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    <link>https://repositorio.ufpb.br/jspui/handle/tede/5435</link>
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        <rdf:li rdf:resource="https://repositorio.ufpb.br/jspui/handle/123456789/38517" />
        <rdf:li rdf:resource="https://repositorio.ufpb.br/jspui/handle/123456789/38432" />
        <rdf:li rdf:resource="https://repositorio.ufpb.br/jspui/handle/123456789/38357" />
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    <dc:date>2026-08-03T13:46:06Z</dc:date>
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  <item rdf:about="https://repositorio.ufpb.br/jspui/handle/123456789/38517">
    <title>Potencial efetivo nas teorias tipo Hořava–Lifshitz</title>
    <link>https://repositorio.ufpb.br/jspui/handle/123456789/38517</link>
    <description>Título: Potencial efetivo nas teorias tipo Hořava–Lifshitz
Autor(es): Lima, André Manzoni de
Orientador: Petrov, Albert
Abstract: In the beggining of the 20th century, Quantum Mechanics and Special Relativity changed radically&#xD;
the basic notions of physics. From the merging of the two theories Quantum Field Theory&#xD;
was born, the basis of the Standard Model of Elementary Particles, which describes three of the&#xD;
four fundamental interactions (electromagnetic and the strong and weak forces). The gravitational&#xD;
interaction is described in a very different setting, namelly the classical General Theory&#xD;
of Relativity, whose formulation is quite distinct from the one used for the other interactions.&#xD;
Initial efforts to place the four interactions into the same conceptual framework were unsuccessful.&#xD;
The reason behind it is that, if treated as a quantum field theory, gravity yields divergent&#xD;
results.&#xD;
Several theories were presented as candidates to put gravity at the same footing as other&#xD;
interactions. One of these theories, proposed by Petr Horava in 2009, consists in enhancing the&#xD;
divergence properties of quantum gravity through the introduction of an anisotropic space-time.&#xD;
As Horava’s proposal changes the notions of space and time essentially, one may ask questions&#xD;
about how the usual quantum field theory models behave under such changes.&#xD;
In this thesis we study two quantum field theory models within the context of Horava-like&#xD;
space-time anisotropy. We calculate the effective potential at one loop order for the scalar QED&#xD;
using two methods. The first, Dirac’s method for constrained systems, does not reffer to any&#xD;
type of gauge choice. In the second method we studied the model with a particular choice of&#xD;
gauge fixing, which led to the appearance of Faddeev-Popov ghosts. We have also studied the&#xD;
Gross-Neveu model, for which we calculated the gap equation, showing the dynamical parity&#xD;
breaking and mass generation under specific circumstances. We calculated the gap equation in&#xD;
the finite temperature case, having found the critical temperature for which the parity breaking&#xD;
occurs. We have also analized the renormalization properties of the theory in the 1=N expasion.&#xD;
Finally, we checked for the possibility of generating the Chern-Simons term for this Gross-&#xD;
Neveu model.
Editor: Universidade Federal da Paraíba
Tipo: Tese</description>
    <dc:date>2018-02-27T00:00:00Z</dc:date>
  </item>
  <item rdf:about="https://repositorio.ufpb.br/jspui/handle/123456789/38432">
    <title>HIgh-energy astroparticle physics as a window into quantum gravity</title>
    <link>https://repositorio.ufpb.br/jspui/handle/123456789/38432</link>
    <description>Título: HIgh-energy astroparticle physics as a window into quantum gravity
Autor(es): Morais, Pedro Henrique
Orientador: Bezerra, Valdir Barbosa
Abstract: The search for quantum gravity signatures in astrophysical observations is one of the central&#xD;
challenges of modern physics. In this thesis, we investigate the phenomenological consequences&#xD;
of scenarios that violate or deform Lorentz symmetries, focusing on extremely high-energy particles&#xD;
produced by cosmic rays and extragalactic sources. We employ a kinematical framework&#xD;
based on Finsler geometry, which enables the description of modified dispersion relations and&#xD;
momentum conservation laws compatible with κ-Poincaré–type symmetries. This approach&#xD;
leads to deformed Lorentz transformations containing terms that are amplified by the particle’s&#xD;
energy, opening the possibility of enhancing Planck-scale effects. The thesis emphasizes two&#xD;
main directions. The first concerns modifications to the lifetimes of relativistic particles, such as&#xD;
