In 1961 the Buhl Foundation established by the power of money the Buhl Chair in Theoretical Physics at Carnegie Mellon. The Buhl Chair, Dr. Fred Gilman, likely does many interesting things, but the only one I know of, is his responsibility to invite a scientist to the Mellon Institute each year to talk about physics.

This generally highly publicized event is the single physics lecture I go to each year, and is always quite enjoyable. For information on the Buhl Chair, and past speakers you can check their website, here which hasn’t been updated since 2005.
This year’s Buhl lecture was extra-exciting (seriously) as earlier that afternoon the Bruce & Astrid McWilliams Center for Cosmology was announced at Carnegie Mellon. This new center, made possibly by the McWilliams, “will strive to unravel the mysteries of the universe.” While this sounds like quite a hard task, they are going to do it multidisciplinarily and so it is hot.
So in continuing the cosmological astro-physics trend, the Buhl Lecture for 2008 was given by Joel Primack and called “A Brief History of Dark Matter.”
Short notes here (long notes, to come):
A Brief History of Dark Matter
Joel Primack, University of California at Santa Cruz
Part I – History.
Fritz Zwicky is the beginning. Described by Primack as “one of the most profound and annoying astronomers of the 20th century,” this man, while studying the Coma Cluster in 1933 realized something was erm… strange. Without getting too much into real physics, Zwicky calculated the mass of the whole Coma cluster, based on how fast the edge galaxies in the cluster were spinning. He also calculated how much mass should be in the cluster based on the number of galaxies and the amount of light reaching us here on Earth. The numbers didn’t match.
So, let’s say we are hanging out, adding up masses of galaxies 100 Mega-parsecs, which means the light we are looking at is 326 million years old, which is around the time the Appalachian Mountains were formed (i.e. no people hanging out). And as we are hanging out looking at this really old light we realize the masses of the Coma Cluster aren’t adding up. We need to brainstorm some solutions for why this could be the case.
Conveniently, Zwicky has done this in his paper. As summarized by Michael Richmond Zwicky discuss four possibilities:
- Stars in the Coma Cluster are different from stars in the Milky Way (which is where we had nearly all our information about masses and light emitted back in 1933).
- The Coma Cluster is not in equilibrium
- The laws of physics are different in the Coma Cluster!
- The Coma Cluster has lots of mass which is not part of the stars
And this is Dark Matter. Of course, Zwicky did not call it that, but that is what he is getting at, lots and lots of mass (more than ten times that which the stars account for) which we cannot see.
Alright, but as discussed Zwicky is sort of a hassle and this wasn’t much to go on, so we can basically leave his work as open question, and move on. Also, I leave it as an exercise to the reader to find a digital version of Zwicky’s 1933 paper, which doesn’t seem to be online. Hint: it was published in 1933 in Helvetica Physica acta – if you do procure this, e-mail me.
So then, some 40 years later, Vera Rubin was also hanging out measuring masses and speeds of galaxies and stars. (This is what astronomers do, have you noticed?) Vera measured the speeds of stars near the center and also at the far reaches of spiral galaxies and found something very counterintuitive, which was the stars near the ends of the spiral arms were moving very fast. Just as fast as those closer to the center. However, the gravity out at the edges should have been much weaker than that near center, which means the galaxy should not have been able to hold in those fast moving edge stars and they should have been sped away from the spiral galaxies.
But if the gravity out at the edges was similar to the gravity much closer to the center of the galaxy then Vera decided their must be much more mass throughout the galaxy than could be seen. And by the early 80s the community was convinced, there was a lot of mass in the universe that we simply could not see.
So theoretical physicists jump in, to what is a new and interesting and open question. Questions like: What is dark matter made of (on a particle level)? How fast does it move? Where can it be found? How can we detect it?
Now unfortunately, I must be a bit critical here. Primack is one of the scientists behind the theory of Cold Dark Matter, so when discussing the other proposals for explaining this lack of mass he … brushes them aside faster than he possibly should. However at this point Cold Dark Matter (CDM) – and the Lambda-CDM model does seem to be the leading candidate for the explanation of dark matter.
