Introduction

Photon and neutron inelastic scattering probes are indispensable for studies of fast dynamics in condensed matter on atomic to microscopic scales. Despite numerous advances, critical gaps exist in current experimental capabilities. Figure 1 shows that no established probe is able to access collective excitation on the nano- to mesoscale. Entering this uncharted region of dynamics is critical for understanding the nature of glass and the liquid-glass transition, which have an impact on many other fields, including biology, yet remain great unsolved mysteries1,2,3,4,5,6,7.

Figure 1: Accessibility of time-length space by different techniques.
figure 1

Time–length and relevant energy–momentum (εQ) space of excitations in condensed matter. Coloured regions show how it is accessed by different inelastic scattering probes: inelastic neutron scattering (INS), inelastic x-ray scattering (IXS), inelastic UV scattering (IUVS) and Brillouin scattering (BLS). The UHRIX spectrometer presented in the paper enters the previously inaccessible region marked in dark green. The energy ε=EfEi and the momentum Q=kfki transfers from initial to final photon/neutron states are measured in inelastic scattering experiments, as shown schematically in the oval inset.

For a long time, since the pioneering experiment of Brockhause and Stewart8 in 1958, only inelastic neutron scattering could measure nanoscale collective dynamics in condensed matter. Inelastic neutron scattering permits extremely small energy transfer resolution but rarely permits access to good momentum transfers, and hence it cannot be used to study disordered systems, whose sound velocities are typically 500–7,000 m s−1.

The advent of intense synchrotron radiation sources in the 1980s culminated in the first observation of inelastic X-ray scattering (IXS) from phonons9. With the third-generation radiation sources of the 1990s, IXS spectrometers were pushed to 1.5 meV spectral resolution and 1.5 nm−1 momentum resolution10,11, resulted in the first breakthroughs10,12 and further systematic studies13,14,15,16,17 of excitations in disordered systems and have since spread worldwide11,18,19,20. However, for almost 20 years these resolutions have not improved. The long Lorentzian tails of the spectral resolution function and the low-scattering cross-section severely compromise the ability of the existing spectrometers to detect important low-energy excitations.

Here we report the first implementation of a conceptually new IXS spectrometer, based on new principles of X-ray monochromatization and spectral analysis. We prove the efficacy of combining novel optical components to create an ultra-high-resolution IXS (UHRIX) spectrometer with unmatched performance in terms of energy and momentum resolution, and spectral contrast. The UHRIX spectrometer opens up uncharted space on the dynamics landscape, shown in dark green in Fig. 1. This is precisely the space of vital importance for the science of disordered systems. UHRIX is perfectly optimized for the latest generation of the synchrotron radiation sources and X-ray free electron laser facilities. We have verified the new spectrometer concept by carrying measurements on liquid glycerol at previously inaccessible regions of energy and momentum transfer.

Results

Spectrometer optical principles

UHRIX spectrometer is the first implementation of an optical concept, based on new principles of X-ray monochromatization and spectral analysis21. It combines flat crystal angular dispersive X-ray optics with collimating and focusing curved mirrors.

The key principle behind UHRIX is to adopt a highly asymmetric Bragg reflection close to backscattering, as an atomic-scale diffraction grating. A relatively large bandwidth is diffracted, but with a large angular dispersion perpendicular to the crystal surface, similar to that in a conventional grating, which diffracts light of different colours into different directions. The strongly divergent ‘rainbow’ of waves from this dispersing element (D) are then intercepted by a Bragg reflection that acts as a wavelength selector (W) by passing only those that emerge within a very narrow angular window—Fig. 2a. The third essential component in this scheme is a collimator (C)—another highly asymmetric Bragg reflection—placed before the dispersing element to ensure that waves incident on the D crystal are close to parallel. The initial collimation-dispersion-{wavelength-selection} (CDW) scheme can be modified to a collimation-dispersion-dispersion-{wavelength-selection} (CDDW) scheme—Fig. 2b—featuring enhanced angular dispersion due to two dispersing elements D1, D2 and in-line scattering geometry. With D-crystals set into extreme backscattering Bragg diffraction, the CDDW transforms into collimation-dispersion-{anomalous-transmission-filter}-dispersion-{wavelength-selection} (CDFDW) scheme with crystals C and W combined into a single collimation-{anomalous-transmission-filter}-{wavelength-selection} (CFW) crystal playing simultaneously the roles of the collimator (C), the anomalous transmission filter sharpening the tails of the spectral function (F) and wavelength selector (W), in three successive asymmetric Bragg reflections22,23.

