-05-20T15:53:33.625425Z

Reference resolution

0 of 0 outbound references displayed

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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 47f69acc-d98f-4bc6-b61a-68606a281c70 · inbound

Neutrinos from explosive transients at the dawn of multi-messenger astronomy cites this paper.

Neutrinos from explosive transients at the dawn of multi-messenger astronomy Fast Neutrino Flavor Conversions can Help and Hinder Neutrino-Driven Explosions

Reference 11

Resolution
unresolved
no resolver link, observed 2026-08-11T16:53:00.363856Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T16:53:00.363856Z digest=sha256:67566d0fe3bc7263d2ef185dbc61632414b41446c383521879eb98becc253149

Observation 1ab02b77-b2f7-4961-a7d7-1e62ba788a28 · inbound

Pauli blocking: probing beyond-mean-field effects in neutrino flavor evolution cites this paper.

Pauli blocking: probing beyond-mean-field effects in neutrino flavor evolution Fast Neutrino Flavor Conversions can Help and Hinder Neutrino-Driven Explosions

Reference 26

Resolution
unresolved
no resolver link, observed 2026-08-11T14:21:07.667873Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T14:21:07.667873Z digest=sha256:b14d4cf4d7729f060d626388d6f578d6967d24dc3809d302c7192756700ab8f3

Observation 6fc84e96-175f-4f45-b538-344ee04ca6ce · inbound

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

Resolution requirements for numerical modeling of neutrino quantum kinetics Fast Neutrino Flavor Conversions can Help and Hinder Neutrino-Driven Explosions

Reference 12

Resolution
unresolved
no resolver link, observed 2026-08-10T15:26:59.369514Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-10T15:26:59.369514Z digest=sha256:b9372504d92e74213e068e0afe4f24a8d36fc58a8693471d36fb2e0da8a6c5fc

Observation 76902721-0c8c-4e30-8184-ce436ffc0a4e · inbound

Collective flavor conversions are interactions of neutrinos with quantized flavor waves cites this paper.

Collective flavor conversions are interactions of neutrinos with quantized flavor waves Fast Neutrino Flavor Conversions can Help and Hinder Neutrino-Driven Explosions

Reference 16

Resolution
unresolved
no resolver link, observed 2026-08-08T14:22:24.878560Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-08T14:22:24.878560Z digest=sha256:0748bbb858a6ba095e29084d2096fbb154ee9401bcffdb4a227131514a13749e

Observation 85835e6a-246b-4680-a11f-1e081e080528 · inbound

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

Predicting the outcome of collisional neutrino flavor conversion Fast Neutrino Flavor Conversions can Help and Hinder Neutrino-Driven Explosions

Reference 21

Resolution
unresolved
no resolver link, observed 2026-08-07T14:58:55.468967Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T14:58:55.468967Z digest=sha256:72f88bb71bb5156ab74892daeda0a5dc0058354af8bbb96c595b0e00fd643a06

Observation 988c4803-2f3e-4159-b9a3-a0036ee4978c · inbound

Comparative Testing of Subgrid Models for Fast Neutrino Flavor Conversions in Core-collapse Supernova Simulations cites this paper.

Comparative Testing of Subgrid Models for Fast Neutrino Flavor Conversions in Core-collapse Supernova Simulations Fast Neutrino Flavor Conversions can Help and Hinder Neutrino-Driven Explosions

Reference 74

Resolution
unresolved
no resolver link, observed 2026-08-07T05:49:20.628901Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-07T05:49:20.628901Z digest=sha256:92b60164f05261db01a14553e8a72ce77db9fd1e2a5765e1f04a4933a2c3d4cd

Observation 8e76a3eb-04b3-407d-9c63-57349ff666e5 · 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 Fast Neutrino Flavor Conversions can Help and Hinder Neutrino-Driven Explosions

Reference 11

Resolution
unresolved
no resolver link, observed 2026-08-06T16:29:11.382664Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-06T16:29:11.382664Z digest=sha256:699c109a778ca304b46fb88aca6b54d46e9e743cef6fbffbfa2a8cdd49c0f04b

Observation c9820842-46f3-4eb6-be18-a172086d6bb4 · inbound

Bifurcated Impact of Neutrino Fast Flavor Conversion on Core-collapse Supernovae Informed by Multi-angle Neutrino Radiation Hydrodynamics cites this paper.

