Excess radiation from axion-photon conversion

Two notable anomalies in radio observations---the excess radiation in the Rayleigh-Jeans tail of the cosmic microwave background, revealed by ARCADE-2, and the twice-deeper absorption trough of the global 21-cm line, identified by EDGES---remain unresolved. These phenomena may have a shared origin, as the enhancement of the 21-cm absorption trough could arise from excess heating. We investigate this scenario through the framework of axionlike particles (ALPs), showing that the resonant conversion of ALPs into photons can produce a photon abundance sufficient to resolve both anomalies simultaneously. Our model naturally explains the observed radio excess between 0.4 and 10 GHz while also enhances the 21-cm absorption feature at 78 MHz. Furthermore, it predicts a novel power-law scaling of the radio spectrum above 0.5 GHz and an additional absorption trough below 30 MHz, which could be verified through cross-detection in upcoming experiments.

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Publication Details

Journal
Physical review. D/Physical review. D.
Published
2025-08-27
DOI
https://doi.org/10.1103/ww3t-xtcz
Citations
2
Primary Topic
Dark Matter and Cosmic Phenomena
Type
article
Field-Weighted Citation Impact
3.74
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article

Excess radiation from axion-photon conversion

Rome Samanta, Gaetano Lambiase, Qingyu Gan, Salvatore Capozzıello et al.
2 citations
Physical review. D/Physical review. D.
Dark Matter and Cosmic Phenomena
3.74
article

Excess radiation from axion-photon conversion

Rome Samanta, Gaetano Lambiase, Qingyu Gan, Salvatore Capozzıello, Andrea Addazi
article en
2 citations

Abstract

Two notable anomalies in radio observations---the excess radiation in the Rayleigh-Jeans tail of the cosmic microwave background, revealed by ARCADE-2, and the twice-deeper absorption trough of the global 21-cm line, identified by EDGES---remain unresolved. These phenomena may have a shared origin, as the enhancement of the 21-cm absorption trough could arise from excess heating. We investigate this scenario through the framework of axionlike particles (ALPs), showing that the resonant conversion of ALPs into photons can produce a photon abundance sufficient to resolve both anomalies simultaneously. Our model naturally explains the observed radio excess between 0.4 and 10 GHz while also enhances the 21-cm absorption feature at 78 MHz. Furthermore, it predicts a novel power-law scaling of the radio spectrum above 0.5 GHz and an additional absorption trough below 30 MHz, which could be verified through cross-detection in upcoming experiments.

Physical review. D/Physical review. D.Vol. 112(6)
University of Salerno (IT), Istituto Nazionale di Fisica Nucleare (IT), Sichuan University (CN), Scuola Superiore Meridionale (IT), University of Naples Federico II (IT)
Openalex Percentile: Top 7%
Dark Matter and Cosmic Phenomena
3.74
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