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Behavior of axion-like particles in smoothed out domain-like magnetic fields

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arxiv 1804.09443 v3 pith:GEV7MZSI submitted 2018-04-25 astro-ph.HE hep-ph

classification astro-ph.HEhep-ph
keywords gammaedgesdomaindomain-likephotonsmoothedwhenabove
verification ladder T0 review T1 audit T2 compute T3 formal

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abstract

Basically, in certain circumstances axion-like particles (ALPs) substantially enhance the photon survival probability $P_{\gamma \to \gamma} ({\cal E})$ of a beam emitted by a far-away source through the mechanism of photon-ALP oscillation (${\cal E}$ denotes the energy). But in order for this to work, an external magnetic field ${\bf B}$ must be present. In several cases ${\bf B}$ is modeled as a domain-like network with `sharp edges': all domains have the same size $L_{\rm dom}$ (set by the ${\bf B}$ coherence length) and the same strength B, but the direction of ${\bf B}$ changes randomly and abruptly from one domain to the next. It is obviously a highly mathematical idealization wherein the components of ${\bf B}$ are discontinuous across the edges (whence the name sharp edges). It is therefore highly desirable to go a step further, and to find out what happens when the edges are smoothed out, namely when the abrupt change of ${\bf B}$ is replaced by a smooth one. Moreover, this step becomes compelling when the photon-ALP oscillation length $l_{\rm osc}$ turns out to be comparable to -- or smaller than -- $L_{\rm dom}$, because in this case the photon survival probability $P_{\gamma \to \gamma} ({\cal E})$ critically depends on the domain shape. In the present paper we propose a smoothed out version of the previous domain-like structure of ${\bf B}$ which incorporates the above changes, and we work out its implications. Even in the present case we are able to solve analytically and exactly the photon/ALP beam propagation equation inside a single smoothed-out domain, thereby evaluating the corresponding $P_{\gamma \to \gamma} ({\cal E})$ exactly. Our results is of particular importance in view of the new generation of gamma-ray detectors, since in such a situation $l_{\rm osc} \lesssim L_{\rm dom}$ occurs just above the TeV scale.

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Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. Full citation record

  1. Line-of-sight magnetic-field propagation effects on axion-like particle constraints from GRB 221009A

    hep-ph 2026-06 unverdicted novelty 5.0 of 10

    Intergalactic magnetic field strength, coherence scale, and stochastic properties significantly alter ALP exclusion contours from GRB 221009A, while host-galaxy and Milky Way fields cause only mild changes.

  2. On the impact of magnetic-field models in galaxy clusters on constraints on axion-like particles from the lack of irregularities in high-energy spectra of astrophysical sources

    astro-ph.HE 2019-08 conditional novelty 5.0 of 10

    For a purely regular magnetic field in the X-ray cavity of NGC 1275, the ALP-photon coupling constraints from Fermi-LAT spectral smoothness are much weaker than for the purely turbulent field assumed in previous work,...

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