Paper Citation Record · LEDGER

Boomerang mechanism explaining the excess radio background

As of 13 August 2026, this Paper Citation Record lists 72 of 72 outbound references and 4 inbound Pith citation observations for arXiv:2509.03441.

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

pith.paper-citation-record.v1
2509.03441 v3

Coverage vector

measured 72 of 72 reference resolution

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Source: paper_references, paper_reference_links, observed 2026-08-05T11:02:37.232998Z

measured 76 of 76 standing notices

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Source: scholarly_work_events, retraction_status_cache, observed 2026-08-13T06:32:02.005865+00:00

measured 4 of 4 inbound itemization

Pith citing papers itemized under the disclosed page cap.

Source: paper_references, paper_reference_links, observed 2026-08-02T10:27:06.369020Z

measured 0 of 1 external citation measurements

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

Source: pith, observed 2026-07-04T18:20:05.178090Z

Reference resolution

72 of 72 outbound references displayed

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External citation measurements

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Outbound references

Observation fdc4f5b4-0b26-4ae5-a9e7-5975ee10a0a0 · outbound

This paper cites ARCADE 2 Measurement of the Extra-Galactic Sky Temperature at 3-90 GHz.

Boomerang mechanism explaining the excess radio background ARCADE 2 Measurement of the Extra-Galactic Sky Temperature at 3-90 GHz

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.013000Z

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Observation 70725b1c-5bf9-4d97-953e-dc1e8ba1313c · outbound

This paper cites The Radio Synchrotron Background: Conference Summary and Report.

Boomerang mechanism explaining the excess radio background The Radio Synchrotron Background: Conference Summary and Report

Reference 2

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.017543Z

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Observation 2f9f71a2-5216-4dc1-8f0d-cbe1194dcdba · outbound

This paper cites The unusual smoothness of the extragalactic unresolved radio background.

Boomerang mechanism explaining the excess radio background The unusual smoothness of the extragalactic unresolved radio background

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.021179Z

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Observation fdbda20d-43ea-49b7-a29e-478a04a1287f · outbound

This paper cites an unresolved cited work.

Boomerang mechanism explaining the excess radio background Unresolved cited work

Reference 4

Resolution: unresolved; raw_fallback, observed 2026-08-05T11:02:38.149220Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 6533dcc5-e7d0-4b35-8b57-dc3953c7f41e · outbound

This paper cites The optical system of the Tenerife Microwave Spectrometer: a window for observing the 10-20 GHz sky spectra.

Boomerang mechanism explaining the excess radio background The optical system of the Tenerife Microwave Spectrometer: a window for observing the 10-20 GHz sky spectra

Reference 5

Resolution: verified exact; local_arxiv, observed 2026-08-05T11:02:37.978984Z

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No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation e6e56174-1e23-4cc8-872b-0612101c5b50 · outbound

This paper cites Probing relic neutrino decays with 21 cm cosmology.

Boomerang mechanism explaining the excess radio background Probing relic neutrino decays with 21 cm cosmology

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.031776Z

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Observation 2bc3febe-eea2-4181-8957-526030f8f186 · outbound

This paper cites Relic neutrino decay solution to the excess radio background.

Boomerang mechanism explaining the excess radio background Relic neutrino decay solution to the excess radio background

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.035173Z

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Observation 7cd68e3f-8f1e-4c70-a4ed-97f2f0e420ad · outbound

This paper cites The Temperature of the Cosmic Microwave Background.

Boomerang mechanism explaining the excess radio background The Temperature of the Cosmic Microwave Background

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.038564Z

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Observation f45e4221-7f66-415b-84aa-b07baec81149 · outbound

This paper cites The Radio Background Below 100 MHz.

Boomerang mechanism explaining the excess radio background The Radio Background Below 100 MHz

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.042180Z

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Observation 5b1e981c-a676-4b4e-aca3-c37336e3babb · outbound

This paper cites Xing and S.

Boomerang mechanism explaining the excess radio background Xing and S

Reference 10

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T11:02:38.140349Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation dcac9186-74ae-43fc-a253-27538c6d15f0 · outbound

This paper cites Neutrino electromagnetic interactions: a window to new physics.