Figure 2: CDW optics: principles and modifications.
figure 2

(a) Schematic of the CDW optics, comprising three asymmetrically cut crystals functioning as a collimator—C, a dispersing element—D and a wavelength selector—W, respectively. (b) CDDW optics is a modification of the CDW scheme augmented with two dispersing elements D1 and D2, ensuring enhanced dispersion rate and in-line scattering geometry. (c) CDFDW optics is another modification of the CDW scheme. Crystals C and W are combined into a single CFW crystal executing three key functions: the collimator—C, an anomalous transmission filter—F and a wavelength selector—W, in successive reflections.

The CDW optics and their modifications provide a very narrow spectral resolution function with steep tails, in combination with unusually large angular acceptance. It performs best at photon energies of 5–10 keV, where undulator flux and momentum resolution are very high. The large angular acceptance, ~\n100 μrad, makes possible to combine the CDW optics with large-angular acceptance collimating optics into a large-angular acceptance analyser system.

The complete UHRIX spectrometer (Fig. 3) comprises a CDDW-type monochromator and a CDFDW-type analyser, based on the CDW operating principle. However, the analyser is more challenging as the ‘source’ is a diverging beam from the sample, rather than a parallel beam from a synchrotron. The analyser therefore requires the combination of a CDW system and the very large-acceptance angle collimating optics.

Figure 3: UHRIX layout.
figure 3

Layout of the UHRIX instrument in the vertical (y,z) scattering plane showing all optical elements and all 15 deflections of the X-ray beam. Rotation of the analyser system in the horizontal plane (x,z) by an angle ϕy about the vertical y axis passing through the sample provides access to photons scattered with a momentum transfer Q=2k sin(ϕy/2). See Methods for more details.

Early experiments had demonstrated the existence of angular dispersion in asymmetric Bragg diffraction24. Various components of the UHRIX spectrometer have been tested separately during the last few years in a series of experiments. The initial CDW design had been tested24,25,26,27 and improved by implementing doubly-dispersive CDFDW22,28,29 and CDDW optics23. A Montel-type two-dimensional (2D) mirror system was designed and tested to work as the large-acceptance angle collimating optics30.

Although various components of the spectrometer have been developed, refined and tested, they have never before been combined in a fully functional spectrometer. The challenge and the final proof of the concept is not just in a proper functioning of each individually intricate element, but in a precise coupling of all optic elements. The flat-crystal CDDW monochromator and curved focusing mirror (Fig. 3) have to be properly designed and coupled to produce not only high spectral flux but also about 10-μm small vertical focal spot size on the sample despite the strong angular dispersion in the CDDW monochromator29. The small size of the secondary source is essential for the collimating mirror to collect photons in the large solid angle Δϕx × Δϕy10 × 10 mrad2 and to produce sufficiently parallel 100 μrad beam for proper coupling with the CDFDW analyser (Fig. 3). Only flawless coupling of all elements may result in the highest resolution and efficiency of the spectrometer.

Spectrometer momentum transfer and spectral resolution functions

The experiments were performed at the undulator beamline 30ID at the Advanced Photon Source. The UHRIX instrument is shown schematically in Fig. 3 and presented in detail in Methods. Once the CDDW monochromator and the Kirkpatrick-Baez (KB) focusing mirrors had brought a large flux 2.4 × 109 ph s−1 of ultra-monochromatic ΔEi=0.25 meV X-rays to a 18(V) × 45(H)-μm2 spot on the sample, it remained to test the new analyser system. Measurements of the momentum and spectral resolution functions, and of IXS spectra, are the ultimate proof of the new concept.

