Behavior of axion-like particles in smoothed out domain-like magnetic fields
arXiv:1804.09443 · doi:10.1103/PhysRevD.98.043018
Abstract
Basically, in certain circumstances axion-like particles (ALPs) substantially enhance the photon survival probability of a beam emitted by a far-away source through the mechanism of photon-ALP oscillation ( denotes the energy). But in order for this to work, an external magnetic field must be present. In several cases is modeled as a domain-like network with `sharp edges': all domains have the same size (set by the coherence length) and the same strength B, but the direction of changes randomly and abruptly from one domain to the next. It is obviously a highly mathematical idealization wherein the components of 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 is replaced by a smooth one. Moreover, this step becomes compelling when the photon-ALP oscillation length turns out to be comparable to -- or smaller than -- , because in this case the photon survival probability critically depends on the domain shape. In the present paper we propose a smoothed out version of the previous domain-like structure of 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 exactly. Our results is of particular importance in view of the new generation of gamma-ray detectors, since in such a situation occurs just above the TeV scale.
30 pages, 14 figures. This version matches the published paper: Phys. Rev. D 98, 043018 (2018)
References in corpus (43)
- Revisiting the bound on axion-photon coupling from Globular Clusters
- Collider Probes of Axion-Like Particles
- Revisiting the SN1987A gamma-ray limit on ultralight axion-like particles
- Evidence for a new light spin-zero boson from cosmological gamma-ray propagation?
- Constraining the mass of dark photons and axion-like particles through black-hole superradiance
- The Milky Way as a Kiloparsec-Scale Axionscope
- The extragalactic background light revisited and the cosmic photon-photon opacity
- An M Theory Solution to the Strong CP Problem and Constraints on the Axiverse
- Hints of the existence of Axion-Like-Particles from the gamma-ray spectra of cosmological sources
- Detecting Axion-Like Particles With Gamma Ray Telescopes
- Cluster Magnetic Fields from Galactic Outflows
- Magnetic Field Seeding by Galactic Winds
- The Quest for an Intermediate-Scale Accidental Axion and Further ALPs
- On the amplification of magnetic fields in cosmic filaments and galaxy clusters
- Signatures of axion-like particles in the spectra of TeV gamma-ray sources
- Constraining the Axion-Photon Coupling with Massive Stars
- The spatial energy spectrum of magnetic fields in our Galaxy
- A 3.55 keV Photon Line and its Morphology from a 3.55 keV ALP Line
- Axion-Like Particles, Cosmic Magnetic Fields and Gamma-Ray Astrophysics
- Effects of Axion-Photon Mixing on Gamma-Ray Spectra from Magnetized Astrophysical Sources
- Detecting Chameleons: The Astronomical Polarization Produced by Chameleon-like Scalar Fields
- The Effect of the AGN Feedback on the Interstellar Medium of Early-Type Galaxies: 2D Hydrodynamical Simulations of the Low-Rotation Case
- On detecting oscillations of gamma rays into axion-like particles in turbulent and coherent magnetic fields
- Photons to axion-like particles conversion in Active Galactic Nuclei
- Irregularity in gamma ray source spectra as a signature of axionlike particles
- 3.55 keV photon lines from axion to photon conversion in the Milky Way and M31
- Sensitivity of the Cherenkov Telescope Array to the detection of axion-like particles at high gamma-ray opacities
- The Spectrum of the Axion Dark Sector
- New Bounds on Axion-Like Particles From the Fermi Large Area Telescope observation of PKS
- Evolution of cosmic filaments and of their galaxy population from MHD cosmological simulations
- Axionic black branes in the k-essence sector of the Horndeski model
- Extragalactic photon-ALP conversion at CTA energies
- Axionic black branes with conformal coupling
- Astrophysical Haloscopes
- Shining light through the Sun
- Probing axion-like particles with the ultraviolet photon polarization from active galactic nuclei in radio galaxies
- Seeing the Invisible Axion in the Sparticle Spectrum
- Searching for Axion-Like Particles with X-ray Polarimeters
- Signatures of photon and axion-like particle mixing in the gamma-ray burst jet
- The potential of large germanium detector arrays for solar-axion searches utilizing the axio-electric effect for detection
- ALP Conversion and the Soft X-ray Excess in the Outskirts of the Coma Cluster
- Photon-axion mixing within the jets of Active Galactic Nuclei and prospects for detection
- The e-ASTROGAM gamma-ray space observatory for the multimessenger astronomy of the 2030s
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- Limits on axion-like particles from Mrk 421 with 4.5-year period observations by ARGO-YBJ and Fermi-LAT
- Blazar VHE spectral alterations induced by photon-ALP oscillations
- 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
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- Constraints on Axion-like Particles from the Observation of GRB 221009A by LHAASO
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- Axion-like Particle Effects on Photon Polarization in High-Energy Astrophysics
- Optical circular polarization induced by axionlike particles in blazars
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- Probing the absorption of gamma-rays by IR radiation from the dusty torus in FSRQs with the Cherenkov Telescope Array
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- Revisiting the evidences for spectral anomalies in distant blazars: new data on the photon-ALP mixing
- Axion-photon conversion in stochastic magnetic fields
- Axion-like Particles and their Possible Impact on the Very High-Energy Spectrum of M87 Observed by LHAASO
- How do Magnetic Field Models Affect Astrophysical Limits on Light Axion-like Particles? An X-ray Case Study with NGC 1275