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This project focuses on the conceptual design of the spin rotator for a proposed electron polarization upgrade of the SuperKEKB. The goal is to achieve the longitudinal electron polarization at the interaction point (IP). In this design, four existing dipoles will be replaced with four rotator magnets on both sides of the IP. The rotator magnet structure consists of dipole-solenoid combined function magnets with skew-quadrupoles installed on top to decouple the x-y plane. The advantage of this design is that the original machine geometry is maintained, and the original machine can be recovered by turning off the solenoid-quadrupole in the rotator magnet. With Bmad, a powerful lattice simulation tool applied to perform the optimizations for this design, the longitudinal spin alignment at the IP reaches a significantly high level, greater than 99.99%. Furthermore, the influence of the installation of the spin rotator on the original machine dynamics is minimized to an acceptable level. / Graduate

We present the results of applying a Fast Boosted Decision Tree (FBDT) algorithm to the task of distinguishing muons from pions in K-Long and Muon (KLM) detector of the Belle II experiment. Performance was evaluated over a momentum range of 0.6 < p < 5.0 GeV/c by plotting Receiver Operating Characteristic (ROC) curves for 0.1 GeV/c intervals. The FBDT model was worse than the benchmark likelihood ratio test model for the whole momentum range during testing on Monte Carlo (MC) simulated data. This is seen in the lower Area Under the Curve (AUC) values for the FBDT ROC curves, achieving peak AUC values around 0.82, while the likelihood ratio ROC curves achieve peak AUC values around 0.98. Performance of the FBDT model in muon identification may be improved in the future by adding a pre-processing routine for the MC data and input variables. / Master of Science / An important task of a high-energy physics experiment is taking the input information provided by detectors, such as the distance a particle travels through a detector, the momentum, and energy deposits it makes, and using that information to identify the particle's type. In this study we test a machine learning model that sorts the particles observed into two categories—muons and pions—by comparing the particle's input values to a threshold value at multiple stages, then assigns a final identity to the particle at the last stage. This is compared to a benchmark model that uses the probabilities that these input variables would be seen from a particle of each type to determine which particle type is most likely. The ability of both models to distinguish muons and pions were tested on simulated data from the Belle II detector, and the benchmark model outperformed the machine learning model.

This project contributes to the research and development studies towards successful commissioning of the SuperKEKB electron-positron collider. This accelerator and storage rings complex aims at delivering the high-luminosity collisions of beams of electrons and positrons needed for the Belle II experiment. Such beams produce parasitic radiation—called “machine-induced backgrounds”, or simply “beam backgrounds” — that have detrimental effects on the experimental apparatus performance and durability. The Beast II effort is dedicated to measuring the beam backgrounds, and aims at testing the predictive power of the background models that were used in various phases of the Belle II design. A second objective is to ensure that the environment is safe for the detector prior to installing it around the beam lines. A major component of beam backgrounds consists of electromagnetic radiation. This study focusses on measuring this radiation at the location of the Belle II electromagnetic calorimeter. The measurements were achieved by placing scintillator crystals at positions representative of the Belle II calorimeter crystals that are the closest to the beam lines, and comparing the data with predictions for different operating parameters of the accelerator. Different phenomena related to machine backgrounds were observed: vacuum scrubbing, the electron-cloud effect, injection-related noise, beam-gas scattering and Touschek losses. Studies on the positron ring showed average background levels 13.5 +/- 3.5 times larger than simulation, whereas that ratio reached O(100-1000) for the electron ring. In the latter, the large uncertainty on the pressure measurements and the gas constituents limit the predictive power of the measurements. Radiation shields were also designed, fabricated, delivered and installed in the detector to protect the electromagnetic calorimeter from radiation coming from the beam lines. / Graduate

