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# Axion dark matter detection by laser induced fluorescence in rare-earth doped materials

## Abstract

We present a detection scheme to search for QCD axion dark matter, that is based on a direct interaction between axions and electrons explicitly predicted by DFSZ axion models. The local axion dark matter field shall drive transitions between Zeeman-split atomic levels separated by the axion rest mass energy m a c 2. Axion-related excitations are then detected with an upconversion scheme involving a pump laser that converts the absorbed axion energy (~hundreds of μeV) to visible or infrared photons, where single photon detection is an established technique. The proposed scheme involves rare-earth ions doped into solid-state crystalline materials, and the optical transitions take place between energy levels of 4f N electron configuration. Beyond discussing theoretical aspects and requirements to achieve a cosmologically relevant sensitivity, especially in terms of spectroscopic material properties, we experimentally investigate backgrounds due to the pump laser at temperatures in the range 1.9 − 4.2 K. Our results rule out excitation of the upper Zeeman component of the ground state by laser-related heating effects, and are of some help in optimizing activated material parameters to suppress the multiphonon-assisted Stokes fluorescence.

## Introduction

The nature of dark matter (DM) is the most long standing question in Big Bang cosmology, and direct searches may shed light on this intriguing mystery. The non-detection of particle DM in the heavy mass range (10 GeV to 10 TeV)1,2,3 has motivated the scientific community to focus theoretical and experimental efforts on much lower mass particles4,5. Among them, a well motivated light particle is the QCD axion6,7, introduced by Peccei-Quinn to solve the strong CP problem8. Axion physical properties are described by several models that can be grouped into the KSVZ9,10 and DFSZ classes11,12,13, depending on zero or full axion coupling strength to leptons, respectively. Even so, an almost model-independent statement holds for the axion mass

$${m}_{a}\simeq 0.6\times {10}^{-4}{\rm{eV}}(\frac{{10}^{11}{\rm{GeV}}}{{f}_{a}}),$$
(1)

where f a is the Peccei-Queen symmetry-breaking energy scale, inversely proportional to the coupling strenghts with standard model particles6,7. A light and stable axion emerges as an ideal DM candidate if large f a are considered. Due to the resulting huge occupation number, galactic halo axions can be described as a classical oscillating field a, with oscillation frequency $${\nu }_{a}={m}_{a}{c}^{2}/h$$ 14. The $${10}^{-6} < {m}_{a} < {10}^{-3}$$ eV axion mass range has since long been favoured by astrophysical and cosmological bounds15, while very recent high-temperature lattice QCD calculations suggest that $${m}_{a}\geqslant 50\,\mu$$eV16.

The axion is intensively searched in haloscope experiments17, mostly based on resonant axion-photon conversion in a static magnetic field via Primakoff effect. The Axion Dark Matter eXperiment (ADMX) is the most sensitive haloscope detector based on high quality factor microwave resonators at cryogenic temperature. ADMX searches have excluded the mass range 1.9 < m a  < 3.69 μeV18,19. The experiment HAYSTAC (formally ADMX-High Frequency)20, designed specifically to search for axions in the 20–100 μeV range (5–25 GHz), has recently reached cosmologically relevant sensitivity at 24 μeV (~5.8 GHz).

The axion-electron coupling, explicitly predicted by DFSZ models11,12,13, can be considered to envisage another class of haloscopes, thereby providing the opportunity to discriminate among axion models in case of detection. Complementary approaches may prove crucial to determine the fractional amount of axions as DM constituent. For instance, inhomogeneous filled cavities, in which the effective axion field is converted to magnetization oscillations of a ferrimagnet, are under study21. In this case, single photon detection is required, and it can be realized by e.g. superconducting circuit devices acting as quantum bits properly coupled to the cavity photons22,23, but as yet their dark count rate still exceeds the axion interaction rate.

Approaches described so far are affected by an extremely poor sensitivity for axion masses above 0.2 meV (~50 GHz), where the effective detector volume is a critical issue. Extension to the mass range up to 1 meV (250 GHz) may be rather accomplished in suitable condensed matter experiments, in which the space parameters hardly accessible to cavity technology could be tackled with the upconversion scheme investigated in this work, whereby cosmological axions cause transitions between Zeeman split levels of suitable atomic species.

As target atoms we consider rare-earth (RE) elements inserted as dopants in crystalline matrices, where they exist as trivalent ions, substitutional for one of the atoms of the host with the same valence state and similar ionic radius. Among RE ions, those with an odd number of 4f electrons are called Kramers ions24, and have electronic doublet levels with magnetic moments of the order of 1–10 Bohr magnetons μ B . Therefore, using Kramers doublets, axion-induced spin transitions can take place in the GHz range with application of moderate magnetic fields. For instance, in Er3+, the calculated splitting spans from 20 to 120 GHz with applied magnetic fields in the interval 0.4 to 2.5 T25, which translates to a large tunability in the favoured cosmological axion mass window.

In the direct axion-electron coupling26,27 the interaction energy is $$({g}_{ae}\mathrm{/2}e)\overrightarrow{\nabla }a\cdot \overrightarrow{\mu }$$, where the term $$({g}_{ae}\mathrm{/2}e)\overrightarrow{\nabla }a$$ plays the role of an effective oscillating field, $$\overrightarrow{\mu }$$ is the electron magnetic moment with electric charge e and $${g}_{ae}$$ is the coupling constant17. Resonant condition is met when the Zeeman splitting energy is m a c 2. As schematized in Fig. 1(a), the axion excitation is upconverted by a pump laser to photons in visible or infrared ranges, where single photon detection with ultra-low dark count rate has been already demonstrated28,29,30.

