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This Week at Physics

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Events During the Week of February 12th through February 19th, 2017

Monday, February 13th, 2017

Plasma Physics (Physics/ECE/NE 922) Seminar
Plasma Material Interaction in Radiation Environments - the Next Grand Challenge- CANCELLED
Time: 12:00 pm
Place: 2317 Engineering Hall
Speaker: Dr. Juergen Rapp, Oak Ridge National Laboratory, USA
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Cosmology Journal Club
An Informal discussion about a broad variety of arXiv papers related to Cosmology
Time: 12:15 pm
Place: 5242 Chamberlin Hall
Abstract: Please visit the following link for more details:
http://cmb.physics.wisc.edu/journal/index.html
Please feel free to bring your lunch!
If you have questions or comments about this journal club, would like to propose a topic or volunteer to introduce a paper, please email Amol Upadhye (aupadhye@wisc.edu).
Host: Amol Upadhye
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Tuesday, February 14th, 2017

Chaos & Complex Systems Seminar
Functional integration and split in the brain
Time: 12:05 pm
Place: 4274 Chamberlin (refreshments will be served)
Speaker: Shun Sasai, UW Department of Psychiatry
Abstract: We often engage in two concurrent but unrelated activities, such as driving on a quiet road while talking over the phone. When the conversation is unrelated to driving, how does the brain manage these two concurrent flows? I will present our recent work showing that a brain may functionally split into two separate 'driving' and 'listening' systems when a listening task is unrelated to concurrent driving, but not when the two tasks are related.
Host: Clint Sprott
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"Physics Today" Undergrad Colloquium (Physics 301)
Direct Dark Matter Detection and LZ
Time: 1:20 pm
Place: 2241 Chamberlin Hall
Speaker: Kimberly J. Palladino, UW Madison Department of Physics
Host: Wesley Smith
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NPAC (Nuclear/Particle/Astro/Cosmo) Forum
Studying Neutrino Oscillations at NOvA: From Experimental Design to Pioneering Analysis
Time: 4:00 pm
Place: 4274 Chamberlin Hall
Speaker: Alexander Radovic, William and Mary
Abstract: The observation of neutrino oscillations provides evidence of physics beyond the standard model, and the precise measurement of those oscillations remains an important goal for the field of particle physics. NOνA is one of the foremost experiments in that field. Taking advantage of a two-detector technique, a tightly focused off-axis view of the NuMI neutrino beam, and a pair of finely instrumented liquid scintillator detectors, NOνA is in a prime position to contribute to precision measurements of the neutrino mass splitting, mass hierarchy, and CP violation.

This presentation will describe the goals and design of the NOνA experiment, and outline how the cutting edge tools of the Deep Learning community are being used to push the limits of that design. The latest oscillation results will be shown, along with a guide to what to expect from NOvA in the coming years.
Host: Sridhara Dasu
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Wednesday, February 15th, 2017

