The Prospect from the Upcoming CMB Experiment LiteBIRD to Discover Axion-like Particles Using Milky Way
Harsh Mehta, Suvodip Mukherjee

TL;DR
This paper proposes a new template-based method to detect axion-like particles through their non-Gaussian signatures in the CMB, demonstrating LiteBIRD's potential to improve constraints on ALP-photon coupling.
Contribution
It introduces a novel non-Gaussian analysis technique for ALP detection in CMB data, tailored for the upcoming LiteBIRD experiment, enhancing sensitivity beyond current bounds.
Findings
Constraints on ALP-photon coupling improved by an order of magnitude.
The method effectively captures non-Gaussian ALP signals in CMB data.
LiteBIRD can probe ALP masses below 10^{-14} eV with high sensitivity.
Abstract
The existence of axion-like particles (ALPs) can be probed from their signatures in the Cosmic Microwave Background (CMB) due to the photon-ALP resonant conversion over the mass range of ALPs that matches with the effective mass of photons in the plasma in the astrophysical systems. Such a conversion can also occur in the Milky Way halo and disk and can cause a unique spatial and spectral distortion. The signal is highly non-Gaussian and cannot be measured precisely by the usual power-spectrum approach. We devise a new technique to search for this signal from the upcoming full-sky CMB experiment LiteBIRD using its multi-frequency band using a template-based spatial profile of the ALP distortion signal. This technique captures the large-scale non-Gaussian aspects of the ALP distortion signal in terms of a spatial template and makes it possible to search for any non-zero ALP signal. We…
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Taxonomy
TopicsDark Matter and Cosmic Phenomena · Particle physics theoretical and experimental studies · Astrophysics and Cosmic Phenomena
