Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess | Paper Citation Record

Observation 3caf327a-b8e0-4332-8696-02c55496d875 · outbound

This paper cites New physics from the polarised light of the cosmic microwave background.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess New physics from the polarised light of the cosmic microwave background

Reference 1

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:19.535379Z

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Observation 5852a4bd-6dc3-4fc3-85c2-b641984cc82d · outbound

This paper cites Cosmic Microwave Background Anisotropies.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Cosmic Microwave Background Anisotropies

Reference 3

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:19.590202Z

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Observation 16747ac5-f3bf-4f96-b4b2-403a43227328 · outbound

This paper cites CMB power spectra and cosmological parameters from Planck PR4 with CamSpec.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess CMB power spectra and cosmological parameters from Planck PR4 with CamSpec

Reference 4

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:19.651014Z

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Observation 45b815ce-a541-495a-8691-9aab8301f5db · outbound

This paper cites Characterization of foreground emission at degree angular scale for CMB B-modes observations. Thermal Dust and Synchrotron signal from Planck and WMAP data.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Characterization of foreground emission at degree angular scale for CMB B-modes observations. Thermal Dust and Synchrotron signal from Planck and WMAP data

Reference 5

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:19.719898Z

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Observation d5d9e778-94d5-4515-9af6-1028c7c90df7 · outbound

This paper cites Fixsen and et al.,Arcade 2 measurement of the absolute sky brightness at 3–90 ghz, The Astrophysical Journal734(2011) 5.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Fixsen and et al.,Arcade 2 measurement of the absolute sky brightness at 3–90 ghz, The Astrophysical Journal734(2011) 5

Reference 6

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:19.785061Z

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Observation 89c2eb23-6c71-4a95-9561-d5b1af3c3844 · outbound

This paper cites An absorption profile centred at 78 megahertz in the sky-averaged spectrum.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess An absorption profile centred at 78 megahertz in the sky-averaged spectrum

Reference 7

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:19.860806Z

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Observation a58dc2b0-b92f-4650-aa3d-33786492a872 · outbound

This paper cites First Light for the First Station of the Long Wavelength Array.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess First Light for the First Station of the Long Wavelength Array

Reference 8

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:19.927980Z

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Observation 04d3881b-1347-4aa3-a1a1-620022fe291c · outbound

This paper cites Haslam, C.J.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Haslam, C.J

Reference 9

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:19.999555Z

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Observation f2451895-da2d-41f9-907b-59727664a846 · outbound

This paper cites ARCADE 2 Observations of Galactic Radio Emission.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess ARCADE 2 Observations of Galactic Radio Emission

Reference 10

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:20.066077Z

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Observation 839026ce-794a-47ab-b6cd-b118effe6f2d · outbound

This paper cites Spectral Index of the Diffuse Radio Background Measured From 100 to 200 MHz.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Spectral Index of the Diffuse Radio Background Measured From 100 to 200 MHz

Reference 11

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:20.210289Z

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Observation 53efa5b8-1cd8-4adf-9c03-de6dae72f110 · outbound

This paper cites Haslam, U.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Haslam, U

Reference 12

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:20.331961Z

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Observation 9b716f21-7700-4ab5-8ea5-69e3c2499edf · outbound

This paper cites Reich and W.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Reich and W

Reference 13

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:20.436714Z

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Observation 566e2a82-cf91-4648-8bae-723f88718c73 · outbound

This paper cites The radio emission from the Galaxy at 22 MHz.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess The radio emission from the Galaxy at 22 MHz

Reference 14

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:20.588648Z

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Observation f14ccdbe-08f3-43f9-afd2-b3e082f241e7 · outbound

This paper cites All-sky Galactic radiation at 45 MHz and spectral index between 45 and 408 MHz.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess All-sky Galactic radiation at 45 MHz and spectral index between 45 and 408 MHz

