Updated Bounds on Axion-Like Particles from X-ray Observations
arXiv:2108.04827 · doi:10.1093/mnras/stac1224
Abstract
In this work we revisit five different point sources within or behind galaxy clusters in order to constrain the coupling constant between axion-like particles (ALPs) and photons. We use three distinct machine learning (ML) techniques and compare our results with a standard analysis. For the first time we apply approximate Bayesian computation to searches for ALPs and find consistently good performance across ML classifiers. Further, we apply more realistic 3D magnetic field simulations of galaxy clusters and compare our results with previously used 1D simulations. We find constraints on the ALP-photon coupling at the level of state-of-the-art bounds with GeV, hence improving on previous constraints obtained from the same observations.
arXiv commentv2: minor changes, 14 pages, 7 figures, 11 tables; matches accepted version to appear in MNRAS
References in corpus (30)
- Scikit-learn: Machine Learning in Python
- The SIMBAD astronomical database
- Axions In String Theory
- The Chandra Source Catalog
- The type IIB string axiverse and its low-energy phenomenology
- Sherpa: a Mission-Independent Data Analysis Application
- The Coma cluster magnetic field from Faraday rotation measures
- The QCD Axion and Moduli Stabilisation
- Magnetic Fields and Faraday Rotation in Clusters of Galaxies
- Search for Spectral Irregularities due to Photon-Axionlike-Particle Oscillations With the Fermi Large Area Telescope
- A New Bound on Axion-Like Particles
- Astrophysical limits on very light axion-like particles from Chandra grating spectroscopy of NGC 1275
- Sardinia Radio Telescope observations of Abell 194 - the intra-cluster magnetic field power spectrum
- The intracluster magnetic field power spectrum in A2199
- Constraints on axion-like particles from X-ray observations of Hydra galaxy cluster
- Magnetic power spectra from Faraday rotation maps - REALMAF and its use on Hydra A
- Constraints on Axion-Like Particles from X-ray Observations of NGC1275
- eROSITA on SRG
- Constraints on Axion-Like Particles from Non-Observation of Spectral Modulations for X-ray Point Sources
- Soft X-ray Excess in the Coma Cluster from a Cosmic Axion Background
- Behavior of axion-like particles in smoothed out domain-like magnetic fields
- beta-model and cooling flows in X-ray clusters of galaxies
- Overview of Approximate Bayesian Computation
- Projected bounds on ALPs from Athena
- The Fourier formalism for relativistic axion-photon conversion, with astrophysical applications
- Searching for Axion-Like Particles with X-ray Polarimeters
- A new probe of Axion-Like Particles: CMB polarization distortions due to cluster magnetic fields
- Constraints on non-resonant photon-axion conversion from the Planck satellite data
- Improving Statistical Sensitivity of X-ray Searches for Axion-Like Particles
- Accelerating the search for Axion-Like Particles with machine learning
Cited by in corpus (7)
- New constraints on light Axion-Like Particles using Chandra Transmission Grating Spectroscopy of the powerful cluster-hosted quasar H1821+643
- Observability of the very-high-energy emission from GRB 221009A
- ALP induced polarization effects on photons from galaxy clusters
- Photon-ALP oscillations inducing modifications to photon polarization
- Magnetohydrodynamics predicts heavy-tailed distributions of axion-photon conversion
- Physics Beyond the Standard Model with Future X-ray Observatories: Projected Constraints on Very-Light Axion-Like Particles with and
- Revisiting the evidences for spectral anomalies in distant blazars: new data on the photon-ALP mixing