UHRIX momentum transfer resolution measurements are presented in Fig. 4a. The spectrometer was tested in two modes, first by accepting the entire beam onto the analyser, which produced the energy resolution shown in Fig. 4b, and momentum resolution ΔQ=0.49 nm−1. A 1-mm horizontal slit was then placed before the analyser to reduce the momentum resolution to ΔQ=0.25 nm−1 and produce the IXS spectra shown in Fig. 5.

Figure 4: UHRIX resolution functions.
figure 4

(a) Momentum transfer resolution ΔQ of the UHRIX instrument measured by the analyser system rotated about y axis with angle ϕy. Open circles: ΔQ=0.49 nm−1, corresponding to the collimating mirror and CDFDW optics being fully open. Solid circles: ΔQ=0.25 nm−1, with a horizontal aperture installed after the collimating Montel optics, to reduce the solid angle of the analyser system acceptance. (b) UHRIX spectral resolution functions measured by scanning the CDDW monochromator energy. Light purple solid circles: the analyser system is at ϕy=0 intercepting the direct focused monochromatic X-ray beam. Dark purple open circles: the analyser system is at ϕy=21.6 mrad (Q=1 nm−1) intercepting X-rays scattered from a strong elastic scatterer, glassy carbon. The black solid line is the convolution of the theoretical spectral functions of the CDDW and CDFDW optics calculated using multi-crystal dynamical theory of X-ray diffraction. Other functions with the same FWHM are shown for comparison: dashed green line—Gaussian; blue dash-dotted line—Lorentzian.

Figure 5: Glycerol IXS spectra, sound velocity and attenuation.
figure 5

IXS spectra of glycerol liquid at 298 K measured at different momentum transfer Q=0.5 nm−1 (a), Q=1 nm−1 (b) and Q=1.4 nm−1 (c), respectively. Dashed dark-blue lines are UHRIX resolution functions. Solid green lines are damped harmonic oscillator (DHO) functions convoluted with the resolution function. Solid red lines are a sum of the two, fitted to the experimental spectra. The dashed light-blue line in c is an IXS spectrum of glycerol measured with a conventional IXS spectrometer at Q=1.5 nm−1 (ref. 31). The apparent sound velocity (d) and the reduced broadening ГQ/Q2 (e) of the acoustic-like modes, obtained from the least-squares fit of the experimental data to the DHO model, are shown with black circles and ±1σ error bars.

UHRIX spectral resolution functions are shown in Fig. 4b, in which only the CDDW monochromator energy is scanned. We show that the spectral line shape measured from the direct beam, and that from the beam diverging from a glassy carbon amorphous sample, are identical. Both results show a 620-μeV spectral bandwidth that was never before achieved with an IXS spectrometer and is in good agreement with the predictions of dynamical diffraction theory. In addition to the factor of three improvements in bandwidth, the UHRIX resolution function exhibits vastly improved contrast. It has an almost Gaussian shape over two orders of magnitude in intensity and is an order of magnitude steeper than the Lorentzian shape that is typical for existing IXS spectrometers. The improved momentum resolution, better spectral resolution and higher contrast are game changers for IXS spectroscopy.

Spectrometer applied to studies of dynamics in glycerol

We have applied our new spectrometer to a study of glycerol, a prototypical glass-forming liquid. Figure 5 shows IXS spectra measured with momentum transfers of Q=1.4, 1.0 and 0.5 nm−1. All the spectra clearly reveal Stokes and anti-Stokes inelastic lines, interpreted as longitudinal acoustic-like modes in glycerol, well resolved from the central elastic line, even at the lowest Q. For comparison, we show measurements in glycerol31 with a state-of-the-art conventional IXS spectrometer at Q=1.5 nm−1—the smallest accessible for such spectrometers. Unlike the UHRIX measurements, the inelastic features appear unresolved as shoulders on the elastic line tail. UHRIX can resolve phonon lines even at Q=0.5 nm−1, due to its high resolution and high contrast capabilities, where conventional spectrometers fail.