The proposed detection scheme is based on electronic transitions between states within a $$4f$$ configuration of the trivalent RE, with positions of the discrete energy levels minimally perturbed by the crystal-field due to the screening action of the 5s and 5p orbitals24. It is immediately evident that a first requirement for the feasibility of such a scheme is related to the the linewidth of the transition driven by the laser, which must be narrower than the energy difference between the atomic levels $$\mathrm{|0}\rangle$$ and $$|i\rangle$$.

Detectability of axions in this scheme can be at first discussed by considering only the thermal excitation of the atomic level as fundamental noise limit. Backgrounds of different nature are left for experimental investigations in the second part of the work.

We consider one mole of target atoms in the ground state $$\mathrm{|0}\rangle$$ and, using Eq. 8 of ref.31, we establish the transition rate to the level $$|i\rangle$$ by axion absorption on resonance:

$${N}_{A}{R}_{i}=8.5\times {10}^{-3}\,(\frac{{\rho }_{a}}{0.4\,{\rm{GeV}}/{{\rm{cm}}}^{3}}){(\frac{{E}_{a}}{330\mu {\rm{eV}}})}^{2}{g}_{i}^{2}(\frac{\overline{{v}^{2}}}{{10}^{-6}{c}^{2}})(\frac{{\rm{\min }}(t,\tau ,{\tau }_{\nabla a})}{{10}^{-6}\,{\rm{s}}})\,{\rm{Hz}},$$
(2)

where $${R}_{i}$$ is the transition rate of a single target atom, N A is the Avogadro number, $${E}_{a}=h{\nu }_{a}$$ is the axion energy, $${g}_{i}$$ is the coupling strength to the target atom and is of the order of one31, and $$\overline{{v}^{2}}$$ is the mean square of the axion velocity. The value $$330\,\mu$$eV (80 GHz) is a midpoint of the Zeeman splitting frequency interval reported for Er3+ in ref.25. As in the considered galactic halo model axions are galaxy dominant component of dark matter, we take for its energy density $${\rho }_{a}$$ the value 0.4 GeV/cm3 obtained from galaxy rotational curves.

The experiment coherence time is set by $${\rm{\min }}(t,\tau ,{\tau }_{\nabla a})$$, where t is the measurement integration time (inverse of the resolution bandwidth), and $${\tau }_{\nabla a}$$ is the axion gradient coherence time at the resonant frequency of the experiment that can be calculated from the axion coherence time $${\tau }_{a}=h/({E}_{a}\overline{{v}^{2}}/{c}^{2})$$ 32. The latter is related to the width of the axion kinetic energy distribution in the laboratory frame. If we assume a Maxwellian velocity distribution in the Galactic rest frame and we take $${(\overline{{v}^{2}})}^{\mathrm{1/2}}\simeq {10}^{-3}c$$ as the local dark matter virial velocity, we get $${\tau }_{a}=91\cdot \mathrm{(330}\,\mu {\rm{e}}V/{m}_{a})\,\mu {\rm{s}}$$, and finally21

$${\tau }_{\nabla a}\simeq 0.68\,{\tau }_{a}=4(\frac{330\,\mu {\rm{eV}}}{{E}_{a}})(\frac{{Q}_{a}}{1.9\times {10}^{6}})\mu {\rm{s}}\mathrm{.}$$
(3)

where the merit factor $${Q}_{a}\equiv 2{\tau }_{a}{\nu }_{a}\simeq 1.9\times {10}^{6}$$ qualifies the axion-microwave linewidth in haloscope experiments.

The lifetime of the Zeeman excited state τ is typically much longer than $${\tau }_{\nabla a}$$, and in the rare-earth doped materials considered in this work is strongly dependent on temperature, intensity of the static magnetic field, dopant concentration33,34,35,36. The magnetic field, beyond splitting degenerate levels and thus opening a channel for resonant axion detection, may also inhibit spin flips and thus increase the lifetime τ of the intermediate level. Lifetimes much longer than ms have been measured in several rare-earth activated optical materials at liquid helium temperature with magnetic fields comparable to those used in this work ($$\sim 0.5$$ T) up to about 3 T34. Incidentally, for a given pump laser intensity, the efficiency of the mentioned upconversion process is greater for longer τ, thus allowing for mitigation of the laser power requirements when large detecting volumes are devised37.

As one might expect, the experiment must be operated in a ultra-cryogenic environment to minimize thermal population of the Zeeman excited level. To establish the working temperature of the apparatus, we treat the pumped crystal as if it were a single photon detector with overall efficiency $$\eta =0.5$$ (including the efficiency of upconversion, the fluorescence collection efficiency and self absorption) and consider thermal excitation of the target ions. For a given temperature T of the doped crystal, the corresponding excitation rate is related to the lifetime of the Zeeman excited level

$${N}_{A}{R}_{t}=\bar{n}/\tau ,$$
(4)

with $$\bar{n}={N}_{A}\,\exp (-{E}_{a}/kT)$$ average number of excited ions in the energy level $${E}_{a}$$, and k the Boltzmann constant. It is worth noticing that the contribution of adjacent Stark sublevels (due to interaction with the crystalline field) is not considered when their energy is much higher than $${E}_{a}$$, as is the case analyzed in this work. To ensure a signal to noise ratio (SNR) of 3 with a statistically significant number of counts within one hour observation time38, the thermal excitation rate settles to $${R}_{t}=6\times {10}^{-3}$$ Hz. If a level lifetime of τ = 1 ms is taken, axions with mass greater than 80 GHz can be searched, provided the active crystal is cooled down to at least 57 mK.

