We consider a 4D model for photon production induced by a refractive index perturbation in a dielectric medium. We show that, in this model, we can infer the presence of a Hawking type effect. This prediction shows up both in the analogue Hawking framework, which is implemented in the pulse frame and relies on the peculiar properties of the effective geometry in which quantum fields propagate, as well as in the laboratory frame, through standard quantum field theory calculations. Effects of optical dispersion are also taken into account, and are shown to provide a limited energy bandwidth for the emission of Hawking radiation. © 2011 The American Physical Society.

Belgiorno, F., Cacciatori, S., Ortenzi, G., Rizzi, L., Gorini, V., Faccio, D. (2011). Dielectric black holes induced by a refractive index perturbation and the Hawking effect. PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY, 83(2) [10.1103/PhysRevD.83.024015].

Dielectric black holes induced by a refractive index perturbation and the Hawking effect

ORTENZI, GIOVANNI;
2011

Abstract

We consider a 4D model for photon production induced by a refractive index perturbation in a dielectric medium. We show that, in this model, we can infer the presence of a Hawking type effect. This prediction shows up both in the analogue Hawking framework, which is implemented in the pulse frame and relies on the peculiar properties of the effective geometry in which quantum fields propagate, as well as in the laboratory frame, through standard quantum field theory calculations. Effects of optical dispersion are also taken into account, and are shown to provide a limited energy bandwidth for the emission of Hawking radiation. © 2011 The American Physical Society.
Articolo in rivista - Articolo scientifico
optical analogue black holes models
English
2011
83
2
024015
none
Belgiorno, F., Cacciatori, S., Ortenzi, G., Rizzi, L., Gorini, V., Faccio, D. (2011). Dielectric black holes induced by a refractive index perturbation and the Hawking effect. PHYSICAL REVIEW D, PARTICLES, FIELDS, GRAVITATION, AND COSMOLOGY, 83(2) [10.1103/PhysRevD.83.024015].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10281/56538
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