High-resolution X-ray emission study for Xe54+\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$^{54+}$$\end{document} on Xe collisions

We report on an experiment conducted at the ESR storage ring aiming at the study of the X-ray emission of Xe54+\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\text {Xe}^{54+}$$\end{document} ions colliding with Xe atoms at a beam energy of 50 MeV/u. The radiation resulting from the ion–atom interaction was observed using a high-resolution spectrometer based on metallic–magnetic calorimeter technology. In order to benchmark the capabilities of these detectors for high-precision atomic physics experiments, we identified several transitions from H-like and He-like xenon and determined their energies. Furthermore, the 1s-Lamb shift in Xe53+\documentclass[12pt]{minimal} \usepackage{amsmath} \usepackage{wasysym} \usepackage{amsfonts} \usepackage{amssymb} \usepackage{amsbsy} \usepackage{mathrsfs} \usepackage{upgreek} \setlength{\oddsidemargin}{-69pt} \begin{document}$$\text {Xe}^{53+}$$\end{document} was estimated using the measured line energies. The results are compared with previous experimental studies and theoretical predictions.


Introduction
X-ray spectroscopy experiments involving highly charged heavy ions have become an indispensable tool for tests of quantum electrodynamic (QED) effects in strong fields [1]. In the past, measurements with H-like and He-like Xe ions have been performed by several groups at different experiment facilities (see, for example, [2][3][4]). In this work, we present the results of an experiment that was conducted at the ESR ion storage ring of GSI [5] utilizing a cryogenic calorimeter detector for high-precision X-ray spectroscopy. Metallicmagnetic calorimeters (MMC) like the maXs-series detectors developed in cooperation with the Kirchhoff-Institute for Physics (KIP) in Heidelberg [6][7][8] combine several advantages over conventional energy-dispersive X-ray photon detectors. They can reach resolving powers of E/ΔE > 6000 [9]-comparable to crystal spectrometers-over a broad spectral acceptance range-comparable to typical semiconductor detectors. Together with an excellent linearity [10] as well as signal rise times up to τ 0 ≈ 100 ns [11] they are particularly well suited for high-precision X-ray studies a e-mail: m.o.herdrich@hi-jena.gsi.de (corresponding author) in atomic and fundamental physics experiments dealing with heavy, highly charged ions. However, in order to achieve this extraordinary performance, a transition from conventional analog to fully digital data processing and analysis is required. Therefore, a software framework for analyzing MMC data has been developed during the course of several experiments conducted at the ion storage facilities of GSI/FAIR in the last years. In the following, the experiment and the MMC detector are briefly described in Sects. 2 and 2.1, respectively. The detailed analysis of the recorded data in Sect. 3 is followed by a short conclusion about the feasibility of using cryogenic microcalorimeter detectors in the context of precision spectroscopy related to fundamental tests of the standard model (see Sect. 4).

Experiment
The experiment is described in detail in [12,13]. It involved an electron-cooled 132 Xe 54+ ion beam at 50 MeV/u beam energy colliding with a Xe gas-jet at the internal target of the ESR ion storage ring. In order to record X-ray photons resulting from the ion-atom inter-action, a maXs-200 detector [7] was positioned in front of the 60 • port of the target chamber. The pixels of this 1 × 8 spectrometer array consist of a gold absorber and a Au:Er-based paramagnetic sensor in a gradiometric configuration with two pixels connected to a SQUIDbased readout and amplification stage. It was mounted with its pixels in vertical orientation (to reduce Doppler broadening) at the tip of the 60 cm long cold finger of a 3 He/ 4 He dilution cryostat in order to achieve the required operation temperature of < 30 mK. The nominal absorption efficiency at 100 keV is 45% with an active detection area of 1 mm 2 per pixel. From previous testing of an identical detector chip, an energy resolution of 62 eV full width at half maximum (FWHM) at 60 keV was reported. The distance between the detector and the interaction point amounted to 2 m resulting in a 2.5 × 10 −7 sr solid angle per pixel. A vacuum window made of diamond was installed on the target chamber, and the X-ray entry window in front of the MMC was made of aluminum-coated Mylar foils as well as a beryllium window for the separation of the surrounding vacuum from air. During the 48 h of almost continuous recording of X-ray radiation at the ESR, a 241 Am source was positioned in front of the detector (offset from the view port into the target chamber) for simultaneous calibration.
We note that an experiment with a similar setup was performed very recently [14]; however, only conventional photon detectors were used. Furthermore, a comparable experiment at even lower collision energies was conducted [15] utilizing a maXs-30 type detector. Though, too few events were detected by the microcalorimeter at that time to perform a proper analysis.

