Events
November
2019
| Event Location: Hennings 201 | Speaker: Shirley Ho (Flatiron/Princeton)
The ever-increase need for accurate prediction for complex non-linear processes leads to large scale dynamical systems whose simulations and analysis make overwhelming and unmanageable demands on computational resources. The evolution of the Universe is one of these complex processes that the computational cost of the traditional full-order numerical simulations is extremely prohibitive.
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November
2019
| Event Location: Hennings 318 | Speaker: Hao Tjeng
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November
2019
| Event Location: Chem B250 2036 Main Mall, UBC Vancouver | Speaker: Thomas F. Rosenbaum Caltech
Why climb mountains when you can tunnel through them? Harnessing quantum tunneling holds great promise to speed up solutions to optimization problems, ranging from design of circuit boards to protein folding. When computers optimize, they are doing the analog of the physical process of annealing. I will discuss experiments on disordered magnets that quantitatively compare quantum and classical annealing, and demonstrate quantum speedup for reasons that can be understood at a microscopic level.
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November
2019
| Event Location: Hennings 201 | Speaker: Alexandre Brolo (UVic)
A variety of new properties emerges in nanostructured metallic materials. These new properties are consequence of the collective excitation of conducting electrons, known as surface-plasmon resonances (SPR). For instance, the color of noble metals, such as gold and silver, can be controlled at the nanoscale by tuning the geometric characteristics of the nanostructures. Surface plasmon (SP) waves can propagate at the surface of thin metal films and this property can be explored for 2D imaging applications.
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November
2019
| Event Location: Brimacombe 311 | Speaker: Stephen Wilson
Abstract: The triangular lattice of antiferromagetically coupled spins has long served as the paradigm of geometric magnetic frustration.
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November
2019
| Event Location: Room 203, Graduate Student Centre (6371 Crescent Road) | Speaker: OSCAR JAVIER HERNANDEZ
Abstract:
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November
2019
| Event Location: TRIUMF Auditorium | Speaker: Chun-Hui Chen (Iowa State)
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November
2019
| Event Location: Hennings 318 | Speaker: 12-1pm: lunch & poster sesson. 1-2pm: Positive Space by Dr. Rachael E. Sullivan (UBC Equity and Inclusion Office)
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November
2019
| Event Location: Hennings 318 | Speaker: Sarah Pearson (Flatiron)
Stellar streams form when a gravitationally bound ensemble of stars tidally
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October
2019
| Event Location: Hennings 201 | Speaker: David Griffiths (Reed)
In electrostatics any excess charge on a conductor goes to the surface. This is due, of course, to the mutual repulsion of like charges. But it depends critically on the precise form of Coulomb's law and on the dimensionality of the conductor. I will discuss some intriguing examples, including the vexed case of a conducting needle.
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October
2019
| Event Location: Brimacombe 311 | Speaker: Liang Wu
Abstract: The fundamental difference between electrons in a solid and those in high-energy physics is the absence of Poincare symmetry in lattice systems.
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October
2019
| Event Location: TRIUMF Auditorium | Speaker: Levon Pogosian (SFU)
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October
2019
| Event Location: Room 318, Hennings Bldg. | Speaker: ARIS CHATZICHRISTOS
Abstract:
It is well established that the properties of many materials change as their thickness is shrunk to the nanoscale, often yielding novel features at the near-surface region that are absent in the bulk. Even though there are several techniques that can study either the bulk or the surface of these materials, there are very few that can scan the near-surface region of crystals and thin films versus depth. Beta detected NMR (β-NMR) is capable of this and therefore has been established as a powerful tool for
material science.
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October
2019
| Event Location: Brimacombe 311 | Speaker: Domenico Giuliano
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October
2019
| Event Location: Hennings 318 | Speaker: Bradley Meyers (UBC)
Pulsars are unparalleled astrophysical tools, yet, after more than 50 years of research, we still do not fully understand the mechanism responsible for their radio emission. To further complicate the matter, the phenomenon of emission intermittency, where the pulsar radio emission ceases unpredictably, is also a mystery.
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October
2019
| Event Location: Hennings 201 | Speaker: James Charbonneau
Climate and energy are prominent topics in the news and in our daily lives. We hear things like doubling the amount of CO2 in the atmosphere will raise the temperature of the Earth by 3 degrees. UBC's sustainability reports tell us that simply heating our classrooms, offices, and labs produces the equivalent of 42,000 tonnes of CO2 a year.
