Greetings from sunny Palo Alto, California, where we’re having the 2005 incarnation of the SLAC Summer Institute, Gravity in the Quantum World and the Cosmos. It’s an annual two-week school, aimed primarily at graduate students in physics, covering topics of interest to SLAC (the Stanford Linear Accelerator Center). Until recently, gravity didn’t qualify as something of interest to anyone working at a particle accelerator, but times have changed — gravity was the subject of SSI in 1998, and again this year. These days, considerations of dark energy, extra dimensions, and string theory are of direct interest to particle physicists.
I got to speak first, giving a three-hour General Relativity Primer. For lecture notes, we handed out my No-Nonsense Introduction to General Relativity that’s been on the web for a while; the online transparencies were scanned in from the actual lectures I gave. The idea was to give a complete intro to GR (metrics, geodesics, tensors, covariant derivatives, curvature, Einstein’s equation, some solutions), aimed at physics graduate students who hadn’t been exposed to GR. (Sadly, there are still plenty of physics grad students who have never been exposed to GR.)
I really wanted to give a blackboard talk, but the organizers talked me out of it, claiming (correctly, as it turns out) that blackboard in SLAC’s lecture hall is practically unreadable. But I didn’t want to use powerpoint, as it’s nearly impossible to move at a pedagogically appropriate pace when you speak from pre-made slides. As a compromise, I wrote the transparencies in real time as I lectured. It worked okay, although I realized that the main test of endurance wasn’t talking for three hours, but rather staring into the light of an overhead projector for three hours as I was writing the transparencies. In the afternoon I fielded questions for another two hours at a discussion section, so the organizers squeezed their money’s worth from me.
Yesterday morning we heard from Alessandra Buonnano on gravitational waves and Gabriella Gonzalez on actual gravitational-wave detectors, such as the LIGO observatory. All seems to be going well at LIGO, and Gabriella mentioned that they’ve even detected something — but it turned out to be an airplane flying overhead. We’re still waiting for the direct detection of an honest gravitational wave.
In the afternoon, we had Ken Nordtvedt talking about testing GR by bouncing lasers and radar signals around the solar system, and Shane Larson talking about the LISA mission. LISA will (assuming all goes according to plan) consist of three satellites flying in formation five million kilometers apart, measuring passing ripples in the geometry of spacetime by bouncing lasers back and forth. What’s that you say? You think the satellites should feature more powerful lasers, and be located twenty million kilometers from each other? Shane has set up a sensitivity curve generator, allowing you to determine how the noise limits of the satellite will change as a function of such parameters. Once you’ve hit on your favorites, it’s up to you to convince NASA to go along.