https://ubc.zoom.us/j/64183011430?pwd=U2lFNXEwSmlBRWVBdTR5OG1ZdlVSZz09
Meeting ID: 641 8301 1430
Passcode: 113399
Ultrafast dynamics of excitons, electrons and phonons in momentum space
| Event Location: via Zoom | Speaker: ÉTIENNE LANTAGNE-HURTUBISE
Abstract:
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| Event Location: Zoom link in description | Speaker: Anthony K. Cheetham - Materials Research Laboratory, UCSB
CM Seminar - Thu, April 8th 10am
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| Event Location: Connect via zoom | Speaker: Douglas Scott (UBC)
1st April has traditionally been a day for japes and high jinks in many realms of life - with science not being entirely excluded! In observance of this day I will review the use of humour in physics and astronomy, focusing on some specific examples, particularly those involving April Fool's Day.
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| Event Location: Zoom link in description | Speaker: Jacob Taylor – University of Maryland
https://ubc.zoom.us/j/64183011430?pwd=U2lFNXEwSmlBRWVBdTR5OG1ZdlVSZz09
Meeting ID: 641 8301 1430
Passcode: 113399
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| Event Location: Connect via Zoom | Speaker: Colby DeLisle (UBC)
Soft factorization has been shown to hold to sub-leading order in QED and to sub-sub-leading order in perturbative quantum gravity, with various loop and non-universal corrections that can be found. In a recent paper, we show that all terms factorizing at tree level can be uniquely identified as boundary terms that exist already in the classical expressions for the electric current and stress tensor of a point particle.
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| Event Location: Connect via zoom | Speaker: Lloyd Knox (UC Davis)
The most precise of the direct measurements of the current rate of cosmic expansion (the Hubble constant) is inconsistent with the even more precise, but indirect, model-dependent inferences. In particular the Riess et al. (2020) measurement is more than four standard deviations higher than the inference based on the standard cosmological model, with its free parameters constrained by Planck satellite observations of the cosmic microwave background.
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| Event Location: via Zoom | Speaker: EDWARD ASHTON
Abstract: (please see this link)
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| Event Location: Connect via zoom | Speaker: Paul Corkum (U Ottawa)
An electron that multiphoton ionizes is immediately subject to the light's electric field that will control its short-term future. This control enables a gas of atoms to produce intense VUV or soft X-ray beams. Since we can precisely control the infrared beam, we can synthesize attosecond soft X-ray pulses - pulses that are the shortest controlled events ever systematically produced. For a complex atom (such as xenon), the recollision electron shares its energy in any multi-electron interaction.
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| Event Location: Zoom link in description | Speaker: Xiaodong Xu, Department of Physics, Department of Materials Science and Engineering
CM Seminar - Thu, March 25, 10am (PST)
https://ubc.zoom.us/j/64183011430?pwd=U2lFNXEwSmlBRWVBdTR5OG1ZdlVSZz09
Meeting ID: 641 8301 1430
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| Event Location: via Zoom | Speaker: Brandon Stuart
Abstract:
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| Event Location: Connect via zoom | Speaker: Susan Clark (Princeton IAS)
Magnetic fields thread our Milky Way Galaxy, influencing interstellar physics from cosmic ray propagation to star formation. The magnetic interstellar medium is also a formidable foreground for experimental cosmology, particularly for the quest to find signatures of inflation in the polarized cosmic microwave background (CMB). Despite its importance across scientific realms, the structure of the Galactic magnetic field is not well understood.
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| Event Location: via Zoom | Speaker: GIACOMO GALLINA
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| Event Location: Connect via zoom | Speaker: Juan Maldacena (Princeton IAS)
Black holes are interesting spacetime configurations predicted by general relativity. When quantum mechanics is taken into account, black holes are found to emit thermal radiation, called "Hawking radiation".
During the past couple of years a surprising new way to compute its entropy has emerged. This result indicates that the black hole formation and evaporation is consistent with standard quantum mechanical laws.
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| Event Location: via Zoom | Speaker: ALEX MAY
Abstract:
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| Event Location: Connect via Zoom | Speaker: Deborah Good, UBC
The success of gravitational wave observations of stellar mass black hole mergers and neutron star mergers has proven that observational gravitational wave astronomy has an important part to play in coming years. However, ground-based laser interferometers can access only a limited portion of the gravitational wave spectrum.
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| Event Location: Connect via zoom | Speaker: Dale E. Gary
Abstract: New Jersey Institute of Technology's Expanded Owens Valley Solar Array (EOVSA) has amply demonstrated the power of radio imaging spectroscopy for imaging and quantitative diagnostics of both the flaring and non-flaring Sun. The unique sensitivity of radio emission to the flaring coronal magnetic field has been dramatically shown in a series of recent papers, along with accelerated-electron diagnostics in the same volume. The coming solar maximum (cycle 25) is slated to peak in 2025-2026, which promises to bring new space- and ground-based instruments together with
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| Event Location: via Zoom | Speaker: MARCUS ANDREW SONIER
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| Event Location: Connect via zoom | Speaker: Tom Davis (FactSet Research Systems)
The connection between physics and finance goes back hundreds of years, and the names of the earliest physicists who studied finance may be surprising. In the 18th century Bernoulli discovered Euler's constant e when investigating compound interest; mo
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| Event Location: Zoom link in description | Speaker: Kate Ross, Colorado State University
https://ubc.zoom.us/j/64183011430?pwd=U2lFNXEwSmlBRWVBdTR5OG1ZdlVSZz09
Meeting ID: 641 8301 1430
Passcode: 113399
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| Event Location: Connect via Zoom | Speaker: Markus Aspelmeyer, University of Vienna
No experiment today provides evidence that gravity requires a quantum description. It has been suggested that one can at least exclude the possibility for semiclassical gravity by performing an experiment whose outcome cannot be explained by a purely classical source mass configuration.