Detector performance
The absolute energy calibration of the detector was performed by fitting a gaussian distribution to the peaks of the well-known lines of the 241 Am calibration source for each pixel individually. The central positions of the peaks were then compared to the corresponding energies reported in the literature. A fit using a secondorder polynomial thereby takes into account the well understood nonlinearities of the detector. Additionally, unavoidable temperature fluctuations of the detector's substrate during the measurement lead to a spectral broadening due to a linear temperature dependance of the sensor's gain behavior. This effect could be mostly compensated by using the baseline level (before the trigger) of each recorded signal as its temperature information. Comparing the measured energies of events associated with the 59.5 keV calibration line to their corresponding sensor temperatures allowed for the calculation of a regression line which was then applied inversely to the rest of the events. An in-depth description of all utilized calibration and correction procedures can be found in [8].
The instrumental energy resolution determined from the line width of the observed calibration line at 26.3 keV is found to be 42.0 eV (FWHM). However, from the characterization of the baseline noise one finds an expected resolution of 38.2 eV [12]. This can be partially explained by a loss of resolution power due to a remaining fraction of uncorrected temperaturedependent gain drift and signal shape (see [16]) artifacts. The line width of the measured X-ray lines from the ion-atom interaction amounts to 77 eV at around 35 keV. This difference to the calibration lines can be partially attributed to the finite size of the gas-jet target resulting in Doppler broadening, but has not been fully understood, yet [8]. Systematic uncertainties from the Doppler broadening between pixels are approximated to be below 4 eV [8]. Additional uncertainties due to calibration errors are also small compared to the overall resolution (approximated mean deviation from literature values are in the order of 1 eV). Therefore, both effects are ignored in the following analysis. During the experiment only two of the eight pixels were connected, therefore limiting the total amount of events available for the analysis.

Experimental data and results
Because of the comparably slow collision of 50 MeV/u and the symmetrical and heavy systems chosen (Xe 54+ on Xe), one can assume an adiabatic exchange of one or more electrons between the fully ionized projectile ions and neutral target atoms [22]. The entire recorded spectrum can be seen in Fig. 1. The most prominent features stem from K-shell transitions (see also Fig. 2) within both collision partners, while L-shell transitions are not observable due to photon absorption in the diamond window and gap filled with air between target and detector. A first evaluation of the measured spectra can be found in [8,23].

Target radiation
At 30 keV, a group of transitions is visible that can be attributed to radiation emitted by the target atoms. It results from subsequent relaxation of excited states into electron vacancies produced by electron transfer from the target into the projectile ions. Observed are K-α transitions from different charge states of xenon with multiple satellite features caused by screening effects. A detailed analysis of this phenomenon is found in [14]. A comparison of energy limits for neutral down to H-like xenon ranges from Xe I K-α 2 : 29,458.3 eV [24] to Lyα 1 : 31,283.9 eV [17]. This matches the recorded spectral features and indicates that in such collisions potentially a multitude of electrons can be stripped from the target atoms. It contains X-ray events (from both pixels combined) from collisions between Xe 54+ at 50 MeV/u and a Xe gas-jet target (blue curve). In red, the fitted model function containing the annotated transitions is overlaid. A preliminary version of the spectrum can be found in [12]

Projectile radiation
Electrons transferred into excited states of the projectile ions through non-radiative electron capture (NRC) [25] also lead to the emission of characteristic X-ray radiation via subsequent cascades. As can be seen in Fig. 1, the projectile radiation is significantly more intense than the radiation from the target. This can be explained by the fact that the NRC process (involving electrons from all target shells) has a much larger cross section for this collision system than the target K-shell vacancy production including electron transfer and direct Coulomb ionization responsible for the target X-rays.

