Events
October
2018
| Event Location: AMPEL 311 | Speaker: Prof. Joe Trodahl from MacDiarmid Institute for Advanced Materials and Nanotechnology, Victoria University of Wellington
Controlling the flow of electronic spin in addition to the charge promises speed and power demand advantages. However, there are as yet few “spintronic” devices on the market, in part due to a lack of intrinsic ferromagnetic semiconductors that would permit full exploitation of the coupled spin/charge technology. To date the only full series of such materials are the mononitrides of the lanthanides, the 14 rare-earth elements.
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October
2018
| Event Location: TRIUMF Auditorium | Speaker: David DeMille (Yale University)
Time-reversal (T) symmetry is observed to be broken in K- and B-meson systems, in a manner consistent with the Standard Model (SM) of electroweak interactions. Violation of T-invariance makes it possible for elementary particles such as the electron to have an electric dipole moment (EDM) along their spin axis. Although the SM prediction for the electron EDM is too small to detect, extensions to the SM frequently predict EDMs within a few orders of magnitude of the current limits.
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October
2018
| Event Location: Henn 318 | Speaker: James Charbonneau
We introduce ComPAIR, an open source, peer feedback and teaching technology developed at UBC that provides students a safe, flexible environment to develop the skill of evaluating another person’s work, and in turn, receive evaluations from their peers. ComPAIR is currently being used by about 40 courses here at UBC and has been installed at three external institutions. Particularly in introductory courses, the effectiveness of peer feedback can be limited by the relative newness of students to both the course content and the skills involved in providing good feedback.
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October
2018
| Event Location: Room B319, Buchanan Building Block B | Speaker: AGUEDA PAULA GRANADOS CONTRERAS
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October
2018
| Event Location: Hennings 318 | Speaker: Toby Brown (MxMaster)
Every star in our Milky Way, and in all other galaxies, was born from the collapse of a cloud of hydrogen gas. The importance of cold gas in galaxy evolution is therefore well established, as is its role as a probe of recent environmental effects on galaxies. However, sensitivity limitations mean the extent to which internal and external processes drive variations in the gas-star formation cycle of galaxies remains unclear.
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October
2018
| Event Location: Henn 309 | Speaker: Yue Shen
This talk introduces an empirical method for determining the excited-state fraction of atoms in a magneto-optical trap (MOT).
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October
2018
| Event Location: Hennings 201 | Speaker: Bill Louis (LANL)
The LSND and MiniBooNE short-baseline neutrino experiments have provided evidence for neutrino oscillations at a mass scale of approximately 1 eV. When combined with oscillation measurements at the solar and atmospheric mass scales, these experiments imply the existence of more than three neutrino mass states and, therefore, one or more "sterile" neutrinos. Such sterile neutrinos, if proven to exist, would have a big impact on particle physics, nuclear physics, and astrophysics, and would contribute to the dark matter of the Universe.
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October
2018
| Event Location: AMPL 311 | Speaker: Dr. Pedro Lopes, from QMI
Fractional Josephson effects comprise some of the main signatures of topological features and quasi-particle fractionalization in Josephson junctions.
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October
2018
| Event Location: TRIUMF Auditorium | Speaker: Bill Louis (Los Alamos National Laboratory)
The MiniBooNE experiment at Fermilab observes an excess of 460.5+-99.0 nue CCQE candidate events in the 200 < E < 1250 MeV energy range, corresponding to a significance of 4.7 sigma. If interpreted in a two-neutrino oscillation model, numu -> nue, the best oscillation fit to the excess has a probability of 21.1%, while the background-only fit has a chisquare probability of 6E-7 relative to the best fit. The MiniBooNE data are consistent in energy and magnitude with the excess events observed by the LSND experiment.
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October
2018
| Event Location: Stay home if you can |
There will be no turkey dinner in Hennings 318. Sorry.
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October
2018
| Event Location: Room 318, Hennings Building | Speaker: NIKITA BERNIER
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October
2018
| Event Location: Hennings 201 | Speaker: Corinne Manogue (Oregon)
The Paradigms in Physics program began 20 years ago at Oregon State University. In those two decades, we not only completely restructured the content trajectory for majors to be more aligned with how professionals think about the content, but we also designed many course activities which reflect not only our own education research but also results from other PER and DBER groups.