Boomerang mechanism explaining the excess radio background Neutrino electromagnetic interactions: a window to new physics

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.048217Z

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Observation 8ccb4203-6191-445b-97f7-832fb2920b28 · outbound

This paper cites an unresolved cited work.

Boomerang mechanism explaining the excess radio background Unresolved cited work

Reference 12

Resolution: unresolved; raw_fallback, observed 2026-08-05T11:02:38.131008Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation e42997b8-844d-4a10-9e3f-5ad8bfe06580 · outbound

This paper cites Axion and neutrino bounds improved with new calibrations of the tip of the red-giant branch using geometric distance determinations.

Boomerang mechanism explaining the excess radio background Axion and neutrino bounds improved with new calibrations of the tip of the red-giant branch using geometric distance determinations

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.054784Z

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Observation e707aab5-2b15-415a-b589-f22e70b4b341 · outbound

This paper cites Upper limit on the neutrino magnetic moment from three years of data from the GEMMA spectrometer.

Boomerang mechanism explaining the excess radio background Upper limit on the neutrino magnetic moment from three years of data from the GEMMA spectrometer

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.058014Z

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Observation abeb292d-a832-4352-ab5a-9c3a84abfcca · outbound

This paper cites an unresolved cited work.

Boomerang mechanism explaining the excess radio background Unresolved cited work

Reference 15

Resolution: unresolved; raw_fallback, observed 2026-08-05T11:02:38.122237Z

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No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 2f7212da-cf37-42ad-b666-50e20e8da79d · outbound

This paper cites The net result is that neutrinos are converted into photons.

Boomerang mechanism explaining the excess radio background The net result is that neutrinos are converted into photons

Reference 16

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T11:02:38.112903Z

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No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation c40c1d48-1615-4a2b-8f82-d9b2f6f23eec · outbound

This paper cites an unresolved cited work.

Boomerang mechanism explaining the excess radio background Unresolved cited work

Reference 17

Resolution: unresolved; raw_fallback, observed 2026-08-05T11:02:38.103751Z

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No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 1ec6a478-783c-4b01-b066-7962e1374a2b · outbound

This paper cites N¨ otzold and G.

Boomerang mechanism explaining the excess radio background N¨ otzold and G

Reference 18

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T11:02:38.095234Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 64806d31-d205-4ea2-b1fc-275a0e95f8a1 · outbound

This paper cites Large neutrino asymmetries from neutrino oscillations.

Boomerang mechanism explaining the excess radio background Large neutrino asymmetries from neutrino oscillations

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.072663Z

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Observation 92246849-1862-4958-9f13-1c837b244f7e · outbound

This paper cites Active-sterile neutrino oscillations in the early Universe: asymmetry generation at low |delta m^2| and the Landau-Zener approximation.

Boomerang mechanism explaining the excess radio background Active-sterile neutrino oscillations in the early Universe: asymmetry generation at low |delta m^2| and the Landau-Zener approximation

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.075763Z

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Observation f1fad09e-da60-4a0f-97f4-d08c6f9cec49 · outbound

This paper cites Enqvist, K.

Boomerang mechanism explaining the excess radio background Enqvist, K

Reference 21

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T11:02:38.086274Z

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No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 382f7a48-dcaf-4982-8740-45970e37347a · outbound

This paper cites Microwave Background Constraints on Mixing of Photons with Hidden Photons.

Boomerang mechanism explaining the excess radio background Microwave Background Constraints on Mixing of Photons with Hidden Photons

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.081193Z

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Observation 00248eae-0010-44cc-9fb6-94aafb85afd0 · outbound

This paper cites Dark Photon Oscillations in Our Inhomogeneous Universe.

Boomerang mechanism explaining the excess radio background Dark Photon Oscillations in Our Inhomogeneous Universe

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.084108Z

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Observation 924480ba-a9d9-46dd-a975-865b796c4a25 · outbound

This paper cites Effective photon mass and (dark) photon conversion in the inhomogeneous Universe.

