Orientador: Pedro Galli Mercadante / Dissertação (mestrado) - Universidade Federal do ABC, Programa de Pós-Graduação em Física, 2012

Ce travail présente la mesure de la section efficace différentielle du boson Z en impulsion transverse (ptz), dans le canal de désintégration electron-positron, avec le détecteur ATLAS au LHC. La mesure utilise 4.64 inverse fb de données de collisions proton-proton, prises en 2011 avec une énergie du centre de masse de 7 TeV. Le résultat est combiné avec une mesure indépendante faite dans le canal muon-antimuon. La mesure est faite jusqu'à ptz = 800 GeV, et a une incertitude typique de 0.5 % pour ptz < 60 GeV, atteignant jusqu'à 5 % vers la fin du spectre. La mesure est comparée avec modèles théoriques et prédictions des générateurs Monte Carlo.

After a long history of searches, a Higgs boson H was discovered by the ATLAS and the CMS experiments at the Large Hadron Collider (LHC) in 2012. Its properties fit well the ones predicted by the Standard Model (SM) of particle physics. However, the SM can not explain other established properties of Nature, such as the existence of Dark Matter. For this reason, models beyond the SM should be considered. Such models often predict the existence of several Higgs bosons and this thesis explores some of those models. In particular, the possibility to discover a charged Higgs boson, which would be a clear sign of physics beyond the SM, is studied. A commonly studied extension of the SM is the framework of two-Higgs-doublet models (2HDMs), where there are five Higgs bosons. By confronting the parameter spaces of some 2HDMs with publically available data from the LHC, the prospects for finding the 2HDM Higgs bosons is presented through the calculation of production cross sections and decay branching ratios in various channels. A new kind of 2HDM, called the Stealth Doublet Model is presented and the properties of the Higgs bosons are studied. In this model, it is shown that in particular the properties of the charged Higgs boson H± have new features not exhibited in earlier studied models. Within the parameter space compatible with the LHC results, the production cross section for H± can be sizeable enough to be experimentally observed. Finally, the discovery prospects at the LHC, for a H± in the pp → tH± process, with the decays H± → HW± and H → bb, is studied in various models beyond the Standard Model. It is shown that for the supersymmetric models, this channel is beyond the discovery reach of the LHC. In some of the other studied models, in particular the Aligned 2HDM, the situation is improved and the channel is feasible.

Thesis (Ph. D.)--Georgia State University, 2008. / Title from file title page. Xiaochun He, committee chair; William Nelson, Steven Manson, Brian Thoms, Douglas Gies, committee members. Description based on contents viewed Aug. 21, 2009. Includes bibliographical references (p. 104-108).

Η παρούσα εργασία εστιάζει στη διαδικασία δημιουργίας του χάρτη απωλειών ρεύματος της δέσμης ηλεκτρονίων κατά μήκος της Tρίτης Πειραματικής Διάταξης για το Συμπαγή Γραμμικό Επιταχυντή του Ευρωπαϊκού Κέντρου Πυρηνικών Ερευνών CERN (Beam Loss Map for Clic Test Facility 3). Ο χάρτης απωλειών χρησιμοποιείται για τον προσδιορισμό των σημείων στα οποία υπάρχει απώλεια ρεύματος των φορτίων της δέσμης. Ο προσδιορισμός των σημείων αυτών είναι πρωτεύουσας σημασίας, τόσο από θεωρητική όσο και από πρακτική πλευρά, επειδή πιθανές απώλειες συνεπάγονται αυξημένους κινδύνους έκθεσης σε ακτινοβολία για τον άνθρωπο, πιθανές βλάβες στα μαγνητικά στοιχεία, αλλά και μείωση της ισχύος της δέσμης. Στο πρώτο μέρος της εργασίας, παρουσιάζεται το Ευρωπαϊκό Κέντρο Πυρηνικών Ερευνών και οι πειραματικές εγκαταστάσεις στις οποίες έγινε η παρούσα εργασία. Στη συνέχεια, περιγράφεται η συλλογή και ανάλυση των δεδομένων με στόχο την χαρτογράφηση των σημείων απώλειας ρεύματος δέσμης στο σύμπλεγμα του CTF3. / The Diploma Thesis focuses on creating the Beam Loss Map for Compact Linear Collider Test Facility 3, at CERN. The goal of the project is the allocation of the points where beam current losses occur. Defining these points is of great importance, because any loss of beam current, especially at the maximum energy of 150 MeV, can induce radiation activation along the machine, which is dangerous for both the hardware and the personnel who need to service the machine. In the first part of the project, CERN, LHC and CLIC are presented. The second part contains data analysis, presentation of the calibration procedure of the BPMs, the new scaling factors and finally the Beam Loss Map for CTF3.

