Gerry Harp

Gerry Harp
Senior Astrophysicist
Degree/Major: 
Ph.D. Physics
Discipline: 
Astrophyiscs, Interstellar communication

Trained as quantum mechanic, Gerry found the possibilities of using the multiple antennas of the Allen Telescope Array to generate beams on the sky – beams that could be far smaller than any single antenna could produce – remarkably exciting. Lured to the SETI Institute by this instrument’s intriguing possibilities, he’s undertaken many studies on beam formation (for SETI research). These include the Array’s ability to produce “negative” beams – useful for cancelling out, or “rejecting”, signals from such man-made noise makers as telecommunications satellites and the on-site, observatory computers.

For Gerry, SETI searches, and trying out new ideas on how signals might be encoded, is all exciting stuff. And while a SETI detection is a dramatic prospect, Gerry points out that the ATA will really push the envelope for radio astronomy too. It’s not just a new instrument for cosmic research; it’s revolutionary. Lately, Gerry has turned to the problem of making images with radio data, and he's very interested in "imaging SETI," which can extract thousands of times as much information from our radio telescope than more conventional SETI processing. This will speed up the SETI search by a similar factor.

Gerry is a late-comer to astronomy, having started his carrer in surface physics and thin film magnetism. Gerry's has expertise in semiconductors, magnetic materials, and low dimensional systems. In this part of his carrer, Gerry learned a great deal about quantum mechanics, diffraction and hologrphy, and his thesis topic was on the development of a new kind of electron holograpy to obtain 3D pictures of atoms. Nowadays, making pictures of atoms is relatively easy thanks to the STM.

Gerry spends free time learning as much as he can about quantum mechanics and, since joining the SETI Institute, gravitation. Einstein's theory of general relativity is not consistent with quantum mechanics even in some very simple thought experiments. Gerry thinks that very soon some astronomical measurements will allow us to probe this inconsistency, and he's looking forward to that.

Technical Description of work: 
Gerry is currently working with the Allen Telescope Array, a radio interferometer telescope owned partly by the SETI Institute. He is lucky enough to sometimes have observing time on this telescope for research (on his own and as a SETI team memeber). Gerry and team look for artificial signals coming from outside our solar system (SETI) and other astrophysical phenomena especially relating to the very thin ionized gas in the almost empty space between stars and galaxies. Gerry is fascinated by quasars which are by far the brightest astronomical objects. Quasars are thought to be enormous black holes at the centers of galaxies that are gradually devouring their host galaxy. The light (and radio waves) from these objects is so strong that they can easily be viewed at a distance of 10 billion light years. Since the universe itself is only 13 billion years old, this means we are looking back more than halfway to the big bang. How could anything be this bright? Sometimes, quasars are seen to generate visible flashes of light with duration of ~15 minutes. This is amazingly small, about the orbital radius of Jupiter. How could anything be so bright? Humans do not entirely understand the physics of quasars, which makes them even more interesting.
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