skip to main content

Vanishing Poynting Observers and Electromagnetic Field Classification in Kerr and Kerr-Newman Spacetimes

Vargas–Rodríguez, H. ; Rosu, H. C. ; Medina–Guevara, M. G. ; Gallegos, A. ; Muñiz–Torres, M. A. Shamir, Muhammad Farasat ; Muhammad Farasat Shamir

Advances in High Energy Physics, 2022-06, Vol.2022, p.1-17 [Revista revisada por pares]

New York: Hindawi

Texto completo disponible

Citas Citado por
  • Título:
    Vanishing Poynting Observers and Electromagnetic Field Classification in Kerr and Kerr-Newman Spacetimes
  • Autor: Vargas–Rodríguez, H. ; Rosu, H. C. ; Medina–Guevara, M. G. ; Gallegos, A. ; Muñiz–Torres, M. A.
  • Shamir, Muhammad Farasat ; Muhammad Farasat Shamir
  • Materias: Accretion disks ; Analysis ; Angular momentum ; Astrophysics ; Classification ; Decomposition ; Electric fields ; Electromagnetic fields ; Electromagnetism ; Light ; Light speed ; Magnetic fields ; Observers ; Relativity ; Spacetime ; Velocity ; Velocity distribution
  • Es parte de: Advances in High Energy Physics, 2022-06, Vol.2022, p.1-17
  • Descripción: We consider electromagnetic fields having an angular momentum density in a locally nonrotating reference frame in Schwarzschild, Kerr, and Kerr-Newman spacetimes. The nature of such fields is assessed with two families of observers, the locally nonrotating ones and those of vanishing Poynting flux. The velocity fields of the vanishing-Poynting observers in the locally nonrotating reference frames are determined using the 3+1 decomposition formalism. From a methodological point of view and considering a classification of the electromagnetic field based on its invariants, it is convenient to separate the consideration of the vanishing-Poynting observers into two cases corresponding to the pure and nonpure fields; additionally, if there are regions where the field rotates with the speed of light (light surfaces), it becomes necessary to split these observers into two subfamilies. We present several examples of relevance in astrophysics and general relativity, such as pure rotating dipolar-like magnetic fields and the electromagnetic field of the Kerr-Newman solution. For the latter example, we see that vanishing-Poynting observers also measure a vanishing super-Poynting vector, confirming recent results in the literature. Finally, for all nonnull electromagnetic fields, we present the 4-velocity fields of vanishing Poynting observers in an arbitrary spacetime.
  • Editor: New York: Hindawi
  • Idioma: Inglés

Buscando en bases de datos remotas, por favor espere

  • Buscando por
  • enscope:(USP_VIDEOS),scope:("PRIMO"),scope:(USP_FISICO),scope:(USP_EREVISTAS),scope:(USP),scope:(USP_EBOOKS),scope:(USP_PRODUCAO),primo_central_multiple_fe
  • Mostrar lo que tiene hasta ahora