The IXS data are modelled by the normalized dynamical structure factor

the variable measured in IXS experiments13, presented here as a sum of the delta function for the elastic component and the damped harmonic oscillator for the inelastic component32. Convolution of S(Q,E)/S(Q) with the instrumental function is used to compare with the experimental results and derive the model parameters fQ, ГQ and ΩQ. See Fig. 5, which also shows the apparent sound velocity and the reduced broadening ГQ/Q2 of the acoustic-like modes in glycerol, obtained from the least-squares fit of the experimental data.

Speed of sound vs in Fig. 5d is flat at Q=1 and 1.4 nm−1, and is smaller than the values measured at larger Q in earlier IXS studies in glycerol liquid12, shown by open circles. At the smallest measured Q=0.5 nm−1, it increases to the level determined by low-frequency techniques33,34, as shown with triangles. At this point the reduced width ГQ/Q2 in Fig. 5e drops down from the constant level measured at larger Q in the present and earlier IXS studies. This indicates a breakdown of the ГQQ2 dependence typical for liquid and glass dynamics in the THZ frequency range discovered in early IXS studies12. The low-frequency measurements in glycerol liquid revealed a linear dependence in Q and much smaller attenuation34. Therefore, breakdown of the Q2 dependence in the intermediate frequency and Q range is a plausible scenario. Breakdown of the Q2 and cross-over to a faster Q4 dependence have been reported in glasses35, and in particular very clearly in glycerol glass at T=150 K16. Our observation of the simultaneous increase of νs and breakdown of Q2 dependence is very similar to the observations reported for glycerol glass16. The results of the present studies in liquid glycerol indicate that such behaviour cannot be taken as a unique identifier of a glass. Our results indicate that similar behaviour occurs in glass-forming liquids at longer time–length scales, compared with those typical for glasses, precisely in the regime that has become accessible with the novel IXS spectrometer demonstrated in this paper.

Discussion

A conceptually new IXS spectrometer was demonstrated, which opens up hitherto inaccessible region of the time- and length-scale landscape of collective excitations in condensed matter. Novel X-ray crystal optics combined with special collimating optics result in unmatched performance. The spectrometer features a spectral resolution function with Gaussian-like steep tails over two orders of magnitude in intensity and sub-meV (620 μeV) bandwidth. The new capabilities are demonstrated by studies of dynamics in glass-forming glycerol liquid, with a momentum transfer resolution of 0.25 nm−1. The moderate working photon energy of 9.1 keV makes this spectrometer practical for most X-ray synchrotron and X-ray free-electron laser (XFEL) facilities.

The optical principles demonstrated here can be further developed towards achieving an even greater spectroscopic performance. Complemented with additional focusing optics and a position sensitive detector, the analyser system can be transformed into a spectrograph imaging single-shot spectra with sub-0.1-meV resolution, as has recently been demonstrated in a proof-of-principle experiment28. A 2D detector would allow single-shot imaging of IXS spectra at different Q-values with sub-0.1-nm−1 resolution. The X-ray spectrometer concept demonstrated here, which combines flat crystal angular dispersive optics with focusing and collimating optics is a new and exciting paradigm, which is highly attractive for a wide range of applications in non-resonant and resonant IXS.

