# Design and Implementation of the ABRACADABRA-10 cm Axion Dark Matter   Search

**Authors:** Jonathan L. Ouellet, Chiara P. Salemi, Joshua W. Foster, Reyco, Henning, Zachary Bogorad, Janet M. Conrad, Joseph A. Formaggio, Yonatan Kahn,, Joe Minervini, Alexey Radovinsky, Nicholas L. Rodd, Benjamin R. Safdi, Jesse, Thaler, Daniel Winklehner, Lindley Winslow

arXiv: 1901.10652 · 2019-04-03

## TL;DR

This paper details the design, construction, and initial data analysis of the ABRACADABRA-10 cm prototype, a novel experiment aiming to detect axion dark matter within a specific mass range.

## Contribution

It introduces the ABRACADABRA-10 cm experimental setup and provides the first search results, establishing a foundation for future axion dark matter detection efforts.

## Key findings

- First axion dark matter search with ABRACADABRA-10 cm
- Development of robust statistical analysis techniques
- Constraints set on axion-photon coupling in the targeted mass range

## Abstract

The past few years have seen a renewed interest in the search for light particle dark matter. ABRACADABRA is a new experimental program to search for axion dark matter over a broad range of masses, $10^{-12}\lesssim m_a\lesssim10^{-6}$ eV. ABRACADABRA-10 cm is a small-scale prototype for a future detector that could be sensitive to QCD axion couplings. In this paper, we present the details of the design, construction, and data analysis for the first axion dark matter search with the ABRACADABRA-10 cm detector. We include a detailed discussion of the statistical techniques used to extract the limit from the first result with an emphasis on creating a robust statistical footing for interpreting those limits.

## Full text

_Full body text omitted from this summary view._ Fetch the complete paper as Markdown: https://tomesphere.com/paper/1901.10652/full.md

## Figures

16 figures with captions in the complete paper: https://tomesphere.com/paper/1901.10652/full.md

## References

33 references — full list in the complete paper: https://tomesphere.com/paper/1901.10652/full.md

---
Source: https://tomesphere.com/paper/1901.10652