In the planned linear accelerator called Compact Linear Collider, CLIC, electrons and positrons will be accelerated to velocities near the speed of light. A limiting factor in accelerating structures are vacuum breakdowns, which are electrical discharges from a surface as a result of a large electric field being applied. In the preparatory studies for the CLIC, Uppsala University in collaboration with The European Organization for Nuclear Research, CERN, is building a DC Spark system to analyze vacuum breakdowns. This system containing large planar electrodes will be cooled down all the way down to around 4 K in order to limit the rate of wich vacuum breakdowns happen. When cooling a system like this, which consists of different components made of different materials there is the question of how the system will be affected. The objective of this project is to investigate how the cooling will affect the stability in terms of stresses and to analyze the cool down time of the system. Another goal is to make a material recommendation for a few parts based on the results. This will be done by simulating the cooling in COMSOL Multiphysics, which is a program that uses finite element analysis to solve complex problems where different branches of physics interact. The conclusion is that the system will most likely be stable as it is and there is no need to redesign it. The choice of recommended material is alumina with the reason being it should cause the least stress and the smallest gap between the electrodes when the cooling is done. There was no big difference in the cool down time between the materials. Further studies and simulations on the system is also recommended since there are many factors not taken into consideration in this study.

Le Modèle Standard de la physique des particules a été renforcé par la récente découverte du très attendu boson de Higgs. Le modèle standard cosmologique a lui relevé le défi de la haute précision des observations cosmologiques et des expériences d'astroparticules. Toutefois, ces deux modèles standards sont encore confrontés à plusieurs problèmes théoriques, comme le problème de naturalité dans le secteur de Higgs du Modèle Standard, ainsi que des problèmes observationnels à l'image des nombreuses preuves de l'existence d'un genre inconnu de matière, appelé Matière Noire, qui représenterait la majeure partie du contenu en matière de l'Univers. Les tentatives visant à résoudre ces problèmes ont conduit au développement de nouveaux modèles physiques au cours des dernières décennies. La supersymétrie est un de ces modèles qui traite du problème du réglage fin dans le secteur de Higgs et fournit de bons candidats à la Matière Noire. Les expériences actuelles de physique des hautes énergies et de haute précision offrent de nombreuses possibilités pour contraindre les modèles supersymétriques. C'est dans ce contexte que cette thèse s'inscrit. En considérant le Modèle Standard Supersymétrique Minimal (MSSM), l'extension supersymétrique la plus simple du Modèle Standard, et son candidat à la Matière Noire, le neutralino, il est montré que les contraintes obtenues en collisionneur pourraient fournir des informations sur une période de l'Univers jeune, l'ère inflationnaire. Il est également démontré que la Détection Indirecte de Matière Noire, en dépit de plusieurs inconvénients, peut se révéler être une technique efficace pour explorer les modèles de Matière Noire supersymétrique. Au-delà du MSSM il est montré que des caractéristiques uniques du candidat à la Matière Noire dans le NMSSM peuvent être explorées aux collisionneurs. L'étude d'un modèle supersymétrique avec une symétrie de jauge étendue, le UMSSM, est également développée. Les caractéristiques d'un autre candidat de la matière noire de ce modèle, le sneutrino droit, sont analysées. Des contraintes plus générales telles que celles provenant d'observables de basse énergie sont finalement prise en compte. / The Standard Model of particle physics has been strengthened by the recent discovery of the long-awaited Higgs boson. The standard cosmological model has met the challenge of the high precision observations in comology and astroparticle physics. However these two standard models face both several theoretical issues, such as the naturalness problem in the Higgs sector of the Standard Model, as well as observational issues, in particular the fact that an unknown kind of matter called Dark Matter accounts for the majority of the matter content in our Universe. Attempts to solve such problems have led to the development of New Physics models during the last decades. Supersymmetry is one such model which addresses the fine-tuning problem in the Higgs sector and provides viable Dark Matter candidates. Current high energy and high precision experiments give many new opportunities to probe the supersymmetric models. It is in this context that this thesis is written. Considering the Minimal Supersymmetric Standard Model (MSSM), the simplest supersymmetric extension of the Standard Model of particle physics, and its conventional Dark Matter candidate, the neutralino, it is shown that collider constraints could provide informations on the very early Universe at the inflation area. It is also demonstrated that the Indirect Detection of Dark Matter, despite several drawbacks, can be a powerful technique to probe supersymmetric Dark Matter models. Beyond the MSSM it is shown that unique characteristics of the Dark Matter candidate in the NMSSM could be probed at colliders. The study of a supersymmetric model with an extended gauge symmetry, the UMSSM, is also developed. The features of another Dark Matter candidate of this model, the Right-Handed sneutrino, are analysed. More general constraints such as those coming from low energy observables are finally considered in this model.

