Covariant power-counting renormalizable gravity: Lorentz symmetry breaking and accelerating early-time FRW universe
Shin'ichi Nojiri, Sergei D. Odintsov

TL;DR
This paper explores a covariant, power-counting renormalizable gravity theory with Lorentz symmetry breaking, proposing vector gravity models that admit inflationary solutions and black hole solutions, advancing quantum gravity research.
Contribution
It introduces a covariant vector gravity model with U(1) symmetry and analyzes its cosmological and black hole solutions, including dispersion relations for gravitons.
Findings
Existence of power-law and de Sitter inflationary solutions.
Derivation of black hole solutions within the model.
Presentation of graviton dispersion relations.
Abstract
We continue the study of covariant power-counting renormalizable gravity constrained by scalar Lagrange multiplier. Lorentz symmetry breaking is investigated in such a theory in comparison with the one in ghost condensation model. Covariant power-counting renormalizable vector gravity which is invariant under gauge symmetry is proposed. Several forms of vector Lagrange multiplier in this theory are discussed. It is shown that covariant scalar/vector gravity under consideration may have power-law or de Sitter accelerating cosmological solution corresponding to inflationary era. Simplest black hole solution is obtained and dispersion relations for graviton are presented.
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