General Backgrounds for higher spin massive particles
arXiv:1711.11535
Abstract
We consider the propagation of totally symmetric bosonic fields on generic background spacetimes. The mutual compatibility of the dynamical equations and constraints severely constrains the set of geometries where consistent propagation is possible. To enlarge this set in this article we allow several background fields to be turned on. We were able to show that massive fields of spin s greater than or equal to three may consistently propagate in a large set of non-trivial spacetimes, such as asymptotically de-Sitter, flat and anti-de-Sitter black holes geometries, as long as certain conditions between the various background fields are met. For the special case of massive spin-2 fields the set of allowed spacetimes is larger and includes domain-wall-type geometries, such as the Freedman-Robertson-Walker metric. We comment on the assumptions underlying our study and on possible applications of our results.
23 pages, no figures
References in corpus (16)
- Resummation of Massive Gravity
- Generalization of the Fierz-Pauli Action
- Universal Limits on Massless High-Spin Particles
- Massive Spin 3/2 Electrodynamics
- Inconsistencies of Massive Charged Gravitating Higher Spins
- String Theory and The Velo-Zwanziger Problem
- Causal Propagation of a Charged Spin 3/2 Field in an External Electromagnetic Background
- On massive spin 2 electromagnetic interactions
- Cubic interaction vertex of higher-spin fields with external electromagnetic field
- Consistent massive graviton on arbitrary backgrounds
- Consistent Non-Minimal Couplings of Massive Higher-Spin Particles
- Linear spin-2 fields in most general backgrounds
- On manifolds admitting the consistent Lagrangian formulation for higher spin fields
- Progress in Gauge Invariant Lagrangian Construction for Massive Higher Spin Fields
- Massive graviton on arbitrary background: derivation, syzygies, applications
- Fundamental fields around compact objects: Massive spin-2 fields, Superradiant instabilities and Stars with dark matter cores