Non Relativistic Limit
Mostrando 1-10 de 10 artigos, teses e dissertações.
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1. Effects of spontaneous symmetry breaking-CPT and Lorentz invariance of the phenomenon the Bose-Einstein / Efeitos da quebra espontânea da simetria-CPT e da invariância de Lorentz no fenômeno da condensação de Bose-Einstein
The Bose-Einstein condensate (BEC), also known as the fifth state of the matter, was predicted theoretically by Albert Einstein in 1925 and verified experimentally 70 years later in 1995. This dissertation addresses the effects of spontaneous broken of the CPT-symmetry and of the invariance Lorentz (also called simply the violation of Lorentz symmetry) in th
Publicado em: 2011
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2. Decaimentos de mésons D e DSJ no modelo C3P0
The Fock-Tani representation is a field theory formalism appropriated for the simultaneous treatment of composite particles and their constituents. The 3P0 model is a typical decay model which considers only OZI-allowed strong decays. The model considers a quark-antiquark pair created with the vacuum quantum numbers in the presence of the initial state meson
IBICT - Instituto Brasileiro de Informação em Ciência e Tecnologia. Publicado em: 2011
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3. Oscilador de Dirac: ImplicaÃÃes da violaÃÃo da simetria de Lorentz e da massa dependente da posiÃÃo.
In this work we study the Dirac Oscillator (DO) in a threefold way. In the first way, we study DO with Lorentz symmetry violation. This violation is implemented through vectorial and an axial terms. We realize a non-relativistic limit and we obtain that the background vector field does not modify the energy spectrum. However, in the case of the background ax
IBICT - Instituto Brasileiro de Informação em Ciência e Tecnologia. Publicado em: 16/07/2008
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4. Cosmologia na teoria de Visser / Cosmology from the Visser s theory
The advent of observational cosmology has led us to conclude that only 4% of whole Universe is composed by known matter (baryons). On the other hand 23% comes from a kind of non barionic dark matter. Moreover the cosmic dynamics is almost fully dominated by the so called dark energy (usually considered a kind of fluid), which corresponds to 73% of the energy
IBICT - Instituto Brasileiro de Informação em Ciência e Tecnologia. Publicado em: 30/08/2006
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5. Cosmologia na teoria de Visser / Cosmology from the Visser s theory
The advent of observational cosmology has led us to conclude that only 4% of whole Universe is composed by known matter (baryons). On the other hand 23% comes from a kind of non barionic dark matter. Moreover the cosmic dynamics is almost fully dominated by the so called dark energy (usually considered a kind of fluid), which corresponds to 73% of the energy
Publicado em: 2006
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6. INFLUÊNCIA DA VIOLAÇÃO DA SIMETRIA DE LORENTZ SOBRE A EQUAÇÃO DE DIRAC E O ESPECTRO DE HIDROGÊNIO / INFLUENCE OF THE BREACH OF LORENTZ SYMMETRY ABOUT EQUATION OF DIRAC AND THE SPECTRUM OF HYDROGEN
Neste trabalho, busca-se investigar a influência de termos violadores de Lorentz e CPT (em acoplamentos "vetoriais"e "axiais") sobre a equação de Dirac, e seu limite não-relativistico. Primeiramente, são obtidas as suas soluções de onda-plana, relação de dispersão e autovalores. Em seguida, o limite de baixas energias é trabalhado e o Hamiltoniano
Publicado em: 2006
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7. Physics of deformed special relativity: relativity principle revisited
In many different ways, Deformed Special Relativity (DSR) has been argued to provide an effective limit of quantum gravity in almost-flat regime. Unfortunately, DSR is up to now plagued by many conceptual problems (in particular how it describes macroscopic objects) which forbids a definitive physical interpretation and clear predictions. Here we propose a c
Brazilian Journal of Physics. Publicado em: 2005-06
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8. Non Relativistic Limit in QFT: a Wilson Renormalization Group Approach in the Minkowski Space
We study the non relativistic limit of a model of fermions interacting through a Chern-Simons field, from a perspective that resembles the Wilson Renormalization Group (WRG) approach. The main difference of our approach to WRG is that instead of working in the Euclidean space, we directly work in Minkowski space. For the nonrelativistic limit this procedure
Brazilian Journal of Physics. Publicado em: 2001-06
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9. On the non-relativistic Casimir effect
We compute the Casimir energy for a massive scalar field constrained between two parallel planes (Dirichlet boundary conditions) in order to investigate its non-relativistic limit. Instead of employing the usual relativistic dispersion relation omega(p) = , we use the non-relativistic one, omega(p) = p²/2m. It
Brazilian Journal of Physics. Publicado em: 2001-03
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10. Influencia do campo de radiação no processo de interferencia eletronica
We develop a non-relativistic quantum formulation for the dynamics of na electron taking into account the effects of the coupling to its own radiation field, which give rise to radiation damping. For this purpose we have applied the Feynman-Vernon approach, obtaining the reduced density operation of the electron via path integrals. In the classical limit, so
Publicado em: 1989