Reference 15

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:20.688557Z

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Observation 73a88c61-4d43-4334-9bad-00474ae6aae9 · outbound

This paper cites Guzm´ an, J.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Guzm´ an, J

Reference 16

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:20.796498Z

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Observation 3aad5bf3-652c-4bc0-afda-b09418a6dac2 · outbound

This paper cites Interpretation of the Extragalactic Radio Background.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Interpretation of the Extragalactic Radio Background

Reference 17

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:20.897818Z

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Observation 98a50cd7-7d0c-4602-97f4-426dccf830c7 · outbound

This paper cites The Radio Background Below 100 MHz.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess The Radio Background Below 100 MHz

Reference 18

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:21.039191Z

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Observation f6c7a532-0279-43ff-bf57-82ad1f70de04 · outbound

This paper cites Concerns about Modelling of the EDGES Data.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Concerns about Modelling of the EDGES Data

Reference 19

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:21.203908Z

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Observation b3ee3411-8465-44f4-a577-44b34d56a350 · outbound

This paper cites On the detection of a cosmic dawn signal in the radio background.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess On the detection of a cosmic dawn signal in the radio background

Reference 20

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:21.307457Z

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Observation 259ea284-a165-4b54-8ca1-e53cce424b7d · outbound

This paper cites A Bayesian approach to modelling spectrometer data chromaticity corrected using beam factors -- I. Mathematical formalism.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess A Bayesian approach to modelling spectrometer data chromaticity corrected using beam factors -- I. Mathematical formalism

Reference 21

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:21.456092Z

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Observation 18085987-8e64-4e68-ae9d-c98cd43450a0 · outbound

This paper cites Sims et al.,A Bayesian approach to modelling spectrometer data chromaticity corrected using beam factors – II.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Sims et al.,A Bayesian approach to modelling spectrometer data chromaticity corrected using beam factors – II

Reference 22

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:21.609751Z

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Observation bcc75a58-f420-4780-b6e9-0a939f00c7b1 · outbound

This paper cites Price, L.J.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Price, L.J

Reference 23

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:21.740729Z

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Observation dd9ecabe-b2e7-4200-8adf-70d9ca24231c · outbound

This paper cites The Array of Long Baseline Antennas for Taking Radio Observations from the Sub-Antarctic.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess The Array of Long Baseline Antennas for Taking Radio Observations from the Sub-Antarctic

Reference 24

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:21.844904Z

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Observation 0a10d122-465a-41ff-ba5d-e3f68262c6a4 · outbound

This paper cites The REACH radiometer for detecting the 21-cm hydrogen signal from redshift 7.5 to 28.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess The REACH radiometer for detecting the 21-cm hydrogen signal from redshift 7.5 to 28

Reference 25

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:22.001067Z

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Observation 6b11d3b2-9ac3-4e36-beac-40bffa713f63 · outbound

This paper cites Possible interaction between baryons and dark-matter particles revealed by the first stars.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Possible interaction between baryons and dark-matter particles revealed by the first stars

Reference 26

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:22.144385Z

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Observation 13a227f0-2dd6-4e5f-8a01-2acac3b864f7 · outbound

This paper cites Constraining Baryon--Dark Matter Scattering with the Cosmic Dawn 21-cm Signal.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Constraining Baryon--Dark Matter Scattering with the Cosmic Dawn 21-cm Signal

Reference 27

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:22.291225Z

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Observation 927c8c3d-85a4-46c0-a713-e7de11d87b9a · outbound

This paper cites Insights on Dark Matter from Hydrogen during Cosmic Dawn.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Insights on Dark Matter from Hydrogen during Cosmic Dawn

Reference 28

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:22.406674Z

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Observation 36395b74-0657-4d01-b31f-2722223cf449 · outbound

This paper cites Signs of Dark Matter at 21-cm?.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Signs of Dark Matter at 21-cm?

