{"id":323,"date":"2025-10-16T20:28:58","date_gmt":"2025-10-16T23:28:58","guid":{"rendered":"https:\/\/www.ccen.ufpb.br\/fisica\/?p=323"},"modified":"2025-10-26T20:49:05","modified_gmt":"2025-10-26T23:49:05","slug":"ii-encontro-paraibano-de-teoria-de-campos","status":"publish","type":"post","link":"https:\/\/www.ccen.ufpb.br\/fisica\/ii-encontro-paraibano-de-teoria-de-campos\/","title":{"rendered":"II Encontro Paraibano de Teoria de Campos"},"content":{"rendered":"<div class=\"wp-block-image\">\n<figure class=\"aligncenter size-full\"><img loading=\"lazy\" decoding=\"async\" width=\"475\" height=\"329\" src=\"https:\/\/www.ccen.ufpb.br\/fisica\/wp-content\/uploads\/sites\/115\/sites\/359\/2025\/10\/Logo-Evento-1.png\" alt=\"\" class=\"wp-image-326\" srcset=\"https:\/\/www.ccen.ufpb.br\/fisica\/wp-content\/uploads\/sites\/115\/sites\/359\/2025\/10\/Logo-Evento-1.png 475w, https:\/\/www.ccen.ufpb.br\/fisica\/wp-content\/uploads\/sites\/115\/sites\/359\/2025\/10\/Logo-Evento-1-300x208.png 300w\" sizes=\"auto, (max-width: 475px) 100vw, 475px\" \/><\/figure>\n<\/div>\n\n\n<p><\/p>\n\n\n\n<p>Nos dias 7 e 8 de novembro de 2025, ser\u00e1 realizado o II Encontro Paraibano de Teoria de Campos, em formato presencial, no Hotel VerdeGreen, em Jo\u00e3o Pessoa.<\/p>\n\n\n\n<p>O evento contar\u00e1 com apresenta\u00e7\u00f5es ministradas por professores da UEPB, UFCG e UFPB, al\u00e9m de pesquisadores de p\u00f3s-doutorado vinculados \u00e0 UFCG e \u00e0 UFPB.<\/p>\n\n\n\n<p>A organiza\u00e7\u00e3o desta edi\u00e7\u00e3o est\u00e1 sob a responsabilidade dos professores Dion\u00edsio Bazeia e Roberto Menezes (coordenador geral), respectivamente dos Departamentos de F\u00edsica e de Ci\u00eancias Exatas.<\/p>\n\n\n\n<p>Com o apoio institucional da Universidade Federal da Para\u00edba (UFPB), do CNPq, da CAPES e da FAPESQ-PB, o encontro tem como principal objetivo fortalecer as a\u00e7\u00f5es e colabora\u00e7\u00f5es entre grupos de pesquisa consolidados na Para\u00edba na \u00e1rea de Teoria de Campos, promovendo o interc\u00e2mbio cient\u00edfico e a integra\u00e7\u00e3o da comunidade acad\u00eamica regional.<\/p>\n\n\n\n<p><\/p>\n\n\n\n<h2 class=\"wp-block-heading\"><div class=\"linha-header\">APRESENTA\u00c7\u00d5ES<\/div><\/h2>\n\n\n\n<blockquote class=\"wp-block-quote is-layout-flow wp-block-quote-is-layout-flow\">\n<p>T\u00edtulos e Resumos<\/p>\n<\/blockquote>\n\n\n\n<p><\/p>\n\n\n\n<p class=\"has-cyan-bluish-gray-background-color has-background\"><strong>Albert Petrov (UFPB)<\/strong><\/p>\n\n\n\n<p><strong><em>Two-Loop corrections to the CFJ Term in a CPT-odd LV Scalar QED<\/em><\/strong><\/p>\n\n\n\n<p class=\" \">In this study, we systematically calculate one-loop corrections to the Lorentz-violating vertices within the framework of CPT-odd Quantum Electrodynamics, encompassing scalar and photon fields in arbitrary gauge. Additionally, we ascertain the finite two-loop corrections to the Carroll-Field-Jackiw term. Furthermore, we analyze the UV divergent component of the two-loop Lorentz-violating correction in the self-energy of the scalar field.