Notes on Relativity and Cosmology - Physics Department, UCSB
Notes on Relativity and Cosmology - Physics Department, UCSB
Notes on Relativity and Cosmology - Physics Department, UCSB
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10.2. DYNAMICS! (A.K.A. TIME EVOLUTION) 293<br />
principle why the pressure P must be positive. Let’s think about what a negative<br />
pressure would mean. A positive pressure is an effect that resists something<br />
being squeezed. So, a negative pressure is an effect that resists something being<br />
stretched. This is also known as a ‘tensi<strong>on</strong>.’ Imagine, for example, a rubber<br />
b<strong>and</strong> that has been stretched. We say that it is under tensi<strong>on</strong>, meaning that it<br />
tries to pull itself back together. A sophisticated relativistic physicist calls such<br />
an effect a ‘negative pressure.’<br />
Let’s look closely at equati<strong>on</strong> (10.4). We see that the universe can in fact ‘sit<br />
still’ <strong>and</strong> remain static if ρ + 3P = 0. If ρ + 3P is negative, then gravity will<br />
in fact be repulsive (as opposed to attractive) the various bits of matter will<br />
accelerate apart. Now, because ρ is typically very large (since it is the density<br />
of energy <strong>and</strong> E = mc 2 ) this requires a truly huge negative pressure. The kinds<br />
of matter that we are most familiar with will never have such a large negative<br />
pressure. However, physicists can imagine that their might possibly be such a<br />
kind of matter.<br />
The favorite idea al<strong>on</strong>g these lines is called “vacuum energy.” The idea is that<br />
empty space itself might somehow have energy. At first, this is a rather shocking<br />
noti<strong>on</strong>. I mean, if it is empty, how can it have energy? But, some reflecti<strong>on</strong> will<br />
tell us that this may simply be a matter of semantics: given the space that we<br />
think is empty (because we have cleared it of everything that we know how to<br />
remove), how empty is it really? In the end, like everything else in physics, this<br />
questi<strong>on</strong> must be answered experimentally. We need to find a way to go out<br />
<strong>and</strong> to measure the energy of empty space.<br />
Now, what is clear is that the energy of empty space must be rather small.<br />
Otherwise, it’s gravitati<strong>on</strong>al effects would screw up our predicti<strong>on</strong>s of, for example,<br />
the orbits of the planets. However, there is an awful lot of ‘empty’ space<br />
out there. So, taken together it might still have some n<strong>on</strong>trivial effect <strong>on</strong> the<br />
universe as a whole.<br />
OK, so why should vacuum energy (the energy density of empty space) have<br />
negative pressure? Well, an important fact here is that energy density <strong>and</strong><br />
pressure are not completely independent. Pressure, after all is related to the<br />
force required to change the size of a system: to smash it or to stretch it out.<br />
On the other h<strong>and</strong>, force is related to energy: for example, we must add energy<br />
to a rubber b<strong>and</strong> in order fight the tensi<strong>on</strong> forces <strong>and</strong> stretch it out. The fact<br />
that we must add energy to a spring in order to stretch it is what causes the<br />
spring to want to c<strong>on</strong>tract; i.e., to have a negative pressure when stretched.<br />
Now, if the vacuum itself has some energy density ρ <strong>and</strong> we stretch the space<br />
(which is just what we will do when the universe exp<strong>and</strong>s) then the new (stretched)<br />
space has more vacuum <strong>and</strong> therefore more energy. So, we again have to add<br />
energy to stretch the space, so there is a negative pressure. It turns out that pressure<br />
is (minus) the derivative of energy with respect to volume P = −dE/dV .<br />
Here, E = ρV , so P = −ρ. Clearly then for pure vacuum energy we have<br />
ρ + 3P < 0 <strong>and</strong> gravity is repulsive. On the other h<strong>and</strong>, combining this with<br />
the appropriate amount of normal matter could make the two effects cancel out<br />
<strong>and</strong> could result in a static universe.