Submitted by Wagner Maciel Castilho (castilho.w@gmail.com) on 2017-12-05T10:53:57Z No. of bitstreams: 1 TeseWagner.pdf: 4189219 bytes, checksum: dbc77f46b31b8872c5aafe68d8a5b7d0 (MD5) / Approved for entry into archive by Pamella Benevides Gonçalves null (pamella@feg.unesp.br) on 2017-12-05T12:38:21Z (GMT) No. of bitstreams: 1 catilho_wm_dr_guara.pdf: 4189219 bytes, checksum: dbc77f46b31b8872c5aafe68d8a5b7d0 (MD5) / Made available in DSpace on 2017-12-05T12:38:21Z (GMT). No. of bitstreams: 1 catilho_wm_dr_guara.pdf: 4189219 bytes, checksum: dbc77f46b31b8872c5aafe68d8a5b7d0 (MD5) Previous issue date: 2017-11-10 / Os fenômenos físicos envolvidos em colisões relativísticas de íons pesados foram estudados utilizando o código hidrodinâmico NeXSPheRIO, com condições iniciais flutuantes evento a evento, caracterizado por tubos de fluxo longitudinais de altas energias. Foram realizadas análises para o espectro de hádrons em função dos momentos transversais pelos cálculos das distribuições de partículas em sete janelas de centralidade de colisão, de acordo com dados publicados pela Colaboração STAR. A coletividade da matéria nuclear formada durante as colisões foi investigada em termos de correlações azimutais entre hádrons. Verificou-se que as estruturas da correlação dependem do momento transversal e da centralidade. Tais estruturas são atribuídas à interação entre um fundo dependente da centralidade e as flutuações de evento a evento na multiplicidade. Como resultado, as correlações observadas são apresentadas por um duplo pico na região do away-side que mudam continuamente para um pico único sob certas circunstâncias. Em termos do modelo do tubo periférico, o fundo é dominado pelo fluxo elíptico que aumenta com a descentralização. Pelos cálculos numéricos, a anisotropia do sistema é estudada quanto aos coeficientes de fluxo harmônico até a quarta ordem, de acordo com os dados da colaboração PHENIX. A anisotropia do fundo contribui para as correlações entre hádrons e pôde ser avaliada pelo método ZYAM. Após sua subtração na produção do sinal de correlação próprio, a estrutura de correlação resultante é uma função da centralidade, plano de evento e do momento transverso de acordo com os dados das colaborações PHENIX e STAR. Mostrou-se que a estrutura do duplo pico no away-side muda continuamente para um pico único com a redução na centralidade. Além disso, em relação à dependência do plano de eventos, a estrutura de duplo pico no away-side evolui para um pico único à medida que o ângulo azimutal das partículas gatilho se move do plano para o da direção fora do plano de eventos. Também foi mostrado que a estrutura resultante do away-side pode ser sensível ao esquema detalhado pelo método ZYAM, particularmente, a subtração do terceiro coeficiente harmônico. Por último, mas não menos importante, a magnitude da correlação diminuiu com o aumento do momento transversal das partículas associadas. Nossas análises apresentaram um acordo razoável com os dados experimentais publicados pela colaboração PHENIX e STAR do RHIC / The physical phenomena involved in relativistic heavy-ion collisions were studied using a hydrodynamic code, NeXSPheRIO, with event-by-event fluctuating initial conditions featured by high-energy longitudinal flux tubes. Analyses were carried out for hadron spectrum as a function of the transverse momentum by the calculations of particle distributions in seven collision centrality windows, according to the data published by the STAR Collaboration. Also, the collectivity of the nuclear matter formed during the collisions was investigated in terms of dihadron azimuthal correlations. The correlation structures were found to be dependent on the transverse momentum and centrality. They are attributed to the interplay between the centrality dependent background and the eventby-event multiplicity fluctuations. As a result, the observed correlations are featured by a double-peak in the away-side region that continuously change to a single peak under certain circumstances. In terms of the peripheral tube model, the background is dominated by the elliptic flow which increases with decreasing centrality. By numerical calculations, the anisotropy of the system is studied regarding the harmonic flow coefficients up to fourth order, in accordance with the existing RHIC data. The background anisotropy contributes to the dihadron correlations, and can be evaluated by the ZYAM method. After it is subtracted from the proper correlation yields, the resultant correlation structure is a function of centrality, event plane and transverse moment, in accordance with the data from the PHENIX and STAR Collaborations. It was shown that the double-peak structure in the away-side continually changes to a single peak as centrality decreases. In addition, concerning the event plane dependence, the double-peak structure in the away-side evolves into a single peak as the azimuthal angle of the trigger particles moves from the in-plane to the out-of-plane direction. It was also shown that the resultant away-side structure can be sensitive to the detailed schemes of the ZYAM method, particularly, to the subtraction of the third harmonic coefficient. Last but not least, the magnitude of the correlation was found to decrease with increasing transverse moment of the associated particles. Our analyses manifestly presented a reasonable agreement with the experimental data published by the PHENIX and STAR Collaborations

