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Simulación de respuesta electromagnética de yacimientos de sulfuros y su relación con posibles emisiones radiométricas
(2018-04-20)
En este documento se consignan los aspectos teóricos, analíticos y procedimentales que dan lugar a simulaciones de respuestas electromagnéticas de distintos modelos de yacimientos de sulfuros, mediante algoritmos de solución ...
Propiedades electromagnéticas del quark top y cambio de sabor
(Universidad Michoacana de San Nicolás de Hidalgo, 2015-03)
It is presented the analytical study for the fifiγ vertex in the context of models that predict flavor-changing neutral currents, which are mediated by a new neutral massive gauge boson, known as Z’. The analysis focuses ...
Scalar quasinormal modes of nonlinear charged black holes in Rastall gravity
(Iop Publishing Ltd, 2019-12-01)
In this paper, the scalar quasinormal modes of nonlinear charged black hole metrics in Rastall gravity is investigated. The electromagnetic tensor presented in the background spacetime possesses a power-law form, and the ...
The action for the (propagating) torsion and the limits on the torsion parameters from present experimental data
(1998-04-23)
Starting from the well established form of the Dirac action coupled to the electromagnetic and torsion field we find that there is some additional softly broken local symmetry associated with torsion. This symmetry fixes ...
The action for the (propagating) torsion and the limits on the torsion parameters from present experimental data
(1998-04-23)
Starting from the well established form of the Dirac action coupled to the electromagnetic and torsion field we find that there is some additional softly broken local symmetry associated with torsion. This symmetry fixes ...
Modeling the bow-shock of Ophiuchi
(Livraria da Física, 2013)
Runaway masive stars are O- and B-type stars with large peculiar veloci- ties. Runaway OB stars can produce stellar bowshocks in the surrounding interstellar medium. Bowshocks develop as arc-shaped structures while the ...
A dualidade Maxwell-Proca-Chern-Simons via Formalismo Simplético de Imersão
(Universidade Federal de Juiz de Fora (UFJF)BrasilICE – Instituto de Ciências ExatasPrograma de Pós-graduação em FísicaUFJF, 2017)
Radiación no térmica asociada a estrellas de gran masa
(2018-11-20)
Uno de los principales desafíos de la astrofísica de altas energías es entender las conexiones que subyacen entre los rayos cósmicos y la radiación no térmica (NT), en particular, en la banda de los rayos γ. Hay extensa ...