No events scheduled

Thursday, February 16th, 2017

R. G. Herb Condensed Matter Seminar
Exploring the analogy between atoms and optical nanoresonators -- atomic metasurfaces, super-scattering, and super-radiant thermal emission
Time: 10:00 am
Place: Chamberlin 5310
Speaker: Zongfu Yu, UW-Madison
Abstract: I will use a few examples to show that the exploration of the analogy between atoms and optical nano-resonators could be quite interesting and useful. In the first example, I will discuss how atoms might help to overcome the most daunting challenges in optical metasurfaces, which promise to revolutionize optical instruments by replacing delicate and expensive lenses with integrated flat components. Then, I will discuss quantum antenna, in an analogy to optical antenna. I will show how to drastically enhance the optical cross section of atoms using topologically nontrivial optical media. Lastly, I will discuss the effect of super-radiance in thermal radiation, which could provide an interesting way to control thermal energy conversion.
Host: Vavilov
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NPAC (Nuclear/Particle/Astro/Cosmo) Forum
Physics with a 10-year Color Movie of 40 Billion Stars and Galaxies
Time: 1:30 pm
Place: 5310 Chamberlin Hall
Speaker: Keith Bechtol, Large Synoptic Survey Telescope
Abstract: Steady advances in telescope and camera technology have allowed us to explore the night sky deeper, wider, and faster with each new generation of instruments. The next major experiment in this endeavor is the Large Synoptic Survey Telescope (LSST), now under construction in Chile, with first light scheduled in 2020. LSST will catalog more stars and galaxies than all previous astronomical surveys combined, and will monitor transient, variable, and moving objects over a ten-year period, generating ~10 million alerts each night. In addition to precision cosmological constraints for dark energy, dark matter, neutrino physics, and inflation, the resulting multipurpose dataset will enable discoveries in time-domain, Galactic, and Solar System astronomy. By turning the night sky into a giant publicly-accessible database, LSST will also create new opportunities for education and public outreach.<br><br>
Host: Sridhara Dasu
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Astronomy Colloquium
Systematic Serendipity: Novel Discoveries in Astronomical Surveys
Time: 3:30 pm
Place: 4421 Sterling Hall, Coffee and cookies 3:30 PM, Talk Begins 3:45 PM
Speaker: Lucianne Walkowicz, Chicago Planetarium
Abstract: As of last year, the Large Synoptic Survey Telescope (LSST) has begun construction on the summit of Cerro Pachon. As the top-rated flagship for ground-based astronomy in the next decade, LSST will provide an unprecedented dataset of 37 billion objects observed in both space and time. The time domain aspect of LSST is an especially promising source of new discoveries: the main survey is expected to generate new samples of thousands of supernovae, cataclysmic variables, stellar flares, and regular variables, amongst other denizens of the time-domain zoo, each one of which will generate an "alert" within 60 seconds of observation. Sorting amongst these transient and variable objects poses a challenging task: transient events of interest must be identified and prioritized, so that valuable follow-up resources (which are easily saturated by the volume of LSST alerts per night) are deployed on the events with the most potential to provide transformative understanding of particular phenomena. For LSST, this task is of course at a beyond-human scale, requiring sophisticated machine learning algorithms to provide real-time characterization and prioritization. However, another challenge looms under the surface of the approaching flood of data: how can truly novel phenomena be recognized and discovered in large datasets? In this talk, I will discuss methods and applications of finding anomalous data in astronomical datasets. Anomaly identification is a powerful means to both discover novel phenomena, as well as to identify problematic data so that it may be cleaned from the database. Lastly, hunting down anomalies is an exciting way to engage citizen scientists in astronomical discovery, whose efforts have repeatedly demonstrated the power of the crowd in uncovering previously-unnoticed phenomena.
Host: Astronomy Department
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NPAC (Nuclear/Particle/Astro/Cosmo) Forum
Unlocking neutrino mysteries with the NOvA experiment
Time: 4:00 pm
Place: 4274 Chamberlin Hall
Speaker: Chris Backhouse, Caltech
Abstract: The 2015 Nobel Prize in Physics was awarded for the discovery of the phenomenon of neutrino oscillations, which implies that neutrinos are not massless as we had previously believed. This raises a wealth of new and intriguing questions. What is the ordering of the neutrino mass states? Might they violate matter/antimatter symmetry? What structure, if any, does the neutrino mixing matrix have? The NOvA experiment directly addresses these questions by measuring changes undergone by a powerful neutrino beam over an 810km baseline, from its source at Fermilab, Illinois to a huge 14kton detector in Ash River, Minnesota. I will give a brief overview of neutrino oscillations, then present our latest results, their implications, and prospects for the future.
Host: Sridhara Dasu
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Friday, February 17th, 2017

Physics Department Colloquium
The basic physics of collisionless magnetic reconnection
Time: 3:30 pm
Place: 2241 Chamberlin hall
Speaker: Michael Hesse, NASA & Birkeland Centre for Space Science
Abstract: Magnetic reconnection is a plasma process, which enables, by means of highly localized physics, the often-explosive release of stored magnetic energy over very large spatial scales. Magnetic reconnection is believed to play a key role in the dynamics of plasmas in a diverse multitude of environments, which include pulsar magnetospheres on one end, and laboratory plasmas on the other. Owing both to this universality and to the impact of reconnection, the underlying physics has been a target or research for quite some time. However, only the advent of advanced computer simulations and, most recently, the revealing space observations of the Magnetospheric Multiscale (MMS) mission have facilitated breakthroughs in our understanding of the critical local physics in the so-called diffusion region. This talk will present recent research results pertaining to the diffusion region. As an introduction, we will review the role reconnection plays as an energy release and conversion process, and briefly look at a variety of applications. We will then focus on reconnection at the Earth’s magnetopause, and will investigate in detail a high-precision numerical simulation of reconnection in this environment. Thereafter, we will look into the role of the reconnection electric field in sustaining the current flow in the inner diffusion region. We will end by demonstrating that complex particle behavior, which leads to population mixing and an effective, thermal, inertia, is critical aspect of this region.
Host: Jan Egedal
Video: https://vod.physics.wisc.edu/media/2017_02_17.m4v
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