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    <link>https://repositorio.ufpb.br/jspui/handle/123456789/4</link>
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    <pubDate>Mon, 06 Apr 2026 12:07:06 GMT</pubDate>
    <dc:date>2026-04-06T12:07:06Z</dc:date>
    <item>
      <title>Gravidade quântica a baixas energias: correções fenomenológicas da mecânica quântica</title>
      <link>https://repositorio.ufpb.br/jspui/handle/123456789/37882</link>
      <description>Título: Gravidade quântica a baixas energias: correções fenomenológicas da mecânica quântica
Autor(es): Sampaio, Kelvin Costa Rocha
Orientador: Lobo, Iarley Pereira
Abstract: This study aims to explore how quantum systems and decoherence characteristics impact&#xD;
the field of quantum gravity, highlighting the importance of phenomenological models&#xD;
that bridge microscopic-scale effects with observable observations. The research includes&#xD;
a review of the theoretical principles of quantum mechanics and relativity, emphasizing&#xD;
suggestions for systematic and stochastic modifications in kinematics inspired by quantum&#xD;
gravity scenarios. Furthermore, the observational consequences and limitations of the&#xD;
models in question are highlighted, connecting the formulated theory to possible effects&#xD;
that can be detected at accessible energies. The findings suggest that, although quantum&#xD;
gravity remains an open challenge, phenomenological analyses may offer interesting clues&#xD;
for future investigations and experiments.
Editor: Universidade Federal da Paraíba
Tipo: TCC</description>
      <pubDate>Fri, 03 Oct 2025 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">https://repositorio.ufpb.br/jspui/handle/123456789/37882</guid>
      <dc:date>2025-10-03T00:00:00Z</dc:date>
    </item>
    <item>
      <title>Um estudo da eletrodinâmica acoplada a férmions e alguns aspectos da mecânica quântica relativística</title>
      <link>https://repositorio.ufpb.br/jspui/handle/123456789/34796</link>
      <description>Título: Um estudo da eletrodinâmica acoplada a férmions e alguns aspectos da mecânica quântica relativística
Autor(es): Guinote, Bárbara Vitória Silva
Orientador: Porfírio, Paulo José Ferreira da Silva
Abstract: This work seeks to explore the foundations of Classical and Quantum Field Theory,&#xD;
establishing a bridge between Classical Mechanics and modern concepts such as symmetry&#xD;
and gauge invariance. It begins by developing the variational and tensorial formalism&#xD;
required to understand the transition from classical physics to field formulations. Then,&#xD;
electromagnetism is examined from the perspective of a gauge theory, with emphasis&#xD;
on the covariance of Maxwell’s equations and the distinction between global and local&#xD;
symmetries. The study also addresses the gauge principle and its role in quantum mechanics.&#xD;
Finally, relativistic quantum mechanics is introduced through the Klein-Gordon and Dirac&#xD;
equations, discussing their solutions, probability currents, and the famous Dirac Sea&#xD;
interpretation. This study aims to provide a solid conceptual and mathematical foundation&#xD;
for understanding the fundamental theories governing physical interactions in various&#xD;
regimes.
Editor: Universidade Federal da Paraíba
Tipo: TCC</description>
      <pubDate>Mon, 05 May 2025 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">https://repositorio.ufpb.br/jspui/handle/123456789/34796</guid>
      <dc:date>2025-05-05T00:00:00Z</dc:date>
    </item>
    <item>
      <title>Um estudo das soluções de buracos negros na relatividade geral</title>
      <link>https://repositorio.ufpb.br/jspui/handle/123456789/34469</link>
      <description>Título: Um estudo das soluções de buracos negros na relatividade geral
Autor(es): Nascimento, Tarcila Ferreira Domingues do
Orientador: Silva, Paulo José Ferreira Porfírio da
Abstract: In this work, we investigate some of the exact solutions for black holes in the context of&#xD;
general relativity, focusing on the Schwarzschild and Reissner-Nordström metrics. Based&#xD;
on the foundations of special relativity, differential geometry, and general relativity, the&#xD;
necessary mathematical framework was developed to analyze these solutions. For the&#xD;
Schwarzschild case, the spacetime structure, the singularity at r = 0, and the event horizon&#xD;
at r = 2GM were examined. The Reissner-Nordström solution was analyzed, revealing&#xD;
the existence of two horizons (r±) and discussing the physical implications of the electric&#xD;
charge Q. The results demonstrate how these theoretical solutions are now supported by&#xD;
observational evidence through modern techniques, such as the first image of a black hole&#xD;
captured by the Event Horizon Telescope.
Editor: Universidade Federal da Paraíba
Tipo: TCC</description>
      <pubDate>Fri, 25 Apr 2025 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">https://repositorio.ufpb.br/jspui/handle/123456789/34469</guid>
      <dc:date>2025-04-25T00:00:00Z</dc:date>
    </item>
    <item>
      <title>Método de aplicação de Redes Neurais Convolucionárias (CNN) para identificação de fusões de galáxias em dados simulados pelo Projeto Illustris</title>
      <link>https://repositorio.ufpb.br/jspui/handle/123456789/33239</link>
      <description>Título: Método de aplicação de Redes Neurais Convolucionárias (CNN) para identificação de fusões de galáxias em dados simulados pelo Projeto Illustris
Autor(es): Almeida, Natali Cristina Moreira de
Orientador: Cavalcante, Hugo Leonardo Davi de Souza
Abstract: Since its origin, the universe has been in constant evolution, which includes the formation&#xD;
and destruction of black holes, galaxies, stars, and other cosmological structures. Observing&#xD;
this evolution allows us to understand, discover, and test models and theories related to the&#xD;
foundations of physics, such as the Big Bang, relativity, the existence of dark matter and dark&#xD;
energy, etc. In addition to experimental observation, theoretical models can be tested in computer&#xD;
simulations, in which theoretical variables can be directly controlled and time accelerated or&#xD;
reversed, allowing analyses that are impossible to perform on real scales. Recent models,&#xD;
however, produce a vast amount of data, which makes their manual analysis difficult. The&#xD;
same is true for the vast amount of images acquired by the Hubble Space Telescope (HST) and&#xD;
James Webb Space Telescope (JWST). To facilitate this analysis, we demonstrate here the use&#xD;
of convolutional neural networks (CNNs) to identify galaxy mergers in data simulated by the&#xD;
Illustris project. We successfully reproduced some results from the literature, improving the&#xD;
hyperparameters of the neural network to allow faster and more reliable convergence. Data&#xD;
collection was performed on open-access platforms, GitHub, and the Space Telescope Science&#xD;
Institute (STSI). The source code developed is also made available to the community so that&#xD;
it can be used in this and other problems and improved. We hope to contribute to the use of&#xD;
neural networks and artificial intelligence not only in astrophysics but also in other problems&#xD;
that require image classification and that have a large database.
Editor: Universidade Federal da Paraíba
Tipo: TCC</description>
      <pubDate>Fri, 25 Oct 2024 00:00:00 GMT</pubDate>
      <guid isPermaLink="false">https://repositorio.ufpb.br/jspui/handle/123456789/33239</guid>
      <dc:date>2024-10-25T00:00:00Z</dc:date>
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