M. A. Anacleto

In this paper, we investigate the relativistic dynamics of a spin-1/2 particle in the presence of a Lorentz-violating background within the framework of effective field theory. We consider a modified Dirac Hamiltonian resulting from a CPT-odd coupling involving the Lorentz-violating gauge tensor from the Standard Model Extension (SME). Effective velocity and force operators are derived from the Heisenberg equations of motion. Using Ehrenfest’s theorem and the correspondence principle, we obtain the classical limit of the dynamics and identify an effective force exhibiting a generalized Lorentz force structure. This formalism is applied to a Penning trap system, known for high-precision measurements of charged particle properties. Our analysis shows that both the axial and cyclotron frequencies undergo corrections due to the Lorentz-violating term, leading to deviations in the particle’s trajectory and offering a potentially observable signature of Lorentz violation in precision experiments. By comparing our results with current limits from high-precision Penning traps, we establish an upper bound for the Lorentz-violating coupling [Formula: see text] for the axial frequency and [Formula: see text] for the cyclotron. These limits are compatible with the interpretation of an effective Lorentz violation consistent with current observational constraints and reinforce the phenomenological nature of the terms in question, aligning with previous analyses based on cosmological birefringence and photon propagation in a Lorentz-violating background.

In this work, we investigate the effects of Lorentz symmetry violation on the absorption cross section and quasinormal modes of a rotating acoustic black hole in (2+1) dimensions. The absorption cross section was analyzed analytically, using the low and high frequency regimes, and numerically, through integration of the radial equation. The results showed that Lorentz violation increases the absorption cross section at all energy scales, with a contribution from the rotation parameter B appearing even in the low frequency regime. For the quasinormal modes, we observed that symmetry breaking decreases the real part of the frequencies and increases the magnitude of the corresponding imaginary part, indicating a faster damping of the oscillations.