An intra-pulse Interaction Point fast feedback system (IPFB) has been designed for the Next Linear Collider (NLC), to correct relative beam-beam misalignments at the Interaction Point (IP). This system will utilise the large beam-beam kick that results from the beam-beam interaction and apply a rapid correction to the beam misalignment at the IP within a single bunch train. A detailed examination of the IPFB system is given, including a discussion of the necessary electronics, and the results of extensive simulations based on the IPFB concept for fast beam correction are presented. A recovery of the nominal luminosity of the NLC is predicted well within the NLC bunch train of 266 ns. The FONT experiment - Feedback On Nanosecond Timescales - was proposed as a direct test of the IPFB concept and was realised at the NLC Test Accelerator at SLAC. As part of FONT, a novel X-band BPM was designed and tested at the NLCTA. The results of these tests with the NLCTA short and long-pulse beam are presented, demonstrating a linear response to the position of the 180 ns long-pulse beam: measurements show a time constant of ~1.5 ns and a precision of better than 20 microns. A novel BPM processor for use at X-band, making use of the difference-over-sum processing technique, is also presented in detail, with results given for both short and long-pulse beams. The FONT design concepts and modification of the IPFB system for use at the NLCTA are described. The design of a fast charge normalisation circuit, to process the difference and sum signals produced by the BPM processor, forming part of the FONT feedback circuit, is detailed extensively. Bench tests of the feedback electronics demonstrate the effectiveness of the normalisation and feedback stages, for which a signal latency of 11 ns was measured. These bench tests also show the correct operation of the normalisation and feedback principles. Finally, the results of a full beam test of the FONT system are presented, during which a system latency of 70 ns was measured. These rigorous tests establish the soundness of the IPFB scheme and show correction of a mis-steered bunch train within the full NLCTA pulse length of 180 ns.

Un des objectifs principaux de l'expérience PHENIX est l'étude de la matière nucléaire soumise à des conditions extrêmes de température et de densité d'énergie. Dans les collisions ultra-relativistes Au+Au à 200~GeV par paires de nucléon, il serait possible de former un état de la matière pour lequel les quarks et les gluons ne seraient plus liés au sein des nucléons mais pourraient évoluer de façon quasi-libre sur des distances plus grandes que la taille caractéristique de ces derniers. Cet état est dénommé le Plasma de Quarks et de Gluons (QGP).<br /><br />L'étude de la production du $\jpsi$, particule lourde formée d'une paire de quarks charme ($c \bar c$), est une des sondes initialement proposée pour étudier le QGP. Une suppression de la production du $\jpsi$ était en effet attendue en présence d'un QGP, en raison de l'écrantage du potentiel de liaison entre les quarks charme le constituant par la présence du milieu dense coloré environnant. De nombreuses mesures du $\jpsi$ ont eu lieu depuis au SPS (CERN) et à RHIC (BNL). Elles ont permis de mettre en évidence non seulement l'existence d'une telle suppression, mais également la présence de mécanismes supplémentaires, rendant plus difficile l'interprétation des résultats correspondants.<br /><br />L'expérience PHENIX est la seule des quatre expériences de RHIC capable de mesurer le $\jpsi$ à rapidité positive via sa désintégration en deux muons. En 2007 des collisions Au+Au à une énergie par paire de nucléons dans le centre de masse $\sqrt{s_{NN}}=200$~GeV ont été réalisées à BNL, ce qui a permis d'augmenter d'un facteur quatre la statistique disponible pour l'étude du $\jpsi$ par rapport aux résultats publiés précédemment. Cette augmentation, ajoutée à la mise en oeuvre de nouveaux détecteurs dans PHENIX, a permis de préciser les mesures précédentes, et de mesurer des observables jusqu'alors inaccessibles telles que l'asymétrie azimutale de la production du $\jpsi$.<br /><br />Ce manuscrit présente la compréhension actuelle de la production de quarkonia et l'utilisation de cette sonde dans l'étude du QGP. L'analyse conduisant à la première mesure de l'anisotropie azimutale du $\jpsi$ à rapidité positive dans les collisions Au+Au à 200~GeV par paire de nucléons est détaillée. Cette mesure devrait permettre de préciser le mécanisme de production du méson, en particulier en ce qui concerne la part de recombinaison des quarks $c$ en $\jpsi$.

In this thesis we employ string perturbation theory in toroidal orbifold models to study aspects of supersymmetry breaking in type IIB string theory. First, we determine the dependence of physical Yukawa couplings on blow-up moduli in models with D3-branes at orbifold singularities. Blow-up moduli are scalar fields describing the size of small blow-up cycles in the compactification geometry. In models implementing moduli stabilisation these fields can acquire F-terms and break supersymmetry. We examine the moduli-dependence of physical Yukawa couplings at string tree-level by computing disk correlation functions involving a Yukawa interaction of visible sector fields and an arbitrary number of blow-up moduli. We perform the calculation for one blow-up insertion explicitly and find that the correlation function vanishes if the blow-up modulus is associated with a small cycle distant to the visible sector. For more than one blow-up insertion we show that all such correlation functions are exponentially suppressed by the compactification volume. We explain how these results are relevant to suppressing soft terms to scales parametrically below the gravitino mass. Further, we determine corrections to holomorphic Yukawa couplings on D3-branes at an orbifold singularity due to non-perturbative effects such as gaugino condensation on a stack of D7-branes. This can be done by calculating a one-loop threshold correction to the gauge coupling on the D7-branes. We show that, if present, the new contributions to Yukawa couplings are not aligned with the tree-level couplings. As the new Yukawa couplings contribute to soft A-terms they are sources of flavour-changing neutral currents. Last we discuss an effect unrelated to supersymmetry breaking. We show that orbifold models with D3-branes at orbifold singularities can exhibit kinetic mixing of different massless Abelian factors. For this to be possible, the relevant U(1) factors have to be associated with more than one orbifold singularity.

The International Muon Ionization Cooling Experiment (MICE) is designed to demonstrate the currently untested technique of ionization cooling. Theoretically, this process can condition the high quality muon beams required to build a neutrino factory or muon collider which will be the next generation of machines for the study of Particle Physics. The beam line to transport muons into the MICE cooling channel lattice cell was installed in December 2009. Step I of the experimental programme, whose goal was to demonstrate that the beam line can generate beams similar to those expected in a neutrino factory cooling channel, was completed in August 2010. Methods were developed to use time difference measurements in the MICE time of flight counters (TOFs) to obtain a transverse spatial resolution of approximately 10 mm and to track muons through the focusing elements of the beam line, thus allowing the trace space vectors of individual muons to be reconstructed and their integrated path length to be calculated. The TOFs were used to make an absolute measurement of the momentum of muons with zero bias and a systematic error of less than 3 MeV/c. The measured trace space vectors of single muons were used to estimate the emittances and approximate optical parameters of eighteen muon beams. The results of beam line simulations were compared with the measurements and, once the effects of experimental resolution had had been included, found to be in good agreement. A sample of individual muons whose phase space vectors had been measured was injected into a simulation of the full MICE cooling channel; the beam was found to be suitable for demonstrating muon cooling, although some fine tuning of the cooling channel optics will eventually be required.