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October
2019
| Event Location: Brimacombe 311 | Speaker: Adam Tsen, University of Waterloo
The recent discoveries of ferromagnetism in single atomic layers have opened a new avenue for two-dimensional (2D) materials research. Not only do they raise fundamental questions regarding the requirements for long-range magnetic order in low-dimensional systems, but they also provide a new platform for the development of spintronic devices. In this talk, I will present a series of studies on the family of layered ferromagnetic semiconductors, CrX3 (X = I, Br, Cl), in the atomically thin limit.
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October
2019
| Event Location: Hennings 318 | Speaker: Seunghwan Lim
The Sunyaev-Zeldovich effect (SZE) provides a promising avenue to explore the properties of gas associated with halos and large-scale structures. However, due to contamination by the primary CMB, as well as foregrounds, projection effects, halo identification, and the beam size of current CMB surveys, it is not a trivial task to extract the signal precisely and accurately.
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October
2019
| Event Location: Hennings 201 | Speaker: Ravindra Bhatt (Princeton)
The decades following the initial discovery of the integer and fractional quantum Hall effects (IQHE/FQHE) in two-dimensional electrons in a strong perpendicular magnetic field led to a detailed understanding of the rich phase diagram and exotic phenomena characterizing various phases. These include charge fractionalization, Abelian and non-Abelian quantum states, topological spin excitations, charge-density-wave phases, to name a few. This body of work paved the way for the new field of topological materials in the 21st century.
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October
2019
| Event Location: AMPEL room 311 | Speaker: Martin Cross
Abstract:
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October
2019
| Event Location: Buchanan A201 1866 Main Mall Block A, UBC campus | Speaker: Dan Friedmann (Chair, Carbon Engineering)
To stem the rise of global temperatures we must reduce CO2 emissions. Recently, a Canadian clean energy company, Carbon Engineering Ltd. has developed an industrially-scalable “Direct Air Capture” technology to address this global problem. This technology removes CO2 directly from the atmosphere and can permanently store it underground. In addition, it can be used to reduce emissions by producing ultra-low carbon synthetic fuels, which can power existing cars, trucks and airplanes without any modifications.
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October
2019
| Event Location: TRIUMF Auditorium | Speaker: Jamie Forrest (U Waterloo)
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October
2019
| Event Location: Hennings 201 | Speaker: Avery Broderick (Waterloo/PI)
Black holes are, without question, one of the most bizarre and mysterious phenomena predicted by Einstein's theory of general relativity. They correspond to infinitely dense, compact regions in space and time, where gravity is so extreme that nothing, not even light, can escape from within. And, their existence raises some of the most challenging questions about the nature of space and time. Over the past few decades, astronomers have identified numerous tantalizing observations that suggested that black holes are real. This past April, the search for confirmat
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October
2019
| Event Location: Brim 311 | Speaker: Jun Zhu
Abstract : The advent of two-dimensional materials with hexagonal crystal symmetry offers a new electronic degree of freedom, namely valley, the manipulation and detection of which could potentially be exploited to form new many-body ground states as well as new paradigms of electronic applications.
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October
2019
| Event Location: Room 4524 (Teaching Room), BC Cancer-Vancouver | Speaker: SHIQIN SU
Abstract:
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October
2019
| Event Location: Hennings 318 | Speaker: Phil Korngut
Recently selected for implementation as the next medium-class mission in NASA's Explorer line, SPHEREx will produce a Near Infrared spectrum for every 6 arcsecond pixel on the celestial sphere. Through the use of cold wide-field optics combined with linear variable filters, this experiment is optimized to probe for signatures of inflation, imprinted on the large-scale structure of the Universe. Key science goals also include surveying the Milky Way for water and other biogenic ices, as well as tracing the history of cosmic light production through fluctuation studies of the NIR
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October
2019
| Event Location: Hennings 201 | Speaker: Carl Haber (LBNL)
Sound was first recorded and reproduced by Thomas Edison in 1877. Until about 1950, when magnetic tape use became common, most recordings were made on mechanical media such as wax, foil, shellac, lacquer, and plastic. Some of these older recordings contain material of great historical interest, but may be in obsolete formats, and are damaged, decaying, or are now considered too delicate to play. Unlike print and latent image scanning, the playback of mechanical sound carriers has been inherently invasive. Recently, techniques, based upon non-contact optical metrology
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October
2019
| Event Location: TRIUMF Auditorium | Speaker: Gregory MacDougall (U Illinois)
Spinel antiferromagnets have long been at the center of research into strong spin-lattice coupling and orbital effects. Among other properties, these materials frequently demonstrate concomitant magnetic and structural phase transitions, heightened magneto-elastic or dielectric response functions, and low-temperature multiferroism. There is very little agreement on the microscopic picture to be associated with these effects, but recent work has shown that mesoscale inhomogeneity can play a key role in raising the susceptibilities of complex materials to external perturbations.
