Superfluid Picture for Rotating Space-Times
George Chapline, Pawel O. Mazur (Lawrence Livermore National, Laboratory, University of South Carolina)

TL;DR
This paper proposes a superfluid condensate model for space-time, showing that rotating gravitational fields like cosmic strings can be described as vortices in a superfluid, leading to G"odel-like metrics and insights into general relativity's limitations.
Contribution
It introduces a novel superfluid-based framework for stationary gravitational fields, connecting cosmic string metrics to superfluid vortices and exploring multi-vortex configurations.
Findings
Cosmic string metrics correspond to superfluid vortices outside the core.
Multiple vortices can produce G"odel-like space-time metrics.
Breakdown of superfluid rigidity explains closed time-like curves.
Abstract
A new prescription, in the framework of condensate models for space-times, for physical stationary gravitational fields is presented. We show that the spinning cosmic string metric describes the gravitational field associated with the single vortex in a superfluid condensate model for space-time outside the vortex core. This metric differs significantly from the usual acoustic metric for the Onsager-Feynman vortex. We also consider the question of what happens when many vortices are present, and show that on large scales a G\"odel-like metric emerges. In both the single and multiple vortex cases the failure of general relativity exemplified by the presence of closed time-like curves is attributed to the breakdown of superfluid rigidity.
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Taxonomy
TopicsCosmology and Gravitation Theories · Black Holes and Theoretical Physics · Pulsars and Gravitational Waves Research
