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Approaches to Quantum Gravity

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100 O. Dreyer<br />

Is<br />

spacetime<br />

fundamental<br />

?<br />

Are<br />

No Uses No Einstein's No<br />

background<br />

Equations<br />

time<br />

used ?<br />

?<br />

Internal<br />

Relativity<br />

Yes Yes Yes<br />

Strings,<br />

LQG, etc.<br />

Volovik<br />

Lloyd<br />

Fig. 7.1. Choices on the road <strong>to</strong> <strong>Quantum</strong> <strong>Gravity</strong>.<br />

uses the Einstein equations <strong>to</strong> formulate the theory. The other possibility is <strong>to</strong> argue<br />

for why the Einstein equations hold true. In section 7.3 we will show how such an<br />

argument can be made. We call this approach Internal Relativity.<br />

7.2 Two views of time<br />

In this section we review two approaches <strong>to</strong> <strong>Quantum</strong> <strong>Gravity</strong> that differ in the<br />

way they view time. The first approach comes from solid state physics; the second<br />

comes from quantum information theory.<br />

7.2.1 Fermi points<br />

In this section we are interested in the low energy behavior of quantum mechanical<br />

Fermi liquids. It turns out that this behavior does not depend on the details of the<br />

model but is rather described by a small number of universality classes. Which<br />

universality class a given model falls in<strong>to</strong> is determined by the <strong>to</strong>pology of the<br />

energy spectrum in momentum space. The best known class is that of a simple<br />

Fermi surface (see figure 7.2Aa). In an ideal free Fermi gas the Fermi surface is<br />

the boundary in momentum space between the occupied and unoccupied states. If<br />

p F is the corresponding momentum then the energy spectrum is given by<br />

E( p) = v F (| p|−p F ). (7.1)<br />

In addition <strong>to</strong> these fermionic degrees of freedom there are also bosonic excitations<br />

given by oscillations of the Fermi surface itself. The dynamics of the fermionic and<br />

bosonic degrees of freedom is described by the Landau theory of Fermi liquids.<br />

The other well known situation is that of a fully gapped system (see figure<br />

7.2Ab). In this case the next available energy level above the Fermi surface is everywhere<br />

separated from it by a non-zero amount . This situation is encountered in<br />

superfluids and superconduc<strong>to</strong>rs.

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