Horndeski extension of the minimal theory of quasidilaton massive gravity
Antonio De Felice, Shinji Mukohyama, Michele Oliosi

TL;DR
This paper extends the minimal quasidilaton massive gravity theory by adding a Horndeski term, ensuring stability, the Vainshtein screening mechanism, and compatibility with local gravity tests, while maintaining a stable de Sitter solution.
Contribution
The paper introduces a Horndeski extension to the minimal quasidilaton theory that preserves degrees of freedom, stability, and screening, advancing the model's physical viability.
Findings
Stable self-accelerating de Sitter solutions across parameter ranges
Propagation speed of gravitational waves matches the speed of light
The extended theory maintains three physical degrees of freedom
Abstract
The minimal theory of quasidilaton massive gravity allows for a stable self-accelerating de Sitter solution in a wide range of parameters. On the other hand, in order for the theory to be compatible with local gravity tests, the fifth force due to the quasidilaton scalar needs to be screened at local scales. The present paper thus extends the theory by inclusion of a cubic Horndeski term in a way that (i) respects the quasidilaton global symmetry, that (ii) maintains the physical degrees of freedom in the theory being three, that (iii) can accommodate the Vainshtein screening mechanism and that still (iv) allows for a stable self-accelerating de Sitter solution. After adding the Horndeski term (and a k-essence type nonlinear kinetic term as well) to the precursor action, we switch to the Hamiltonian language and find a complete set of independent constraints. We then construct the…
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