Le collisionneur SuperKEKB, dédié à l'expérience Belle II, prévoit une très haute luminosité, inégalée à ce jour. Son objectif est de fournir une luminosité instantanée de 8x10³⁵ cm⁻²s⁻¹ en mettant en collision des faisceaux minuscules au point d'interaction (IP) sur la base du schéma "nano-beam". Par conséquent, un excellent contrôle de l'orbite du faisceau à l’IP est nécessaire pour assurer un recouvrement géométrique optimal entre les deux faisceaux en collision, et ainsi maximiser la luminosité. Dans ce cadre, cette thèse présente le développement et l'implémentation d'un système de monitoring rapide de la luminosité de SuperKEKB basé sur des détecteurs en diamant sCVD. Pour atteindre une précision relative aussi élevée et couvrir une gamme dynamique de luminosité élevée, le processus de diffusion Bhabha radiatif à très petit angle est utilisé, dont la section efficace d’interaction est très importante et relativement bien connue. Des détecteurs diamant sCVD, dont le signal est rapide et qui ont une bonne tolérance au rayonnement, sont utilisés pour détecter les particules chargées dans les gerbes électromagnétiques induites par l’interaction entre les particules Bhabha diffusées et perdues dans le tube à vide du faisceau, et dans les autres matériaux, en particulier un radiateur, à des emplacements choisis spécialement en aval de l'IP, dans les deux anneaux LER et HER. Une simulation de bout en bout du système d'asservissement de l'orbite du faisceau à l'IP basé sur notre signal de luminosité rapide et précis a été réalisé, qui comprend: une estimation du signal du détecteur de diamant sCVD, basé sur des mesures de laboratoire à l'aide d'une source radioactive, la construction de séquences de signal représentative de SuperKEKB comprenant les bruits de fond à un seul faisceau et les particules diffusées par le processus Bhabha, un traitement du signal de luminosité, et la simulation de l'asservissement de l'orbite. Il a été possible de vérifier la faisabilité de ce système pour maintenir la très haute luminosité de SuperKEKB en présence des mouvements du sol et a de déterminer la précision relative du signal de luminosité rapide qu'il est possible d'obtenir toutes les 1 ms. Au cours des phases de mise en service de SuperKEKB, la phase 2 et le début de la phase 3, notre moniteur de luminosité rapide basé sur des détecteurs en diamant sCVD a été installé et utilisé avec succès. Les processus de perte de faisceau, principalement ceux provenant des processus de Bremsstrahlung et de Touschek, ont été étudiés en détail et, par rapport à la simulation, un bon accord a été trouvé. Lors de la mise en service de la collision, des signaux de luminosité intégrés toutes les secondes étaient fournis en continu pour le réglage des paramètres des faisceaux à l'IP. En outre, un signal de luminosité intégré toutes les 1 ms avec la précision relative attendue a également été fourni et utilisé comme entrée du système d'asservissement de l'orbite à l'IP, notamment pour des premiers tests conduits avec succès avec des décalages de faisceau horizontaux introduits volontairement. Davantage de tests de ce système d'asservissement sont attendus pour assurer son bon fonctionnement en continu à l'avenir. Cette thèse présente le développement et l’application d’un système de surveillance rapide de la luminosité basé sur les détecteurs de sCVD diamant de SuperKEKB. / SuperKEKB is at the foremost frontier of high luminosity e⁺e⁻ colliders, dedicated to the Belle-II experiment. It aims to provide an instantaneous luminosity of 8x10³⁵ by involving extremely tiny beams colliding at the Interaction Point (IP) based on the "nano-beam scheme". Therefore, excellent control of its beam orbit at the IP is required to ensure the optimum geometrical overlap between the two colliding beams, and thereby maximize the luminosity. Besides, effective instrumentation to diagnose the behavior of the beam at the IP and possible beam interactions between bunches along the train are also quite essential during the long and rather difficult process of machine tuning towards the nominal beam parameters. This thesis presents the development and application of a fast luminosity monitoring system based on sCVD diamond detectors at SuperKEKB, including: (1),train integrated luminosity signals every 1 ms which will be used as input to the dithering orbit feedback system, its relative precision is expected to be better than 1% when luminosity reaches 10³⁴ (2), sensitive train integrated luminosity signals over a large luminosity dynamic range every 1 s which