Black-bounce solutions in a k-essence theory under the effects of bumblebee gravity

In the present study, we analyze the effects of violation of Lorentz symmetry for black-bounce solutions in a $k$-essence theory that has the form of a power law for the configuration $n=1\mathrm{/}3$. We perform such analysis for a known model explored in previous work ${\mathrm{\Sigma }}^2=x^2+a^2$ and complement the proposal with a new black-bounce model for the area functions ${\mathrm{\Sigma }}_1^2=\sqrt{x^4+d^4}$. This model has the Schwarzschild-de Sitter asymptomatic behavior for $x\to -\mathrm{\infty }$, and we investigate the scalar field, potential, and energy conditions for both models. We have shown that the violation of Lorentz symmetry can be generated through $k$-essence without the need for an additional field. These results corroborate the validation of other previously investigated wormhole solutions.