Reference 29

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:22.552780Z

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Observation 59e5fb32-29ad-48e6-942b-0afa26837e5d · outbound

This paper cites Severely Constraining Dark Matter Interpretations of the 21-cm Anomaly.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Severely Constraining Dark Matter Interpretations of the 21-cm Anomaly

Reference 30

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:22.671773Z

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Observation 6e5c4630-9e18-442b-b532-3372f7a14c17 · outbound

This paper cites New Physics in the Rayleigh-Jeans Tail of the CMB.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess New Physics in the Rayleigh-Jeans Tail of the CMB

Reference 31

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:22.800780Z

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Observation 0471b07e-6671-4f0f-82a9-e0a62f4dcebe · outbound

This paper cites The EDGES 21 cm Anomaly and Properties of Dark Matter.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess The EDGES 21 cm Anomaly and Properties of Dark Matter

Reference 32

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:22.889775Z

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Observation 66fe2cae-5d12-42e6-8966-f354d94711be · outbound

This paper cites Constraints on Superconducting Cosmic Strings from the Global $21$-cm Signal before Reionization.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Constraints on Superconducting Cosmic Strings from the Global $21$-cm Signal before Reionization

Reference 33

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:22.994216Z

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Observation 54a5878c-2a7b-4e56-a7cc-a57adadc4904 · outbound

This paper cites Axion-Photon Conversion and Effects on 21cm Observation.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Axion-Photon Conversion and Effects on 21cm Observation

Reference 34

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:23.063170Z

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Observation 5518a2d7-0374-43d4-a9d4-3bd42c8067fa · outbound

This paper cites Axion-photon-dark photon oscillation and its implication for 21 cm observation.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Axion-photon-dark photon oscillation and its implication for 21 cm observation

Reference 35

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:23.136287Z

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Observation 6a9b39db-fba0-4b27-a1fe-be8fd26f4183 · outbound

This paper cites The role of soft photon injection and heating in 21 cm cosmology.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess The role of soft photon injection and heating in 21 cm cosmology

Reference 36

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:23.230713Z

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Observation a4ff7180-de49-4316-911f-77e263a05299 · outbound

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

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Probing relic neutrino decays with 21 cm cosmology

Reference 37

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:23.298582Z

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Observation 3cbcc1b2-7e14-4fcf-a6a2-69d7a01ac03c · outbound

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

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Relic neutrino decay solution to the excess radio background

Reference 38

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:23.348611Z

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Observation 2386ac14-73ad-4a9a-bcee-f03420f2f79f · outbound

This paper cites A dark matter interpretation for the ARCADE excess?.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess A dark matter interpretation for the ARCADE excess?

Reference 39

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:23.379293Z

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Observation cb9e187d-3326-4225-8910-2ea7cc177f1f · outbound

This paper cites A closer look at dark photon explanations of the excess radio background.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess A closer look at dark photon explanations of the excess radio background

Reference 40

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:23.431251Z

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Observation d72fe35d-2c1b-4e3f-9d3c-4cea5bb3a031 · outbound

This paper cites Raffelt and L.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Raffelt and L

Reference 41

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:23.475617Z

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Observation d87ef468-1a7b-46b2-b76e-0ef9b91417a6 · outbound

This paper cites Signatures of axion-like particles in the spectra of TeV gamma-ray sources.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Signatures of axion-like particles in the spectra of TeV gamma-ray sources

Reference 42

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:23.546726Z

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Observation 9273a77a-f220-4e7d-b3c9-6b08cc33661a · outbound

This paper cites Constraints on millicharged dark matter and axion-like particles from timing of radio waves.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Constraints on millicharged dark matter and axion-like particles from timing of radio waves

Reference 43

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:23.600016Z

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Observation bebea464-c207-4c5c-a227-ccc1077c01ef · outbound

This paper cites Excess Radiation from Axion-Photon Conversion.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Excess Radiation from Axion-Photon Conversion

