School of Physics

Frequency Standards and Metrology

Many modern developments in a technological society are based on high quality clocks and oscillators. One can think of examples such as the Global Positioning System (GPS) satellite system, radar, fibre optical communications, even mobile phones. The goal of the FSM Group is the development of new frequency standards with two endpoints in mind: to improve systems that are based on high quality clocks and oscillators (such as those listed above), and the use of these as precision tools to test the foundations of physics. We have already used our oscillators to make the most sensitive test of one of the founding theories of modern physics: Einstein's Theory of Relativity. In the near future we will use our devices to test new theories of cosmology, and to search for evidence of "new physics" that goes beyond the present conception of physics. We are dedicated to commercialising our inventions and thus hold patents in conjunction with industry. Our research programs include strong international and industrial collaborations, please keep reading for more details.

For ease of administration, and to reflect the difference in technologies, the FSM research group has been divided into Microwave and Optical Divisions. However, the goals of the group are shared by all its members, and in fact the techniques used across the entire group are ubiquitous. If you wish to know more about the projects and Research Staff within these divisions, then please click on the links listed below. If you can't find what you need, or if there is too little information to satisfy you, then please don't hesitate to contact the person listed after each of the listed projects (click on their name). Also, if you are interested in joining our group as a Postgraduate Researcher (Honours, Masters, Ph.D.) follow this link. We are keen to invite Postdoctoral Researchers and Visiting Academics to contribute to our research programs. A summary of the group's publications may be found here. For further information on either division, follow the link from the title of each section below.

Optical Division (Optical Frequency Synthesis, Optical Clocks, Femtosecond Pulsed Lasers, Laser Cooling)


For general information about this Division contact A/Prof. Andre Luiten

For teaching materials in courses taught by Andre, Tom Stace or John McFerran go here.

Microwave Division

For general information about this Division contact:


Professor Michael Tobar
.

Light, radio-waves and X-rays are all just different parts of the spectrum of electromagnetic radiation. Our perception of their differing nature arises because the energy of the energy carrier, the photon, varies by many orders of magnitude between these different types of radiation, and also because the wavelengths of these types of radiation are so different. This makes the light behave differently in space and interact with matter in strongly variable ways. Our eyes can respond to different frequencies of visible light by revealing them as different colours. However, because the frequency of visible light is so high (e.g. green light corresponds to 564 trillion cycles per second) it has been impossible, until very recently, to measure the exact frequency of an optical signal i.e. to follow the time varying phase of a light beam. In just a few tens of places around the world it has now become possible to perform this task with relative ease. In our laboratory we can synthesise and measure the frequency of radiation at any chosen place in the visible spectrum. We do this using a highly innovative technique ("the frequency comb") that avoids many of the pitfalls of traditional methods: the importance of this approach is recognised in the awarding of the 2005 Nobel Prize in Physics to Ted Hänsch and Jan Hall. These high quality light signals can be used in high accuracy spectroscopy and thereby used to test certain aspects of Quantum Mechanics. It is necessary to develop many other technologies to support this work, and you can read more about our development of the optical synthesiser, our two optical atomic clocks, and our frequency stabilised lasers by following the link from the title.

This division is directed towards creating extremely high frequency stable and low noise microwave oscillators. Topics include:

1. Testing fundamental physics with precision measurement

2. Precision frequency synthesis

3. Low noise frequency and phase techniques

4. Measurement of electonic and magnetic properties of materials

5. Novel high-Q microwave and millimetre wave resonators

This pursuit is being undertaken at temperatures ranging from room temperature (300 K) to liquid helium temperature (4.2 K). Applications extend from commercial to fundamental metrology and physics. We are Physicists, so our main endeavour is to undertake exciting physics experiments. However, we are also aware of "spin-off" applications. Much of our work has been patented and commercialised and the development of this technology has helped us to build new tools that can in turn be used for fundamental physics applications. Our group undertakes projects that are suitable for the Engineering Technologist to the most fundamentally inclined Physicist.

Contact Profile Address

Professor Andre Luiten

Professor
Academic Staff (Physics)

Telephone Number
6488 7028

Fax Number
6488 1014

Email Address
andre@physics.uwa.edu.au

Home Page
http://www.fsm.physics.uwa.edu.au
http://www.physics.uwa.edu.au/page/115450

Contact Profile Address

W/Prof Michael Tobar

Winthrop Professor/ARC Australian Laureate Fellow
Academic Staff (Physics)

Telephone Number
6488 3443

Fax Number
6488 1235

Email Address
mike@physics.uwa.edu.au

Home Page
http://www.physics.uwa.edu.au/~mike