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October
2018
| Event Location: TRIUMF Auditorium | Speaker: Rod Clark (Lawrence Berkeley National Lab)
Where does the Periodic Table end? What is the mass of the heaviest atomic nucleus? With the addition of four new elements in 2015, the seventh row of the table is now complete, but answers to such basic questions remain elusive. I will present a brief review of the current status of the topic, and recent controversies in the field, including the failure to directly determine the atomic number, Z, and mass number, A, of many of the newly discovered superheavy isotopes. Then I will turn to describing new efforts to address outstanding issues.
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October
2018
| Event Location: Henn 318 | Speaker: Lincoln D. Carr, Colorado School of Mines, Golden, Colorado, USA
There are now over 300 quantum simulators on at least 10 separate architectures with long coherence times and controlled dynamics. These experimental systems have generated tremendous excitement about driven interacting quantum systems resulting in physics ranging from time crystals to dynamical many-body localization. The quantum ratchet adds a new feature to periodic driving: a preferred direction in both time and space, i.e., parity and time-reversal symmetry-breaking. By studying weakly interacting ultracold bosons in a quantum ratchet on a ring in position, mome
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October
2018
| Event Location: Hennings Building - RM 202 (6224 Agricultural Road) UBC | Speaker: Rainer Blatt
Since the mid-1990s, we have seen how computers and many of their applications can be enhanced using quantum physics. This is timely since "Moores law", for the continuing development of conventional computers, will not apply to ever-smaller electronic components governed by quantum physics. All computations, in our heads or in computational devices, rely on the real physical processes of data input, data representation in a memory, data manipulation using algorithms and finally, data output.
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October
2018
| Event Location: AMPEL 311 | Speaker: Dr. Bernhard Keimer, Max Planck Institute for Solid State Research
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October
2018
| Event Location: Hennings 318 | Speaker: Holger Baumgardt (University of Queensland)
Supermassive black holes are thought to exist in the centres of most massive galaxies and their masses have been found to correlate strongly with the properties of their host galaxies like overall luminosity or central velocity dispersion. Yet it is unknown what processes have established these correlations and if and how they continue towards lower mass systems. In my talk I will present results from our search for massive black holes in ultra-compact dwarf galaxies in nearby galaxies and in massive globular clusters of the Milky Way.
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September
2018
| Event Location: Room 309, Hennings Building | Speaker: Byron Wilson
Abstract:
Introduction: Stereotactic Radiosurgery is the delivery of a large, highly focused radiation dose to well defined targets in the brain. This thesis explores linac-based inverse planning algorithms that can be implemented to improve the dosimetric and delivery performance of Volumetric ModulatedArc Therapy treatments for these indications.
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September
2018
| Event Location: Hennings 201 |
Our group is investigating the mechanics of a key structural protein, collagen, which is comprised of three chains that coil to make a triple helix. Collagen is the fundamental structural protein in vertebrates and is widely used as biomaterial, for example as a substrate for tissue engineering. In spite of its prevalence and mechanical importance in biology, the mechanics of collagen is surprisingly unresolved.
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September
2018
| Event Location: Hennings 201 | Speaker: Nancy Forde (SFU)
Our group is investigating the mechanics of a key structural protein, collagen, which is comprised of three chains that coil to make a triple helix. Collagen is the fundamental structural protein in vertebrates and is widely used as biomaterial, for example as a substrate for tissue engineering. In spite of its prevalence and mechanical importance in biology, the mechanics of collagen is surprisingly unresolved.
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September
2018
| Event Location: AMPL 311 | Speaker: Stéphane Ouvry, Université Paris Sud
I will first give a review of the thermodynamics of the anyon model and the Lowest Landau Level (LLL) anyon model (i.e. anyons coupled to a strong external magnetic field), in relation to that of the Calogero model and Haldane fractional statistics. Then I will construct explicitly an $N$-body kernel which maps Calogero eigenstates onto anyonic eigenstates (arXiv: 1805.09899).
