### 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 original | English |
---|---|

Número de artículo | 214004 |

Publicación | Journal of Physics A: Mathematical and Theoretical |

Volumen | 46 |

N.º | 21 |

DOI | |

Estado | Published - 31 may 2013 |

### Huella dactilar

### ASJC Scopus subject areas

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

### Citar esto

*Journal of Physics A: Mathematical and Theoretical*,

*46*(21), [214004]. https://doi.org/10.1088/1751-8113/46/21/214004

}

*Journal of Physics A: Mathematical and Theoretical*, vol. 46, n.º 21, 214004. https://doi.org/10.1088/1751-8113/46/21/214004

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

Resultado de la investigación: Review article

TY - JOUR

T1 - Biaxially symmetric solutions to 4D higher spin gravity

AU - Iazeolla, Carlo

AU - Sundell, Per

PY - 2013/5/31

Y1 - 2013/5/31

N2 - 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.

AB - 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.

UR - http://www.scopus.com/inward/record.url?scp=84878132191&partnerID=8YFLogxK

U2 - 10.1088/1751-8113/46/21/214004

DO - 10.1088/1751-8113/46/21/214004

M3 - Review article

AN - SCOPUS:84878132191

VL - 46

JO - Journal of Physics A: Mathematical and Theoretical

JF - Journal of Physics A: Mathematical and Theoretical

SN - 1751-8113

IS - 21

M1 - 214004

ER -