New constraints on light Axion-Like Particles using Chandra Transmission Grating Spectroscopy of the powerful cluster-hosted quasar H1821+643

TL;DR

This study uses high-resolution Chandra X-ray spectra of a quasar in a galaxy cluster to set new constraints on light Axion-Like Particles, improving previous limits and highlighting future research prospects with upcoming missions.

Contribution

First application of detailed magnetic field modeling to constrain ALPs using Chandra spectra of a cluster-hosted quasar, achieving more stringent bounds than previous studies.

Findings

Excluded ALP-photon coupling > 6.3 x 10^{-13} GeV^{-1} for masses < 10^{-12} eV at 99.7% credibility.

Demonstrated the effectiveness of turbulent magnetic field modeling in constraining ALPs.

Highlighted the potential of future X-ray missions like Athena for ALP research.

Abstract

Axion-Like Particles (ALPs) are predicted by several Beyond the Standard Model theories, in particular, string theory. In the presence of an external magnetic field perpendicular to the direction of propagation, ALPs can couple to photons. Therefore, if an X-ray source is viewed through a magnetised plasma, such as a luminous quasar in a galaxy cluster, we may expect spectral distortions that are well described by photon-ALP oscillations. We present a $571 \ \mathrm{ks}$ combined High and Low Energy Transmission Grating (HETG/LETG) Chandra observation of the powerful radio-quiet quasar H1821+643, hosted by a cool-core cluster at redshift $0.3$. The spectrum is well described by a double power-law continuum and broad$+$narrow iron line emission typical of type-1 Active Galactic Nuclei (AGN), with remaining spectral features $< 2.5\%$. Using a cell-based approach to describe the turbulent cluster magnetic field, we compare our spectrum with photon-ALP mixing curves for 500 field realisations assuming that the thermal-to-magnetic pressure ratio remains constant up to the virial radius. At $99.7\%$ credibility and taking $\beta = 100$, we exclude all couplings $g_\mathrm{a\gamma} > 6.3 \times 10^{-13} \ {\mathrm{GeV}}^{-1}$ for most ALP masses $< 10^{-12} \ \mathrm{eV}$. Our results are moderately more sensitive to constraining ALPs than the best previous result from Chandra observations of the Perseus cluster, albeit with a less constrained field model. We reflect on the promising future of ALP studies with bright AGN embedded in rich clusters, especially with the upcoming Athena mission.