Search for solar axions produced through the axion-electron coupling $g_{ae}$ using a new GridPix detector at CAST

TL;DR

This paper reports a new search for solar axions via the axion-electron coupling using a novel detector at CAST, setting improved limits on axion couplings with potential implications for axion physics.

Contribution

Introduction of a new GridPix detector at CAST with machine learning background suppression, leading to improved limits on axion-electron and axion-photon couplings.

Findings

No significant axion signal detected.

Set new upper limit on $g_{ae} imes g_{a ext{γ}}$.

Derived competitive limit on $g_{a ext{γ}}$.

Abstract

We present a search for solar axions produced through the axion-electron coupling $(g_{ae})$ using data from a novel 7-GridPix detector installed at the CERN Axion Solar Telescope (CAST). The detector, featuring ultra-thin silicon nitride windows and multiple veto systems, collected approximately 160 hours of solar tracking data between 2017-2018. Using machine learning techniques and the veto systems, we achieved a background rate of $1.06\times 10^{-5}\,\text{keV}^{-1}\text{cm}^{-2}\text{s}^{-1}$ at a signal efficiency of about $80\,\%$ in the $0.2$-$8\,\text{keV}$ range. Analysis of the data yielded no significant excess above background, allowing us to set a new upper limit on the product of the axion-electron and axion-photon couplings of $g_{ae}\cdot g_{a\gamma} < 7.35\times 10^{-23}\,\text{GeV}^{-1}$ at $95\,\%$ confidence level. This result improves upon the previous best helioscope limit and demonstrates the potential of GridPix technology for rare event searches. Additionally, we derived a limit on the axion-photon coupling of $g_{a\gamma} < 9.0\times 10^{-11}\,\text{GeV}^{-1}$ at $95\,\%$ CL, which, while not surpassing CAST's best limit, provides complementary constraints on axion models.