will be sent to the SuperKEKB control room as immediate observable for machine collision tuning, and (3) bunch integrated luminosity signals every 1 s with sufficient relative precision to monitor the collision performance for each single bunch. To achieve such high relative precision and cover a large luminosity dynamic range, the radiative Bhabha process events at vanishing scattering angle will be measured, whose interaction cross-section is quite large and reasonably well known. The sCVD diamond detectors, which have fast signal formation and good radiation tolerance, were used to detect the charged particles in the secondary showers induced by the interaction between the lost Bhabha scattered particles and the beam pipe and specific radiator materials at carefully chosen locations downstream of the IP in both the LER and HER. A start-to-end simulation was performed on the dithering orbit feedback system using fast, precise luminosity signal as input, which includes: sCVD diamond detector signal estimation based on laboratory measurements with a radioactive source, signal sequence construction at SuperKEKB including single beam backgrounds and Bhabha scattered particles, luminosity signal procession, dithering orbit feedback simulation. It enabled verifying the feasibility of this system to maintain very high luminosity in the presence of ground motion, in particular it determined the relative precision of the fast luminosity signal every 1 ms. Besides, the radiation damage of the sCVD diamond detectors in the LER was also estimated based on a FLUKA simulation and applying the NIEL hypothesis. During the Phase-2 and early Phase-3 commissioning periods of SuperKEKB, our fast luminosity monitor based on sCVD diamond detectors was installed and operated successfully. Single beam loss processes, mainly Bremsstrahlung and Touschek, were studied in detail and compared with the simulation, showing good agreement. During the collision commissioning, train and bunch integrated luminosity signals every 1 s were provided for machine tuning. e.g. the vertical beam sizes were determined with the vertical offset scan technique based on our luminosity signals, both the average and for the individual bunches, which is very important and useful for the collision and IP local optics tuning during the long and rather difficult process of SuperKEKB machine tuning towards the nominal beam parameters. Besides, a train integrated luminosity signal every 1 ms with the expected relative precision was also provided and used as input to the dithering orbit feedback system for its first successful tests with deliberately introduced horizontal beam-beam offsets. More tests on the dithering orbit feedback system are expected to ensure its future continuous operation.

Nous étudions la sensibilité de Belle II avec 50 ab-1 de données sur l'angle βc du triangle d'unitarité, avec une mesure en fonction du temps de l'asymétrie de CP dans les désintégrations des mésons D0. Nous montrons que cette mesure est limitée statistiquement, avec une incertitude totale attendue de l'ordre de 3°. La mesure de βc nécessite la reconstruction de trajectoires de particules de très faible impulsion, impactée par le bruit de fond induit par SuperKEKB. Deux échelles PLUME vont être utilisées pour étudier ce bruit de fond. Ici, une étude des performances de PLUME est effectuée. Ainsi, la résolution spatiale avec des traces à 0° et 36° est mesurée, de 1,8 µm et 3,5µm respectivement. Par ailleurs nous proposons d'améliorer la mesure des faibles impulsions en utilisant la charge déposée par la particule dans le trajectomètre interne au silicium. L'estimateur permet d'améliorer par 2% la résolution sur l'impulsion pour les particules n'atteignant pas le trajectomètre interne. / We are studying the sensitivity of Belle II with 50 ab-1 data to the βc angle of the c-u unitarity triangle, with a time-dependent measurement of the CP asymmetry in the D0 decays. We show that such a measurement is still statistically limited, with a total expected incertitude of 3°.This measurement relies on the reconstruction of soft momenta, impacted by the SuperKEKB induced background.Two PLUME ladders will be used to study this background, therefore a study on the performances of PLUME was performed. The spatial resolution is of 1.8 µm and 3.5 µm for 0° and 36° tilted tracks respectivelly.We also propose to improve the estimation of soft momenta using the energy depositions of charged particles in the silicon layers of the inner tracker. Our estimator improves by approximately 2 % the resolution on momentum for particles which do not penetrate the central tracking system.