<\/p>\n\n\n\n<hr class=\"wp-block-separator has-alpha-channel-opacity\" \/>\n\n\n\n<p><\/p>\n\n\n\n<p class=\"has-cyan-bluish-gray-background-color has-background\"><strong>Danilo Moreira (UEPB)<\/strong><\/p>\n\n\n\n<p><strong><em>Buracos negros de Lifshitz-Born-Infeld efetivos<\/em><\/strong><\/p>\n\n\n\n<p>Neste trabalho apresentamos uma solu\u00e7\u00e3o de buracos negros assintoticamente Lifshitz com Eletrodin\u00e2mica n\u00e3o-linear guiada pela presen\u00e7a de um termo de Born-Infeld. A solu\u00e7\u00e3o tem car\u00e1ter efetivo, emergindo em cen\u00e1rios de viola\u00e7\u00e3o da covari\u00e2ncia geral, e generaliza alguns resultados pr\u00e9vios da Literatura.&nbsp;<\/p>\n\n\n\n<hr class=\"wp-block-separator has-alpha-channel-opacity\" \/>\n\n\n\n<p><\/p>\n\n\n\n<p class=\"has-cyan-bluish-gray-background-color has-background\"><strong>Dionisio Bazeia (UFPB)<\/strong><\/p>\n\n\n\n<p><em><strong>Deformed kinks, vortices, and magnetic&nbsp;monopoles<\/strong><\/em><\/p>\n\n\n\n<p>Defect structures play a significant role in high energy physics, appearing in various contexts. Among the most well-known localized defect configurations are kinks, vortices, and magnetic monopoles which naturally arise in one, two, and three spatial dimensions, respectively. In this talk, I will begin by reviewing some of the key features of kinks, vortices, and monopoles that were developed in the past century. I will then discuss how introducing modifications to the underlying models can lead to novel phenomena, radically altering the defect profiles and incorporating internal deformations of current interest not only in high energy physics but also in other areas of nonlinear science.<\/p>\n\n\n\n<hr class=\"wp-block-separator has-alpha-channel-opacity\" \/>\n\n\n\n<p><\/p>\n\n\n\n<p class=\"has-cyan-bluish-gray-background-color has-background\"><strong>Eduardo Passos (UFCG)<\/strong><\/p>\n\n\n\n<p><strong><em>Lorentz-violating higher derivative gravity<\/em><\/strong><\/p>\n\n\n\n<p>We present a proposal for higher-derivative gravity that violates Lorentz invariance. Through this model, we investigate how LIV affects the equations of motion in the context of the weak gravitational field. The dispersion relation and the Feynman propagator are also analyzed.<\/p>\n\n\n\n<hr class=\"wp-block-separator has-alpha-channel-opacity\" \/>\n\n\n\n<p><\/p>\n\n\n\n<p class=\"has-cyan-bluish-gray-background-color has-background\"><strong>Elias Brito Alves (UFPB)<\/strong><\/p>\n\n\n\n<p><strong><em>Acoplamento n\u00e3o-m\u00ednimo em teorias f(R,T) e f(R,L,T).<\/em><\/strong><\/p>\n\n\n\n<p>A cosmologia passa por um per\u00edodo de crise e algumas perguntas est\u00e3o sem ind\u00edcio de resposta. A teoria da Relatividade Geral parece n\u00e3o dar conta de explicar os fen\u00f4menos como Energia Escura, Mat\u00e9ria Escura e a Tens\u00e3o de Hubble. Diante disso, modifica\u00e7\u00f5es da Relatividade Geral surgem como forma de explicar tais fen\u00f4menos, com destaque para teorias f(R,T) e f(R,L,T).&nbsp; Elas s\u00e3o extens\u00f5es da teoria f(R) e acoplam, de forma n\u00e3o-m\u00ednima, geometria e mat\u00e9ria, gerando novas equa\u00e7\u00f5es de campo que conseguem se ajustar melhor a dados observacionais. A palestra ir\u00e1 mostrar alguns resultados em cosmologia e astrof\u00edsica destas teorias e como elas podem indicar uma dire\u00e7\u00e3o para responder as quest\u00f5es em aberto sobre o universo.