## Results

We demonstrate here that we are able to resolve the involved transitions in a rare-earth doped material, that is a prerequisite for the feasibility of the proposed detection scheme. We then focus our experimental investigations on possible backgrounds induced by the pump laser at cryogenic temperatures and sub-Tesla magnetic field. The samples utilized in these measurements have 1% and 0.01% Er3+ -dopant nominal concentration, which correspond to $$1.4\cdot {10}^{20}$$ and $$1.4\cdot {10}^{18}$$ ions/cm3, with three $$4f$$ electrons for each ion available as axion targets. Crystals with dopant concentrations well below 0.1% have been the subject of much scientific investigation for photon-echo-based optical data storage and data processing, owing to their narrow $$4f-4f$$ transition linewidths and long optical coherence times (see ref.34 and references therein). In this work we are interested in the behavior of higher concentration samples to maximize the axion interaction rate given by Eq. (2) for a given laser-pumped, active detector volume. Moreover, the 1% concentration samples allow for higher sensitivity to laser related backgrounds in the measurements described in this section.

### Zeeman splitting of the 4I15/2,5/2

We consider the electronic ground state $${}^{2S+1}L_{J}$$ of the erbium Kramers ion, the $${}^{4}I_{\mathrm{15/2}}$$. The interaction with the crystal-field splits the $$2J+1$$ magnetic sublevels into eight ($$J+\mathrm{1/2}$$) Kramers doublets, labeled by $$|{M}_{J}|$$, namely the absolute value of the J projection on the crystal optical axis c, $$|{M}_{J}|=\mathrm{15/2},\mathrm{13/2},\ldots \mathrm{,\; 3/2},\mathrm{1/2}$$. Through application of a magnetic field parallel to the c-axis, each Kramers doublet splits into two magnetic components: $${}^{4}I_{\mathrm{15/2,|}{M}_{J}|,-}$$ and $${}^{4}I_{\mathrm{15/2,|}{M}_{J}|,+}$$. In YLiF4:Er3+, the lowest Kramers doublet is the $${}^{4}I_{\mathrm{15/2,5/2}}$$. To determine its splitting under application of a 370 mT magnetic field, we measure the wavelength of transitions coupling the Zeeman components of the ground $${}^{4}I_{\mathrm{15/2,5/2}}$$ and the $${}^{4}I_{\mathrm{9/2,}\,\mathrm{9/2}}$$ excited level by laser induced fluorescence (LIF) measurements.

In Fig. 2 we report the results obtained with the 0.01% concentration sample, where different incident laser polarization orientations (orthogonal and parallel to the crystallographic axis c) allow for a better detectability of possible transitions between Zeeman-split ground and excited states. The fluorescence spectrum displays sharp, well-separated lines. Among the observed transitions, only $${}^{4}I_{\mathrm{15/2,}\,\mathrm{5/2,}+}\to \,{}^{4}I_{\mathrm{9/2,}\,\mathrm{9/2,}-}$$ ($${\lambda }_{1}=809.029$$ nm) and $${}^{4}I_{\mathrm{15/2,}\,\mathrm{5/2,}-}\to \,{}^{4}I_{\mathrm{9/2,}\,\mathrm{9/2,}+}$$ ($${\lambda }_{4}=808.955$$ nm) are unambiguously identified. With the displayed data it is then not possible to determine whether the energy levels differences $${\rm{\Delta }}{E}_{31}=73.9$$μeV, $${\rm{\Delta }}{E}_{42}=77.7$$ $$\mu$$eV and $${\rm{\Delta }}{E}_{21}=62.5$$ $$\mu$$eV, $${\rm{\Delta }}{E}_{43}=66.4$$μeV represent the ground state or the excited level $${}^{4}I_{\mathrm{9/2,}\,\mathrm{9/2}}$$ splittings. We accomplish this task by laser excitation of the thermal population in the Zeeman-split first excited Stark level of the ground state. Independently of this limitation, the plots in Fig. 2 demonstrate that we are able to resolve the Zeeman splitting and therefore that it is possible to monitor the population of the upper Zeeman component of the ground state. Clearly, at $$T=2$$ K thermal excitation of the level still prevents us from assigning a detection sensitivity to the present apparatus, but before we get to cool the sample to hundreds of mK temperatures, a thorough investigation of the pump laser related noise is accomplished as described in the following sections.

The LIF measurements in Fig. 2 have been repeated with the 1% concentration sample. In this case the Zeeman transition is hardly resolved due to increased transition linewidths, ascribable to spin cross relaxation processes due to direct interactions among Er3+ ions36,39. However, such a limitation might be overcome in the high magnetic field and low temperature regime, required to achieve ultimate sensitivity in the proposed axion detection scheme. For instance, in a 0.1% concentration sample of YLiF4:Er3+, authors have investigated the four transitions connecting the Zeeman sublevels of the ground and lowest $${}^{4}F_{\mathrm{9/2}}$$ excited state and demonstrated that their linewidth can be as narrow as $$\sim 1$$ MHz40. The applied magnetic field was about 3 T and measurements were conducted below 4 K by Zeeman-switched optical-free-induction decay technique. These results, together with our findings, foster the development of a few liters detector with intermediate concentration active materials, matching the axion-induced transition rate in Eq. 2 to dark count rates in available single photon counters28,29,30. As a final additional remark, we note that an intermediate concentration sample would allow for increasing the axion-electron interactions of six orders of magnitude compared to a gaseous target prepared by buffer cooling techniques41.