Boomerang mechanism explaining the excess radio background Effective photon mass and (dark) photon conversion in the inhomogeneous Universe

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.086994Z

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Observation 31a36a13-b654-42da-890b-b6b591af6d06 · outbound

This paper cites Shaping Dark Photon Spectral Distortions.

Boomerang mechanism explaining the excess radio background Shaping Dark Photon Spectral Distortions

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.090047Z

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Observation 9d7c9098-e612-445b-afc9-e0b9b3e9fe84 · outbound

This paper cites an unresolved cited work.

Boomerang mechanism explaining the excess radio background Unresolved cited work

Reference 26

Resolution: unresolved; raw_fallback, observed 2026-08-05T11:02:38.077372Z

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No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 8bed0e6c-64e7-40d9-8312-7a7041b06d7a · outbound

This paper cites Cosmological bounds on neutrino degeneracy improved by flavor oscillations.

Boomerang mechanism explaining the excess radio background Cosmological bounds on neutrino degeneracy improved by flavor oscillations

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.096350Z

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Observation a91033a1-0c79-46e9-a966-82e04b18ecee · outbound

This paper cites Neutrino Electromagnetic Properties.

Boomerang mechanism explaining the excess radio background Neutrino Electromagnetic Properties

Reference 28

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Observation 1139f80e-2f72-41d0-bbe2-0dd94a70bd9b · outbound

This paper cites Indications for a Nonzero Lepton Asymmetry from Extremely Metal-Poor Galaxies.

Boomerang mechanism explaining the excess radio background Indications for a Nonzero Lepton Asymmetry from Extremely Metal-Poor Galaxies

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.101984Z

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Observation 2540358b-73ef-4f8c-9f72-db9d445a0db4 · outbound

This paper cites Fukugita and T.

Boomerang mechanism explaining the excess radio background Fukugita and T

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.104715Z

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Observation c1a54569-3c6e-4fd6-9629-d212e7f9a081 · outbound

This paper cites Exploring the robustness of stellar cooling constraints on light particles.

Boomerang mechanism explaining the excess radio background Exploring the robustness of stellar cooling constraints on light particles

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.107595Z

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Observation 7bb6fb3e-d8fb-4b43-987b-eb3dc7cd4aeb · outbound

This paper cites Reconciling the CAST and PVLAS Results.

Boomerang mechanism explaining the excess radio background Reconciling the CAST and PVLAS Results

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.110686Z

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Observation 6d1b2b79-0d93-46f6-a747-dd9dc9648f31 · outbound

This paper cites The split majoron model confronts the NANOGrav signal and cosmological tensions.

Boomerang mechanism explaining the excess radio background The split majoron model confronts the NANOGrav signal and cosmological tensions

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.113953Z

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Observation 425795f4-865b-4757-9190-620ec377e1c4 · outbound

This paper cites Naturally Light Dirac and Pseudo-Dirac Neutrinos from Left-Right Symmetry.

Boomerang mechanism explaining the excess radio background Naturally Light Dirac and Pseudo-Dirac Neutrinos from Left-Right Symmetry

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.117015Z

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Observation 6e596b3f-a07a-4c1d-9857-ef1403d93491 · outbound

This paper cites Probing Pseudo-Dirac Neutrinos with Astrophysical Sources at IceCube.

Boomerang mechanism explaining the excess radio background Probing Pseudo-Dirac Neutrinos with Astrophysical Sources at IceCube

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.120038Z

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Observation ec285af2-59b9-472e-88d3-a0685c90bd9e · outbound

This paper cites Right-Handed Neutrinos at LHC and the Mechanism of Neutrino Mass Generation.

Boomerang mechanism explaining the excess radio background Right-Handed Neutrinos at LHC and the Mechanism of Neutrino Mass Generation

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.123146Z

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Observation 0e89cd17-5581-4d37-8937-6c2213a768a6 · outbound

This paper cites Evidence for Neutrino Oscillations from the Observation of Electron Anti-neutrinos in a Muon Anti-Neutrino Beam.