Doppler correction and comparison to theoretical predictions
Observed K-shell transitions are shifted to higher energies compared to the target radiation due to a Doppler shift at the used observation angle resulting from the relativistically moving projectiles: With a beam energy of E kin = 50.43 ± 0.09 MeV/u (calculated from the applied electron cooler voltage of 27.70 ± 0.05 kV at an electron beam current of 100 mA) and an observation angle of θ = 60 ± 1 • a Doppler shift of f = 1.1269 ± 0.0064 is expected. A model of superposed normal distributed peaks for all identified transition lines is fitted to the spectrum to extract the measured line positions. The most prominent K-α-and K-β-transition energies E * from hydrogen-like xenon (see Table 1 and Fig. 3) are then used to perform a linear fit against the binding energies E i -assumed to be known from our theoretical predictions [17]-of the participating excited states: This not only yields a more precise value for the actual Doppler shift but also allows to estimate the common ground state binding energy E f = 41,299.93 ± 2.78 eV (uncertainty taken from the fit). The resulting Doppler correction factor of f = 1.125534 ± 9.8 ×10 −5 is in good agreement with the expectation. Assuming that the beam energy is well known, this yields a corrected observation angle of 60.21 ± 0.03 • . At a distance of 2 m this gives rise to a difference of 7.39 ± 0.92 mm to the assumed ideal detector position at 60 • in regards to the interaction point (a reasonable finding consistent with previous experiments). Using the spectrum itself to perform a Doppler correction eliminates these kinds of systematic errors arising from difficult to control experimental uncertainties (like the exact detector and target positions). Having multiple line positions and spectral features within the same spectrum is an immediate advantage of using high-resolution, broad range MMC detectors compared to conventional detection methods.
Because of an unresolved superposition of the two transitions from the 2s1 /2 and 2p 1 /2 states of ≈ 7 eV, the Ly-α 2 lines were excluded from the fit. Besides K-shell transitions in hydrogen-like xenon, several lines stemming from helium-like xenon ions were 125 Page 4 of 9 Eur. Phys. J. D (2023) 77 :125 Fig. 2 Displayed are the level schemes for hydrogen (left) and helium-like xenon ions (right). The observed K-α (blue, dashdot) and K-β (red, long dash) transitions are highlighted. The respective binding energies were taken from our theoretical predictions [17] calculated using the MDFGME code (see [18] and refs. there in): It includes finite nuclear size effects (experimental charge radius from [19]), nuclear recoil contributions including relativistic corrections as well as first-and second-order QED corrections. For the two-electron calculations, more details can be found in [20,21]  The photon energies are given in relation to the moving emitter reference frame and include the statistical uncertainties resulting from fitting errors as well as systematic uncertainties from the Doppler correction. Additionally, the corresponding initial excited state binding energy and transition energy from our theoretical predictions [17] are given identified as well (see Table 2). This means, that in some collisions two electrons were transferred from the target atoms to the projectiles at once. A comparison between measured line positions with theoretical predictions shows an overall good agreement within the boundaries of statistical and systematic uncertainty. The 1s 2p 1 P 1 → 1s 2 1 S 0 line is overlapped by a second transition from the 1s 2p 3 P 2 state and could not be resolved.

