Using the Moon as a Low-Noise Seismic Detector for Strange Quark Matter

Talso Chui
Jet PropulsionLaboratory



Abstract:

Strange Quark Matter (SQM) made of up, down and strange quarks has been postulated by Witten [/Phys. Rev D 30/, 279, 1984]. SQM is nearly charge neutral and has density of nuclear matter (10^14 gm/cm^3). Witten also suggested that SQM formed shortly after the Big Bang is a viable candidate for dark matter. As suggested by de Rujula and Glashow [/Nature/ /312/, 734, 1984], a nugget of SQM may traverse a body releasing detectable seismic energy along a straight line. The Moon, being much quieter seismically than the Earth, would be an ideal place for detecting SQM. We will review previous searches for SQM to illustrate the unique parameter space to be explored by a proposal to use the Moon as a low-noise detector for SQM. We will discuss possible detection schemes by using a single seismometer, and by using an International Lunar Seismic Network. Development of a sensitive seismometer and its electronics will also be presented.