Introduction to neutrino oscillation's fenomenology, in vacuum and matter

Orientador: Marcelo Moraes GuzzoDissertação (mestrado) - Universidade Estadual de Campinas, Instituto de Fisica Gleb WataghinResumo: O objetivo deste trabalho é produzir um texto didático que sirva como base para alunos de física, ao ingressarem na área da fenomenologia de neutrinos. Introduz-se o modelo de mistura de neutrinos no vácuo, baseado no conceito de superposição de estados. Mostra-se que esta hipótese leva ao fenômeno da oscilação de sabor, o qual se propõe ser uma solução para o problema do neutrino solar. Mostra-se que a oscilação que ocorre no vácuo entre o Sol e a Terra não pode explicar os dados experimentais, sendo necessária a inclusão dos efeitos da matéria solar. O meio solar leva a uma alteração nas previsões devido a efeitos de ressonância. O conjunto de fenômenos que ocorrem devido a presença e à distribuição do meio solar, chamado efeito MSW, leva à verdadeira solução do problema do neutrino solar. Faz-se um ajuste simples no modelo, encontrando o melhor ajuste aos dados de SuperKamiokande. Com o modelo ajustado, mostra-se a concordância com os dados de HomestakeAbstract: The subject of this work is to produce a didactic text that can be used by physics students as a basis when incoming on the neutrinos phenomenology area. We introduce the neutrinos mixing model in vacuum, based on the concept of state superposition. We show that this hypothesis leads to avor oscillation phenomenon, the one is proposed to be a solution to the solar neutrino problem. We show that vacuum oscillations between the Sun and the Earth cannot explain the experimental data, making necessary the inclusion of solar matter effects. The solar medium leads to modifications on the predictions because of resonance effects. The set of phenomenon that takes place due to the presence and to the distribution of solar medium, called MSW effect, leads to the real solution of the solar neutrino problem. We make a simple fit on the models parameters, finding the best fit to de SuperKamiokande data set. With the model fitted, we show that it agrees with Homestake dataMestradoTeoria Geral das Particulas e CamposMestre em Físic

The Alice Collaboration

8301-4919c924

First proton-proton collisions at the LHC as observed with the ALICE detector: Measurement of the charged-particle pseudorapidity density at √s = 900 GeV

On 23rd November 2009, during the early commissioning of the CERN Large Hadron Collider (LHC), two counter-rotating proton bunches were circulated for the first time concurrently in the machine, at the LHC injection energy of 450 GeV per beam. Although the proton intensity was very low, with only one pilot bunch per beam, and no systematic attempt was made to optimize the collision optics, all LHC experiments reported a number of collision candidates. In the ALICE experiment, the collision region was centred very well in both the longitudinal and transverse directions and 284 events were recorded in coincidence with the two passing proton bunches. The events were immediately reconstructed and analyzed both online and offline. We have used these events to measure the pseudorapidity density of charged primary particles in the central region. In the range |η|<0.5, we obtain dNch/dη=3. 10±0. 13(stat.)±0. 22(syst.) for all inelastic interactions, and dNch/dη=3.51±0. 15(stat.)±0. 25(syst.) for non-single diffractive interactions. These results are consistent with previous measurements in proton-antiproton interactions at the same centre-of-mass energy at the CERN SppS̄ collider. They also illustrate the excellent functioning and rapid progress of the LHC accelerator, and of both the hardware and software of the ALICE experiment, in this early start-up phase