### Laser-induced thermal noise

To assess heating effects in the active detector volume, we focus on the population of the first excited Stark (crystal-field) sublevel $${}^{4}I_{\mathrm{15/2,15/2}}$$, that has a strong thermal coupling with the ground energy level. To enhance the sensitivity of our tests, we use the 1% concentration sample. The crystal-field splittings of Er3+ ions in YLiF4 have been calculated and measured by previous authors42,43 and for the $${}^{4}I_{\mathrm{15/2,15/2}}$$ sublevel the separation from the ground state is $${E}_{{\rm{S}}1}=17$$ cm−1 (2.11 meV). If E Sj are the Stark sublevels energies of the $${}^{4}I_{\mathrm{15/2}}$$ level, the occupation probability of the first excited Stark level is proportional to $${e}^{-{E}_{{\rm{S}}1}/kT}/(1+{\sum }_{j=1}^{{M}_{J}}\,{e}^{-{E}_{{\rm{Sj}}}/kT})$$, where the sum is well approximated with the first two terms. As the fluorescence intensity F is proportional to the laser intensity I times the level occupation number $$\bar{n}$$, we model a possible heating effect with the term $$\beta I$$ in expression $$F(T,I)\simeq \alpha I\,\exp [-{E}_{{\rm{S}}1}/(kT+\beta I)]$$, where α, β are empirical parameters determined from a fit to the data.

From the data shown in the inset of Fig. 3, we infer that the β parameter is compatible with zero within one standard deviation, which allows us to limit the temperature increase to less than 4.5 mK/[W/cm2]. We stress that such limit is obtained in an unfavorable upconversion scheme, where the de-excitation takes place also through non radiative channels as shown in Fig. 1(c). Therefore we can assign the temperature of the thermal bath to the entire crystal and calculate the ratio of the populations of the same Stark level at two different temperatures T 1 and T 2. Such ratio is then compared to the LIF peak areas.

As shown in Fig. 3, with the pump laser tuned to the transition $${}^{4}I_{\mathrm{15/2,15/2}}\to {}^{4}I_{9/\mathrm{2,9/2}}$$, we obtain peaks that differ only in their area for $${T}_{1}=2.16$$ K and $${T}_{2}=1.93$$ K. The Er(1%):YLF crystal is immersed in superfluid He, and these points are obtained under λ-point operation at which bubbling disturbances are eliminated. A small satellite line is present on the right side of the main peak at both temperatures, which hinders an accurate fitting of the data. Therefore we compare the areas of the main peaks at $${T}_{1}=2.16$$ K and $${T}_{2}=1.93$$ K by summing the amplitudes of the data recorded at four wavelengths around resonance. The ratio of $$3.6\pm 0.3$$ is in agreement with the expected value, confirming the assumption made in the introduction to calculate the rate of excited atoms via thermal bath temperature.

In addition, we confirm experimentally (Fig. 4) that also the population of the Zeeman-split levels follows Boltzmann statistics. In this case, the pump laser is set to probe the populations of the Zeeman-split levels of the first excited Stark sublevel ($${}^{4}I_{\mathrm{15/2,}\,\mathrm{15/2,}+}$$ and $${}^{4}I_{\mathrm{15/2,}\,\mathrm{15/2,}-}$$). As a larger splitting is expected for this level as compared to the ground state43, by pumping the transitions to the Zeeman levels of the $${}^{4}I_{\mathrm{9/2,9/2}}$$, the previously measured energy differences (Fig. 2) can also be precisely identified. In fact, from the wavelengths reported in the first column of Table 1, we obtain the splitting of the first excited Stark level $${\rm{\Delta }}{E}_{e}\equiv {\rm{\Delta }}{E}_{13}={\rm{\Delta }}{E}_{42}^{\text{'}}=164.4$$ $$\mu$$eV and $${\rm{\Delta }}{E}_{12}^{\text{'}}={\rm{\Delta }}{E}_{43}^{\text{'}}=75.6$$ $$\mu$$eV, where the indices are assigned as described in the inset of Fig. 4. The latter value is consistent with the average of $${\rm{\Delta }}{E}_{31}=73.9$$ $$\mu$$eV, $${\rm{\Delta }}{E}_{42}=77.7$$μeV obtained from data in Fig. 2. Consequently, we take the average $${\rm{\Delta }}{E}_{g}\equiv ({\rm{\Delta }}{E}_{21}+{\rm{\Delta }}{E}_{43}\mathrm{)/2}=64.5\,\mu$$eV as the searched splitting of the ground state. To further confirm proper identification of the Zeeman split levels, we can use the ratios of reported g factors in the same material oriented with its c-axis parallel to the magnetic field43. We obtain $${\rm{\Delta }}{E}_{g}/{\rm{\Delta }}{E}_{e}=0.39$$, in agreement with $${g}_{||}\mathrm{[15/2,5/2]/}{g}_{||}\mathrm{[15/2,15/2]=3.137/7.97=0.39}\pm 0.01$$. The ground state splitting value we measured at 0.37 mT is also in fair agreement with theoretical values reported in ref.25.

