A search for hep solar neutrinos at the Sudbury Neutrino Observatory

Thesis (Ph.D.)--University of Washington, 2016-08

The role of nuclear physics in supernovae and the evolution of neutron stars, Neutrino Opacities, Equation of State, Transport Coefficients, and Dark Matter Production

Thesis (Ph.D.)--University of Washington, 2016-08

Seattle Campus Master Plan Draft EIS - Notice of Availability

This is a public notice for the availability of the Seattle Campus Master Plan Draft EIS. It provides information on the Campus Master Plan, EIS alternatives analyzed, a link to the plan and EIS, and notification of a public hearing.

Seattle Campus Master Plan Draft Environmental Impact Statement (EIS)

This is a SEPA Environmental Impact Statement as required by State regulations for analyzing the potential impacts of implementing the proposed Seattle Campus Master Plan for the University of Washington. Five action alternatives and the No Action Alternative have been analyzed for 15 elements of the environment.

Eine Pädagogik von multinationalen Online Seminaren (Webinaren) in Echtzeit im Rahmen des Blended Learning-Konzepts

Online-Meetings in Echtzeit oder auch Webinare sind eine hervorragende Möglichkeit, mit den Gruppen auf virtuellem Wege kommunizieren zu können. Dieser Aspekt beinhaltet ein enormes Potential für die internationale und nationale Zusammenarbeit von unterschiedlichen Bildungsanbietern. Während Online-Konferenzen in der Geschäftswelt bereits zum Alltag gehören, ist man im Bildungsbereich noch weit davon entfernt Webinare als integrativen Bestandteil der Lehre anzusehen. Eingebunden in ein "Blended Learning"-Szenario erwiesen sich Webinare als ein effizientes Tool für die transnationale Kooperation von Gruppen. Sogar Großveranstaltungen können als Online-Event durchgeführt werden. Es bedarf jedoch einer sorgfältigen Planung und Inhaltserstellung, um aus einem Webinar eine attraktive Lehrveranstaltung für die Lernenden werden zu lassen. (DIPF/Orig.)

A Search for Muon Neutrinos in Coincidence with Gamma-Ray Bursts in the Southern Hemisphere Sky Using the IceCube Neutrino Observatory

The origin of observed ultra-high energy cosmic rays (UHECRs, energies in excess of $10^{18.5}$ eV) remains unknown, as extragalactic magnetic fields deflect these charged particles from their true origin. Interactions of these UHECRs at their source would invariably produce high energy neutrinos. As these neutrinos are chargeless and nearly massless, their propagation through the universe is unimpeded and their detection can be correlated with the origin of UHECRs. Gamma-ray bursts (GRBs) are one of the few possible origins for UHECRs, observed as short, immensely bright outbursts of gamma-rays at cosmological distances. The energy density of GRBs in the universe is capable of explaining the measured UHECR flux, making them promising UHECR sources. Interactions between UHECRs and the prompt gamma-ray emission of a GRB would produce neutrinos that would be detected in coincidence with the GRB’s gamma-ray emission. The IceCube Neutrino Observatory can be used to search for these neutrinos in coincidence with GRBs, detecting neutrinos through the Cherenkov radiation emitted by secondary charged particles produced in neutrino interactions in the South Pole glacial ice. Restricting these searches to be in coincidence with GRB gamma-ray emis- sion, analyses can be performed with very little atmospheric background. Previous searches have focused on detecting muon tracks from muon neutrino interactions fromthe Northern Hemisphere, where the Earth shields IceCube’s primary background of atmospheric muons, or spherical cascade events from neutrinos of all flavors from the entire sky, with no compelling neutrino signal found. Neutrino searches from GRBs with IceCube have been extended to a search for muon tracks in the Southern Hemisphere in coincidence with 664 GRBs over five years of IceCube data in this dissertation. Though this region of the sky contains IceCube’s primary background of atmospheric muons, it is also where IceCube is most sensitive to neutrinos at the very highest energies as Earth absorption in the Northern Hemisphere becomes relevant. As previous neutrino searches have strongly constrained neutrino production in GRBs, a new per-GRB analysis is introduced for the first time to discover neutrinos in coincidence with possibly rare neutrino-bright GRBs. A stacked analysis is also performed to discover a weak neutrino signal distributed over many GRBs. Results of this search are found to be consistent with atmospheric muon backgrounds. Combining this result with previously published searches for muon neutrino tracks in the Northern Hemisphere, cascade event searches over the entire sky, and an extension of the Northern Hemisphere track search in three additional years of IceCube data that is consistent with atmospheric backgrounds, the most stringent limits yet can be placed on prompt neutrino production in GRBs, which increasingly disfavor GRBs as primary sources of UHECRs in current GRB models.

