Adapted from P. Coles, 1999, The Routledge Critical
Dictionary of the New Cosmology, Routledge Inc., New York. Reprinted
with the author's permission. To order this book click here:
http://www.routledge-ny.com/books.cfm?isbn=0415923549
According to the standard Big Bang theory,
the early Universe was sufficiently hot for all the matter in it to be
fully ionised. Under these conditions, electromagnetic radiation was
scattered very efficiently by matter, and this scattering kept the
Universe in a state of thermal equilibrium. Eventually the Universe
cooled to a temperature at which electrons could begin to recombine
into atoms, and this had the effect of lowering the rate of
scattering. This happened at what is called the recombination era of
the thermal history of the Universe. At some point, when
recombination
was virtually complete, photons ceased to scatter at all and began to
propagate freely through the Universe, suffering only the effects of
the cosmological redshift. These photons reach present-day observers
as the cosmic microwave background radiation (CMB). This radiation
appears to come from a spherical surface around the observer such that
the radius of the shell is the distance each photon has travelled
since it was last scattered at the epoch of recombination. This
surface is what is called the last scattering surface.
To visualise how this effect arises, imagine that you are in a large
field filled with people screaming. You are screaming too. At some
time t = 0 everyone stops screaming simultaneously. What will you
hear? After 1 second you will still be able to hear the distant
screaming of people more than 330 metres away (the speed of sound in
air, vs, is about 330 m/s). After 3 seconds you will
be able to hear
distant screams from people more than 1 kilometre away (even though
those distant people stopped screaming when you did). At any time t,
assuming a suitably heightened sense of hearing, you will hear some
faint screams, but the closest and loudest will be coming from people
a distance vst away. This distance defines a
`surface of last
screaming' and this surface is receding from you at the speed of
sound. Similarly, in a non-expanding universe, the surface of last
scattering would recede from us at the speed of light. Since our
Universe is expanding, the surface of last scattering is actually
receding at about twice the speed of light. This leads to the
paradoxical result that, on their way to us, photons are actually
moving away from us until they reach regions of space that are
receding at less than the speed of light. From then on they get closer
to us. None of this violates any laws of physics because all material
objects are locally at rest.
When something is hot and cools down it can undergo a phase
transition. For example, hot steam cools down to become water, and
when cooled further it becomes ice. The Universe went through similar
phase transitions as it expanded and cooled. One such phase
transition, the process of recombination discussed above, produced the
last scattering surface. When the Universe was cool enough to allow
the electrons and protons to fall together, they `recombined' to form
neutral hydrogen. CMB photons do not interact with neutral hydrogen,
so they were free to travel through the Universe without being
scattered. They decoupled from matter. The opaque Universe then became
transparent.
Imagine you are living 15 billion years ago. You would be surrounded
by a very hot opaque plasma of electrons and protons. The Universe is
expanding and cooling. When the Universe cools down below a critical
temperature, the fog clears instantaneously everywhere. But you would
not be able to see that it has cleared everywhere because, as you look
into the far distance, you would be seeing into the opaque past of
distant parts of the Universe. As the Universe continues to expand and
cool you would be able to see farther, but you would always see the
bright opaque fog in the distance, in the past. That bright fog is the
surface of last scattering. It is the boundary between a transparent
and an opaque universe and you can still see it today, 15 billion
years later.
Although the surface of last scattering has a temperature of 3000 K,
the cosmic microwave background photons now have a temperature of
about 3 K. This factor-of-1000 reduction in temperature is the result
of the factor-of-1000 expansion between the time the photons were
emitted and now. The photons have cooled and become redshifted as a
result of the expansion of the Universe. For example, when the
Universe is three times bigger than it is now, the CMB will have a
temperature of about 1 K.
The last scattering surface is sometimes called the cosmic
photosphere, by analogy with the visible `surface' of the Sun where
radiation produced by nuclear reactions is last scattered by the solar
material. The energy source for the Sun's photons is not in the
photosphere: it comes from nuclear fusion at the centre of the Sun.
Similarly, the CMB photons were not created at the surface of last
scattering: they were produced at a much earlier epoch in the
evolution of the Universe. A tiny fraction (about one in a billion) of
these photons, however, were created by recombination transitions at
the last scattering surface. There should therefore be very weak
emission lines in the black-body spectrum of the CMB
radiation, but none has yet been detected.
Some interesting properties of the last scattering surface are
illustrated in the Figure overleaf. Here, space is represented as
two-dimensional. The time t since the Big Bang is the vertical
axis; T
is the temperature of the CMB and z is the redshift (for
simplicity,
the expansion of the Universe is ignored). The plane at the top
corresponds to the Universe now. As stationary observers we move
through time (but not space), and we are now at the apex of the cone
in the Now plane. When we look around us into the past, we can see
only photons on our past light cone. CMB photons travel from the waxy
circle in the last scattering surface along the surface of the light
cone to us. The unevenness of the circle represents
temperature fluctuations at the last scattering surface. The bottom
two planes are at fixed times, while the Now plane moves upwards. As
it does, the size of the observable Universe (the diameter of the wavy
circle) increases. The object which emitted light at C is currently at
C', and the light emitted at C is currently entering our telescopes at
the apex of the cone. Points A and C are on opposite sides of the sky.
If the angle between B and C is greater than a few degrees, then B and
C have never been able to exchange photons with each other, so they
cannot even know about each other at the time of last scattering. How
can it be that their temperatures are the same? This is the essence of
the cosmological horizon problem, and was one of the motivations for
the inflationary Universe theory.
Last scattering surface. The last
scattering surface represented as a
flat sheet. The expansion of the Universe is ignored in this diagram.
LAST SCATTERING SURFACE