The intriguing connection between black holes’ evaporation and physics of solitons is opening novel roads to finding observable phenomena. It is known from the inverse scattering transform that velocity is a fundamental parameter in solitons theory. Taking this into account, the study of Hawking radiation by a moving soliton gets a growing relevance. However, a theoretical context for the description of this phenomenon is still lacking. Here, we adopt a soliton geometrization technique to study the quantum emission of a moving soliton in a one-dimensional model. Representing a black hole by the one soliton solution of the Sine-Gordon equation, we consider Hawking emission spectra of a quantized massless scalar field on the soliton-induced metric. We study the relation between the soliton velocity and the black hole temperature. Our results address a new scenario in the detection of new physics in the quantum gravity panorama.
%0 Journal Article
%1 2399-6528-2-5-055016
%A Villari, Leone Di Mauro
%A Marcucci, Giulia
%A Braidotti, Maria Chiara
%A Conti, Claudio
%D 2018
%J Journal of Physics Communications
%K myown quantum-gravity
%N 5
%P 055016
%T Sine-Gordon soliton as a model for Hawking radiation of moving black holes and quantum soliton evaporation
%U http://stacks.iop.org/2399-6528/2/i=5/a=055016
%V 2
%X The intriguing connection between black holes’ evaporation and physics of solitons is opening novel roads to finding observable phenomena. It is known from the inverse scattering transform that velocity is a fundamental parameter in solitons theory. Taking this into account, the study of Hawking radiation by a moving soliton gets a growing relevance. However, a theoretical context for the description of this phenomenon is still lacking. Here, we adopt a soliton geometrization technique to study the quantum emission of a moving soliton in a one-dimensional model. Representing a black hole by the one soliton solution of the Sine-Gordon equation, we consider Hawking emission spectra of a quantized massless scalar field on the soliton-induced metric. We study the relation between the soliton velocity and the black hole temperature. Our results address a new scenario in the detection of new physics in the quantum gravity panorama.
@article{2399-6528-2-5-055016,
abstract = {The intriguing connection between black holes’ evaporation and physics of solitons is opening novel roads to finding observable phenomena. It is known from the inverse scattering transform that velocity is a fundamental parameter in solitons theory. Taking this into account, the study of Hawking radiation by a moving soliton gets a growing relevance. However, a theoretical context for the description of this phenomenon is still lacking. Here, we adopt a soliton geometrization technique to study the quantum emission of a moving soliton in a one-dimensional model. Representing a black hole by the one soliton solution of the Sine-Gordon equation, we consider Hawking emission spectra of a quantized massless scalar field on the soliton-induced metric. We study the relation between the soliton velocity and the black hole temperature. Our results address a new scenario in the detection of new physics in the quantum gravity panorama.},
added-at = {2018-05-20T21:51:59.000+0200},
author = {Villari, Leone Di Mauro and Marcucci, Giulia and Braidotti, Maria Chiara and Conti, Claudio},
biburl = {https://www.bibsonomy.org/bibtex/272d67c699588b477b1edc6aaa6ec82a5/nonlinearxwaves},
interhash = {43dc4f59817c1e2fc0e7bd884516a40a},
intrahash = {72d67c699588b477b1edc6aaa6ec82a5},
journal = {Journal of Physics Communications},
keywords = {myown quantum-gravity},
number = 5,
pages = 055016,
timestamp = {2018-05-20T21:51:59.000+0200},
title = {Sine-Gordon soliton as a model for Hawking radiation of moving black holes and quantum soliton evaporation},
url = {http://stacks.iop.org/2399-6528/2/i=5/a=055016},
volume = 2,
year = 2018
}