That is as far as our LIF measurement of the ground level splitting is concerned. As for the investigations of possible laser-induced deviations from Boltzmann statistics, we consider the peak areas of LIF measured for the levels $${}^{4}I_{\mathrm{15/2,}\,\mathrm{15/2,}+}$$ and $${}^{4}I_{\mathrm{15/2,}\,\mathrm{15/2,}-}$$. The data displayed in Fig. 4. are fitted to a Lorentzian curve in the form $$F(\lambda )={y}_{0}+2\frac{A}{\pi }\cdot \frac{w}{\mathrm{4(}\lambda -{\lambda }_{c}{)}^{2}+{w}^{2}}$$ and the results are reported in Table 1. The ratio $$A\mathrm{(1)/}A\mathrm{(4)}=0.69$$ and $$A\mathrm{(2)/}A\mathrm{(3)}=0.64$$ is in fair agreement with 0.69 expected ratio at $$T=4.2$$ K. At $$T=1.93$$ K we obtain $$A\mathrm{(1)/}A\mathrm{(4)}=0.35$$ and $$A\mathrm{(2)/}A\mathrm{(3)}=0.48$$, which averages to a value compatible with the calculated one 0.37.

### Multiphonon background

In the data reported in Fig. 4. (lower side) the apparatus sensitivity allows observation of an out-of-resonance fluorescence level. To understand the physical origin of this background, we measure its intensity for values of pump laser wavelength in a wide range (corresponding to 10300–12360 cm−1), as shown in Fig. 5. The LIF measured with the pump laser tuned to transition $${}^{4}I_{\mathrm{15/2}}\to {}^{4}I_{\mathrm{9/2}}$$ is also plotted for comparison.

A similar exponential behaviour has been previously reported in Er:YLF and has been explained in terms of multiphonon-assisted, side-band absorption44. The RE manifolds $${E}_{\mathrm{1,2}}$$ can be in fact excited even by a nonresonant pump photon $${E}_{1} < E < {E}_{2}$$, when the missing/excess energy is bridged by absorption/emission of phonons via Anti-Stokes and Stokes processes, respectively. The related absorbed intensity is theoretically given by:

$$I(E)=I({E}_{1}){e}^{-{\alpha }_{{\rm{S}}}(E-{E}_{1})}+I({E}_{2}){e}^{-{\alpha }_{{\rm{A}}S}({E}_{2}-E)}$$
(5)

where $${\alpha }_{{\rm{S}}}$$ and $${\alpha }_{{\rm{A}}S}$$ are the Stokes and Anti-Stokes coefficients, described in the model45 through expressions:

$${\alpha }_{{\rm{S}}}={(\hslash {\omega }_{{\rm{eff}}})}^{-1}\,\mathrm{ln}\,(\frac{p}{{S}_{0}(n+\mathrm{1)}}-1)$$
(6)
$${\alpha }_{{\rm{AS}}}={\alpha }_{{\rm{S}}}+\mathrm{1/}kT\mathrm{.}$$
(7)

In Eq. (6), $$\hslash {\omega }_{{\rm{eff}}}$$ is the crystal effective phonon energy, p is the number of photons needed to bridge the energy gap, $$n$$ is the average occupation number and $${S}_{0}$$ the Huang-Rhys coefficient that represents the electron-phonon coupling strength. Typical values of $$\hslash {\omega }_{{\rm{eff}}}$$ are smaller than 200 cm−1 in bromides, greater than 400 cm−1 in oxides46, and in YLF the value 400 cm−1 is reported.

The strong suppression of the LIF observed in our 4.2 K data as soon as the pumping wavelength differs from the pure electronic transition wavelength (Fig. 5) is ascribable to the expected suppression of the AS component with temperature (from eq. 7) and the exponential growth for increasing wavelengths is then mainly due to the Stokes process. Fitting of data with wavelength greater than 850 nm give an absorption coefficient $${\alpha }_{{\rm{S}}}=9.2\cdot {10}^{-3}$$ cm−1, in agreement with the value reported in ref.47. Ground state absorption measurements allow to estimate a $$2\cdot {10}^{-20}$$ cm2 cross section of the pure electronic transition (circled data in Fig. 5) and thus to quantify the upconversion efficiency and the multiphonon side band relative amplitude. This type of background hinders the application of the present scheme to axion detection, unless a suitable combination of rare-earth dopant, pumping pathway and matrix is chosen. In particular, relevant suppression of the background should be accomplished in low phonon energy host matrices46 or, as suggested by Eq. (5), by exploiting pumping schemes with larger $$E-{E}_{1}$$. It is worth mentioning that an ultimate laser-induced background might also originate from impurity absorption, the same process that is currently limiting the efficiency of optical refrigeration48,49,50.

## Discussion

We have discussed a solid-state approach for direct detection of axion dark matter, and established the most important experimental parameters necessary to reach cosmologically relevant sensitivity in DFSZ models. The effect of the continuous, coherent axion field is searched in the excitation of the Zeeman upper component $$|i\rangle$$ of the ground state of rare earth ions in crystalline matrices, at the energy scale $${\rm{\Delta }}{E}_{g}$$, corresponding to transitions in the $$\sim 100$$ GHz range. The population of this excited level is probed by a pump laser tuned to the transition to a fluorescent level within the same $$4f$$ atomic configuration, so as to convert the axion excitation into photons, detectable with state-of-the-art single-photon detectors. Assuming thermal excitation of the excited Zeeman level as fundamental noise limit, the active detector volume must be cooled down to ultracryogenic temperatures. The rate of thermal excitation of the $$|i\rangle$$ atomic level is directly related to its lifetime τ, and the temperature of less than $$\lesssim 0.3$$ K, at which the final experiment must be performed, has been estimated for 80 GHz axion-induced transitions and τ = 1 ms by requiring SNR $$\gtrsim 3$$. As long as $$\tau \geqslant 1\,$$ ms, a high upconversion efficiency is also ensured for tens of W/cm2 pumping intensity.

