Bumblebee gravity perturbations decouple exactly into gravitational and vector sectors, with gravitational modes dynamically immune to Lorentz violation and odd-even parities strictly isospectral.
Shadow of slowly rotating kalb-ramond black holes
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Non-metricity in bumblebee gravity modifies neutrino-antineutrino annihilation energy deposition, oscillation phases, and lensing-induced flavor transition probabilities in a specific black hole spacetime.
citing papers explorer
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Gravitational-Bumblebee perturbations: Exact decoupling and isospectrality
Bumblebee gravity perturbations decouple exactly into gravitational and vector sectors, with gravitational modes dynamically immune to Lorentz violation and odd-even parities strictly isospectral.
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The role of non-metricity on neutrino behavior in bumblebee gravity
Non-metricity in bumblebee gravity modifies neutrino-antineutrino annihilation energy deposition, oscillation phases, and lensing-induced flavor transition probabilities in a specific black hole spacetime.