Reference 44

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:23.654735Z

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Observation 84f3e3ce-8879-48be-98eb-a17e1aa750c9 · outbound

This paper cites Cosmological constraints on axionic dark radiation from axion-photon conversion in the early Universe.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Cosmological constraints on axionic dark radiation from axion-photon conversion in the early Universe

Reference 45

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:23.701606Z

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Observation 4597e576-41f9-40d6-9b97-a0c789d7fd12 · outbound

This paper cites Influence of primordial magnetic fields on 21 cm emission.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Influence of primordial magnetic fields on 21 cm emission

Reference 46

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:23.772936Z

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Observation 70e6ddcc-6785-4f1f-ab25-90ece3766926 · outbound

This paper cites Primordial magnetic fields and the HI signal from the epoch of reionization.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Primordial magnetic fields and the HI signal from the epoch of reionization

Reference 47

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:23.831177Z

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Observation 47fb79c3-b81d-4816-b41c-0d8a3050db41 · outbound

This paper cites Revisiting primordial magnetic fields through 21-cm physics: Bounds and forecasts.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Revisiting primordial magnetic fields through 21-cm physics: Bounds and forecasts

Reference 48

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:23.881020Z

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Observation f64fe95d-ba49-4b04-8483-66eb7b900a0f · outbound

This paper cites Shaping Dark Photon Spectral Distortions.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Shaping Dark Photon Spectral Distortions

Reference 49

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:23.927631Z

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Observation 9100b34a-8f0b-413c-b393-e40294f4d441 · outbound

This paper cites Revisiting Dark Photon Constraints from CMB Spectral Distortions.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Revisiting Dark Photon Constraints from CMB Spectral Distortions

Reference 50

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:24.007076Z

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Observation 3631a5b6-b4df-4204-9bb5-8ec4f4c249fc · outbound

This paper cites The Atacama Cosmology Telescope: DR6 Constraints on Extended Cosmological Models.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess The Atacama Cosmology Telescope: DR6 Constraints on Extended Cosmological Models

Reference 51

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:24.059356Z

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Observation b74482c8-0e91-4ae6-9832-e2d8783bf59b · outbound

This paper cites Constraints on dark radiation from cosmological probes.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Constraints on dark radiation from cosmological probes

Reference 54

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:24.111623Z

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Observation b13cc536-e68f-4480-8cf5-fb5cf4a20116 · outbound

This paper cites Mangano and P.D.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Mangano and P.D

Reference 55

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:24.207124Z

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Observation 624f6062-d88e-4303-ba3b-b7a54ed178e3 · outbound

This paper cites Baumann,Cosmology, Cambridge University Press (7, 2022), 10.1017/9781108937092.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Baumann,Cosmology, Cambridge University Press (7, 2022), 10.1017/9781108937092

Reference 56

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:24.279005Z

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Observation 79c23a59-8e50-4318-b866-59a420b50e77 · outbound

This paper cites Guth,Inflationary universe: A possible solution to the horizon and flatness problems, Physical Review D23(1981) 347.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Guth,Inflationary universe: A possible solution to the horizon and flatness problems, Physical Review D23(1981) 347

Reference 57

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:24.325386Z

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Observation d5eefe83-77af-40e7-b98e-842927754f43 · outbound

This paper cites Linde,A new inflationary universe scenario: a possible solution of the horizon, flatness, homogeneity, isotropy and primordial monopole problems,Physics Letters B108 (1982) 389.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Linde,A new inflationary universe scenario: a possible solution of the horizon, flatness, homogeneity, isotropy and primordial monopole problems,Physics Letters B108 (1982) 389

Reference 58

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:24.391735Z

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Observation 6ac6664d-a76a-44ab-a5d6-dca5204ab17b · outbound

This paper cites Mukhanov and G.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Mukhanov and G

