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This thesis presents results from three strands of experimental work aimed towards establishing more reproducible, higher energy, and more accurately measured electron beams generated by a laser-driven plasma accelerator. The first experiment calibrated two types of detector frequently used to measure the bunch charge in laser wakefield accelerator experiments, namely scintillating screens and image plates. The experiments undertaken at the DAFNE beam test facility in Frascati, Italy, confirmed that the fluorescence signal from Kodak Lanex Regular screens varies linearly with the charge density for a nanosecond elec- tron bunch for charge densities in the range between ρ = 2 × 10⁻⁷ ^C/_m² to ρ = 10−5 ^C/_m². A sensitivity measurement of FUJIFILM BAS-IP MS image plates resulted in a sensitivity of SMS = (0.0487 ± 0.0028 ) PSL, which is 2.4 times higher than had been assumed prior to this work. The second strand aimed at improving the operation of the capillary discharge waveguide by re-designing the discharge circuit and the waveguide housing. The experiment showed that combining a glow discharge circuit with the pulsed discharge circuit of the capillary discharge waveguide reduced electrical noise, the timing jitter between the trigger pulse and the discharge, and the voltage required to initially break down the capillary gas for pressures below 10 mbar and above 150 mbar. The size of the housing of the capillary discharge waveguide was reduced in all three dimensions by an average of 60 %, enabling the device to be used in future staging experiments, and an open design of the housing eliminated the possibility of unwanted discharges. The new capillary design performed without flaw in the Astra-Gemini experiment and no disadvantages compared with the old housing were found. The third strand of work describes an experiment undertaken with the Astra-Gemini laser at the Central Laser Facility of the Rutherford Appleton Laboratory, United Kingdom. The improved capillary discharge waveguide was used to generate GeV-scale electron beams with good reproducibility. Beams of electrons with energies above 900 MeV, and with root- mean-square divergence of 3.5 mrad, were observed for a plasma density of 2.2 × 10¹⁸ cm⁻³ and a peak input laser power of 55 TW. The variation of the maximum electron energy with the plasma density was measured and found to agree well with simple models. The energy spectra of the generated electron beams exhibited good shot-to-shot reproducibility, with the observed variations attributable to the measured shot-to-shot jitter of the laser parameters. Two methods for correcting the effect of beam pointing variations on the measured energy spectrum were tested and it was found that using a thin Lanex screen in front of the electron spectrometer was easy to implement and did not degrade the recorded energy spectrum. The first observation of temporal compression of a laser pulse within a plasma channel with simultaneous electron acceleration to energies higher than 500 MeV is also presented. This measurement suggests that the pulse compresses linearly from the back as predicted by theory.

Le blazar Mrk 501 possède un spectre d'émission non thermique présentant deux composantes. La première, dominant entre le domaine radio et celui des rayons X, correspond à l'émission synchrotron du jet magnétisé, tandis que l'origine de la seconde, dans le domaine gamma de haute énergie, demeure encore sujette à discussion. Jusqu'en 1999, ce dernier domaine d'énergie n'avait été couvert qu'entre 100 MeV et 4 GeV, ainsi qu'au-dessus de 300 GeV. La mise en place de l'expérience CELESTE a comblé la fenêtre d'énergie manquante : observation de l'émission Tcherenkov produite par les rayons gamma d'énergie entre 50 et 350 GeV pénétrant l'atmosphère. Source variable, Mrk 501 a ainsi été observée en 2000 et 2001, détectée en 2000 avec calcul de son flux permettant de contraindre les modèles d'émission à haute énergie.<br />Cette thèse présente la démarche effectuée jusqu'à la détection de Mrk 501 : dans un premier temps, par la validation de l'analyse utilisée sur des observations de la nébuleuse du Crabe, chandelle standard des télescopes Tcherenkov atmosphériques ; puis la détermination des coupures d'analyse, dépendantes de la région du ciel pointée, à partir d'observations du blazar Mrk 421, de même déclinaison que Mrk 501, dont la forte activité permet une détection claire. Enfin, des simulations, tenant compte de la qualité de l'atmosphère et améliorées pour mieux reproduire le détecteur, ont permis d'établir la surface effective de l'instrument pour en déduire le flux de Mrk 501 entre avril et juin 2000. Ce flux a été comparé avec un modèle d'émission de type synchrotron self-Compton et avec des données prises en rayons X. Elles indiquent que Mrk 501 apparaissait légèrement plus actif durant cette période par rapport au reste de l'année et à l'année 2001. Une limite supérieure au flux est calculée pour l'ensemble des autres mesures. C'est une première mesure dans le domaine d'énergie 50 - 350 GeV (gamme représentant les limites en énergie pour lesquelles le taux de comptage, c'est-à-dire la convolution du spectre de l'astre avec la surface effective de collection de l'instrument, se révèle supérieur à 20 % du maximum de comptage). Elle apporte des contraintes sur la position du maximum d'émission Compton inverse et tend à favoriser, dans ce cas précis, des processus d'émission X et gamma par deux populations d'électrons différentes (la variation dans le domaine X est faible comparée à celle du domaine gamma).