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October
2019
| Event Location: Room 309, Hennings Bldg | Speaker: ILARIA CAIAZZO
Abstract:
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September
2019
| Event Location: Hennings 318 | Speaker: Tilman Troester (Edinburgh)
Baryonic processes that alter the large-scale distribution of gas, and thus the matter power spectrum, such as AGN feedback, are one of the the main systematics in current and future weak lensing surveys. Left uncorrected, these effects will bias the inferred properties of dark matter and dark energy that these surveys are designed to measure. Characterising the distribution of gas is thus of vital importance if these surveys are to be exploited to their full potential.
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September
2019
| Event Location: Hennings 201 | Speaker: Frank Close (University of Oxford)
Trinity was the codename for the test explosion of the atomic bomb in New Mexico on 16 July 1945. Frank Close tells the story of: the bomb's metaphorical father, Rudolf Peierls (Prof. Close's one time mentor in Oxford); his intellectual son, the atomic spy Klaus Fuchs; and the ghosts of the security services in Britain, the USA and USSR. Frank will reveal new insights from MI5 files in the British National Archives, and documents of the FBI and KGB.
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September
2019
| Event Location: Room 318 Hennings, 6224 Agricultural Road | Speaker: ERICH LEISTENSCHNEIDER
Abstract:
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September
2019
| Event Location: BRIM 311 | Speaker: Lance Cooley
Abstract : Magnets are unarguably the "killer app" of superconductivity, with medical imaging magnets comprising an annual $2 billion market that consumes about 1000 tons of superconductor per year, and magnets for large science projects contributing a similar share.
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September
2019
| Event Location: Room 203 of the Graduate Student Centre (6371 Crescent Road) | Speaker: PASCAL ALEXANDER NIGGE
Abstract:
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September
2019
| Event Location: Hennings 318 | Speaker: Eve Lee (McGill)
From gas-poor Earths to gas-rich Jupiters, planets come in a variety of sizes. I will describe the physics behind the diversity of exoplanets - how the core and gas assembly processes give rise to the observed distribution of radii and orbital periods. Basic astrophysical considerations of gas dynamical friction, gravitational scattering, collisional mergers, and gas accretion by cooling inform us that planets smaller than Neptune likely emerged in situ, in the late stages of disk evolution.
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September
2019
| Event Location: TRIUMF Auditorium | Speaker: Frank Close (Oxford U)
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September
2019
| Event Location: Hennings 201 | Speaker: David Zimmerman (UVic)
David Zimmerman is Professor of History at the University of Victoria, British Columbia, Canada. He is the author of "Britain's Shield: Radar and the Defeat of the Luftwaffe"; "Top Secret Exchange: The Tizard Mission and the Scientific War"; "The Great Naval Battle of Ottawa"; "Coastal Fort: A History of Fort Sullivan, Maine"; and "Maritime Command Pacific: The Royal Canadian Navy in the Pacific during the Early Cold War".
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September
2019
| Event Location: TRIUMF Auditorium | Speaker: Jessica McIver (UBC)
Advanced LIGO and Advanced Virgo are currently in the middle of their third observing run, and releasing open public event alerts for the first time. The LIGO-Virgo collaboration has issued 28 un-retracted candidate event alerts as of September 11th, 2019, potentially adding dozens more known compact binary object mergers to the eleven confident detections from the first two Advanced-era observing runs. I'll give an overview of the process of detecting, characterizing, and assessing the significance of gravitational wave signals registered in Advanced LIGO data.
