Abstract

The particular structure of Galileon interactions allows for higher-derivative terms while retaining second order field equations for scalar fields and Abelian p-forms. In this work we introduce an index-free formulation of these interactions in terms of two sets of Grassmannian variables. We employ this to construct Galileon interactions for mixed-symmetry tensor fields and coupled systems thereof. We argue that these tensors are the natural generalization of scalars with Galileon symmetry, similar to p-forms and scalars with a shift-symmetry. The simplest case corresponds to linearised gravity with Lovelock invariants, relating the Galileon symmetry to diffeomorphisms. Finally, we examine the coupling of a mixed-symmetry tensor to gravity, and demonstrate in an explicit example that the inclusion of appropriate counterterms retains second order field equations.

Highlights

  • These include scalar theories with field equations containing derivatives up to second order instead of strictly second order [12]

  • The particular structure of Galileon interactions allows for higher-derivative terms while retaining second order field equations for scalar fields and Abelian p-forms

  • In this work we introduce an index-free formulation of these interactions in terms of two sets of Grassmannian variables. We employ this to construct Galileon interactions for mixedsymmetry tensor fields and coupled systems thereof. We argue that these tensors are the natural generalization of scalars with Galileon symmetry, similar to p-forms and scalars with a shift-symmetry

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Summary

Preliminaries on anticommuting variables

Given that the actions for Galileons are highly non-linear, they appear rather complicated and employ a large number of indices. Extending the bosonic (degree-0) coordinates (xi) by these degree-1 variables essentially means that we are going to write down actions on a graded (super)manifold M. These variables satisfy the following properties: θiθj = −θjθi , χiχj = −χjχi , θiχj = χjθi. In curved space and for more general choices of coordinates, the epsilon symbol is to be replaced by the epsilon tensor, i.e. the value of integrals like (2.9) can depend on spacetime position. These integral formulas are pivotal in our formulation, since the Lagrangians will always involve integration over the graded variables

Scalar and p-form Galileons in the graded formalism
Galileons for mixed-symmetry tensor fields
The mixed-symmetry Galileon for a single species
Relation to Lovelock gravity
Multiple species and generalized mixed-symmetry Galileons
Covariant tensor Galileons
Preliminaries on covariant tensors
Covariantization of the mixed-symmetry Galileon
Discussion and conclusions
Scalars in flat space-time
Scalars in curved space-time
Two-forms in curved space-time
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