Biaxially symmetric solutions to 4D higher spin gravity

Carlo Iazeolla, Per Sundell

Resultado de la investigación: Review article

14 Citas (Scopus)

Resumen

We review some aspects of biaxially symmetric solutions to Vasiliev's equations in four-dimensional spacetime with a negative cosmological constant. The solutions, which activate bosonic fields of all spins, are constructed using gauge functions, projectors and deformed oscillators. The deformation parameters, which are formally gauge invariant, are related to generalized electric and magnetic charges in asymptotic weak-field regions. Alternatively, the solutions can be characterized in a dual fashion using 0-form charges which are higher spin Casimir invariants built from combinations of curvatures and all their derivatives that are constant on shell and well-defined everywhere.

Idioma originalEnglish
Número de artículo214004
PublicaciónJournal of Physics A: Mathematical and Theoretical
Volumen46
N.º21
DOI
EstadoPublished - 31 may 2013

Huella dactilar

Symmetric Solution
Gages
Gravity
Gravitation
Charge
Gauge Function
gravitation
Invariant
Cosmological Constant
projectors
electric charge
Projector
Well-defined
Shell
Gauge
Space-time
Curvature
curvature
oscillators
Derivatives

ASJC Scopus subject areas

  • Statistical and Nonlinear Physics
  • Statistics and Probability
  • Modelling and Simulation
  • Mathematical Physics
  • Physics and Astronomy(all)

Citar esto

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Biaxially symmetric solutions to 4D higher spin gravity. / Iazeolla, Carlo; Sundell, Per.

En: Journal of Physics A: Mathematical and Theoretical, Vol. 46, N.º 21, 214004, 31.05.2013.

Resultado de la investigación: Review article

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