Hamiltonian vs stability in alternative theories of gravity

Abstract

When a Hamiltonian density is bounded by below, we know that the lowest-energy state must be stable. One is often tempted to reverse the theorem and therefore believe that an unbounded Hamiltonian density always implies an instability. The main purpose of this presentation (which summarizes my work with E. Babichev, C. Charmousis and A. Lehébel) is to pedagogically explain why this is erroneous. Stability is indeed a coordinate-independent property, whereas the Hamiltonian density does depend on the choice of coordinates. In alternative theories of gravity, like k-essence or Horndeski theories, the correct stability criterion is a subtler version of the well-known "Weak Energy Condition" of general relativity. As an illustration, this criterion is applied to an exact Schwarzschild-de Sitter solution of a Horndeski theory, which is found to be stable for a given range of its parameters, contrary to a claim in the literature.

9 pages, 2 figures, uses the LaTeX class file "moriond.cls", contribution to the 2019 Gravitation session of the 54th Rencontres de Moriond

References in corpus (5)

• Stability of a black hole and the speed of gravity waves within self-tuning cosmological models
• Time-dependent spherically symmetric covariant Galileons
• Cosmological self-tuning and local solutions in generalized Horndeski theories
• Hamiltonian vs stability and application to Horndeski theory
• Linear perturbation analysis of hairy black holes in shift-symmetric Horndeski theories: Odd-parity perturbations