Reference 59

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:24.431720Z

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Observation f304002f-9522-490d-8a32-181ee563076b · outbound

This paper cites Peccei and H.R.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Peccei and H.R

Reference 60

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:24.483278Z

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Observation 6a271911-bb8f-4306-9d7d-45bf5b5ef616 · outbound

This paper cites Preskill, M.B.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Preskill, M.B

Reference 61

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:24.536117Z

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Observation 34352091-7c02-4bb9-8ad7-c41392ca32c4 · outbound

This paper cites Yamaguchi, M.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Yamaguchi, M

Reference 62

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:24.594570Z

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Observation 105ac6ec-a567-4370-ba86-a8413ce7df79 · outbound

This paper cites Sikivie,Axions, domain walls, and the early universe,Physical Review Letters48(1982) 1156.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Sikivie,Axions, domain walls, and the early universe,Physical Review Letters48(1982) 1156

Reference 63

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:24.655541Z

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Observation 93ae7f23-e37c-44a6-bf5c-2544d2d3a048 · outbound

This paper cites Graf and F.D.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Graf and F.D

Reference 64

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:24.694972Z

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Observation 07003b29-8410-45d4-8f3e-b3b75d3b4cf9 · outbound

This paper cites Probing the axion-photon coupling: phenomenological and experimental perspectives. A snowmass white paper.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Probing the axion-photon coupling: phenomenological and experimental perspectives. A snowmass white paper

Reference 65

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:24.770954Z

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Observation ecad6514-9726-4d01-b1fe-47145ffb5524 · outbound

This paper cites Landau, E.M.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Landau, E.M

Reference 66

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:24.879383Z

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Observation 043c075e-b3e5-4e25-9a44-8ce850e5e497 · outbound

This paper cites Turner and L.M.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Turner and L.M

Reference 67

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:24.996224Z

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Observation 0a429ac5-95ac-4062-9d2a-5f058b835c34 · outbound

This paper cites Addazi, S.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Addazi, S

Reference 68

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.096437Z

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Observation 53818890-7ce0-43bf-85e7-5a193cbb71ce · outbound

This paper cites Ratra,Cosmological’seed’magnetic field from inflation,Astrophysical Journal, Part 2-Letters (ISSN 0004-637X), vol.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Ratra,Cosmological’seed’magnetic field from inflation,Astrophysical Journal, Part 2-Letters (ISSN 0004-637X), vol

Reference 69

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.250292Z

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Observation 2a46fa61-6caf-49ab-ac83-fedf37d03842 · outbound

This paper cites Kobayashi and M.S.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Kobayashi and M.S

Reference 70

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.278910Z

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Unavailable: canonical work link unavailable.

Observation 3a16ed21-eeb9-4a09-ab99-509a4b1b65c8 · outbound

This paper cites Magnetogenesis during inflation and preheating in the Starobinsky model.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Magnetogenesis during inflation and preheating in the Starobinsky model

Reference 71

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.287226Z

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Observation 9263ee3e-c8d1-4b35-ad48-9de8be9eeadc · outbound

This paper cites The generation of helical magnetic field in a viable scenario of Inflationary Magnetogenesis.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess The generation of helical magnetic field in a viable scenario of Inflationary Magnetogenesis

Reference 72

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.295463Z

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Observation 3b29df81-b73d-48ec-8bf8-f9b207939445 · outbound

This paper cites Challenges in Inflationary Magnetogenesis: Constraints from Strong Coupling, Backreaction and the Schwinger Effect.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Challenges in Inflationary Magnetogenesis: Constraints from Strong Coupling, Backreaction and the Schwinger Effect

Reference 73

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.301071Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 08b43a02-bac0-4ea8-b0a4-62285d48e96d · outbound

This paper cites On the challenges in the choice of the non-conformal coupling function in inflationary magnetogenesis.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess On the challenges in the choice of the non-conformal coupling function in inflationary magnetogenesis