<\/p>\n\n\n\n<hr class=\"wp-block-separator has-alpha-channel-opacity\" \/>\n\n\n\n<p><\/p>\n\n\n\n<p class=\"has-cyan-bluish-gray-background-color has-background\"><strong>Francisco Brito (UFCG)<\/strong><\/p>\n\n\n\n<p><strong><em>Some topics in q-deformed systems&nbsp;<\/em><\/strong><\/p>\n\n\n\n<p>In this talk we shall discuss recent applications in systems that are governed by q-deformed algebras.<\/p>\n\n\n\n<hr class=\"wp-block-separator has-alpha-channel-opacity\" \/>\n\n\n\n<p><\/p>\n\n\n\n<p class=\"has-cyan-bluish-gray-background-color has-background\"><strong>Josecl\u00e9cio Dutra Dantas (UFCG)<\/strong><\/p>\n\n\n\n<p><strong><em>Energia escura com contribui\u00e7\u00e3o do tipo cuscuton<\/em><\/strong><\/p>\n\n\n\n<p>Estudamos a din\u00e2mica de uma evolu\u00e7\u00e3o com energia escura introduzindo um termo do tipo cuscuton&nbsp;na lagrangiana do campo escalar.&nbsp; Fazemos uso de um formalismo de primeira ordem que nos permite resolver as equa\u00e7\u00f5es de movimento de maneira anal\u00edtica. Exploramos alguns modelos&nbsp;de maneira a entender como a contribui\u00e7\u00e3o do tipo cuscuton&nbsp;modifica a evolu\u00e7\u00e3o c\u00f3smica.<\/p>\n\n\n\n<hr class=\"wp-block-separator has-alpha-channel-opacity\" \/>\n\n\n\n<p><\/p>\n\n\n\n<p class=\"has-cyan-bluish-gray-background-color has-background\"><strong>Jos\u00e9 Jamilton Rodrigues (UEPB)<\/strong><\/p>\n\n\n\n<p><strong><em>A Tilted Kerr-Newman Black Hole Engine for Fast Radio Bursts<\/em><\/strong><\/p>\n\n\n\n<p>We propose that misaligned, charged, and rotating (Kerr-Newman) black holes constitute a distinct class of progenitors for Fast Radio Bursts (FRBs). In our model, a misalignment between the magnetic and spin axes generates an oscillating dipole that radiates powers of P \u223c&nbsp;1040&nbsp;erg s\u207b\u00b9, accounting for the observed energetics of FRBs. Furthermore, we demonstrate how a coherent synchrotron maser mechanism in the surrounding plasma efficiently up-converts the engine&#8217;s fundamental kilohertz frequency to the observed gigahertz band. This model provides a self-contained explanation for both the power and frequency of FRBs, presenting a robust alternative to conventional magnetar-based theories.<\/p>\n\n\n\n<hr class=\"wp-block-separator has-alpha-channel-opacity\" \/>\n\n\n\n<p><\/p>\n\n\n\n<p class=\"has-cyan-bluish-gray-background-color has-background\"><strong>Jos\u00e9 Grim\u00e1rio de Lima J\u00fanior (UFCG)<\/strong><\/p>\n\n\n\n<p><strong><em>Efeitos T\u00e9rmicos no Termo de CFJ no Modelo de Rarita-Schwinger<\/em><\/strong><\/p>\n\n\n\n<p>Neste trabalho, estudamos o termo de CFJ na teoria de um campo de gauge acoplado a um campo de spin-3\/2, na presen\u00e7a de um vetor axial constante, considerando os efeitos da temperatura a partir do formalismo de tempo imagin\u00e1rio. O objetivo \u00e9 verificar como os efeitos t\u00e9rmicos influenciam as propriedades f\u00edsicas no modelo de Rarita-Schwinger com Viola\u00e7\u00e3o de Lorentz.