Boomerang mechanism explaining the excess radio background Evidence for Neutrino Oscillations from the Observation of Electron Anti-neutrinos in a Muon Anti-Neutrino Beam

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.126321Z

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Observation 77dacd3c-dc0b-49e8-9007-294c68b4b820 · outbound

This paper cites Updated MiniBooNE Neutrino Oscillation Results with Increased Data and New Background Studies.

Boomerang mechanism explaining the excess radio background Updated MiniBooNE Neutrino Oscillation Results with Increased Data and New Background Studies

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.129764Z

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Observation a57b2620-5c11-4c37-8184-e067f799f514 · outbound

This paper cites Results from the Baksan Experiment on Sterile Transitions (BEST).

Boomerang mechanism explaining the excess radio background Results from the Baksan Experiment on Sterile Transitions (BEST)

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.133107Z

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Observation 0ef3489d-753d-4786-ac46-a972f02f2778 · outbound

This paper cites Abbasi et al.

Boomerang mechanism explaining the excess radio background Abbasi et al

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.136266Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1c7af00a-1699-4734-a4f8-4dd79b5f686f · outbound

This paper cites Updated global analysis of neutrino oscillations in the presence of eV-scale sterile neutrinos.

Boomerang mechanism explaining the excess radio background Updated global analysis of neutrino oscillations in the presence of eV-scale sterile neutrinos

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.139394Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7749d4fa-656b-43ae-8d38-0cdc214e265f · outbound

This paper cites New Clues About Light Sterile Neutrinos: Preference for Models with Damping Effects in Global Fits.

Boomerang mechanism explaining the excess radio background New Clues About Light Sterile Neutrinos: Preference for Models with Damping Effects in Global Fits

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.142572Z

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Unavailable: canonical work link unavailable.

Observation 8984aa42-b0b8-4e95-9ae2-f0c9af726ad3 · outbound

This paper cites Wolfenstein, Different Varieties of Massive Dirac Neu- trinos, Nucl.

Boomerang mechanism explaining the excess radio background Wolfenstein, Different Varieties of Massive Dirac Neu- trinos, Nucl

Reference 43

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T11:02:38.062047Z

Source-reported events for the cited work

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Observation 300a95b0-3848-435c-95d9-fd3b13f41afe · outbound

This paper cites an unresolved cited work.

Boomerang mechanism explaining the excess radio background Unresolved cited work

Reference 44

Resolution: unresolved; raw_fallback, observed 2026-08-05T11:02:38.051821Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation ea0e905e-b5b8-4467-89fb-5d123100ffb9 · outbound

This paper cites an unresolved cited work.

Boomerang mechanism explaining the excess radio background Unresolved cited work

Reference 45

Resolution: unresolved; raw_fallback, observed 2026-08-05T11:02:38.042873Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 90faaa09-3ca7-4995-9ca1-5222548a1d4a · outbound

This paper cites Pseudo-Dirac Scenario for Neutrino Oscillations.

Boomerang mechanism explaining the excess radio background Pseudo-Dirac Scenario for Neutrino Oscillations

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.155106Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f33c5447-6106-4c16-b648-1a784dc7d02c · outbound

This paper cites Quasi Dirac neutrino oscillations.

Boomerang mechanism explaining the excess radio background Quasi Dirac neutrino oscillations

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.158419Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7c3af8aa-ca1c-4bdb-9317-b329b92e5a53 · outbound

This paper cites Pseudo-Dirac Neutrinos in the New Standard Model.

Boomerang mechanism explaining the excess radio background Pseudo-Dirac Neutrinos in the New Standard Model

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.161519Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 86e148ac-5f8d-4163-aced-bd9d0cfadc6b · outbound

This paper cites Vissani and A.

Boomerang mechanism explaining the excess radio background Vissani and A

Reference 49

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T11:02:38.033355Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation e90e89a3-1776-4716-85d7-bb9945d91402 · outbound

This paper cites Probing BSM Neutrino Physics with Flavor and Spectral Distortions: Prospects for Future High-Energy Neutrino Telescopes.

Boomerang mechanism explaining the excess radio background Probing BSM Neutrino Physics with Flavor and Spectral Distortions: Prospects for Future High-Energy Neutrino Telescopes

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.167519Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d752d3e2-0e5f-465a-91f2-22537bf238e7 · outbound

This paper cites IceCube Flavor Ratios with Identified Astrophysical Sources: Towards Improving New Physics Testability.

