Abstract

In this Letter we derive acoustic black hole metrics in the (3+1) and (2+1)-dimensional Abelian Higgs model with Lorentz symmetry breaking. In this set up the sound waves lose the Lorentz boost invariance and suffer a ‘birefringence’ effect. We have found acoustic black holes and respective Hawking temperatures depending on the Lorentz violating parameter. Furthermore, we obtain an acoustic Kerr-like black hole metric with the Lorentz violating term affecting its rate of loss of mass. We also have shown that for suitable values of the Lorentz violating parameter a wider spectrum of particle wave function can be scattered with increased amplitude by the acoustic black hole.

Highlights

  • Acoustic black holes possess many of the fundamental properties of the black holes of general relativity and have been extensively studied in the literature [1,2,3,4,5,6]

  • In 1974, Hawking combining Einstein’s General Relativity and Quantum Mechanics announced that classically a black hole does not radiate, but when we consider quantum effects emits thermal radiation at a temperature proportional to the horizon surface gravity

  • We have shown that for suitable values of the Lorentz violating parameter a wider spectrum of particle wave function can be scattered with increased amplitude by the acoustic black hole

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Summary

INTRODUCTION

Acoustic black holes possess many of the fundamental properties of the black holes of general relativity and have been extensively studied in the literature [1,2,3,4,5,6]. The purpose of this paper is considering the idea of the Lorentz symmetry breaking theories suggested in the seminal paper in Superstring Theory [16] and further developed in Quantum Field Theory and General Relativity [17,18,19,20] to investigate the relativistic version of acoustic black holes from the Abelian Higgs model [5] with Lorentz symmetry breaking. We derive acoustic black hole metrics in the (3+1) and (2+1)-dimensional Abelian Higgs model with Lorentz symmetry breaking. The effects of this set up is such that the fluctuations of the fluids are affected.

THE LORENTZ-VIOLATING MODEL
THE DISPERSION RELATION
LORENTZ VIOLATING CANONICAL ACOUSTIC BLACK HOLE
CONCLUSIONS
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