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| Where does the evidence lead? (Photograph: H Armstrong Roberts/Corbis) |
In my last three major posts (I, II and III) I've been talking you through a mystery: the integrated Sachs-Wolfe mystery. This post will be able to be read on its own, but it you will appreciate it much more if you have also read them. In today's post I will be playing detective, examining the evidence, looking for leads and weighing up the various possible solutions to the mystery. Like any good mystery there are hints as to what the resolution might be, but like any good mystery story some of these hints might turn out to be just be red herrings, so we need to be careful.
At the beginning of my most recent post in this series I warned you that it would be my most technical post to date, but encouraged you to stick with it. With this post, the situation is the opposite. That post contained the details of the actual measurement that was made, which is necessarily going to be somewhat dry and technical. This post, however, speculates about what might have caused the effect. As you'll soon see, solving the mystery potentially requires modifications to our understanding of fundamental physics or the initial conditions of the universe. All very exciting stuff, so congratulations for making it to this point.
An overview
of the case:
Before
embarking on the detective work, let me recap the first three posts
in this series. In the first post, I introduced what the integrated
Sachs-Wolfe effect is. It is the very subtle heating and cooling of
light as it passes through over and under dense regions of the
universe. In the second post I explained that this effect is so small
that it almost certainly will never be observed directly. The only
hope we have to observe it is to look for statistical correlations
between the temperature of light on the sky and the density of the
matter that the light travelled through to reach us. Only the cosmic microwave background (CMB) is uniform enough that such a statistical
correlation could ever be observed. In the last instalment, I told
you of a particular measurement that intended to detect this ISW
effect by looking at extreme over and under densities in the
universe. The measurement appeared to be a success because it did
measure a correlation. The only problem, and the source of the
mystery, is that the size of the correlation is far too big to be
from the ISW effect.
Something
in those structures is heating/cooling the CMB, but what?