In the proposed scheme it is important to address a thorough experimental study of pump laser-related backgrounds. As a first step we have probed the population of atomic levels close to the ground state via LIF measurements in the temperature range 1.9–4.2 K. Our main finding is that the pump laser does not affect the thermal population of the Zeeman excited level at least up to a few W/cm2 intensity. In addition, we have shown that it is crucial to optimize the pumping pathway and crystal properties to minimize scattering of the pump photons on crystal phonons (Stokes process).

As for the detection scheme via laser induced fluorescence, at 4.2 K and with 370 mT magnetic field, we have demonstrated that the four transitions coupling the Zeeman levels of the ground and the excited $${}^{4}I_{\mathrm{9/2}}$$ can be resolved in the lowest concentration YLiF4:Er3+ sample (0.01%). This was not possible in the 1% sample. However, the spin population dynamics in Kramers ions strongly depends on applied magnetic field, temperature, dopant concentration and species, and we argue that a tradeoff between these parameters can be found for the proposed experiment feasibility. A few liters active volume ensures ~mHz axion and thermal transition rates, corresponding to statistically relevant counts of upconverted photons in a measurement time of a few hours. Fortuitously, the dark count rate of state-of-the-art single photon detectors holds below the transition rate in the detector active volume.

We are witnessing a blooming of table-top experiments pursuing new observables for axion DM direct detection51,52,53,54,55,56,57. In such a multifaceted, dynamic scenario, our complementary proposal aims to probe the uncovered few hundred μeV axion mass region by exploiting the axion-electron interaction predicted in the DFSZ models.

## Methods

The $$5\times 5\times 5$$ mm3 volume, Er3+:YLiF4 crystals used in this work were grown with the Czochralski method. The starting raw material were powders of LiF, YF3 and ErF3 with 5 N purity (99.999%), provided by AC Materials (Tampa, Fl., USA). They have 1% and 0.01% Er3+-dopant concentration (atomic percent substitution for Y3+). The growth was carried out in high purity (5 N) Argon controlled atmosphere. The pulling rate was 0.5 mm/h, the rotation rate 5 rpm and the temperature of the melt was computer-controlled around 880 °C to maintain a constant diameter of the boule; the seed was an undoped YLF monocrystal oriented along the c axis. The crystals resulted of good quality, free of internal cracks, microbubbles or inclusions. The structural analysis by Laue X-ray diffraction checked the mono-crystalline feature, and allowed the orientation of the boules along crystallographic axes.

To allow for Zeeman studies at LHe and superfluid He temperatures, the samples were housed in an immersion dewar located between two NdFeB magnetic discs that produced a field of 370 mT at the sample position. The c-axis of the crystal was parallel to the magnetic field direction. As shown in Fig. 1(b), the sample fluorescence is collected orthogonally to the laser pump propagation direction and coupled to the photon detector by means of a mirror M and a quartz guide. With optical filters we suppress scattered pump radiation at signal wavelengths, and at the InGaAs photodiode we detect the 1.5 μm component of the overall infrared fluorescence spectrum (see Fig. 1(c)). The employed optical source is a cw Ti:sapphire laser, which can be finely tuned by rotating intracavity ethalons. Zeeman studies are conducted around 809 nm wavelength, while laser-induced backgrounds are investigated at 810.1 nm. The laser linewidth is $$\leqslant 2$$ GHz (1–2 pm), comparable with the detected transitions widths. The incident light polarization angle is varied by means of a half-wave plate. A typical value of laser intensity used in our measurements is 10 W/cm2, compatible with 0.1 upconversion efficiency in trivalent ions37. For the laser noise studies the pump laser was chopped at 15 Hz to allow phase-sensitive detection.

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## References

1. 1.

Aprile, E. et al. First dark matter search results from the XENON1T experiment. Phys. Rev. Lett. 119, 181301-1–181301-6 (2017).

2. 2.

Akerib, D. S. et al. Results from a search for dark matter in the complete LUX exposure. Phys. Rev. Lett. 118, 021303-1–021303-8 (2017).

3. 3.

Agnese, R. et al. Projected sensitivity of the SuperCDMS SNOLAB experiment. Phys. Rev. D 95, 082002-1–082002-17 (2017).

4. 4.

Essig, R., Mardon, J. & Volansky, T. Direct detection of sub-GeV dark matter. Phys. Rev. D 85, 076007-1–076007-9 (2012).

5. 5.

Kouvaris, C. & Pradler, J. Probing Sub-GeV dark matter with conventional detectors. Phys. Rev. Lett. 118, 031803-1–031803-5 (2017).

6. 6.

Wilczek, F. Problem of strong P and T invariance in the presence of instantons. Phys. Rev. Lett. 40, 279–282 (1978).

7. 7.

Weinberg, S. A new light boson? Phys. Rev. Lett. 40, 223–226 (1978).

8. 8.

Peccei, R. D. & Quinn, H. R. CP conservation in the presence of pseudoparticles. Phys. Rev. Lett. 38, 1440–1443 (1977).

9. 9.

Kim, J. E. Weak-interaction singlet and strong CP invariance. Phys. Rev. Lett. 43, 103–107 (1979).

10. 10.

Shifman, M., Vainshtein, A. & Zakharov, V. Can confinement ensure natural CP invariance of strong interactions? Nucl. Phys. B 166, 493–506 (1980).

11. 11.

