6:30 pm, Thursday February 20^th 2020

 The Braggs lecture theatre in the Braggs building

University of Adelaide (North Terrace campus)

On the 2019 Nobel Prize

“A short history of the universe – as we understand it today”

Prof. Rachel Webster

University of Melbourne

Abstract:

Most of the universe is made of Hydrogen; indeed, in the early universe, there were essentially no elements heavier than Hydrogen and Helium. During this talk Professor Webster will trace the history of the universe, using Hydrogen as the primary focus. She will explain the bits we understand and some of the key questions we are addressing today.  The efforts of Australian astronomers will be highlighted, as well as some of the new telescopes that will be operating in the next few years. 

The Bronze Bragg medals and merit certificates will be presented at the lecture.

The medals are awarded for highest achievement in Physics in 2019 in the SACE Stage 2 assessments and IB Higher Level Physics, with certificates being for students who achieved a merit or a grade of 7.

The Claire Corani Memorial Lecture

The South Australian lecture in the

2019 AIP Women in Physics Lecture Tour

at 6:30pm–7:45pm on Tuesday 20^th August 2019

in the Napier 102 Lecture Theatre
Napier Building, the University of Adelaide, North Terrace campus.

Abstract: They are small, neutral and often in a spin, and so much more than ‘just’ part of the atom. Neutrons are the sub-atomic particles that are here to save the world. This trusty particle can be called on to discover the details that no other can fathom. From the shape of a virus and how a drug can disable it, to keeping electrons flowing in the next generation of batteries. Neutrons truly are today’s super particle

Biography: Dr Helen Maynard-Casely is an Instrument Scientist based at ANSTO (the Australian Nuclear Science and Technology Organisation) where she uses neutrons to investigate the materials that make up our solar system. She has a PhD in high-pressure physics from the University of Edinburgh and has been lucky enough to have collected data in facilities all over the world.

The Claire Corani Memorial prizes, available for award to the top second-year female Physics student at each SA university in 2018, will be presented at the lecture.

Wednesday 3rd of April 2019 at 8pm
Kerr Grant Lecture Theatre
2nd Floor, Physics Building
The University of Adelaide
North Terrace, Adelaide

The Evolutionary Map of the Universe

Professor Ray Norris
CSIRO Astronomy & Space Science &
Western Sydney University

Abstract: The m Australian Square Kilometre Array Pathfinder (ASKAP) telescope is nearing completion in Western Australia. One of the key projects driving it is EMU – the Evolutionary Map of the Universe – which has an ambitious goal of studying the sky at radio wavelengths in unprecedented detail, boldly going where no telescope has gone before. Our scientific goal is to figure out how galaxies evolved in the early days of the Universe and how they evolve to the Universe we see today, with stars, planets, rocks, trees, and astronomers. What will we find? How will it change our view of how we got to be here? What is the role of black holes in regulating the growth of galaxies? And given that the most spectacular discoveries in astronomy are unexpected, we will be watching especially carefully for serendipitous discoveries that pop up in the data.

Bio: Professor Ray Norris is a British/Australian astronomer with CSIRO Astronomy & Space Science and Western Sydney University, who researches how galaxies formed and evolved after the Big Bang, and also researches the astronomy of  Aboriginal Australians. He frequently appears on radio and TV, featured in the stage show “The First Astronomers” with Wardaman elder Bill Yidumduma Harney, and has written the novel “Graven Images”.  He was educated at Cambridge University, and University of Manchester, UK, and moved to Australia to join CSIRO, where he became Head of Astrophysics in 1994, and then Deputy Director of the Australia Telescope, and Director of the Australian Astronomy Major National Research Facility, before returning in 2005 to active research. He currently leads an international project (EMU, or Evolutionary Map of the Universe) to understand the origin and evolution of galaxies, using the new Australian SKA Pathfinder radio-telescope nearing completion in Western Australia, and is also pioneering the WTF project to discover the unexpected in astronomical data.

Free – visitors welcome –  booking not required (*Please note – university security locks entrance doors at 8pm sharp*)

Thursday 28^th of February 2019 at 6.30 to 7.45 pm
Napier 102 lecture theatre, 1^st floor, Napier Building
University of Adelaide

Optical Tweezers ‘Demystified’

Assoc. Professor Bruce Wedding

University of South Australia

Since their invention 32 years ago, optical tweezers have become a powerful tool utilised in a wide variety of experiments in biology and physics. Optical tweezers use light to trap microscopic objects as small as 10 nm using radiation pressure from a focused laser beam. These trapped particles can then be manipulated and forces on the particles in the trap can be measured. The first designs of optical tweezers used high power lasers and expensive optical hardware. Recently however, simple and inexpensive apparatus for undergraduate laboratories can produce a single beam optical tweezer to trap micron-sized particles. Such a system in undergraduate laboratories and the resulting student engagement will be presented.

