New perturbative black hole solutions in an explicit spacetime-symmetry-breaking gravity EFT, with derived observables including three-horizon metrics when two coefficients are active.
Explicit spacetime-symmetry breaking and the dynamics of primordial fields
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abstract
We study the effects of explicit spacetime-symmetry breaking on primordial tensor fluctuations using an effective-field theory for Lorentz/CPT violation. We find that the graviton is still massless, but that the propagation speed of tensor modes is modified, and we obtain a constraint on the coefficient determining the symmetry breaking on the order of $10^{-15}$ from the recent measurements of the speed of gravity. Due to the symmetry breaking, the de-Sitter phase is modified, and during this inflationary epoch, the power spectrum assumes a slow oscillation around the general-relativity limit; further, we find that the primordial tensor power spectrum retains its scale invariance, but that the amplitude is modified. We also find that the modes which become subhorizon during radiation domination acquire a phase shift proportional to the coefficient for Lorentz violation.
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Perturbative black-hole and horizon solutions in gravity with explicit spacetime-symmetry breaking
New perturbative black hole solutions in an explicit spacetime-symmetry-breaking gravity EFT, with derived observables including three-horizon metrics when two coefficients are active.