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dc.contributor.author
Coppola, Máximo  
dc.contributor.author
Gomez Dumm, Daniel Alberto  
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Noguera, S.  
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Scoccola, Norberto Nerio  
dc.date.available
2025-08-05T09:58:33Z  
dc.date.issued
2024-03  
dc.identifier.citation
Coppola, Máximo; Gomez Dumm, Daniel Alberto; Noguera, S.; Scoccola, Norberto Nerio; Masses of magnetized pseudoscalar and vector mesons in an extended NJL model: The role of axial vector mesons; American Physical Society; Physical Review D; 109; 5; 3-2024; 1-30  
dc.identifier.issn
2470-0010  
dc.identifier.uri
http://hdl.handle.net/11336/267938  
dc.description.abstract
We study the mass spectrum of light pseudoscalar and vector mesons in the presence of an external uniform magnetic field B, considering the effects of the mixing with the axial-vector meson sector. The analysis is performed within a two-flavor NJL-like model which includes isoscalar and isovector couplings together with a flavor mixing ’t Hooft-like term. The effect of the magnetic field on charged particles is taken into account by retaining the Schwinger phases carried by quark propagators, and expanding the corresponding meson fields in proper Ritus-like bases. The spin-isospin and spin-flavor decomposition of meson mass states is also analyzed. For neutral pion masses it is shown that the mixing with axial vector mesons improves previous theoretical results, leading to a monotonic decreasing behavior with B that is in good qualitative agreement with lattice QCD (LQCD) calculations, both for the case of constant or B-dependent couplings. Regarding charged pions, it is seen that the mixing softens the enhancement of their mass with B. As a consequence, the energy becomes lower than the one corresponding to a pointlike pion, improving the agreement with LQCD results. The agreement is also improved for the magnetic behavior of the lowest ρ+ energy state, which does not vanish for the considered range of values of B---afact that can be relevant in connection with the occurrence of meson condensation for strong magnetic fields.  
dc.format
application/pdf  
dc.language.iso
eng  
dc.publisher
American Physical Society  
dc.rights
info:eu-repo/semantics/openAccess  
dc.rights.uri
https://creativecommons.org/licenses/by-nc-sa/2.5/ar/  
dc.subject
Quantum chromodynamics  
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Quark models  
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Strong magnetic fields  
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Mesons  
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Física de Partículas y Campos  
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Ciencias Físicas  
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CIENCIAS NATURALES Y EXACTAS  
dc.title
Masses of magnetized pseudoscalar and vector mesons in an extended NJL model: The role of axial vector mesons  
dc.type
info:eu-repo/semantics/article  
dc.type
info:ar-repo/semantics/artículo  
dc.type
info:eu-repo/semantics/publishedVersion  
dc.date.updated
2025-08-01T12:47:32Z  
dc.identifier.eissn
2470-0029  
dc.journal.volume
109  
dc.journal.number
5  
dc.journal.pagination
1-30  
dc.journal.pais
Estados Unidos  
dc.description.fil
Fil: Coppola, Máximo. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina. Comisión Nacional de Energía Atómica. Gerencia del Área de Investigaciones y Aplicaciones no Nucleares. Gerencia de Física (Centro Atómico Constituyentes); Argentina  
dc.description.fil
Fil: Gomez Dumm, Daniel Alberto. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Departamento de Física; Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina  
dc.description.fil
Fil: Noguera, S.. Universidad de Valencia; España  
dc.description.fil
Fil: Scoccola, Norberto Nerio. Comisión Nacional de Energía Atómica. Gerencia del Área de Investigaciones y Aplicaciones no Nucleares. Gerencia de Física (Centro Atómico Constituyentes); Argentina. Consejo Nacional de Investigaciones Científicas y Técnicas; Argentina  
dc.journal.title
Physical Review D  
dc.relation.alternativeid
info:eu-repo/semantics/altIdentifier/url/https://link.aps.org/doi/10.1103/PhysRevD.109.054014  
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info:eu-repo/semantics/altIdentifier/doi/http://dx.doi.org/10.1103/PhysRevD.109.054014