Progress towards fabrication of Th:229-doped high energy band-gap crystals for use as a solid-state optical frequency reference

TL;DR

This research advances the development of a solid-state optical frequency reference using Th:229-doped high energy band-gap crystals, demonstrating promising host materials and experimental feasibility for detecting nuclear transitions.

Contribution

The paper reports the evaluation of various high energy band-gap crystals for Th:229 doping and presents initial experimental results with LiCAF as a promising host material.

Findings

LiCAF identified as the most suitable host crystal

Mock experiment with $^{232}$Th shows high SNR potential

Feasibility of detecting Th:229 nuclear transition demonstrated

Abstract

We have recently described a novel method for the construction of a solid-state optical frequency reference based on doping $^{229}$Th into high energy band-gap crystals. Since nuclear transitions are far less sensitive to environmental conditions than atomic transitions, we have argued that the $^{229}$Th optical nuclear transition may be driven inside a host crystal resulting in an optical frequency reference with a short-term stability of $3\times10^{-17}<\Delta f/f <1\times10^{-15}$ at 1 s and a systematic-limited repeatability of $\Delta f/f \sim 2 \times 10^{-16}$. Improvement by $10^2-10^3$ of the constraints on the variability of several important fundamental constants also appears possible. Here we present the results of the first phase of these experiments. Specifically, we have evaluated several high energy band-gap crystals (Th:NaYF, Th:YLF, Th:LiCAF, Na$_2$ThF$_6$, LiSAF) for their suitability as a crystal host by a combination of electron beam microprobe measurements, Rutherford Backscattering, and synchrotron excitation/fluorescence measurements. These measurements have shown LiCAF to be the most promising host crystal, and using a $^{232}$Th doped LiCAF crystal, we have performed a mock run of the actual experiment that will be used to search for the isomeric transition in $^{229}$Th. This data indicates that a measurement of the transition energy with a signal to noise ratio (SNR) greater than 30:1 can be achieved at the lowest expected fluorescence rate.