K-α satellite peaks
There is no apparent reason to assume that the second electron always has to be captured into the ground state of the helium-like system. Thus, one expects to find Kshell transitions for two electron configurations with the second electron in a higher orbital as well. Both, the Ly-α 1 and Ly-α 2 lines seem to exhibit small satellites on their lower energy edges. The analysis of the Ly-α 1 satellite yields a plateau with a center distance of 123.0 eV in relation to the main peak and a line broadening  The energies are given with respect to the moving emitter's frame of reference and contain uncertainties both from fitting errors and from the used Doppler correction. Furthermore, the table includes the absolute difference between the measured energies and several theoretical predictions from Johnson [26], Drake [27] and Artemyev [28] to 100 eV. A calculation was performed using FAC [29] exploring all possible transition energies and branching ratios for Ly-α 1 -like transitions with an additional electron in the 2p-orbitals. The second charge in the L-shell partially shields the electric field of the nucleus acting upon the other electron, thus reducing its binding energy. As a result, since the K-shell binding energy is less effected by the L-electron's shielding effect, the overall K-α-transition energy of the system is reduced. In total, two groups of lines are found. Their position coincides with the observed satellites. The transition strength weighted average line energy for the Ly-α 1 satellite yields a distance of 109.4 eV to the main peak and a width of σ = 25 eV. Taking into account the measured X-ray's line width of 77 eV, the resulting total width of the plateau is expected to be 96.8 eV which fits the observed spectral feature's properties well. Therefore, we attribute these peaks to satellite features of the Ly-α lines. However, due to low statistics an exact determination is not possible. Although the simultaneous transfer of three or more electrons from the target to the projectile ions cannot be ruled out completely, no indication of the occurrence was observed.

Comparison to previous experiment findings
In the past, similar experiments were conducted by other groups measuring K-α-transition energies in different charge states of xenon. For example, a single-pass collision experiment using Xe ions as projectiles on a thin carbon foil was performed at the LISE beam line of GANIL, France [2]: The reported transition energies for K-α 1 (31,278 ±10 eV) and 1s 2p 3 P 1 → 1s 2 1 S 0 (30,209.6 ± 3.5 eV) agree with the results presented in this work. In both experiments, occasionally more than one electron was captured from the target, leading to an unavoidable mixture of transitions from different charge states of Xe ions in the final spectra. However, in comparison to the Ge-based semiconductor detector used at LISE, the higher resolving power of the MMC detector enabled the simultaneous observation of both H-like and He-like transitions as separate lines. This not only eliminates the need to disentangle potentially overlapping transitions during the analysis, but also allows for a more direct comparison of the energies and intensities of these lines.
Another high-resolution measurement of highly char ged Xe ions was performed using a different type of microcalorimeter (Si-thermistor based) detector at an 125 Page 6 of 9 Eur. Phys. J. D (2023) 77 :125 Fig. 4 The spectrum shows details of recorded Doppler-shifted lines stemming from K-shell transitions emitted from both hydrogen-and helium-like xenon projectile ions up the the series limit electron-beam ion-trap (EBIT) at the Lawrence Livermore National Laboratory, USA [4]: Again, the experimental findings for the K-α 1 (31,284.9 ± 1.8 eV) as well as the y-(1s 2p 3 P 1 → 1s 2 1 S 0 , 30,207.1 ± 1.4 eV) and z-(1s 2s 3 S 1 → 1s 2 1 S 0 , 30,128.6 ± 1.3 eV) lines of the helium-like system are in good agreement with results of our current work. Though, in principle MMCs are expected to have a higher intrinsic resolution power than semiconductor-based calorimeters [30], the absorber volume of the maXs-200 pixels was optimized for a higher energy range (up to 200 keV compared to 100 keV of the Si thermistor). Because of that, both, the MMC and the semiconductor-based EBIT calorimeter system (ECS) used at by Thorn et al. yield a comparable energy resolution of around 35-40 eV (FWHM) in the region of interest around 35 keV. However, despite the similar energy resolutions, a higher precision was achieved at the EBIT. This can be partially explained by the fact that during the ESR measurement fewer events were recorded overall. More importantly though, the line widths of transitions stemming from the fast moving projectile ions were broadened to 77 eV as briefly discussed in Sect. 2.1. This highlights the inherent property of the EBIT measurement of not requiring a Doppler correction or being effected by other relativistic effects compared to the ion-atom collision. However, performing the experiment at an ion storage ring might still be advantageous as a projectile beam of clean isotopes and a well defined charge state is available for the collision. Less overlapping transitions of different charge states are present in the resulting spectrum and even transitions from higher orbitals with quantum numbers n > 2 are observable up to the continuum edge as shown in Fig. 4.