Interest in microfluidics is also a rapidly expanding area of research and the use of microchips as miniature chemical reactors, so called ‘Labs-on-a-Chip’ is increasingly common. Microfluidic channels are now complex and combine several functions on a single chip. Fluid flow details are important but relatively few experimental methods are available to probe the flow in a confined geometry. We can use optical trapping of a small dielectric particle to probe the fluid flow in microfluidic channels.

Rather than using the optical trap to position and release a particle for independent velocimetry measurement, we map the fluid flow by measuring the hydrodynamic force acting on a trapped particle. The flow rate of a dilute aqueous electrolyte flowing through a microchannel has been mapped using a small (1 µm diameter) silica particle. Such flow mapping is time efficient, reliable, and can be used in low-opacity suspensions flowing in microchannels of various geometries.

The Bronze Bragg medals and certificates will be presented at the lecture. The medal is awarded for highest achievement in Physics in 2018 in the SACE Stage 2 assessments, with certificates being for students who achieved a merit.

 The presentation and lecture will be held in the Napier 102 Lecture Theatre, Napier Building, 1^st floor, University of Adelaide, North Terrace, north from Pulteney St., at 6.30pm. Members of the public are warmly invited to attend. We are obliged for security reasons to keep the front door of the building attended, so please arrive before 6.30pm. Bookings are not available. The doors must be closed if all seats are taken.

Enquires: Email via aip_branchsecretary_sa@aip.org.au  mob: 0427 711 815.

Wednesday 5th of September 2018 at 8pm
Kerr Grant Lecture Theatre
2nd Floor, Physics Building
University of Adelaide
North Terrace, Adelaide

Dr. Sabrina Einecke
University of Adelaide

Abstract: When the term gamma radiation pops up, associations with radioactive hazards may arise. Do we have to be afraid of gamma radiation from space? Fortunately, we don’t have to be, because the Earth’s atmosphere protects us. Unfortunately, it also prevents us from directly observing this radiation from Earth. But it is in the nature of man to be curious to overcome these obstacles to investigate this vicious radiation from space. In 1961, a satellite was the first to detect gamma rays from space. At about the same time, the Cherenkov radiation was discovered – a radiation that is emitted when charged particles move through a medium at the speed of light. This led to a new technique, capable of measuring gamma rays from Earth, and paving the way for ground-based gamma-ray astronomy. However, it took 30 years until an appropriate experiment discovered the first gamma-ray emitting astrophysical source. Since then, hundreds of sources of Galactic and extragalactic origin have been discovered, and higher energies and sensitivities have been reached. The Cherenkov Telescope Array will exceed current experiments in a multitude of aspects: With more than 100 telescopes in 3 sizes at 2 locations equipped with state-of-the-art technologies, it will cover an area of 10 square kilometres on the ground, and it will provide a new view of the sky at energies of up to 300 TeV  – more than a 1000 billion times the energy of visible light. With its unprecedented capabilities, it will refine our knowledge tremendously and will mark the beginning of a new era of gamma-ray astronomy. Deeper insights into this field will be subject of this presentation.

Bio: Born around the time when Cherenkov telescopes made their first discovery, Sabrina Einecke is observing the extreme gamma-ray universe for more than 8 years. She took her first steps in gamma-ray astronomy with the ground-based experiments MAGIC, FACT and CTA. Completing research stays at the Columbia University in New York, she expanded her interests to the utilisation of machine learning approaches to combine a variety of multi-wavelength data to fully exploit the information that is available. This also led to her PhD thesis with the title “The Data Mining Guide to the Galaxy”. According to the German Physical Society, it has been among the best in Germany in 2017. After finishing her PhD studies in Germany, she moved to Australia and now supports the University of Adelaide as a postdoctoral research fellow. Her research focuses on Active Galactic Nuclei – the most extreme objects in the Universe – and data analysis using cutting-edge techniques from the fields of artificial intelligence and machine learning – crucial for handling the immense amount of data collected by next-generation experiments.