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        <rdf:li rdf:resource="https://repositorio.ufpb.br/jspui/handle/123456789/37676" />
        <rdf:li rdf:resource="https://repositorio.ufpb.br/jspui/handle/123456789/37429" />
        <rdf:li rdf:resource="https://repositorio.ufpb.br/jspui/handle/123456789/37423" />
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    <dc:date>2026-04-22T22:43:52Z</dc:date>
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  <item rdf:about="https://repositorio.ufpb.br/jspui/handle/123456789/37676">
    <title>Influência conjunta da polarização e da coerência da luz no experimento da dupla fenda sob uma perspectiva quântica</title>
    <link>https://repositorio.ufpb.br/jspui/handle/123456789/37676</link>
    <description>Título: Influência conjunta da polarização e da coerência da luz no experimento da dupla fenda sob uma perspectiva quântica
Autor(es): Barbosa, Natália Érika Laurentino
Orientador: Bernardo, Bertúlio de Lima
Abstract: In this research, we studied the wave-particle duality through quantifiers of visibility and&#xD;
distuinguishability by the complementary principle. We used the unified density matrix&#xD;
formalism of coherence and polarization as the basis for this study. If we have information&#xD;
on the path, the interference pattern is destroyed and the photon behaves like a particle,&#xD;
on the other hand, a maximum contrast pattern is verified when there is no information&#xD;
on the path taken, a wave-like behavior. To witness the wave-particle duality using the&#xD;
visibility V and distinguishability D quantifiers derived in the research, we present several&#xD;
physical examples and show that it is possible to verify the behavior of photons, quantified&#xD;
through the principle of complementarity by means of the inequality D2 + V&#xD;
2 ≤ 1.
Editor: Universidade Federal da Paraíba
Tipo: Dissertação</description>
    <dc:date>2020-07-29T00:00:00Z</dc:date>
  </item>
  <item rdf:about="https://repositorio.ufpb.br/jspui/handle/123456789/37429">
    <title>Modelos generalizados de Chern-Pontryagin e uma nova teoria de espinores não-locais</title>
    <link>https://repositorio.ufpb.br/jspui/handle/123456789/37429</link>
    <description>Título: Modelos generalizados de Chern-Pontryagin e uma nova teoria de espinores não-locais
Autor(es): Silva, Ramires Nascimento da
Orientador: Silva, Paulo José Ferreira Porfírio da
Abstract: This thesis discusses modified theories of gravitation, exploring aspects inherent to causality,&#xD;
unitarity, renormalizability, Lorentz invariance and CPT symmetry breaking, with emphasis&#xD;
on the original results extracted from two new categories of models: i) generalized Chern-&#xD;
Pontryagin gravity models; and ii) the non-local spin-1/2 field model, in Minkowski&#xD;
space. In the first case, we formulate a new class of modified gravity models in 4&#xD;
dimensions, whose action is characterized by an arbitrary function of the Ricci scalar&#xD;
and the topological Chern-Pontryagin term ∗RR. Within this framework, we derive the&#xD;
gravitational field equations and solve them for a particular model fI (R, ∗RR) = R+β(∗RR)2&#xD;
and fII(R, ∗RR) = R + αR2 + β(∗RR)2, considering two ansatzes: the slowly rotating&#xD;
Schwarzschild metric and first-order perturbations of Gödel-type metrics. For the former,&#xD;
considering slowly rotating Schwarzschild metric, we find a first-order correction to the&#xD;
frame dragging effect boosted by the parameter L, which characterizes the departures from&#xD;
general relativity results. We show that generalized four-dimensional Chern-Pontryagin&#xD;
models admit a scalar-tensor representation, whose explicit form presents two scalar fields:&#xD;
Φ, a dynamical degree of freedom (scalaron). In contrast, the second, ϕ, is a non-dynamical&#xD;
degree of freedom, which arises coupled with the Chern-Pontryagin topological term ∗RR,&#xD;
that is, ϕ ∗RR, which is nothing more than the gravitational Chern-Simons term. In the&#xD;
latter model, we create a novel nonlocal spin-1/2 field theory in which the form factors&#xD;
depend on the Dirac operator rather than on the d’Alembert operator. At the classical&#xD;
level, we investigate the dispersion relation of free spin-1/2 particles and find that it&#xD;
increasingly deviates from the standard case as the nonlocal effects become relevant. At&#xD;
the quantum level, we compute the fermionic one-loop effective action for the nonlocal&#xD;
spin-1/2 theory with Yukawa coupling and show that the contributions of nonlocal effects&#xD;
are significant in the UV limit. At the same time, in the IR they are suppressed by a UV&#xD;
cutoff scale, which has been chosen to coincide with the nonlocality scale Λ. We minimally&#xD;
couple a U(1) gauge field to the non-local spin-1/2 field theory and explicitly demonstrate&#xD;
that this theory is gauge invariant. Finally, we obtain a nonlocal version of the Pauli&#xD;
equation and the impact of the nonlocality on the gs-factor of massive particles.
