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Kiefer C. Quantum gravity

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322 INTERPRETATION<br />

the existence of life, and a particular efficient process in this respect is photosynthesis.<br />

The huge entropy capacity of the environment comes in this case from<br />

the high temperature gradient between the hot Sun and the cold empty space:<br />

few high-energy photons (with small entropy) arrive on Earth, while many lowenergy<br />

photons (with high entropy) leave it. Therefore, also the thermodynamic<br />

arrow of time points towards cosmology: how can gravitationally condensed objects<br />

like the Sun come from in the first place?<br />

Another important arrow of time is the quantum-mechanical arrow. The<br />

Schrödinger equation is time-reversal invariant, but the measurement process,<br />

either through<br />

• a dynamical collapse of the wave function, or<br />

• an Everett branching<br />

distinguishes a direction; cf. Section 10.1. We have seen that growing entanglement<br />

with other degrees of freedom leads to decoherence. The local entropy<br />

thereby increases. Again, decoherence only works if a special initial condition—a<br />

condition of weak entanglement—holds. But where can this come from?<br />

The last of the main arrows is the gravitational arrow of time. Although<br />

the Einstein field equations are time-reversal invariant, gravitational systems in<br />

Nature distinguish a certain direction: the universe as a whole expands, while<br />

local systems such as stars form by contraction, for example, from gas clouds. It<br />

is by this gravitational contraction that the high temperature gradients between<br />

stars such as the Sun and the empty space arise. Because of the negative heat<br />

capacity for gravitational systems, homogeneous states possess a low entropy,<br />

whereas inhomogeneous states possess a high entropy—just the opposite than<br />

for non-gravitational systems.<br />

An extreme case of gravitational collapse is the formation of black holes.<br />

We have seen in Section 7.1 that black holes possess an intrinsic entropy, the<br />

‘Bekenstein–Hawking entropy’ (7.17). This entropy is much bigger than the entropy<br />

of the object from which the black hole has formed. If all matter in the<br />

observable universe were in a single gigantic black hole, its entropy would be<br />

S BH ≈ 10 123 k B (Penrose 1981). Black holes thus seem to be the most efficient<br />

objects for swallowing information. A ‘generic’ universe would thus basically<br />

consist of black holes. Since this is not the case, our universe must have been<br />

started with a very special initial condition. Can this be analysed further? Close<br />

to the big bang, the classical theory of general relativity breaks down. A possible<br />

answer can thus only come from quantum <strong>gravity</strong>.<br />

In the following, we shall adopt the point of view that the origin of irreversibility<br />

can be traced to the structure of the Wheeler–DeWitt equation. As<br />

can be seen, for example, from the minisuperspace case in (8.15), the potential<br />

term is highly asymmetric with respect to the scale factor a ≡ exp(α): in particular,<br />

the potential term vanishes near the ‘big bang’ α →−∞.Thispropertyis<br />

robust against the inclusion of (small) perturbations, that is, degrees of freedom<br />

describing density fluctuations or gravitational waves (cf. Section 8.2). Denoting

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