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  • About
  • The Global ETD Search service is a free service for researchers to find electronic theses and dissertations. This service is provided by the Networked Digital Library of Theses and Dissertations.
    Our metadata is collected from universities around the world. If you manage a university/consortium/country archive and want to be added, details can be found on the NDLTD website.
1

RPA relativística para ressonâncias gigantes isovetoriais /

Socolowski Jr., O, (Otávio) January 1994 (has links)
Orientador: Alfredo Pio Noronha Rodrigues Galeão / Banca: Diógenes Galetti / Banca: Brett V. Carlson / Resumo: Utilizamos o modelo hidrodinâmico de emissão contínua de partículas para estudar vários dados experimentais do SPS/CERN. Dados sobre razões de partículas estranhas das colaborações WA85 e WA97 são usados para determinar um conjunto de condições iniciais para o fluxo hidrodinâmico. Testamos a autoconsistência do modelo estudando outros dados experimentais com as mesmas condições iniciais que reproduziram as razões de partículas estranhas. Mostramos que os espectros em massa transversal de NA35, WA85, NA49 e WA97 podem ser bem reproduzidas. A grande vantagem dessa abordagem (além de ser corroborada pelos modelos microscópicos) é que ela pode resolver, de um modo natural, alguns dos problemas enfrentados pelo modelo usual de freeze-out: possíveis altas densidades de partículas, pequena abundância de píons e temperatura incorreta do 'ômega' / Abstract: We use the hydrodynamical model of continuous particle emission to study several ex- perimental data from SPS/CERN. Data on strange particle ratios from WA85 and WA97 Collaborations are used to determine a set of initial conditions for the hydrodynamical flow. We test the self-consistency of the model by studying several other experimental data by using the same initial conditions that reproduce strange particle ratios. We show that the transverse mass spectra from WA35, WA85, NA49 and WA97 can be well repro- duced. We also reproduce particle abundances, including the tt one. The big advantage of this approach (in addition to being corroborated by microscopical models) is that it may solve, in a natural way, some of the problems met by the standard hydrodynamical approach with sudden freeze-out: possible too high densities, too small pion abundance and wrong 'ômega' temperature / Mestre

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