Boomerang mechanism explaining the excess radio background IceCube Flavor Ratios with Identified Astrophysical Sources: Towards Improving New Physics Testability

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.170563Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 218386a4-bf39-472c-b899-e62c5fa28a7e · outbound

This paper cites Fundamental physics with the diffuse supernova background neutrinos.

Boomerang mechanism explaining the excess radio background Fundamental physics with the diffuse supernova background neutrinos

Reference 52

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.173571Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1a6ec86c-0cb6-4aeb-997c-b9c7beb6014b · outbound

This paper cites Constraints on pseudo-Dirac neutrinos using high-energy neutrinos from NGC 1068.

Boomerang mechanism explaining the excess radio background Constraints on pseudo-Dirac neutrinos using high-energy neutrinos from NGC 1068

Reference 53

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.176540Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0c3dd9eb-b37c-40cf-a180-cd3758e077a2 · outbound

This paper cites Revisiting pseudo-Dirac neutrino scenario after recent solar neutrino data.

Boomerang mechanism explaining the excess radio background Revisiting pseudo-Dirac neutrino scenario after recent solar neutrino data

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.179679Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2171a2db-0273-41fa-876a-71dda6f230d4 · outbound

This paper cites Constraining super-light sterile neutrinos at Borexino and KamLAND.

Boomerang mechanism explaining the excess radio background Constraining super-light sterile neutrinos at Borexino and KamLAND

Reference 55

Resolution: verified exact; local_arxiv, observed 2026-08-05T11:02:37.582352Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 047f4c97-2685-4a24-85e2-9b163dafa720 · outbound

This paper cites an unresolved cited work.

Boomerang mechanism explaining the excess radio background Unresolved cited work

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.186122Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation dc186764-a0c4-4b94-9b62-2dad7781d3ef · outbound

This paper cites Search for sterile neutrinos in MINOS and MINOS+ using a two-detector fit.

Boomerang mechanism explaining the excess radio background Search for sterile neutrinos in MINOS and MINOS+ using a two-detector fit

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.189169Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3b559d05-febb-4d1c-80cb-64f1429e4182 · outbound

This paper cites Dual-Baseline Search for Active-to-Sterile Neutrino Oscillations in NOvA.

Boomerang mechanism explaining the excess radio background Dual-Baseline Search for Active-to-Sterile Neutrino Oscillations in NOvA

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.192463Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4947207b-ba13-439d-8e75-13d337e7d1f0 · outbound

This paper cites Pseudo-Dirac Neutrinos, a Challenge for Neutrino Telescopes.

Boomerang mechanism explaining the excess radio background Pseudo-Dirac Neutrinos, a Challenge for Neutrino Telescopes

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.195378Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 6c017c18-4417-44c6-a331-f647693498ce · outbound

This paper cites SN1987A still shining: A Quest for Pseudo-Dirac Neutrinos.

Boomerang mechanism explaining the excess radio background SN1987A still shining: A Quest for Pseudo-Dirac Neutrinos

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.198657Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 00bdc1b5-ec33-4705-b172-6fa5979fb3dd · outbound

This paper cites $pp$ Solar Neutrinos at DARWIN.

Boomerang mechanism explaining the excess radio background $pp$ Solar Neutrinos at DARWIN

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.201724Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d77f9f02-5249-447f-8a90-6ea986a83f2a · outbound

This paper cites an unresolved cited work.

Boomerang mechanism explaining the excess radio background Unresolved cited work

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.204618Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5081e517-0991-404a-b813-5d037690e771 · outbound

This paper cites Pseudo-Dirac Neutrinos and Relic Neutrino Matter Effect on the High-energy Neutrino Flavor Composition.

Boomerang mechanism explaining the excess radio background Pseudo-Dirac Neutrinos and Relic Neutrino Matter Effect on the High-energy Neutrino Flavor Composition

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.207410Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 0e22cd5c-f4b3-4be8-948c-94e32da26cee · outbound

This paper cites Carloni, Y.