1s-Lamb shift of hydrogen-like xenon
By definition, the 1s-Lamb shift of hydrogen-like xenon amounts to the difference between the real ground state binding energy and the value predicted by Dirac theory for the interaction of a single 1s-electron with a point like nucleus (−41,346.80 eV). The resulting value of 46.87 ± 2.78 eV is in excellent agreement with our theoretical prediction (47.094 eV, [17]) and calculations by V. A. Yerokhin (46.920 eV, [31]). Compared to previous experimental results (54 ± 10 eV [2]), a higher accuracy was achieved due to the better energy resolution of the MMC detector in comparison to the Ge detector (reported 270 eV FWHM in the region of interest [2]).

Conclusion and outlook
In the present study, the results achieved are strongly affected by the moderate counting statistics. A long distance between the detector and interaction point due to geometrical constraints of the setup and a small detector area because of missing pixels reduced the available solid angle of the observation. Additionally, many of the temperature correction procedures that were developed over the period of subsequent experiment campaigns were not yet available at the time of this experiment, thus further reducing the final energy resolution. Nevertheless, quite accurate results for the transition energies could be obtained. Overall, the findings are in a good agreement with both theoretical predictions as well as previous experimental findings. Taking into account that this was one of the first experiments utilizing a maXs-series detector for atomic physics measurements at an ion storage ring, it proves the feasibility of future beam times exploiting the excellent performance of these detectors. In particular, the recorded spectrum did contain almost no background events even without applying time coincidence filtering. Systematic uncertainties stemming from difficult to predict experiment setup parameters like the position of the gas-jet within the target chamber or even the slight shift of the detector position due to thermal contraction during the cool-down phase could be mostly eliminated by using multiple highly resolved lines within the same recorded spectrum.
Meanwhile, detectors of the maXs-series have been improved significantly. The newly designed maXs-30 [8] and -100 [9] detectors consist of 8 × 8 pixels with an increased active detection area and correct several issues that occurred over time. For example, temperature sensitive pixels have been added to allow for an intrinsic temperature correction of the obtained spectra. Accompanying the changes to the hardware, calibration and measurement procedures have been updated as well. Furthermore, the maXs-detector family will be integrated into the heterogeneous detector environment of the FAIR complex which is currently being built [32]. This allows for them to be used, e.g., with particle detectors to perform coincidence measurements and further improve their accuracy by suppressing background events. This could help with a better identification of small spectral features like the discussed satellite structures found near the Lyα lines. Such an application has been recently demonstrated in the first high-resolution measurement of Kα transitions in He-like uranium U 90+ at the electron cooler of the CRYRING@ESR low energy ion storage ring of FAIR [33]. Further experiments utilizing MMC detectors for high-precision atomic physics experiments involving highly charged ions in storage rings like CRYRING@ESR are already planned. ated within the SPARC collaboration and was supported in part by the ExtreMe Matter Institute EMMI at the GSI Helmholtzzentrum für Schwerionenforschung, Darmstadt. Funding Open Access funding enabled and organized by Projekt DEAL. We acknowledge financial support by the European Union and the federal state of Thuringia via Thüringer Aufbaubank within the ESF Project (2018 FGR 0080). The work was supported by the BMBF Grant 05P12VHFA5.

Data Availability Statement
This manuscript has no associated data or the data will not be deposited. The data that support the findings of this study are available upon reasonable request from the authors.

Conflict of interest
The authors declare no conflict of interest. The funders had no role in the design of the study; in the collection, analyses, or interpretation of data; in the writing of the manuscript; or in the decision to publish the results.
Ethics approval Not applicable.

Consent for publication Not applicable.
Code availability Not applicable.
Open Access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecomm ons.org/licenses/by/4.0/.