Develops a Lagrangian path integral formulation for non-projectable Hořava gravity and computes one-loop divergences in (2+1) dimensions, verifying cancellation of linear-in-frequency terms to extract beta functions for Newton constant and λ.
Data Tables for Lorentz and CPT Violation
2 Pith papers cite this work, alongside 1,403 external citations. Polarity classification is still indexing.
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For a Dirac particle in an Einstein-Gauss-Bonnet black hole, the radial force operator is F = -mM/r^2 + 8mξM^2/r^5, the gradient of the EGB gravitational potential.
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Quantizing non-projectable Ho\v{r}ava gravity with Lagrangian path integral
Develops a Lagrangian path integral formulation for non-projectable Hořava gravity and computes one-loop divergences in (2+1) dimensions, verifying cancellation of linear-in-frequency terms to extract beta functions for Newton constant and λ.
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Dynamics for Spin-$1/2$ Particles in Einstein-Gauss-Bonnet Gravity
For a Dirac particle in an Einstein-Gauss-Bonnet black hole, the radial force operator is F = -mM/r^2 + 8mξM^2/r^5, the gradient of the EGB gravitational potential.