Saber ou não saber? Eis a questão

O presente relatório surge com a finalidade de expor diversas diretrizes desenvolvidas, no âmbito do Mestrado em Educação Pré-Escolar e Ensino do 1.º Ciclo do Ensino Básico. Centralizado nas práticas educativas, este documento rege-se pela contextualização dos ambientes educativos onde, enquanto estagiária, realizei as práticas de ensino supervisionadas. Numa análise crítica e reflexiva, são explanadas as experiências e aprendizagens originadas nestes dois períodos. Aqui, fala-se sobre a criatividade e motivação na aquisição de conhecimento, assim como os seus benefícios para e na criança. Deste modo é importante dar voz à criança e saber ouvir o que esta tem para nos dizer, num sentido de orientação e estímulo das suas aprendizagens. É também debatida a importância de um livro ou como somos modelos de comportamentos para a criança, além do modo que se desenrola a comunicação entre um aluno e um professor e se, efetivamente, a escola portuguesa é inclusiva. Considera-se a teoria versus a prática como instrumento de aquisição de saberes, para nós educadores/professores. São, ainda, delineados dois projetos desenvolvidos – um deles na educação pré-escolar e outro no 1.º Ciclo de Ensino Básico – que se focam nas perspetivas e bem-estar da criança/aluno, relativamente ao/à jardim de infância/escola. Não descurando aspetos centrais da profissionalização, o presente relatório apresenta-se como objetivo de descrição e análise do meu desenvolvimento enquanto agente de educação. Enquanto formação inicial, a prática possibilitou-me a concretização de objetivos, além de coadjuvar a metamorfose dos conhecimentos curriculares em profissionais, complementando com experiências memoráveis e indispensáveis para a construção do meu ser pessoal e profissional.

Poemas de Amanda Ponce

- Me rehúso- Amor de ladina

Amanda Lorza de Ayala, Magistrada de la Sala Civil de Santiago de Cali

Amanda Lorza de Ayala, magistrada de la Sala Civil de Santiago de Cali, en su despacho. Foto en primer plano de su cara. Fotografía tomada el 3 de Mayo de 1994

Ter ou ser? Eis a questão: O efeito moderador das características de personalidade sobre a relação entre o person-job fit e o engagement

Dissertação de Mestrado apresentada ao ISPA - Instituto Universitário

Search for heavy neutrinos in $D_s$ decays with the CMS detector at LHC

This thesis presents a search for a sterile right-handed neutrino $N$ produced in $D_s$ meson decays, using proton-proton collisions collected by the CMS experiment at the LHC. The data set used for the analysis, the B-Parking data set, corresponds to an integrated luminosity of $41.7\,\textrm{fb}^{-1}$ and was collected during the 2018 data-taking period. The analysis is targeting the $D_s^+\rightarrow N(\rightarrow\mu^{\pm}\pi^{\mp})\mu^{+}$ decays, where the final state muons can have the same electric charge allowing for a lepton flavor violating decay. To separate signal from background, a cut-based analysis is optimized using requirements on the sterile neutrino vertex displacement, muon and pion impact parameter, and impact parameter significance. The expected limit on the active-sterile neutrino mixing matrix parameter $|V_{\mu}|^2$ is extracted by performing a fit of the $\mu\pi$ invariant mass spectrum for two sterile neutrino mass hypotheses, 1.0 and 1.5 GeV. The analysis is currently blinded, following the internal CMS review process. The expected limit ranges between approximately $10^{-4}$ for a 1.0 GeV neutrino to $7\times10^{-5}$ for a 1.5 GeV neutrino. This is competitive with the best existing results from collider experiments over the same mass range.