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September
2018
| Event Location: TRIUMF Auditorium | Speaker: Brad Filippone (Caltech)
Symmetry principles are basic tenets for our theory of fundamental interactions. While they have been essential in building the theory, it is in their violations were major breakthroughs have often occurred. We will discuss how searches for symmetry violations can play a key role in elucidating the details of the fundamental forces. We will focus on the role of past and future precision measurements using free neutrons.
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September
2018
| Event Location: Hennings 318 | Speaker: Andrea Bellini (Space Telescope Science Institute)
With the advent of the Gaia mission, astrometry is experiencing a renaissance. Although Gaia will make important breakthroughs in many different areas, stars in the crowded central fields of globular clusters and at the faint end of the color-magnitude diagram are out of Gaia's reach. However, the stable environment of space makes the Hubble Space Telescope (HST) an excellent astrometric tool. Its diffraction-limited resolution allows it to distinguish and measure positions and brightnesses for faint stars all the way to the center of most globular clusters.
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September
2018
| Event Location: Hennings 201 | Speaker: Douglas Scott
The Cosmic Gravitational Wave Background (CGB) is a
hypothesized relic radiation field that, if detected, would give us
clues to the earliest moments of the history of the Universe. In this
talk, accessible to students and non-experts, I will describe the
physical processes that can give rise to a CGB, novel features including
a net polarization of the gravitational waves (as distinct from the
polarization of cosmic microwave background photons), and methods of
detection. I will also discuss the ability of the proposed Laser
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September
2018
| Event Location: Hennings 318 | Speaker: Dr. Alberto Nocera, Research Associate at SBQMI
Over the past decade, Resonant Inelastic X-Ray Scattering spectroscopy (RIXS) has been established as a powerful technique to study the energy-momentum structure of charge, orbital, lattice, and magnetic excitations of strongly correlated materials.
The computation of RIXS spectra starting from model Hamiltonians is often a formidable task because of the absence of accurate many-body tools,
particularly when many orbitals are active. In most cases, exact diagonalization (ED) techniques are used which restricts clusters to a relatively small size.
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September
2018
| Event Location: Hennings 318 | Speaker: Jean-Luc Margot (Dept. Earth, Planetary & Space Sciences Dept. Physics & Astronomy, UCLA)
Profound developments in our understanding of the Earth, Moon, and other planetary bodies have been enabled by rotation studies. I will describe the application of a new Earth-based radar technique that enables high-precision measurements of planetary spin states and provides powerful probes of planetary interior structure and processes.
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September
2018
| Event Location: UBC Life Building | Speaker: Francois Bouchet
Dr. Francois Bouchet will describe current observations that precisely constrain the nature of the Cosmos in which we live, leading to radical ideas for the origin of the structures within it. These touch on questions such as: How did the Universe originate? What is it made of? Why is it the way that it is? What is the nature of the Dark Matter and Dark Energy that dominate the Universe? How do we actually learn about these? And what are the new mysteries that our observations are revealing?
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September
2018
| Event Location: Hennings 201 | Speaker: Sarah Keller (Univ. Washington)
(No prior knowledge of biology is required for this talk!) For decades, scientists have argued about how living cell membranes acquire and maintain regions enriched in particular lipid and protein types. One of the more contentious theories has been that lipids and proteins spontaneously phase separate within the plane of the membrane to create liquid regions that differ in their composition. Physicists have long observed this type of demixing in simple artificial membranes. Clear identification of the same transition in a living biological system has heretofore been elusive.
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September
2018
| Event Location: CEME 1210 | Speaker: HUAI-CHE (KEN) YEH
Abstract:
We study the noncommutative geometry associated to matrices of N quantum dots in the matrix models. The earlier work established a surface embedded in flat R^3 from three Hermitian matrices. We construct coherent states corresponding to points in the emergent geometry and find the original matrices determine not only shape of the emergent surface, but also a unique Poisson structure. We prove that commutators of matrix operators correspond to Poisson brackets. Through our construction, we can realize arbitrary noncommutative membranes embedded in R^3.
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September
2018
| Event Location: AMPL 311 | Speaker: Pr. Marcel Franz from UBC
Inclusion of topological phenomena in condensed matter physics over the past 10 years ushered a revolution in this field. As a result of the new theoretical insights entire classes of materials with exotic properties have been discovered, including topological insulators, Dirac and Weyl semimetals as well as topological superconductors containing Majorana fermions. In this talk I will give a brief review of these developments and discuss an intriguing connection noticed recently by Kitaev between one such topological system – the Sachdev-Ye-Kitaev model – and the horizon of a black hole.