Boomerang mechanism explaining the excess radio background Carloni, Y

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.210254Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation aa4c96c4-fbf2-464a-8001-92d63b4e219b · outbound

This paper cites JUNO as a Probe of the Pseudo-Dirac Nature using Solar Neutrinos.

Boomerang mechanism explaining the excess radio background JUNO as a Probe of the Pseudo-Dirac Nature using Solar Neutrinos

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.213090Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation ae2e2adc-5367-41aa-8816-a91aabe81dec · outbound

This paper cites Hampel et al.

Boomerang mechanism explaining the excess radio background Hampel et al

Reference 66

Resolution: verified fuzzy; raw_fallback, observed 2026-08-05T11:02:38.024379Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 41981ca0-1594-42fc-9927-b32b10c8ac36 · outbound

This paper cites an unresolved cited work.

Boomerang mechanism explaining the excess radio background Unresolved cited work

Reference 67

Resolution: unresolved; raw_fallback, observed 2026-08-05T11:02:38.014891Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 736c6752-d260-4b16-a57e-99a1f2ed783b · outbound

This paper cites Direct Evidence for Neutrino Flavor Transformation from Neutral-Current Interactions in the Sudbury Neutrino Observatory.

Boomerang mechanism explaining the excess radio background Direct Evidence for Neutrino Flavor Transformation from Neutral-Current Interactions in the Sudbury Neutrino Observatory

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.221362Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9d7e713b-4551-4c3c-a47a-c3cc0ea721bb · outbound

This paper cites Solar 8B and hep Neutrino Measurements from 1258 Days of Super-Kamiokande Data.

Boomerang mechanism explaining the excess radio background Solar 8B and hep Neutrino Measurements from 1258 Days of Super-Kamiokande Data

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.224251Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 3e251904-1b88-49f8-98de-e378aa757ab6 · outbound

This paper cites The EDGES signal: An imprint from the mirror world?.

Boomerang mechanism explaining the excess radio background The EDGES signal: An imprint from the mirror world?

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.227077Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 1b0dd334-f2f7-445d-915b-218dae2bec6b · outbound

This paper cites Dark photon limits: a handbook.

Boomerang mechanism explaining the excess radio background Dark photon limits: a handbook

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.229911Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 834f6a26-17b2-4c2a-9162-dec394452320 · outbound

This paper cites Constraints on photon mass and dark photon from the Jovian magnetic field.

Boomerang mechanism explaining the excess radio background Constraints on photon mass and dark photon from the Jovian magnetic field

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-05T11:02:37.232998Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Pith citing papers

Observation fe19db82-04fa-42e8-b257-6de1d1ea7571 · inbound

How neutrinos could help solving cosmological anomalies and tensions cites this paper.

How neutrinos could help solving cosmological anomalies and tensions Boomerang mechanism explaining the excess radio background

Reference 2

Resolution: verified exact; arxiv_id, observed 2026-06-12T01:08:15.692110Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 44a56f99-699e-4a11-810b-3dabf4bc41f9 · inbound

Non-adiabatic transitions in the density matrix formalism cites this paper.

Non-adiabatic transitions in the density matrix formalism Boomerang mechanism explaining the excess radio background

Reference 22

Resolution: verified exact; local_arxiv, observed 2026-07-04T16:39:57.516689Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.

Observation 14dcfbf5-d6fc-4b6d-83a6-77478a6b112c · inbound

Non-adiabatic transitions in the density matrix formalism cites this paper.

Non-adiabatic transitions in the density matrix formalism Boomerang mechanism explaining the excess radio background

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-02T10:27:06.369020Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation c9d8030f-1f50-4866-8166-40dc1cfd14ed · inbound

Probing Scalar Non-Standard Neutrino Interactions using High-Energy Astrophysical Neutrinos cites this paper.

Probing Scalar Non-Standard Neutrino Interactions using High-Energy Astrophysical Neutrinos Boomerang mechanism explaining the excess radio background

Reference 199

Resolution: verified exact; local_arxiv, observed 2026-07-04T18:20:05.179539Z

Source-reported events for the cited work

No event found in the named queried sources as of 2026-08-13T06:32:02.005865+00:00.