<\/p>\n\n\n\n<hr class=\"wp-block-separator has-alpha-channel-opacity\" \/>\n\n\n\n<p><\/p>\n\n\n\n<p class=\"has-cyan-bluish-gray-background-color has-background\"><strong>Kl\u00e9cio Lima (UFCG)<\/strong><\/p>\n\n\n\n<p><strong><em>Thermal Casimir Effect in a Neutron Star Spacetime: A Thermo Field Dynamics Approach<\/em><\/strong><\/p>\n\n\n\n<p>This study investigates the thermal Casimir effect in the curved spacetime of a neutron star within the framework of Thermo Field Dynamics (TFD). Starting from the scalar field action coupled to gravity, we derive the renormalized energy\u2013momentum tensor and extend the Stefan\u2013Boltzmann law to include gravitational redshift and curvature corrections through the Tolman\u2013Oppenheimer\u2013Volkoff (TOV) metric. The analysis incorporates both spatial compactification and finite temperature, allowing a unified description of the Casimir energy and pressure inside and outside the star. Analytical expressions are obtained for the high- and low-temperature limits, revealing how strong gravity modifies the thermal and vacuum contributions of quantum fields. The results demonstrate that curvature and redshift significantly alter the local vacuum energy density, offering new insights into the interplay between quantum vacuum phenomena and compact astrophysical objects such as neutron stars.<\/p>\n\n\n\n<hr class=\"wp-block-separator has-alpha-channel-opacity\" \/>\n\n\n\n<p><\/p>\n\n\n\n<p class=\"has-cyan-bluish-gray-background-color has-background\"><strong>Marcos Anacleto (UFCG)<\/strong><\/p>\n\n\n\n<p><strong><em>The self-dual Lorentz violating model: quantization, scattering and dual equivalence<\/em><\/strong><\/p>\n\n\n\n<p>In this work, we analysis the dynamics, at the quantum level, of the self-dual field minimally coupled to bosons with Lorentz symmetry breaking. We quantize the model by applying the Dirac bracket canonical quantization procedure. In addition, we test the relativistic invariance of the model by computing the boson-boson elastic scattering amplitude. Therefore, we show that the Lorentz symmetry breaking has been restored at the quantum level. We finalize our analysis by computing the dual equivalence between the self-dual model with Lorentz symmetry breaking coupled with bosonic matter and the Maxwell-Chern-Simons with Lorentz invariance violation coupled with bosonic field.<\/p>\n\n\n\n<hr class=\"wp-block-separator has-alpha-channel-opacity\" \/>\n\n\n\n<p><\/p>\n\n\n\n<p class=\"has-cyan-bluish-gray-background-color has-background\"><strong>Matheus Le\u00e3o (UFPB)<\/strong><\/p>\n\n\n\n<p><strong><em>Modelos de dois campos reais na presen\u00e7a de impurezas<\/em><\/strong><\/p>\n\n\n\n<p>Esta apresenta\u00e7\u00e3o diz respeito ao trabalho (D. Bazeia, M. A. Liao, and M. A. Marques, Chaos, Solitons &amp; Fractals 192, 115950 (2025)), que trata de sistemas de dois campos escalares reais dopados com impurezas em 1 + 1 dimens\u00f5es. Mostramos que impurezas podem ser introduzidas de modo a preservar parte dos setores BPS de um modelo homog\u00eaneo can\u00f4nico, recuperado quando a impureza tende a zero. Exemplificamos esses resultados com alguns modelos interessantes de potencial qu\u00e1rtico e mostramos que a estrutura interna e comportamento assint\u00f3tico das configura\u00e7\u00f5es de campo podem mudar significativamente. Destacamos ainda outras consequ\u00eancias da dopagem, que incluem a cria\u00e7\u00e3o de novos setores BPS, ao tornar poss\u00edvel a satura\u00e7\u00e3o do v\u00ednculo de Bogomol\u2019nyi sob condi\u00e7\u00f5es de contorno que se mostravam incompat\u00edveis com esse v\u00ednculo na teoria homog\u00eanea.