Dans ce travail, nous caractérisons la production des baryons multi-étranges Xi et Omega dans des collisions Au+Au produites au RHIC où l'on attend l'éventuelle formation d'une matière de quarks et de gluons déconfinés (QGP). Nous analysons avec l'expérience STAR les collisions obtenues à une énergie de 62 GeV, intermédiaire entre celle atteinte au SPS (17 GeV) et l'énergie nominale du RHIC (200 GeV). Les spectres en impulsions transverses, les taux de production et l'écoulement elliptique sont mesurés avec différentes méthodes permettant une estimation pertinente des incertitudes systématiques. Ces résultats sont comparés à des modèles statistiques et hydrodynamiques que nous avons adaptés à l'énergie de 62 GeV. Les propriétés chimiques et dynamiques du milieu ainsi obtenues indiquent la formation d'un milieu au moins partiellement thermalisé et suggèrent la formation d'un état comparable à 62 GeV et à 200 GeV.

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No description available.

Intensity-Duration-Frequency (IDF) curves are among the standard design tools for various engineering applications, such as storm water management systems. The current practice is to use IDF curves based on historical extreme precipitation quantiles. A warming climate, however, might change the extreme precipitation quantiles represented by the IDF curves, emphasizing the need for updating the IDF curves used for the design of urban storm water management systems in different parts of the world, including Canada. This study attempts to construct the future IDF curves for Saskatoon, Canada, under possible climate change scenarios. For this purpose, LARS-WG, a stochastic weather generator, is used to spatially downscale the daily precipitation projected by Global Climate Models (GCMs) from coarse grid resolution to the local point scale. The stochastically downscaled daily precipitation realizations were further disaggregated into ensemble hourly and sub-hourly (as fine as 5-minute) precipitation series, using a disaggregation scheme developed using the K-nearest neighbor (K-NN) technique. This two-stage modeling framework (downscaling to daily, then disaggregating to finer resolutions) is applied to construct the future IDF curves in the city of Saskatoon. The sensitivity of the K-NN disaggregation model to the number of nearest neighbors (i.e. window size) is evaluated during the baseline period (1961-1990). The optimal window size is assigned based on the performance in reproducing the historical IDF curves by the K-NN disaggregation models. Two optimal window sizes are selected for the K-NN hourly and sub-hourly disaggregation models that would be appropriate for the hydrological system of Saskatoon. By using the simulated hourly and sub-hourly precipitation series and the Generalized Extreme Value (GEV) distribution, future changes in the IDF curves and associated uncertainties are quantified using a large ensemble of projections obtained for the Canadian and British GCMs (CanESM2 and HadGEM2-ES) based on three Representative Concentration Pathways; RCP2.6, RCP4.5, and RCP8.5 available from CMIP5 – the most recent product of the Intergovernmental Panel on Climate Change (IPCC). The constructed IDF curves are then compared with the ones constructed using another method based on a genetic programming technique. The results show that the sign and the magnitude of future variations in extreme precipitation quantiles are sensitive to the selection of GCMs and/or RCPs, and the variations seem to become intensified towards the end of the 21st century. Generally, the relative change in precipitation intensities with respect to the historical intensities for CMIP5 climate models (e.g., CanESM2: RCP4.5) is less than those for CMIP3 climate models (e.g., CGCM3.1: B1), which may be due to the inclusion of climate policies (i.e., adaptation and mitigation) in CMIP5 climate models. The two-stage downscaling-disaggregation method enables quantification of uncertainty due to natural internal variability of precipitation, various GCMs and RCPs, and downscaling methods. In general, uncertainty in the projections of future extreme precipitation quantiles increases for short durations and for long return periods. The two-stage method adopted in this study and the GP method reconstruct the historical IDF curves quite successfully during the baseline period (1961-1990); this suggests that these methods can be applied to efficiently construct IDF curves at the local scale under future climate scenarios. The most notable precipitation intensification in Saskatoon is projected to occur with shorter storm duration, up to one hour, and longer return periods of more than 25 years.

New high-K isomers have been populated in Ta and W by bombarding thick targets with pulsed 238U beams at 1600 MeV. The new inelastically excited multi-quasiparticle states include Kpi = 21/2- and 29/2- 3-quasiparticle isomers in 181Ta and Kpi = 7- and (16+) isomers in 186W. The Kpi = (16+) state in 186w has t1/2&ge;3 ms and extends the 4-quasiparticle isomer systematics beyond the limit accessible with fusion-evaporation reactions, using stable beams and targets, for the first time. In addition, a t1/2&ge;1 ms 3-quasiparticle isomeric state feeding a strongly coupled rotational band has been populated in Ta by nucleon transfer. The excitation energies of the intrinsic states are compared to predictions of blocked BCS calculations. A different study of high-K states used a radioactive 14C beam at 67 MeV to investigate the high-spin structure of Os. New rotational bands built on multi-quasiparticle states with Kpi = 5-, 7-, 9-, 10+ and 15+ are observed. The first crossing of the ground-state band at I = 14 h, is interpreted as involving a high-K t-band structure and explained using a two-band mixing model. The structure at higher angular momentum is dominated by intrinsic states, that exhibit a dramatic loss of isomerism. Potential-energy-surface calculations, with Lipkin-Nogami pairing, show these configurations to be triaxial, accounting for the breakdown in K conservation. The relation between the K projection and the total angular momentum is investigated for these non-axial states.