Now, to explain the last thirty years of work in this field in a paragraph, physicists came up with possible explanations for the type of particles that could possibly make up the dark matter. CDM calls for matter that we can’t see, but isn’t much more specific than that. One possibility could be matter that does not interact with normal matter, except through gravity, possibly some sort of very heavy particle that is similar to a neutrino. Or there could be an abundance of large objects of normal matter that just emits very little (or no) radiation, however this seems unlikely. Simulations tend to favor the first idea, lots of heavy particles that we can’t see. Other proposals involve modifying newtonian dynamics to account for the mass, and revising our definitions of gravity but people don’t seem to like these.
Part II – Pretty.
Primack then moved on to lighter material. Explaining how as you travel further away from us you can see galaxies that look different, as they are younger, he showed images taken from the Hubble Ultra Deep Field. He additionally showed a video of the Millennium Simulation by the Max-Planck Institute. This is a 10 billion particle simulation that attempts to show the possible dark matter distribution in the universe, and gives some sense of scale.
Primack also gave the quick numbers that everyone wants to hear. How much of the universe is dark matter? His current estimates put Cold Dark Matter at 25% and Dark Energy at 70% (note again bias towards the CDM model). He also has an interesting representation of that, which I will re-post here:

© Joel Primack & Nancy Ellen Abrams
(And further I will ignore any sort of distortion given to the percentages by the choice of visualization by cartoon pyramid.)
Videos shown:
Part III – What’s Next.
As Primack believes CDM has nailed it, what is left is actually finding experimental evidence of dark matter – and he thinks this will be done by 2010. He suggests ways this might occur.
- We could produce dark matter. The Large Hadron Collider could possibly produce micro black holes, super symmetric particles, or other particles which could be candidates for dark matter particles. Experiments should begin at the LHC in June 2008.
- We could infer dark matter’s existence through the use of the Planck Surveyor, a cute little satellite, who among other things plans to go find lots of gravitational lensing. It should launch on Halloween this year. (it is really a cat dressed up as a satellite)
- According to NASA’s description of GLAST, The Gamma-ray Large Area Space Telescope – it will: “Search for signs of new laws of physics and what composes the mysterious Dark Matter.” Yes that is right we will determine dark matter with “new laws of physics.” Look forward to that on May 16th, 2008.
- We could also directly detect dark matter using my third favorite noble gas, Xenon! Yes the Large Underground Xenon Detector is an experiment where you put a bunch of Xenon in a cave deep underground and then wait. and hope. and maybe they even pray, for some dark matter particle to crash into the Xenon. So far, nothing, but they keep using more Xenon, so maybe they will get there soon. New results coming this fall.
Conclusion
Within the next two years we might find evidence of dark matter, any sort of material that is invisible on the electromagnetic spectrum, or we may not. Each of the experiments above may turn up nothing and we may be left having to admit that it is possible we have framed the problem incorrectly. As this New York Times article explains dark matter is a practical necessity to make the current theories work.
To give a single example, our understanding (or lack thereof) of gravity has always been a bit of a problem for physicists, it doesn’t quite mesh with quantum mechanics and relativity, and it may not work as we expect when we begin to probe the depths of our universe – and thus may have introduced such a concept as dark matter/energy to fill a void that was only imagined.
But this is how science works, we design tests for the hypotheses that we have, and if these fail we create new hypotheses and new tests. So, now we non-physicists wait for one of these experiments to result in actual experimental evidence for dark matter. Remember to check back in two years to see if Primack was on his game and we are a few steps closer to figuring out what roughly 22% (and more likely 96%) of the universe actually is composed of.
If in the meantime you need some light and physicsy reading material you can check out Primack’s book (co-written with Nancy Ellen Abrams), The View from the Center of the Universe which I have not read and therefore will not comment on the quality of the writing or science within.