<\/p>\n\n\n\n<hr class=\"wp-block-separator has-alpha-channel-opacity\" \/>\n\n\n\n<p><\/p>\n\n\n\n<p class=\"has-cyan-bluish-gray-background-color has-background\"><strong>Matheus Marques (UFPB)<\/strong><\/p>\n\n\n\n<p><strong><em>First-order framework for scalar field models with impurities<\/em><\/strong><\/p>\n\n\n\n<p>In this talk, we present a first-order framework for impurity-doped scalar field models. The method relies on the introduction of a tensor that can be forced to have null divergence under specific conditions. In the static case, we consider the inclusion of an auxiliary vector function whose divergence gives the energy density of the system. Aspects of stability are also discussed.<\/p>\n\n\n\n<hr class=\"wp-block-separator has-alpha-channel-opacity\" \/>\n\n\n\n<p><\/p>\n\n\n\n<p class=\"has-cyan-bluish-gray-background-color has-background\"><strong>Matheus Paganelly (UFPB)<\/strong><\/p>\n\n\n\n<p><strong><em>V\u00f3rtices Globais no cen\u00e1rio de viola\u00e7\u00e3o da simetria de Lorentz<\/em><\/strong><\/p>\n\n\n\n<p>Essa&nbsp;apresenta\u00e7\u00e3o ilustra os estudos da influ\u00eancia da viola\u00e7\u00e3o da simetria de Lorentz em estruturas globais bidimensionais. \u00c9&nbsp;demonstrado que estruturas neutras n\u00e3o s\u00e3o afetadas em tal cen\u00e1rio. Por outro lado, \u00e9 observado um comportamento n\u00e3o usual para o campo el\u00e9trico de&nbsp;estruturas carregadas&nbsp;e para uma extens\u00e3o do tipo Born-Infeld.<\/p>\n\n\n\n<hr class=\"wp-block-separator has-alpha-channel-opacity\" \/>\n\n\n\n<p><\/p>\n\n\n\n<p class=\"has-cyan-bluish-gray-background-color has-background\"><strong>Paulo Porf\u00edrio (UFPB)<\/strong><\/p>\n\n\n\n<p><em>U<strong>ma nova teoria de campos n\u00e3o local para f\u00e9rmions de spin 1\/2<\/strong><\/em><\/p>\n\n\n\n<p>Propomos uma nova teoria n\u00e3o local para f\u00e9rmions de spin 1\/2 na qual o fator de forma depende do operador de Dirac, em vez do operador de d\u2019Alembert. Nesse cen\u00e1rio, exploramos alguns aspectos cl\u00e1ssicos e qu\u00e2nticos dessa nova teoria. No regime cl\u00e1ssico, investigamos a rela\u00e7\u00e3o de dispers\u00e3o de part\u00edculas livres de spin 1\/2 e constatamos que ela se desvia progressivamente do caso padr\u00e3o \u00e0 medida que os efeitos n\u00e3o locais se tornam relevantes. No regime qu\u00e2ntico, calculamos a a\u00e7\u00e3o efetiva fermi\u00f3nica de um la\u00e7o para a teoria n\u00e3o local de spin 1\/2 com acoplamento de Yukawa e mostramos que as contribui\u00e7\u00f5es dos efeitos n\u00e3o locais s\u00e3o significativas no limite ultravioleta (UV), enquanto no infravermelho (IR) elas s\u00e3o suprimidas por uma escala de corte UV, escolhida para coincidir com a escala de n\u00e3o localidade. Acoplamos minimamente um campo de calibre U(1) \u00e0 teoria de f\u00e9rmions n\u00e3o local e demonstramos explicitamente que essa teoria \u00e9 invariante de calibre. Por fim, obtemos uma vers\u00e3o n\u00e3o local da equa\u00e7\u00e3o de Pauli e avaliamos o impacto da n\u00e3o localidade no fator g de part\u00edculas massivas.