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September
2019
| Event Location: BRIM 311 | Speaker: Ulrich Hoefer
Abstract:
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September
2019
| Event Location: Room 158, Irving K. Barber, 1961 East Mall | Speaker: FIRAS HASAN MOOSVI
Abstract:
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September
2019
| Event Location: Room 200, Graduate Student Centre (6371 Crescent Road) | Speaker: EMILY ALTIERE
Abstract:
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September
2019
| Event Location: Hennings 318 | Speaker: Todd Henry (RECONS Institute / Georgia State University)
The nearest stars and their companions provide the fundamental framework upon which all of stellar astronomy is based, for individual stars, stellar multiples, and entire stellar populations. We live in exciting times, as our map of the Sun's neighbors becomes enriched with details of other solar systems that will ultimately play key roles in our search for life elsewhere.
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September
2019
| Event Location: BRIM 311 | Speaker: Nathan Wiebe, University of Washington
We provide the first method for fully quantum generative training of quantum Boltzmann machines with both visible and hidden units while using quantum relative entropy as an objective. This is significant because prior methods were not able to do so due to mathematical challenges posed by the gradient evaluation. We present two novel methods for solving this problem.
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September
2019
| Event Location: Hennings 201 | Speaker: Nathan Wiebe (U Washington)
In recent years, quantum experiments have become increasingly complicated, with modern experiments pushing the limits of even our best supercomputers to simulate. This increased complexity has made quantum devices challenging to model, which in turn makes them both difficult to control in quantum technologies and also exceedingly difficult to understand. In this talk, I will show how ideas from machine learning and statistical inference can be used to probe complex quantum systems. In particular, we will show how these methods can allow us to identify common pathologies in
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September
2019
| Event Location: Brim 311 | Speaker: Julia Link
Abstract: In the hydrodynamic regime it is possible to investigate the universal collision-dominated dynamics of the isolated electron fluid, while the couplings to the lattice and to impurities becomes secondary. An important transport property is the shear viscosity which describes whether the electron fluid behaves laminar or turbulent. The ratio shear viscosity over entropy is bounded from below and is an indicator for how strongly the system is interacting [Kovtun].
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September
2019
| Event Location: TRIUMF Auditorium | Speaker: Yoshitaka Kuno (Osaka U)
Muon to electron conversion is a process which violates the conservation of charged lepton flavor. It is forbidden in the Standard Model, but new physics beyond the SM predict its sizable rate. New experiments under preparation in Japan and the US will start soon in a few years, aiming at improvement of four orders of magnitude, with new innovative muon sources. This talk will discuss Its physics motivation, and an outlook on the experiments.
Special seminar in honour of Toshio Numao.
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September
2019
| Event Location: TRIUMF Auditorium | Speaker: Hongbo Zhu (Chinese Academy of Sciences, IHEP)
We found a Higgs boson and are learning more its properties with collision data from the Large Hadron Collider (LHC) and its future upgrade HL-LHC. But to unveil the fundamental nature of this particle and to explore potential new physics, we would need high energy electron-positron colliders with high luminosity. In this talk, I will introduce such an initiative from China, the Circular Electron Positron Collider (CEPC). I will discuss its science case, the conceptual design, and the status and prospects of the project.
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September
2019
| Event Location: Hennings 318 | Speaker: Norbert Werner (MTA-Eötvös University)
Most galaxies comparable to or larger than the mass of the Milky Way host hot, X-ray emitting atmospheres, and many such galaxies are radio sources. Hot atmospheres and radio jets and lobes are the ingredients of radio-mechanical active galactic nucleus (AGN) feedback. While a consensus has emerged that such feedback suppresses cooling of hot cluster atmospheres, less attention has been paid to massive galaxies where similar mechanisms are at play.
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September
2019
| Event Location: Room 309, Hennings Bldg | Speaker: JENNIFER LEANNE MOROZ
Abstract:
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September
2019
| Event Location: Hennings 201 | Speaker: Jason Barnes (U Idaho)
NASA recently selected the Dragonfly quadcopter, on which I serve as Deputy Principal Investigator, as the fourth mission in its New Frontiers program of planetary missions. Dragonfly will land on the surface of Saturn's hazy moon Titan to explore prebiotic chemistry, to evaluate its habitability, and look for chemical biosignatures. Titan is one of just 4 planetary bodies that has both a thick atmosphere and a solid surface - Venus, Earth, and Mars are the others.
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