Bose-Einstein graviton condensate in a Schwarzschild black hole
Jorge Alfaro, Dom\`enec Espriu, Luciano Gabbanelli

TL;DR
This paper models black holes as Bose-Einstein condensates of gravitons by extending the Einstein-Hilbert action with a chemical potential, deriving equations akin to the Gross-Pitaevskii equation, and analyzing solutions within the black hole interior.
Contribution
It introduces a grand-canonical ensemble approach to graviton condensates in black holes, deriving new equations and solutions that describe the condensate's behavior inside the horizon.
Findings
Condensate vanishes outside the horizon
Non-zero condensate exists inside the black hole
Exact solution for the graviton wave function in the interior
Abstract
We analyze in detail a previous proposal by Dvali and G\'omez that black holes could be treated as consisting of a Bose-Einstein condensate of gravitons. In order to do so we extend the Einstein-Hilbert action with a chemical potential-like term, thus placing ourselves in a grand-canonical ensemble. The form and characteristics of this chemical potential-like piece are discussed in some detail. We argue that the resulting equations of motion derived from the action could be interpreted as the Gross-Pitaevskii equation describing a graviton Bose-Einstein condensate trapped by the black hole gravitational field. After this, we proceed to expand the ensuring equations of motion up to second order around the classical Schwarzschild metric so that some non-linear terms in the metric fluctuation are kept. Next we search for solutions and, modulo some very plausible assumptions, we find out…
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