<\/p>\n\n\n\n<hr class=\"wp-block-separator has-alpha-channel-opacity\" \/>\n\n\n\n<p><\/p>\n\n\n\n<p class=\"has-cyan-bluish-gray-background-color has-background\"><strong>Ramires Nascimento da Silva (UFCG)<\/strong><\/p>\n\n\n\n<p><strong><em>Extens\u00f5es Topol\u00f3gicas em Teorias Modificadas da Gravita\u00e7\u00e3o<\/em><\/strong><\/p>\n\n\n\n<p>Nos \u00faltimos anos, os modelos estendidos da gravita\u00e7\u00e3o, formulados por meio da introdu\u00e7\u00e3o de termos invariantes topol\u00f3gicos, t\u00eam despertado crescente interesse, especialmente por oferecerem alternativas \u00e0 Relatividade Geral na descri\u00e7\u00e3o de fen\u00f4menos cosmol\u00f3gicos, astrof\u00edsicos e na f\u00edsica de altas energias. Nesse contexto, destacam-se os modelos de Chern\u2013Simons e os modelos generalizados de Chern\u2013Pontryagin, que, al\u00e9m de compartilharem determinadas solu\u00e7\u00f5es com a Relatividade Geral, podem \u2014 sob condi\u00e7\u00f5es espec\u00edficas \u2014 induzir a quebra expl\u00edcita das simetrias de Lorentz e CPT. Neste trabalho, apresentamos resultados relevantes associados a tais modelos, com \u00eanfase na an\u00e1lise da consist\u00eancia das solu\u00e7\u00f5es de buracos negros com rota\u00e7\u00e3o lenta e na investiga\u00e7\u00e3o de perturba\u00e7\u00f5es de primeira ordem em m\u00e9tricas tipo-G\u00f6del homog\u00eaneas, para dois prot\u00f3tipos espec\u00edficos.<\/p>\n\n\n\n<hr class=\"wp-block-separator has-alpha-channel-opacity\" \/>\n\n\n\n<p><\/p>\n\n\n\n<p class=\"has-cyan-bluish-gray-background-color has-background\"><strong>Roberto Menezes (UFPB)<\/strong><\/p>\n\n\n\n<p><strong><em>O Modelo BNRT<\/em><\/strong><\/p>\n\n\n\n<p>Nesta apresenta\u00e7\u00e3o falarei do modelo BNRT, sua origem e suas aplica\u00e7\u00f5es ao longo das d\u00e9cadas.&nbsp; &nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Nos dias 7 e 8 de novembro de 2025, ser\u00e1 realizado o II Encontro Paraibano [&hellip;]<\/p>\n","protected":false},"author":401,"featured_media":326,"comment_status":"closed","ping_status":"","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[10],"tags":[],"class_list":["post-323","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-eventos"],"_links":{"self":[{"href":"https:\/\/www.ccen.ufpb.br\/fisica\/wp-json\/wp\/v2\/posts\/323","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.ccen.ufpb.br\/fisica\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.ccen.ufpb.br\/fisica\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.ccen.ufpb.br\/fisica\/wp-json\/wp\/v2\/users\/401"}],"replies":[{"embeddable":true,"href":"https:\/\/www.ccen.ufpb.br\/fisica\/wp-json\/wp\/v2\/comments?post=323"}],"version-history":[{"count":12,"href":"https:\/\/www.ccen.ufpb.br\/fisica\/wp-json\/wp\/v2\/posts\/323\/revisions"}],"predecessor-version":[{"id":338,"href":"https:\/\/www.ccen.ufpb.br\/fisica\/wp-json\/wp\/v2\/posts\/323\/revisions\/338"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.ccen.ufpb.br\/fisica\/wp-json\/wp\/v2\/media\/326"}],"wp:attachment":[{"href":"https:\/\/www.ccen.ufpb.br\/fisica\/wp-json\/wp\/v2\/media?parent=323"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.ccen.ufpb.br\/fisica\/wp-json\/wp\/v2\/categories?post=323"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.ccen.ufpb.br\/fisica\/wp-json\/wp\/v2\/tags?post=323"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}