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arXiv · 1302.6581

Microscopic Picture of Non-Relativistic Classicalons

Felix Berkhahn·Sophia Müller·Florian Niedermann·Robert Schneider
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Abstract

A theory of a non-relativistic, complex scalar field with derivatively coupled interaction terms is investigated. This toy model is considered as a prototype of a classicalizing theory and in particular of general relativity, for which the black hole constitutes a prominent example of a classicalon. Accordingly, the theory allows for a non-trivial solution of the stationary Gross-Pitaevskii equation corresponding to a black hole in the case of GR. Quantum fluctuations on this classical background are investigated within the Bogoliubov approximation. It turns out that the perturbative approach is invalidated by a high occupation of the Bogoliubov modes. Recently, it was proposed that a black hole is a Bose-Einstein condensate of gravitons that dynamically ensures to stay at the verge of a quantum phase transition. Our result is understood as an indication for that claim. Furthermore, it motivates a non-linear numerical analysis of the model.

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Felix Berkhahn, Sophia Müller, Florian Niedermann, Robert Schneider. 2013-02-26. Microscopic Picture of Non-Relativistic Classicalons. https://doi.org/10.1088/1475-7516%2F2013%2F08%2F028

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