Spectrometer details

The experiments were performed at the undulator beamline 30ID at the Advanced Photon Source36. The layout of the UHRIX instrument is shown schematically in Fig. 3. The undulator X-ray source and the water-cooled double-crystal diamond pre-monochromator were tuned to a nominal X-ray photon energy Ei=9.1315, keV of the UHRIX instrument. Final monochromatization of X-rays incident on the sample was achieved with a hybrid diamond-silicon CDDW monochromator23, a modification of the CDFDW analyser22. An asymmetrically cut 200-μm-thick silicon (220) crystal plate used as the CFW element in the CDFDW optics was replaced with a 100-μm-thick asymmetrically cut diamond (133) plate. Unlike silicon, the thin diamond plate is practically transparent for the 9-keV photons and therefore functions as a CW element in the CDDW optics. The substitution with the diamond CW element resulted in a very small energy bandwidth ΔEi=0.25 meV, a threefold increase in the aperture of the accepted beam, a reduction in the cumulative angular dispersion rate of X-rays emanating from the monochromator for better focusing on a sample, a sufficient angular acceptance matching the angular divergence of an undulator source (10 μrad) and a very high spectral efficiency of 65% due to low X-ray absorption in the thin diamond crystal. The CDDW monochromator energy Ei can be scanned by simultaneous rotation of the two D-crystals, as indicated by rotation angles and in Fig. 3. A downstream KB mirror system focused X-rays on the sample to a spot. A flux of 2.4 × 109 photons/s was delivered to the sample.

Analyser system

The most critical but unexplored component before our experiment was the analyser system comprising a collimating optics and the CDFDW crystal analyser22. A Montel-type 2D mirror system was used as the collimating optics30. As predicted, the Montel optics collected X-rays in a solid angle Δϕx × Δϕy10 × 10 mrad2 and collimated them to a beam with a much smaller divergence Δψx × Δψy90(V) × 230(H) μrad2. The vertical angular spread Δψx was well matched to the 105 μrad angular acceptance of the CDFDW analyser22 and ensured its high efficiency. Keeping the horizontal angular spread Δψy small was also important, to avoid broadening of the CDFDW spectral bandwidth. For the backscattering CDW-type optics, the broadening was estimated as (ref. 21), that is, ΔE0.24 meV in our case, which was within acceptable limits. The measured values of the angular spread Δψy × Δψx correspond to the angular size (Δys/fM) × (Δxs/fM) of the secondary source (sample) seen from the centre of the Montel optics at a focal distance of fM=0.2 m, emphasizing the importance of the small secondary source size for proper functioning of the analyser system.

Collimating optics

The collimating Montel optics, manufactured by Incoatec GmbH, consisted of two parabolically shaped, 120-mm-long surfaces coated with laterally graded 100 W–C bilayers (Göbel mirrors), arranged perpendicularly and side-by-side30. An almost 50% reflectivity of the Montel optics (70% from each surface) was measured with the analyser system set at ϕy=0 looking into the direct focused beam. The angular spread of X-rays from the Montel optics was measured with a Si(220) channel-cut crystal installed downstream temporarily for this measurements. In this case, X-rays were scattered from a 1-mm-thick amorphous carbon plate sample, and the analyser system set to ϕy22 mrad (Q=1 nm−1).

Momentum transfer resolution

Momentum transfer resolution of the instrument was limited by two factors: the angular spread of the incident beam and the angular acceptance of the analyser system. The incident beam divergence due to focusing onto the sample is 0.4(V) × 0.8(H) mrad2 and therefore can add only a small broadening of 0.016(V) × 0.037(H) nm−2 to the momentum transfer resolution. Although the vertical and horizontal angular acceptance of the Montel optics were the same, that of the analyser system in the vertical plane was presently limited to Δϕx=0.75 mrad by the 90-mm-length of the D-crystals in the CDFDW optics used in this experiments. The angular acceptance of the analyser system in the horizontal plane made the main contribution to the momentum transfer resolution function.

With no sample installed, the focused beam propagating in the forward direction was used to align the collimating Montel and the downstream CDFDW optics, and to measure the UHRIX resolution functions. Rotation of the analyser system in the horizontal plane by an angle ϕy about the vertical axis passing through the sample provided access to photons scattered with a momentum transfer Q=2ki sin(ϕy/2).

Sample

The liquid glycerol sample (T=298 K) was contained between two 12-μm-thick Kapton windows with a separation of 1.5 mm, matched to the X-ray absorption length. To avoid possible radiation damage, the liquid was pumped through the container.

Additional information

How to cite this article: Shvyd’ko, Y. et al. High-contrast sub-millivolt inelastic X-ray scattering for nano- and mesoscale science. Nat. Commun. 5:4219 doi: 10.1038/ncomms5219 (2014).