Reference 74

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.308439Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b7e1f727-0bb5-4e29-be7a-2281b30979fa · outbound

This paper cites Inflationary Magnetogenesis without the Strong Coupling Problem.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Inflationary Magnetogenesis without the Strong Coupling Problem

Reference 75

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.313803Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation b9ca3bc1-ecb1-4d66-ac3c-c1f2de72e350 · outbound

This paper cites Probing the reheating phase through primordial magnetic field and CMB.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Probing the reheating phase through primordial magnetic field and CMB

Reference 76

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.322001Z

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Unavailable: canonical work link unavailable.

Observation 0adaefea-4cd0-4dea-a5de-478799fa0eaa · outbound

This paper cites Large-scale magnetic fields from dilaton inflation in noncommutative spacetime.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Large-scale magnetic fields from dilaton inflation in noncommutative spacetime

Reference 77

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.329929Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation fe50ac7e-3ea4-4d01-af40-7da7d5691303 · outbound

This paper cites Primordial Magnetic Fields From String Cosmology.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Primordial Magnetic Fields From String Cosmology

Reference 78

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.350734Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 64c13a51-fe3a-4495-be15-ad7a9042f384 · outbound

This paper cites Pre-reheating Magnetogenesis in the Kinetic Coupling Model.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Pre-reheating Magnetogenesis in the Kinetic Coupling Model

Reference 79

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.361465Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a9940bce-c596-4697-8066-647a0cdc1838 · outbound

This paper cites Inflationary magnetogenesis with reheating phase from higher curvature coupling.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Inflationary magnetogenesis with reheating phase from higher curvature coupling

Reference 80

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.370418Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 57345889-4ef5-4805-852b-7f8cd122a59a · outbound

This paper cites Magnetic fields from inflation: The CMB temperature anisotropies.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Magnetic fields from inflation: The CMB temperature anisotropies

Reference 81

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.383534Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation d040c2c3-fa00-4639-97bd-c7e1fca3d11c · outbound

This paper cites Cosmological Magnetic Fields: Their Generation, Evolution and Observation.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Cosmological Magnetic Fields: Their Generation, Evolution and Observation

Reference 82

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.390630Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 7d902f2b-76b5-4e82-9695-551acb5672dc · outbound

This paper cites Insight into primordial magnetic fields from 21-cm line observation with EDGES experiment.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Insight into primordial magnetic fields from 21-cm line observation with EDGES experiment

Reference 83

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.396651Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 147794da-f069-4d45-a31b-f31ee06c143b · outbound

This paper cites Statistical Properties of Scale-Invariant Helical Magnetic Fields and Applications to Cosmology.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Statistical Properties of Scale-Invariant Helical Magnetic Fields and Applications to Cosmology

Reference 84

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.402640Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 4cb39529-81b9-4d2b-a18d-031b9c413d13 · outbound

This paper cites Kahniashvili, A.G.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Kahniashvili, A.G

Reference 85

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.409638Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 69af20fe-c865-46bf-aa93-05761f0dcc99 · outbound

This paper cites Phase Transition Generated Cosmological Magnetic Field at Large Scales.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Phase Transition Generated Cosmological Magnetic Field at Large Scales

Reference 86

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.414875Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 2b8dbcf7-dba2-4f46-bde4-fcfa17fa9442 · outbound

This paper cites Ruling out 3 keV warm dark matter using 21 cm-EDGES data.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Ruling out 3 keV warm dark matter using 21 cm-EDGES data

Reference 88

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.422916Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e6e9d4e1-f406-4923-b25d-8b4694856786 · outbound

This paper cites Sisk-Reyn´ es, J.H.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Sisk-Reyn´ es, J.H

Reference 89

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.428456Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a0148230-aaef-45ec-b0a8-4742c9192363 · outbound

This paper cites Conlon, F.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Conlon, F

Reference 90

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.435227Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation cf7b2250-8aba-4815-ba1e-187833e3ac67 · outbound

