Scalar field as a Bose-Einstein condensate in a Schwarzschild-de Sitter spacetime release_rev_b955623e-ba0b-4a6a-a7e1-41f392e9ae50

by Elías Castellanos, Celia Escamilla-Rivera, Claus Lämmerzahl and Alfredo Macías

Released as a article .

2015  

Abstract

In this paper we analyze some properties of a scalar field configuration, where it is considered as a trapped Bose-Einstein condensate in a Schwarzschild-de Sitter background spacetime. In a natural way, the geometry of the curved spacetime provides an effective trapping potential for the scalar field configuration. This allows us to explore some thermodynamical properties of the system. Additionally, the curved geometry of the spacetime also induces a position dependent self-interaction parameter, which can be interpreted as a kind of gravitational Feshbach resonance, that could affect the stability of the cloud and could be used to obtain information about the interactions among the components of the system..
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Type  article
Stage   submitted
Date   2015-12-10
Version   v1
Language   en ?
arXiv  1512.03118v1
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