Valorisation …………………………………………………………………………………………………….………96 1.3.2 XRF X-ray fluorescence (XRF) spectrometry is used to determine the elemental composition of a sample [10]. One variant of this technique, known as total reflection X-ray fluorescence (TXRF) [11], can be used to detect nanoparticles deposited on a flat surface, for example, or to trace the positions of heavy ions in organic monolayers or thick Langmuir-Blodgett films [12-16]. The multilayer coatings used in monochromators are essential in the analysis of low intensity emittance, in the case of light elements such as Li, Be, B, C, N [10]. The latter elements have a relatively low fluorescence yield. This factor, coupled with strong absorption in the sample itself, greatly reduces the intensity of the measured signal. Accordingly, the detection of light elements with XRF is difficult without multilayer coatings. Compared to single layers, the multilayers used in energy-dispersive techniques have a higher integrated reflectivity (over the Bragg peak), which makes it possible to detect light elements. These materials make the fine-tuning of reflectivity, of the position, of the reflectionpeak wavelength and of the angle of incidence a matter of routine. For the purpose of detecting B (K emission line) at angles of incidence close to 45°, for example, La/B4C and Mo/B4C multilayers were used [17]. One XRF-based application (grazing-incidence X-ray reflectivity) involves the angular-dependent measurement of samples to give depth-profiles of selected elements and details of the density of individual layers [18]. With this technique, unlike secondary ion mass spectrometry (SIMS), XPS depthprofiling, Rutherford backscattering spectroscopy (RBS) and other methods that involve sample sputtering, the sample is not damaged by incident X-rays. It also means that the XRF yield (including angular-dependent information) can be measured inhouse (using a standard lab reflectometer with an X-ray tube), thus avoiding the need for restricted and expensive access to equipment at ion centres, synchrotrons, etc. The 1.4 Multilayers for wavelengths above 6.6 nm 1.4.1 The properties and interactions of materials Based on their optical properties (high contrast and low absorption of 6 nm light), La and B were selected [4]. However, LaB6-which is thermodynamically favourable (enthalpy of formation ΔH =-160 kJ/mol [23])-is formed in La/B multilayers [24, 25]. Chemical interactions between La and B result in the formation of interface zones between the layers in a stack, which reduces optical contrast and, as a result, reflectivity [26]. One way to limit compound formation in La/B multilayers is to intentionally deposit (or pre-deposit) the compound, instead of one (or both) of the layers. One requirement is that this compound should be thermodynamically stable, so that it will not dissolve if it interacts with the other layers in a stack. However, this can result in the formation of superfluous amounts of compound in the interface zones, which impairs optical contrast. The enthalpy...