This paper cites Constraining resonant photon-axion conversions in the Early Universe.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Constraining resonant photon-axion conversions in the Early Universe

Reference 91

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.441117Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation f6aa2085-3523-4f8e-a09a-4c63fe67dba4 · outbound

This paper cites Potential of radio telescopes as high-frequency gravitational wave detectors.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Potential of radio telescopes as high-frequency gravitational wave detectors

Reference 92

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.446667Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 78b589cc-3e8c-42b0-9ac5-c71b123ca807 · outbound

This paper cites Upper limits on the amplitude of ultra-high-frequency gravitational waves from graviton-photon mixing.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Upper limits on the amplitude of ultra-high-frequency gravitational waves from graviton-photon mixing

Reference 93

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.452712Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5c1fdc1d-3701-4bb6-81b3-317cc9ae666e · outbound

This paper cites Gravitational Waves from Primordial Magnetic Fields via Photon-Graviton Conversion.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Gravitational Waves from Primordial Magnetic Fields via Photon-Graviton Conversion

Reference 94

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.459093Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation a29da6c0-0c29-4d8b-a241-d39e390a95d3 · outbound

This paper cites Vernstrom, D.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Vernstrom, D

Reference 95

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.465705Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation e7bc9c57-a504-4032-bbd3-1327ea417410 · outbound

This paper cites Galluzzi, M.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Galluzzi, M

Reference 96

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.471725Z

Source-reported events for the cited work

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Observation 91723b27-4b36-49ad-8588-ef0f108bb835 · outbound

This paper cites Ysard and G.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Ysard and G

Reference 97

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.476979Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 01febc0a-18a6-442d-9050-62c010860dcf · outbound

This paper cites Singal, L.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Singal, L

Reference 98

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.482943Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 04caede5-e99f-46db-971d-1416bdf5e6da · outbound

This paper cites Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Cosmology at Low Frequencies: The 21 cm Transition and the High-Redshift Universe

Reference 99

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.490360Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 5e1332d4-9be9-4e03-8d2c-b8262e172017 · outbound

This paper cites 21-cm cosmology.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess 21-cm cosmology

Reference 100

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.498781Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation bbb0ca4f-dd34-48bd-b3e8-85185d2a023d · outbound

This paper cites 21-cm Tomography of the Intergalactic Medium at High Redshift.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess 21-cm Tomography of the Intergalactic Medium at High Redshift

Reference 101

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.504323Z

Source-reported events for the cited work

Unavailable: canonical work link unavailable.

Observation 9143c21b-858c-41a8-8e2a-55d7db2598e5 · outbound

This paper cites Enhanced global signal of neutral hydrogen due to excess radiation at cosmic dawn.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Enhanced global signal of neutral hydrogen due to excess radiation at cosmic dawn

Reference 102

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.510354Z

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Unavailable: canonical work link unavailable.

Observation 5c4e87a8-d7a1-4deb-8bed-43e7af7808fd · outbound

This paper cites Wouthuysen,On the excitation mechanism of the 21-cm (radio-frequency) interstellar hydrogen emission line.,AJ57(1952) 31.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Wouthuysen,On the excitation mechanism of the 21-cm (radio-frequency) interstellar hydrogen emission line.,AJ57(1952) 31

Reference 103

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.517725Z

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Observation 9e46f258-f012-4c88-9de8-8489c213d68e · outbound

This paper cites Field,Excitation of the hydrogen 21-cm line,Proceedings of the IRE46(1958) 240–250.

Axion-Photon Conversion in FLRW with Primordial Magnetic Fields: Explaining the Radio Excess Field,Excitation of the hydrogen 21-cm line,Proceedings of the IRE46(1958) 240–250

Reference 104

Resolution: unresolved; no resolver link, observed 2026-08-04T19:14:25.522904Z

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Unavailable: canonical work link unavailable.

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