Zhitnitsky, A. On possible suppression of the axion hadron interactions. Sov. J. Nucl. Phys. 31, 260–268 (1980).

12. 12.

Dine, M., Fischler, W. & Srednicki, M. A simple solution to the strong CP problem with a harmless axion. Phys. Lett. B 104, 199–202 (1981).

13. 13.

Dine, M. & Fischler, W. The not-so-harmless axion. Phys. Lett. B 120, 137–141 (1983).

14. 14.

Sikivie, P. Experimental tests of the “invisible” axion. Phys. Rev. Lett. 51, 1415–1417 (1983).

15. 15.

Raffelt, G. Astrophysical axion bounds. In M. Kuster, B. Beltrán, G. Raffelt (eds.) Axions, vol. 741 of Lecture Notes in Physics, 51 (Springer Verlag, 2008).

16. 16.

Borsanyi, S. et al. Calculation of the axion mass based on high-temperature lattice quantum chromodynamics. Nature 539, 69–71 (2016).

17. 17.

Marsh, D. J. E. Axion cosmology. Phys. Rep. 643, 1–79 (2016).

18. 18.

Asztalos, S. J. et al. SQUID-Based Microwave Cavity Search for Dark-Matter Axions. Phys. Rev. Lett. 104, 041301-1–041301-4 (2010).

19. 19.

Sloan, J. V. et al. Limits on axion-photon coupling or on local axion density: Dependence on models of the MilkyWay’s dark halo. Phys. Dark Universe 14, 95–102 (2016).

20. 20.

Brubaker, B. M. et al. First results from a microwave cavity axion search at 24 μeV. Phys. Rev. Lett. 118, 061302-1–061302-5 (2017).

21. 21.

Barbieri, R. et al. Searching for galactic axions through magnetized media: The QUAX proposal. Phys. Dark Universe 15, 135–141 (2017).

22. 22.

Wallraff, A. et al. Strong coupling of a single photon to a superconducting qubit using circuit quantum electrodynamics. Nature 431, 162–167 (2004).

23. 23.

Tabuchi, Y. et al. Coherent coupling between a ferromagnetic magnon and a superconducting qubit. Science 349, 405–408 (2015).

24. 24.

Liu, G. Electronic energy level structure. In Guokui, L. & Bernard, J. (eds) Spectroscopic Properties of Rare Earths in Optical Materials, vol. 83 of Springer Series in Material Science, 1–94 (Springer, 2005).

25. 25.

Marino, R. et al. Energy level structure and optical dephasing under magnetic field in Er+: LiYF4 at 1.5 μm. J. Lumin. 169, Part B, 478–482 (2016).

26. 26.

Krauss, L., Moody, J., Wilczek, F. & Morris, D. E. Calculations for cosmic axion detection. Phys. Rev. Lett. 55, 1797–1800 (1985).

27. 27.

Barbieri, R., Cerdonio, M., Fiorentini, G. & Vitale, S. Axion to magnon conversion. A scheme for the detection of galactic axions. Phys. Lett. B 226, 357–360 (1989).

28. 28.

Hadfield, R. H. Single-photon detectors for optical quantum information applications. Nat. Photon. 3, 696–705 (2009).

29. 29.

Schuck, C., Pernice, W. H. P. & Tang, H. X. Waveguide integrated low noise NbTiN nanowire single-photon detectors with milli-Hz dark count rate. Sci. Rep. 3, 1893-1–1893-6 EP (2013).

30. 30.

Dreyling-Eschweiler, J. et al. Characterization, 1064 nm photon signals and background events of a tungsten TES detector for the ALPS experiment. J. Mod. Opt. 62, 1132–1140 (2015).

31. 31.

Sikivie, P. Axion dark matter detection using atomic transitions. Phys. Rev. Lett. 113, 201301-1–201301-5 (2014).

32. 32.

Turner, M. S. Periodic signatures for the detection of cosmic axions. Phys. Rev. D 42, 3572–3575 (1990).

33. 33.

Macfarlane, R. M. & Shelby, R. M. Coherent transient and holeburning spectroscopy of rare earth ions in solids. In A.A.Kaplyanskii & Macfarlane, R. M. (eds.) Spectroscopy of Solids Containing Rare Earth Ions, 51–184 (North-Holland, Amsterdam, 1987).

34. 34.

Thiel, C. W., Böttger, T. & Cone, R. L. Rare-earth-doped materials for applications in quantum information storage and signal processing. J. Lumin. 131, 353–361 (2011).

35. 35.

Lutz, T. et al. Modification of phonon processes in nanostructured rare-earth-ion-doped crystals. Phys. Rev. A 94, 013801-1–013801-5 (2016).

36. 36.

Cruzeiro, E. Z. et al. Spectral hole lifetimes and spin population relaxation dynamics in neodymium-doped yttrium orthosilicate. Phys. Rev. B 95, 205119-1–205119-11 (2017).

37. 37.

Krupke, W. Performance of laser-pumped quantum counters. IEEE J. Quant. Electron. 1, 20–28 (1965).

38. 38.

Lamoreaux, S. K., van Bibber, K. A., Lehnert, K. W. & Carosi, G. Analysis of single-photon and linear amplifier detectors for microwave cavity dark matter axion searches. Phys. Rev. D 88, 035020-1–035020-6 (2013).

39. 39.

Böttger, T., Sun, Y., Thiel, C. W. & Cone, R. L. Spectroscopy and dynamics of Er3+:Y2SiO5 at 1.5 μm. Phys. Rev. B 74, 075107-1–075107-8 (2006).