Orientador: Prof. Dr. Alex Gomes Dias / Coorientador: Prf. Dr. Alexandre Alves / Tese (doutorado) - Universidade Federal do ABC, Programa de Pós-Graduação em Física, Santo André, 2018.

Orientador: Jun Takahashi / Dissertação (mestrado) - Universidade Estadual de Campinas, Instituto de Fisica Gleb Wataghin / Made available in DSpace on 2018-08-11T10:25:44Z (GMT). No. of bitstreams: 1 Souza_RafaelDerradide_M.pdf: 5190148 bytes, checksum: 9951aed4d9ff0a2b1db393891c1ac465 (MD5) Previous issue date: 2008 / Resumo: Reações nucleares envolvendo núcleos pesados em energia de colisão no limite relativístico são estudadas para conhecer as leis e características da matéria em condições extremas de energia e temperatura. Em uma colisão de núcleos pesados no regime relativístico, milhares de partículas são produzidas. Neste trabalho, estudamos a produção de partículas analisando os dados de colisões de íons pesados relativísticos, medidos pelo experimento STAR do acelerador RHIC, com uma abordagem estatístico-termodinâmica. Usando o formalismo grande-canônico, foram feitos estudos da dependência dos parâmetros termodinâmicos com o volume dos sistemas formados em colisões de íons de ouro ( 197 Au) nas energias de 62,4 e 200 GeV por par de núcleon e colisões de íons de cobre ( 63 Cu) na energia de 200 GeV por par de núcleon. Observou-se que o grau de equilíbrio do setor de estranheza é equivalente entre os sistemas criados em colisões centrais de íons de cobre e os criados em colisões periféricas de íons de ouro na energia de 200 GeV por par de núcleon. Também foi analisada a dependência dos parâmetros termodinâmicos com relação à rapidez das partículas produzidas na reação e os resultados mostraram um forte aumento dos potenciais químicos bariônico e de estranheza para as regiões longitudinais das distribuições de rapidez. Finalmente, foi verificada a dependência dos resultados obtidos em função da energia depositada na reação (ps N N), observando-se uma boa consistência com o comportamento geral de resultados de outros trabalhos encontrados na literatura / Abstract: Nuclear reactions in the relativistic regime are studied to understand the laws and characteristics of nature under extreme conditions of high energy density and temperature. In these collisions, a large number of particles is produced. In this work, we study the particle production mechanism using a statistical thermal approach analysing data measured by the STAR experiment at RHIC. Using a grand-canonical approach a study of the volume dependence of the thermodynamical parameters of the systems formed in gold-gold (197 Au ) collisions at 62.4 and 200 GeV per nucleon pair and copper-copper (63 Cu ) collisions at 200 GeV per nucleon pair was performed. This study showed that the equilibrium is indeed achieved and that, even in the strangeness sector, equilibrium is achieved in the case of most central gold-gold collisions. The dependence of the thermodyna-mical parameters on the particle rapidity was also analysed and the results showed an increase of the baryon and strange chemical potentials with rapidity. Finally, the dependence of the results on the energy deposited in the reaction was verified within a fairly good agreement with the general behaviour of results obtained in similar studies from literature / Mestrado / Física / Mestre em Física