muons and pions. Along this line, we show that time dilation receives specific corrections in&#xD;
deformed relativity scenarios, making particle lifetimes a promising observable for experimental&#xD;
tests, whether in muon beam experiments or atmospheric showers. The second direction examines&#xD;
the kinematics of two-body decays, especially π →μ +ν, considering different momentum&#xD;
composition laws compatible with Deformed Special Relativity (DSR). Although the corrections&#xD;
are small, they can affect the relative production of muons and neutrinos in showers initiated&#xD;
by ultra-high-energy cosmic rays, contributing to the ongoing discussion of the muon puzzle.&#xD;
We also investigate the extragalactic and atmospheric propagation of ultra-high-energy photons,&#xD;
whose behavior is sensitive to alterations in the dispersion relation. In Lorentz Invariance Violation&#xD;
(LIV)/DSR scenarios, processes such as pair production may have their thresholds shifted,&#xD;
modifying the transparency horizon of the Universe and potentially altering the development of&#xD;
gamma-ray induced atmospheric showers. The results indicate that extremely high-energy astrophysical&#xD;
messengers—atmospheric muons, neutrinos, and ultra-high-energy photons—provide&#xD;
a privileged laboratory for probing quantum spacetime effects. Thus, this thesis establishes a&#xD;
coherent phenomenological framework linking models of modified relativity with observations&#xD;
in particle astrophysics, highlighting realistic observational avenues for testing quantum gravity&#xD;
hypotheses.
Editor: Universidade Federal da Paraíba
Tipo: Tese</description>
    <dc:date>2026-02-27T00:00:00Z</dc:date>
  </item>
  <item rdf:about="https://repositorio.ufpb.br/jspui/handle/123456789/38357">
    <title>Quantum dynamics beyond lorentz invariance</title>
    <link>https://repositorio.ufpb.br/jspui/handle/123456789/38357</link>
    <description>Título: Quantum dynamics beyond lorentz invariance
Autor(es): Silva, Gislaine Varão da
Orientador: Bezerra, Valdir Barbosa
Abstract: Many approaches to quantum gravity predict the existence of a minimal length associated&#xD;
with the Planck scale, leading to modifications in the relations between energy, momentum,&#xD;
and position, which may in turn affect Lorentz symmetry. In this thesis, we investigate&#xD;
these effects in both systematic and stochastic scenarios, with particular emphasis on&#xD;
their low-energy manifestations. In the first part, we analyze systematic effects derived&#xD;
from modified dispersion relations (MDRs) motivated by quantum gravity. We show that&#xD;
the nonrelativistic limit of general MDRs leads to a deformed nonrelativistic Schrödinger&#xD;
equation containing fractional and nonlocal terms in the Hamiltonian. These terms&#xD;
modify quantum kinematics and allow the establishment of experimental bounds on MDR&#xD;
parameters using low-energy systems. We further demonstrate that certain MDRs with&#xD;
fractional powers give rise to a dynamics described by fractional quantum mechanics at&#xD;
low energies, associated with an effectively fractal geometry in the infrared. We also&#xD;
study stochastic effects associated with Planck-scale fluctuations in MDRs, modeling&#xD;
a stochastic violation of Lorentz symmetry. Performing the stochastic average leads&#xD;
to a Lindblad equation that describes a mechanism of gravitational decoherence in the&#xD;
nonrelativistic regime. We apply this formalism to gravitational Schrödinger cat states&#xD;
(gravcats), revealing the competition between gravitationally induced entanglement and&#xD;
decoherence driven by Planckian fluctuations, and allowing us to estimate the scales&#xD;
at which such effects become relevant. In the second part, we analyze an additional&#xD;
scenario based on noncommutative spacetimes, showing that the deformation of the energy&#xD;
composition rule characteristic of the κ-Minkowski spacetime induces quantum correlations&#xD;
between two systems, even in the nonrelativistic limit. These results demonstrate that&#xD;
low-energy quantum systems provide a novel avenue to test Lorentz symmetry, either&#xD;
through systematic deformations or stochastic violations. The infrared regime has the&#xD;
potential to amplify Planck-suppressed corrections, thereby providing new opportunities&#xD;
to test effective quantum gravity models in tabletop experiments.
Editor: Universidade Federal da Paraíba
Tipo: Tese</description>
    <dc:date>2026-02-23T00:00:00Z</dc:date>
  </item>
  <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>
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