Hamiltonian structure of Horava gravity
arXiv:1106.2131 · doi:10.1103/PhysRevD.84.104019
Abstract
The Hamiltonian formulation of Horava gravity is derived. In a closed universe the Hamiltonian is a sum of generators of gauge symmetries, the foliation-preserving diffeomorphisms, and vanishes on shell. The scalar constraint is second class, except for a global, first-class part that generates time reparametrizations. A reduced phase space formulation is given in which the local part of the scalar constraint is solved formally for the lapse as a function of the 3 metric and its conjugate momentum. In the infrared limit the scalar constraint is linear in the square root of the lapse. For asymptotically flat boundary conditions the Hamiltonian is a sum of bulk constraints plus a boundary term that gives the total energy. This energy expression is identical to the one for Einstein-aether theory which, for static spherically symmetric solutions, is the usual Arnowitt-Deser-Misner energy of general relativity with a rescaled Newton constant.
8 pages, no figures. v2: added references, corrected minor typographical errors. v3: matches PRD version
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- The constraints of post-quantum classical gravity
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- The anisotropic coupling of gravity and electromagnetism in Hořava-Lifshitz theory
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- Cosmological Perturbations in Restricted f(R)-Gravity
- Phenomenologically viable gravitational theory based on a preferred foliation without extra modes
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