Bifurcated Impact of Neutrino Fast Flavor Conversion on Core-collapse Supernovae Informed by Multi-angle Neutrino Radiation Hydrodynamics Fast Neutrino Flavor Conversions can Help and Hinder Neutrino-Driven Explosions

Reference 16

Resolution
verified exact
arxiv_id, observed 2026-05-16T15:31:04.360878Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-05-16T15:30:29.222217Z digest=sha256:0f92017bb19e26d6bc8288f5220e0113c6f0f483b0f17f1dab7603d35fd8c1e8

Observation fc013b71-8bec-4e36-baac-85f7b7c59219 · inbound

Intermittent Turbulence, Fast Flavor Conversion, and Observable Supernova Probes cites this paper.

Intermittent Turbulence, Fast Flavor Conversion, and Observable Supernova Probes Fast Neutrino Flavor Conversions can Help and Hinder Neutrino-Driven Explosions

Reference 4

Resolution
verified exact
arxiv_id, observed 2026-05-16T13:37:57.382782Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-05-16T13:32:59.244112Z digest=sha256:604cbd793766bae7d0b974ae211b05be6152b17b6ac25c1e0ac02e697b9afa79

Observation 9493dda3-ff84-4d7e-9b43-ca260d5cda5b · inbound

Collective neutrino-antineutrino pair oscillations cites this paper.

Collective neutrino-antineutrino pair oscillations Fast Neutrino Flavor Conversions can Help and Hinder Neutrino-Driven Explosions

Reference 41

Resolution
verified exact
arxiv_id, observed 2026-05-11T23:56:16.100158Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-05-07T15:58:06.378902Z digest=sha256:eff7f769cfeb7edd722276332d9a42ea61d7b0b00e32c9f4aa0b1c5e19cda4b4

Observation 90091c98-6a25-40c0-bbb0-065537b00b2f · inbound

Neutrino Flavor Conversion Shapes the Rate of Failed Core-collapse Supernovae cites this paper.

Neutrino Flavor Conversion Shapes the Rate of Failed Core-collapse Supernovae Fast Neutrino Flavor Conversions can Help and Hinder Neutrino-Driven Explosions

Reference 55

Resolution
verified exact
arxiv_id, observed 2026-05-20T15:53:33.626816Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-05-20T15:53:30.768047Z digest=sha256:3ac8c884ea9335a6ec742aedf2f99c43cc3ae4172bd9ee3751e7a8bda027f82c

Observation 7498ce0a-2b7e-4e8f-bf9d-21c11dccb136 · inbound

Flavor Conversion Enhances or Suppresses Supernova Explodability Independent of the Progenitor Mass cites this paper.

Flavor Conversion Enhances or Suppresses Supernova Explodability Independent of the Progenitor Mass Fast Neutrino Flavor Conversions can Help and Hinder Neutrino-Driven Explosions

Reference 57

Resolution
verified exact
arxiv_id, observed 2026-05-20T08:13:08.452284Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-14T06:32:32.682623+00:00.

source=pdf_text observed=2026-05-20T08:10:13.936279Z digest=sha256:d8eeb408c54882459dffb2f18c589eb843971913379f5585a8d4612a4311dc75

Observation 3010200b-4833-4499-9fed-274449a8b511 · inbound

Solar-System Abundances of $p$-Nuclides Probe Collective Neutrino Oscillations in Supernovae cites this paper.

Solar-System Abundances of $p$-Nuclides Probe Collective Neutrino Oscillations in Supernovae Fast Neutrino Flavor Conversions can Help and Hinder Neutrino-Driven Explosions

Reference 66

Resolution
unresolved
no resolver link, observed 2026-08-01T23:35:16.739772Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-01T23:35:16.739772Z digest=sha256:e8f5f9923eed1f87e92d5e9223d93a16a72444fcb6c1198c1d2cc65259f54654

Observation 8db8bda9-163e-4ef4-a8d0-efcb17cf3270 · inbound

Neutrino quantum kinetics for fast flavor conversion in a time-dependent environment cites this paper.

Neutrino quantum kinetics for fast flavor conversion in a time-dependent environment Fast Neutrino Flavor Conversions can Help and Hinder Neutrino-Driven Explosions

Reference 29

Resolution
unresolved
no resolver link, observed 2026-08-11T00:25:59.382448Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

source=pdf_text observed=2026-08-11T00:25:59.382448Z digest=sha256:8573f07372bae606145329eb6612a50ed677f3ba640164542cabb76654b6a0fe