L’utilisation de réseaux optiques dans la géométrie de diffraction conique a connu ces dernières décennies un essor remarquable dans les domaines UV et X grâce à ses propriétés particulières: absence de l’écrantage derrière les traits du réseau aux incidences rasantes, faible dispersion angulaire limitant l’étirement temporel, efficacité de diffraction élevée. Son usage s’est imposé pour la monochromatisation d’impulsions ultra-brèves. C’est aussi l’une des deux options retenues par la Nasa pour le spectrographe à réseau de l’Observatoire à rayon X de la future mission Lynx. Ce travail de thèse contribue au développement de méthodes numériques pour modéliser les effets de diffraction par des réseaux dans une géométrie encore peu étudiée sous cet aspect. La complexité de cette étude réside dans le couplage inhérent entre les deux états fondamentaux de polarisation. Du point de vue numérique, il impose un calcul ‘’vectoriel’’, là où, en géométrie classique des calculs scalaires suffisent. Notre travail s’est appuyé sur les méthodes numériques de calcul de diffraction par des structures périodiques déjà développées dans le cadre de la géométrie classique. Ces méthodes sont basées sur la théorie différentielle, qui consiste à propager une série d’ondes planes au travers de la zone modulée. La méthode différentielle employée est complétée par l’usage de l’algorithme de propagation de la matrice réflectivité. On contourne ainsi certains problèmes de convergence. Dans la partie théorique de ce travail, ces algorithmes sont étendus pour s’adapter aux cas de géométrie oblique. Sur cette base théorique, nous avons pu développer un code de calcul, nommé COROX, fonctionnant dans toutes les géométries d’utilisation. Un certain nombre de réseau types ont été étudiés, tant en géométrie oblique que classique, pour mettre en évidence, non seulement les efficacités de diffraction mais encore les effets de polarisation, (paramètres de Stokes et matrice de Müller) ainsi que les phases spectrales. Des propriétés intéressantes ont été remarquées, comme l’existence d’une composante circulaire non négligeable diffractée par réseau lamellaire quand l’onde incidente polarisée à 45° par rapport au plan du réseau. Le comportement de la phase spectrale est également une donnée significative pour une future gestion d’impulsions ultra-brèves. Des mesures de diffraction ont été effectuées sur la ligne Métrologie du Synchrotron SOLEIL, sur un réseau blazé de 150 traits/mm. Un accord raisonnable entre efficacités mesurées et calculées est constaté si l’on tient compte de la forte rugosité du réseau étudié. / The conical geometry of optical grating diffraction has been suggested and studied, in the last 10 years, for cutting edge applications in the VUV and X-ray domains, due to its specific properties such as: absence of screen inside the grating grooves at grazing incidence, low angular dispersion which limits the temporal spread of short pulses, very high diffraction efficiencies. It has been accepted as the first choice technology for VUV short pulses monochromatization. It is also one of the two options selected by NASA, for the grating spectrograph of the future X-ray Observatory of the Lynx mission. This thesis reports our contribution to the development of numerical methods in order to model the effects of diffraction by optical gratings in this still little studied geometry. This study is made more complex by an inherent coupling between the two fundamental polarization modes. From the numerical aspect, it requires performing “vectorial” computations, whereas, in a classical diffraction geometry, scalar computations are sufficient. Our work is based on numerical methods already developed for modeling optical diffraction by periodic structures in the framework of classical geometry. These methods are using on the differential theory, whose main concept is propagating a set of plane waves throughout the modulated area. We use the differential method together with an algorithm of reflectivity matrix propagation. It overcomes some of the convergence issues. In the theoretical part of this work, reflectivity matrix algorithms are extended to the case of oblique geometry. On these theoretical grounds, we developed a computation code, named COROX, which can be applied in any geometry. A number of typical grating cases have been studied, both in the conical and of le classical one. The output is not only the diffraction efficiencies, but also the polarization properties (Stokes parameters, Müller matrix), as well as the spectral phases. Interesting properties have been noticed, such as the presence of a non-negligible circularly polarized component diffracted from a lamellar grating when the incident wave is linearly polarized at 45° from the grating plane. The spectral phase behavior is also a significant data for an eventual shape tayloring of ultrashort pulses. Diffraction efficiency measurements have been performed on the Metrology beamline of Synchrotron SOLEIL, using a 150 lines/mm blazed grating as a test object. A reasonable agreement between measured and computed efficiencies has been obtained, provided that the rather high roughness of this grating is taken into account.

The objective of this research is to develop and design front-end analog circuits for Capacitive Micromachined Ultrasound Transducers (CMUTs) and optical grating MEMS microphone. This work is motivated by the fact that with micro-scaling, MEMS sense capacitance gets smaller in a CMUT array element for intravascular ultrasound imaging, which has dimensions of 70um x 70um and sub pico-farad capacitance. Smaller sensors lead to a lower active-to-parasitic ratio and thus, degrads sensitivity. Area and power requirements are also very stringent, such as the case of intravascular catheter implementations with CMOS-First CMUT fabrication approach. In this implementation, capacitive feedback charge amplifier is an alternative approach to resistive feedback amplifiers. Capacitive feedback charge amplifier provides high sensitivity, small area, low distortion and saving power. This approach of charge amplifiers is also suitable in capacitive microphones where it provides low power and high sensitivity. Another approach to overcome capacitive detection challenges is to implement optical detection. In the case of biomimetic microphone structure, optical detection overcomes capacitive detection's thermal noise issues. Also with micro-scaling, optical detection overcomes the increased parasitics without any sensitivity degradation, unlike capacitive detection. For hearing aids, along with sensitivity, battery life is another challenge. We propose the use of 1-bit front-end sigma-delta ADC for overall improved hearing aid power efficiency. Front-end interface based on envelope detection and synchronous detection schemes have also been designed. These interface circuits consume currents in microampere range from a 1.5V battery. Circuit techniques are used for maximizing linear range and signal handling with low supplies. The entire front end signal processing with Vertical Cavity Surface Emitting Laser (VCSEL) drivers, photodiodes, filters and detectors is implemented on a single chip in 0.35um CMOS process.