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September
2018
| Event Location: Hennings 318 | Speaker: Francois Bouchet (Institut d'Astrophysique de Paris)
Please join us before the Colloquium in Hennings 318 for coffee, tea and snacks at 2:45 pm
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September
2018
| Event Location: Hennings 201 | Speaker: Pisin Chen (Nat. Taiwan Univ.)
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September
2018
| Event Location: TRIUMF Auditorium | Speaker: Mirko Miorelli (TRIUMF)
Electromagnetic probes represent a fundamental tool to study nuclear structure and dynamics. The perturbative nature of the electromagnetic interaction allows for a clean connection between calculated nuclear structure properties and measured cross sections. Ab initio methods
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September
2018
| Event Location: Hennings 318 | Speaker: Harold Steinacker
Quantized comological spacetimes and higher spin gauge theory in the IKKT model
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August
2018
| Event Location: Hennings 309B | Speaker: Markus Frembs, University College London
Contextuality—the obstruction to describing quantum mechanics in a classical statistical way—has been proposed as a resource that powers quantum computing. The measurement-based model provides a concrete manifestation of contextuality as a computational re
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August
2018
| Event Location: TRIUMF Auditorium | Speaker: Olivia Di Matteo (U Waterloo/Institute for Quantum Computing)
The field of quantum computing has grown rapidly over the last decade. Physical systems with high double-digit numbers of qubits are expected within the coming year. As the machines continue to grow in size, they will be able to run increasingly sophisticated quantum algorithms. Some of these algorithms, such as Shor's factoring algorithm, will have serious repercussions on parts of our cryptographic infrastructure. This leads to an important question: how big of a quantum computer do we need to run an algorithm? To do so fault-tolerantly? Moreover, how long will it take?
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August
2018
| Event Location: Room 318, Hennings Building | Speaker: ALAN MANNING
Abstract:
A major goal of the Magnetic Resonance Imaging (MRI) community is myelin quantification. MRI contrast depends on tissue microstructure, so quantitative models require good understanding of Nuclear Magnetic Resonance (NMR) physics in these complex, heterogeneous environments. In this thesis, we study the underlying physics behind two different 1 H contrast mechanisms in white and grey matter tissue: T 1 relaxation and the recently developed Inhomogeneous Magnetization Transfer (ihMT).
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August
2018
| Event Location: TRIUMF Auditorium | Speaker: Roland Diehl (Max Planck Institute for Extraterrestrial Physics Garching)
Gamma-ray lines from cosmic sources display the action of nuclear reactions in cosmic sites. The gamma rays at such characteristic energies result from nuclear transitions following radioactive decays or high-energy collisions with excitation of nuclei. The gamma-ray line and its associated special continuum from the annihilation of positrons at 511 keV falls into the same energy window, although of different origin.
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August
2018
| Event Location: AMPEL #311 | Speaker: Kyle Wamer
A lattice of interacting Majorana modes can occur in a superconducting film on a topological insulator in a magnetic field. The phase diagram as a function of interaction strength for the square lattice was analyzed recently using a combination of mean field theory and field theory and was found to include second order phase transitions. One of these corresponds to sponta- neous breaking of an emergent U(1) symmetry, for attractive interactions.
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August
2018
| Event Location: Room 311, Brimacombe Building | Speaker: SHADI BALANDEH
Abstract:
Hole doped bismuth perovskite is one of the rare examples of a three-dimensional high transition temperature superconducting oxide (Tc = 34K) without a transition metal cation. The undoped compound, BaBiO3, also shows closely interlinked electronic and structural phase transitions and a controversial insulating mechanism. Understanding the electronic structure of the parent compound, BaBiO3, can give valuable insight into both its superconducting mechanism, in particular, and into the physics of the perovskites family, in general.
