Extraction of CP Properties of the H(125) Boson Discovered in Proton-Proton Collisions at sqrt(s) = 7 and 8 TeV with the CMS Detector at the LHC

In this thesis we build a novel analysis framework to perform the direct extraction of all possible effective Higgs boson couplings to the neutral electroweak gauge bosons in the H → ZZ^(*) → 4l channel also referred to as the golden channel. We use analytic expressions of the full decay differential cross sections for the H → VV' → 4l process, and the dominant irreducible standard model qq ̄ → 4l background where 4l = 2e2μ,4e,4μ. Detector effects are included through an explicit convolution of these analytic expressions with transfer functions that model the detector responses as well as acceptance and efficiency effects. Using the full set of decay observables, we construct an unbinned 8-dimensional detector level likelihood function which is con- tinuous in the effective couplings, and includes systematics. All potential anomalous couplings of HVV' where V = Z,γ are considered, allowing for general CP even/odd admixtures and any possible phases. We measure the CP-odd mixing between the tree-level HZZ coupling and higher order CP-odd couplings to be compatible with zero, and in the range [−0.40, 0.43], and the mixing between HZZ tree-level coupling and higher order CP -even coupling to be in the ranges [−0.66, −0.57] ∪ [−0.15, 1.00]; namely compatible with a standard model Higgs. We discuss the expected precision in determining the various HVV' couplings in future LHC runs. A powerful and at first glance surprising prediction of the analysis is that with 100-400 fb^-1, the golden channel will be able to start probing the couplings of the Higgs boson to diphotons in the 4l channel. We discuss the implications and further optimization of the methods for the next LHC runs.

Caracterização físico-química e avaliação dos níveis de elementos-traço em sedimentos de manguezais das baías da Ilha Grande e de Sepetiba, RJ, por metodologias de digestão ácida assistidas por micro-ondas

O presente trabalho teve como objetivo principal comparar dois métodos de extração de elementos-traço em sedimentos que são assistidos por radiação micro-ondas. Foram coletadas amostras de sedimentos superficiais em um manguezal localizado na baía da Ilha Grande e em três manguezais localizados na baía de Sepetiba, RJ. As amostras de sedimentos coletadas foram secas, destorroadas e peneiradas. Sub-amostras foram submetidas a análises de caracterização física e química. Os métodos de extração de elementos-traço comparados foram o EPA-3051A e o método água régia assistido por micro-ondas. Os elementos-traço analisados foram: Cd, Cr, Cu, Ni, Pb e Zn. As concentrações dos elementos-traço nos extratos produzidos foram determinadas por FAAS (Espectrometria de absorção atômica com chama). Foram encontradas nos sedimentos dos manguezais estudados concentrações acima dos níveis estabelecidos pela Resolução CONAMA 344/2004 para os elementos-traço: Cd, Ni, Pb e Zn. Os resultados mostraram que as capacidades de extração de elementos-traço dos métodos EPA-3051A e água régia assistido por micro-ondas variam em função das características físico-químicas dos sedimentos. A análise estatística pela técnica de regressão linear simples mostrou que as duas metodologias são estatisticamente similares apenas para o Cr e os valores dos coeficientes de determinação (R2) obtidos obedeceram à seqüência: Cu > Pb > Zn > Ni > Cr > Cd. Na análise pela técnica estatística de regressão linear múltipla ocorreram melhorias estatisticamente significativas nos coeficientes de determinação quando foram incluídas as seguintes variáveis independentes: potencial redox e fósforo total para o Cd, argila para o Cr, areia para o Ni e fósforo total para o Pb e para o Zn

Gauge Invariant Spectral Cauchy Characteristic Extraction of Gravitational Waves in Computational General Relativity

We present a complete system for Spectral Cauchy characteristic extraction (Spectral CCE). Implemented in C++ within the Spectral Einstein Code (SpEC), the method employs numerous innovative algorithms to efficiently calculate the Bondi strain, news, and flux.

Spectral CCE was envisioned to ensure physically accurate gravitational wave-forms computed for the Laser Interferometer Gravitational wave Observatory (LIGO) and similar experiments, while working toward a template bank with more than a thousand waveforms to span the binary black hole (BBH) problem’s seven-dimensional parameter space.

The Bondi strain, news, and flux are physical quantities central to efforts to understand and detect astrophysical gravitational wave sources within the Simulations of eXtreme Spacetime (SXS) collaboration, with the ultimate aim of providing the first strong field probe of the Einstein field equation.

In a series of included papers, we demonstrate stability, convergence, and gauge invariance. We also demonstrate agreement between Spectral CCE and the legacy Pitt null code, while achieving a factor of 200 improvement in computational efficiency.

Spectral CCE represents a significant computational advance. It is the foundation upon which further capability will be built, specifically enabling the complete calculation of junk-free, gauge-free, and physically valid waveform data on the fly within SpEC.