Abstract

Analogue models of (and for) gravity have a long and distinguished history dating back to the earliest years of general relativity. In this review article we will discuss the history, aims, results, and future prospects for the various analogue models. We start the discussion by presenting a particularly simple example of an analogue model, before exploring the rich history and complex tapestry of models discussed in the literature. The last decade in particular has seen a remarkable and sustained development of analogue gravity ideas, leading to some hundreds of published articles, a workshop, two books, and this review article. Future prospects for the analogue gravity programme also look promising, both on the experimental front (where technology is rapidly advancing) and on the theoretical front (where variants of analogue models can be used as a springboard for radical attacks on the problem of quantum gravity).

Highlights

  • The basic physics is this: A moving fluid will drag sound waves along with it, and if the speed of the fluid ever becomes supersonic, in the supersonic sound waves will never be able to fight their way back upstream [376, 387, 391, 389]

  • The features of general relativity that one typically captures in an “analogue model” are the kinematic features that have to do with how fields are defined on curved spacetime, and the sine qua non of any analogue model is the existence of some “effective metric” that captures the notion of the curved spacetimes that arise in general relativity. (At the very least, one might wish to capture the notion of the Minkowski geometry of special relativity.) the verbal description above can be converted into a precise mathematical and physical statement, which is the reason that analogue models are of physical interest

  • There were several papers in the 1980’s using an acoustic analogy to investigate the propagation of shockwaves in astrophysical situations, most notably those of Moncrief [268] and Matarrese [259, 17Indeed historically, though not of direct relevance to general relativity, analogue models played a key role in the development of electromagnetism – Maxwell’s derivation of his equations for the electromagnetic field was guided by a rather complicated analogue model in terms of spinning vortices of aether

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Summary

Introduction

I cherish more than anything else the Analogies, my most trustworthy masters. They know all the secrets of Nature, and they ought least to be neglected in Geometry. Supersonic fluid flow can generate a “dumb hole”, the acoustic analogue of a “black hole”, and the analogy can be extended all the way to mathematically demonstrating the presence of phononic Hawking radiation from the acoustic horizon. This particular provides (at least in principle) a concrete laboratory model for curvedspace quantum field theory in a realm that is technologically accessible to experiment. There are many other “analogue models” that may be useful for this or other reasons – some of the analogue models are interesting for experimental reasons, others are useful for the way they provide new light on perplexing theoretical questions. By that stage the interested reader will have had a quite thorough introduction to the ideas, techniques, and hopes of the analogue gravity programme

Going further
The Simplest Example of an Analogue Model
Background
Geometrical acoustics
Physical acoustics
General features of the acoustic metric
Example: vortex geometry
Example: slab geometry
Example
Regaining geometric acoustics
Generalizing the physical model
External forces
The role of dimension
Adding vorticity
Simple Lagrangian meta-model
The years 1981–1999
The year 2000
The year 2001
The year 2002
The year 2003
The year 2004
The year 2005
Historical Period
Optics
Acoustics
Electro-mechanical analogy
Motivation
A Catalogue of Models
Classical sound
Eikonal approximation
Abstract linear electrodynamics
Nonlinear electrodynamics
Summary
Normal mode meta-models
Bose–Einstein condensates
BEC models in the eikonal approximation
The Heliocentric universe
Slow light
Basics
Trans-Planckian problem
Modified dispersion relations
Subluminal dispersion relations
Superluminal dispersion relations
General conditions for Hawking radiation
Open issues
Solid state and lattice models
Horizon stability
Analogue spacetimes as background gestalt
Super-radiance
Cosmological geometries
Bose novae: an example of the reverse flow of information?
Future Directions
Back reaction
Equivalence principle
Emergent gravity
Quantum gravity – phenomenology
Quantum gravity – fundamental models
Conclusions
Full Text
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