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August
2018
| Event Location: Brimacombe 311 | Speaker: Jae-Hoon Park, ( Max Plank )
Large spin-orbit coupling makes the magnetic eigenstate of the total angular momentum state with an admixed spin state and induces unusual magnetic behaviors. In cooperation with the crystal field, it could introduce the Kramers doublet in the magnetic ion site. Then the magnetism is described with the so-called spin-orbit coupled isospin 1/2, and the system often displays novel quantum magnetism behaviors. On the other hand, the admixed spin states possibly introduce anisotropic spin-spin interactions involving the inter-site hopping.
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June
2018
| Event Location: TRIUMF Auditorium | Speaker: Costel Petrache (Université de Paris Sud)
The breaking of symmetries in quantum systems is one of the key issues in nuclear physics. In particular, the spontaneous symmetry breaking in rotating nuclei leads to exotic collective modes, like the wobbling and chiral motions, which are unique fingerprints of triaxiality in nuclei and have been intensively studied in recent years.
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May
2018
| Event Location: AMPL 311 | Speaker: Mark Blamire, Department of Materials Science, University of Cambridge, UK
The discovery in 2010, using superconductor / ferromagnet / superconductor Josephson junctions, that it is possible to controllably create triplet Cooper pairs in which the electrons have parallel spins created the field of superconducting spin electronics (superspintronics) [1]. However, even if triplet pairing implies that supercurrents can carry spin, this is not in itself sufficient to create functioning superspintronic devices. In parallel, a variety of other interactions between singlet superconductivity and magnetism have been actively explored.
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May
2018
| Event Location: TRIUMF Auditorium | Speaker: Martin Fertl (U Washington)
Neutrino flavor oscillation experiments prove that neutrinos do have nonzero masses. Extensions to the Standard Model of Particle Physics have been developed to explain the non-zero masses and can be directly tested by a measurement of the absolute neutrino mass scale. The mass of the electron antineutrino can be determined from the highest precision measurement of the beta-decay spectrum of tritium around its endpoint region (Q = 18.6 keV). The current state of the art experiment stretches all technological limits to probe the range of the electron antineutrino mass down to 200meV.
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May
2018
| Event Location: See event website | Speaker: Multiple Science Departments at UBC
Join us for The University of British Columbia’s 2018 Science Rendezvous festival. Science Rendezvous is an annual festival held across Canada showcasing the Art in Science. This year’s theme is “Full S.T.E.A.M. Ahead!” and will emphasize science, technology, engineering, art, and math (STEAM) research and innovation.
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May
2018
| Event Location: TRIUMF Auditorium | Speaker: Paul Lecoq (CERN)
The future generation of radiation detectors is more and more demanding on timing performance for a wide range of applications, such as time of flight (TOF) techniques for PET cameras and particle identification in nuclear physics and high energy physics detectors, precise event time tagging in high luminosity accelerators and a number of photonic applications based on single photon detection. A target of 10ps coincidence time resolution in TOFPET scanners would introduce a paradigm shift in PET imaging.
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May
2018
| Event Location: TRIUMF Auditorium |
Understanding the origin of the elements is one of the major challenges of modern astrophysics. The rapid neutron-capture process, or r-process, is one of the fundamental ways that stars produce the elements listed along the bottom 2/3 of the periodic table, but key aspects of the r-process are still poorly understood. I will describe three major advances in the last few years that have succeeded in confirming neutron star mergers as an important site of the r-process.
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April
2018
| Event Location: Room 1221, Forest Sciences Building | Speaker: Ian Affleck et al
The Stewart Blusson Quantum Matter Institute is pleased to invite you to attend the workshop: 30 years of AKLT: Interacting Systems in Low Dimensions
INTERNATIONAL SYMPOSIUM CELEBRATING 30 YEARS OF THE AFFLECK-KENNEDY-LIEB-TASAKI PARADIGM
Invited Speakers
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April
2018
| Event Location: Room 309, Hennings Building | Speaker: Jennifer Moroz
The accuracy of Pharmacokinetic model fit parameters is highly sensitive to the quality of the contrast-time curves acquired in the tissue of interest and within a blood vessel feeding the tissue. The later curve is commonly referred to as the arterial input function (AIF). It is difficult to measure the AIF in pre-clinical studies in mice due to their small body size and limited number of vessels of a sufficient size. As a result, several groups will use a population averaged curve from the literature.
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April
2018
| Event Location: Room 309, Hennings Building | Speaker: Steffen Henkelmann
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