Modified dispersion from isotropic Lorentz-violating operators in the gravitational SME produces birefringence and polarization mixing in gravitational waves, with explicit waveforms for binary black holes and new bounds on the coefficients from GW170817 and GWTC-3 data.
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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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Propagation effects of Lorentz violation in gravitational waves
Modified dispersion from isotropic Lorentz-violating operators in the gravitational SME produces birefringence and polarization mixing in gravitational waves, with explicit waveforms for binary black holes and new bounds on the coefficients from GW170817 and GWTC-3 data.
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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.