Editor: Universidade Federal da Paraíba
Tipo: Tese</description>
    <dc:date>2025-08-29T00:00:00Z</dc:date>
  </item>
  <item rdf:about="https://repositorio.ufpb.br/jspui/handle/123456789/37423">
    <title>Um estudo do desvio da luz no formalismo de campo forte</title>
    <link>https://repositorio.ufpb.br/jspui/handle/123456789/37423</link>
    <description>Título: Um estudo do desvio da luz no formalismo de campo forte
Autor(es): Moreira, Antonio Lucas Araujo
Orientador: Nascimento, José Roberto Soares do
Abstract: In this master thesis, we work out light deflection using the strong field approach and&#xD;
apply the results in the study of gravitational lensing. This formalism becomes useful when&#xD;
the light gets close to a photon sphere, where null geodesics trace circular orbits. In this&#xD;
limit, the impact parameter of the photon approaches the critical impact parameter, and&#xD;
if it is less than that the photon falls into the event horizon. We start assuming a static,&#xD;
spherically symmetric and asymptotically flat metric and then we apply this formalism to&#xD;
the Schwarzschild, Reissner-Nordström and black-bounce metrics. In the strong field limit,&#xD;
the integral for the light deflection diverges, so that we have to extract the divergent term&#xD;
and express the result in terms of some parameters. Ultimately, we define observables&#xD;
in the context of gravitational lensing with the purpose of distinguishing between those&#xD;
metrics from future experimental data.
Editor: Universidade Federal da Paraíba
Tipo: Dissertação</description>
    <dc:date>2023-07-26T00:00:00Z</dc:date>
  </item>
  <item rdf:about="https://repositorio.ufpb.br/jspui/handle/123456789/37183">
    <title>Gravitação Invariante de Weyl: teoria e aplicações</title>
    <link>https://repositorio.ufpb.br/jspui/handle/123456789/37183</link>
    <description>Título: Gravitação Invariante de Weyl: teoria e aplicações
Autor(es): Duarte, Mauro Parnaiba
Orientador: Romero Filho, Carlos Augusto
Abstract: The present thesis is dedicated to the study of the Weyl Invariant Gravitational Theory, a&#xD;
modification and reinterpretation of the original theory proposed by Hermann Weyl. Initially,&#xD;
&#xD;
we present in detail the construction of Weyl’s theory. Next, we develop a gauge-invariant for-&#xD;
mulation for the unified theory of Weyl. This formulation consists of a proposal that renders&#xD;
&#xD;
both the metric tensor and the Weyl field invariant quantities under gauge transformations.&#xD;
With this, it is possible to construct a gauge-invariant proper time definition, in addition to&#xD;
allowing the description of the coupling between geometric fields and matter. In this way,&#xD;
we obtain a new alternative theory of gravitation. An important aspect emphasized in the&#xD;
thesis is that the Weyl geometric 1-form can be formally interpreted as a massive vector&#xD;
field, which refers us to the theory proposed in 1936 by the Romanian physicist Alexandru&#xD;
Proca, who aimed to describe the interaction and dynamics of massive spin-1 bosons. As&#xD;
an application of the field equations of the Weyl invariant theory, we investigate a solution&#xD;
in the weak-field regime. Furthermore, we study in detail the propagation of gravitational&#xD;
waves in this new modified theory of gravity. Finally, we propose an alternative approach to&#xD;
the problem of the origin of dark matter. We show that, for appropriate values of the free&#xD;
parameter of the adopted model, the Weyl field, during the matter-dominated, era, exhibits&#xD;
the expected behavior for a dark matter candidate.
Editor: Universidade Federal da Paraíba
Tipo: Tese</description>
    <dc:date>2025-08-22T00:00:00Z</dc:date>
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