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On the space of solutions of the Hořava theory at the kinetic-conformal point

2017/05/31 by Jorge Bellorín, Jorge Bellorin, Alvaro Restuccia · 6 citations
Mathematics · Physics and Astronomy · #Advanced Differential Geometry Research #Cosmology and Gravitation Theories #Covariant Hamiltonian field theory #Differential geometry #Formalism (music) #Geometric Analysis and Curvature Flows #Hamiltonian (control theory) #Homogeneous #Isotropy #Lagrange multiplier #Lagrangian #Minimal coupling #gr-qc #hep-th

paper · pdf · doi:10.1007/s10714-017-2298-4

published in General Relativity and Gravitation 49(10) (Springer Science+Business Media) · v3: Eqs. (2.7), (3.9) and (3.10) have been corrected, with no consequences on the main results. Some references added, some typos corrected

openalex created_date 2017/06/05 · openalex publication_date 2017/09/16 · arxiv created 2017/10/18 · arxiv updated 2017/10/19 · openalex updated_date 2026/08/05

Abstract

The nonprojectable Horava theory at the kinetic-conformal point is defined by setting a specific value of the coupling constant of the kinetic term of the Lagrangian. This formulation has two additional second class-constraints that eliminate the extra mode. We show that the space of solutions of this theory in the Hamiltonian formalism is bigger than the space of solutions in the original Lagrangian formalism. In the Hamiltonian formalism there are certain configurations for the Lagrange multupliers that lead to solutions that cannot be found in the original Lagrangian formulation. We show specific examples in vacuum and with a source. The solution with the source has homogeneous and isotropic spatial hypersurfaces. The enhancement of the space of solutions leaves the possibility that new solutions applicable to cosmology, or to other physical systems, can be found in the Hamiltonian formalism.

Citations