40. 40.

Wannemacher, R. et al. Zeeman-switched optical-free-induction decay and dephasing in YLiF4:Er3+. Phys. Rev. B 40, 4237–4242 (1989).

41. 41.

Santamaria, L. et al. Axion dark matter detection by laser spectroscopy of ultracold molecular oxygen: a proposal. New J. Phys. 17, 113025-1–113025-7 (2015).

42. 42.

Couto dos Santos, M. A. et al. Absorption and fluorescence of Er3+-doped LiYF4: measurements and simulation. J. Alloys Comp. 275–277, 435–441 (1998).

43. 43.

Kulpa, S. M. Optical and magnetic properties of Er3+ in LiYF4. J. Phys. Chem. Solids 36, 1317–1321 (1975).

44. 44.

Auzel, F. Upconversion and anti-Stokes processes with f and d ions in solids. Chem. Rev. 104, 139–174 (2004).

45. 45.

Auzel, F. Multiphonon-assisted anti-Stokes and Stokes fluorescence of triply ionized rare-earth ions. Phys. Rev. B 13, 2809–2817 (1976).

46. 46.

Walsh, B. M., Lee, H. R. & Barnes, N. P. Mid infrared lasers for remote sensing applications. J. Lumin. 169, Part B, 400–405 (2016).

47. 47.

Chen, Y. & Auzel, F. Investigation of multiphonon assisted side band absorptions in rare-earth-doped halide glasses and crystals. J. non-cryst. Solids 184, 278–281 (1995).

48. 48.

Seletskiy, D. V. et al. Laser cooling of solids to cryogenic temperatures. Nat. Photon. 4, 161–164 (2010).

49. 49.

Melgaard, S., Seletskiy, D., Polyak, V., Asmerom, Y. & Sheik-Bahae, M. Identification of parasitic losses in Yb:YLF and prospects for optical refrigeration down to 80K. Opt. Express 22, 7756–7764 (2014).

50. 50.

Di Lieto, A. et al. Influence of other rare earth ions on the optical refrigeration efficiency in Yb:YLF crystals. Opt. Express 22, 28572–28583 (2014).

51. 51.

Budker, D., Graham, P. W., Ledbetter, M., Rajendran, S. & Sushkov, A. O. Proposal for a Cosmic Axion Spin Precession Experiment (CASPEr). Phys. Rev. X 4, 021030-1–021030-10 (2014).

52. 52.

Arvanitaki, A. & Geraci, A. A. Resonantly detecting axion-mediated forces with Nuclear Magnetic Resonance. Phys. Rev. Lett. 113, 161801-1–161801-5 (2014).

53. 53.

Rybka, G. et al. Search for dark matter axions with the Orpheus experiment. Phys. Rev. D 91, 011701-1–011701-5 (2015).

54. 54.

Kahn, Y., Safdi, B. R. & Thaler, J. Broadband and resonant approaches to axion dark matter detection. Phys. Rev. Lett. 117, 141801-1–141801-6 (2016).

55. 55.

Silva-Feaver, M. et al. Design overview of DM radio pathfinder experiment. IEEE Trans. Appl. Supercond. 27, 1–4 (2017).

56. 56.

Group, M. W. et al. Dielectric haloscopes: A new way to detect axion dark matter. Phys. Rev. Lett. 118, 091801-1–091801-6 (2017).

57. 57.

Crescini, N. et al. The QUAX-g p g s experiment to search for monopole-dipole axion interaction experiment to search for monopole-dipole axion interaction. Nucl. Instr. Meth. A 842, 109–113 (2017).

58. 58.

Tkachuk, A. M., Razumova, I. K., Mirzaeva, A. A., Malyshev, A. V. & Gapontsev, V. P. Up-conversion and population of excited erbium levels in LiY1−x ErxF4 (x = 0:003−1) crystals under CW InGaAs laser-diode pumping. Optics and Spectroscopy 92, 67–82 (2002).

## Author information

### Affiliations

1. #### Dip. di Fisica e Astronomia and INFN, Sez di Padova, Via F. Marzolo 8, I-35131, Padova, Italy

• Caterina Braggio
• , Giovanni Carugno
• , Federico Chiossi
•  & Marco Guarise
2. #### Dip. di Fisica and INFN, Largo Bruno Pontecorvo, 3, I-56127, Pisa, Italy

• Alberto Di Lieto
•  & Mauro Tonelli

4. #### INFN, Istituto Nazionale di Fisica Nucleare, Sez. di Napoli, Complesso Universitario di M.S. Angelo, Via Cintia, Napoli, Italy

•  & Jordanka Tasseva
5. #### INFN, Laboratori Nazionali di Legnaro, Viale dell’Università 2, I-35020, Legnaro, Italy

• Antonello Ortolan
•  & Giuseppe Ruoso
6. #### Agenzia Spaziale Italiana (ASI), Contrada Terlecchia, I-75100, Matera, Italy

• Luigi Santamaria

### Contributions

M.G., P.M., L.S. and J.T. made Zeeman splitting measurements in Figure 2. C.B., F.C. assessed thermal population of levels as reported in Figs 3 and 4 and investigated multiphonon-assisted processes (Figure 5). C.B. wrote the manuscript. G.C., A.O. and G.R. helped in revising the manuscript and contributed during the experiments. A.D. and M.T. prepared and characterized the samples. All authors commented on the manuscript.

### Competing Interests

The authors declare that they have no competing interests.

### Corresponding author

Correspondence to Caterina Braggio.