Abstract
| Outline of the lecture:
The lecture will cover the searches for dark
matter axions based on the microwave cavity
experiment of Sikivie. The topics will begin
with a brief overview of halo dark matter, and
the axion as a candidate. The principle of
resonant conversion of axions in an external
magnetic field will be described, and practical
considerations in optimizing the experiment as a
signal-to-noise problem. A major focus of the
lecture will be the two complementary strategies
for ultra-low noise detection of the microwave
photons - the "photon-as-wave" approach (i.e.
conventional heterojunction amplifiers and soon
quantum-limited SQUID devices), and
"photon-as-particle" (i.e. Rydberg-atom
single-quantum detection). Experimental results
will be presented; these experiments have already
reached well into the range of sensitivity to
exclude plausible axion models, for limited
ranges of mass. The lecture will conclude with
a discussion of future plans and challenges for
the microwave cavity experiment. |