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| Event Location: Connect via zoom | Speaker: Ryan Trainor (Franklin & Marshall)
Lyman-alpha emission is produced ubiquitously by excited hydrogen, so it is a powerful tracer of the interactions among gas, stars, and AGN that shape galaxy formation. However, the resonant scattering of this emission line makes its interpretation complex. In this talk, I will describe three related surveys of galaxies at z~2-3 that make use of Lyman-alpha emission: the Keck Baryonic Structure Survey (KBSS), the KBSS-Lya, and the Keck Lyman Continuum Survey (KCLS).
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| Event Location: via Zoom | Speaker: VINCENT WAI SUM WONG
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| Event Location: Connect via zoom | Speaker: Andre Marziali (UBC)
While motorsports events can appear to the general viewing public as a parade of cars driving around tracks in circles, in reality race drivers operating their cars at the grip limit are constantly on a razor's edge, balancing and adjusting the behavior of the car with a variety of inputs and techniques that are foreign to the average road driver.
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| Event Location: Zoom | Speaker: Eva Pavarini - Institute for Advanced Simulation, Forschungszentrum Jülich
https://ubc.zoom.us/j/64183011430?pwd=U2lFNXEwSmlBRWVBdTR5OG1ZdlVSZz09
Meeting ID: 641 8301 1430
Passcode: 113399
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| Event Location: Zoom | Speaker: Hans Boschker, Max-Planck-Institute for Solid State Physics Stuttgart, Germany
https://ubc.zoom.us/j/68506225698?pwd=S2ZBRGsrbzZBQVVZZFNwYk5ZSEduQT09
Meeting ID: 685 0622 5698
Passcode: 113399
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| Event Location: Connect via Zoom | Speaker: Steve Carlip, UC Davis
It has been suggested that Planck-scale "spacetime foam" could have significant macroscopic consequences, perhaps even offering a way to address the cosmological constant problem. I will describe progress in constructing a locally spherically symmetric minisuperspace model with a positive cosmological constant that may shed light on th
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| Event Location: Virtual | Speaker: PHAS undergraduate program advisors and student representatives
Are you a first year UBC student interested in physics or astronomy degree programs? Or, you are just curious in general, wondering what students in PHAS programs study? Join us on Monday, March 1st at 5:30pm for "Meet Your Major" - chat with PHAS academic advisors and student representatives to learn more about options available for you!
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| Event Location: Connect via zoom | Speaker: Brice Menard (Johns Hopkins)
Is your data too complex? This can help. In this talk, we will introduce the scattering transform, a novel approach to extract information from complex data. We will explain its principle and show that it shares mathematical similarities with convolutional neural nets — but it does not require any training and is interpretable! We will demonstrate its power by applying it to datasets in astronomy, cosmology and oceanography for parameter estimation and outlier detection.
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| Event Location: Connect via zoom | Speaker: P&A graduate students
We'll find out about research happening in several different areas of Physics & Astronomy.
Come and support our graduate students in the Departmental heat of the annual 3-minute thesis competition!
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| Event Location: Zoom | Speaker: NATHAN EVETTS
Abstract:
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| Event Location: Zoom link in description | Speaker: Ralph Ernstorfer, Fritz Haber Institute of the Max Planck Society
https://ubc.zoom.us/j/64183011430?pwd=U2lFNXEwSmlBRWVBdTR5OG1ZdlVSZz09
Meeting ID: 641 8301 1430
Passcode: 113399
Ultrafast dynamics of excitons, electrons and phonons in momentum space
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| Event Location: Connect via Zoom | Speaker: Luis Lehner (Perimeter Institute)
Within systems producing gravitational waves detectable by current gravitational wave detectors, those that also yield electromagnetic signals are particularly interesting. Binary neutron stars do so in a spectacular way, which has been illustrated by the event GW170817.
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| Event Location: Connect via zoom | Speaker: Sarah Greenstreet (UWashington)
We discovered two new dynamical populations of astero
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| Event Location: via Zoom | Speaker: ALON HERSHENHORN
Abstract:
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| Event Location: Connect via zoom | Speaker: Max Tegmark (MIT)
A central goal of physics is to discover mathematical
patterns in data. For example, after four years of analyzing data
tables on planetary orbits, Johannes Kepler started a scientific
revolution in 1605 by discovering that Mars' orbit was an ellipse. I
describe how we can automate such tasks with machine learning and not
only discover symbolic formulas accurately matching datasets
(so-called symbolic regression), equations of motion and conserved
quantities, but also auto-discover which degrees of freedom are most
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| Event Location: Zoom link in description | Speaker: Erica Carlson, Purdue University
https://ubc.zoom.us/j/64183011430?pwd=U2lFNXEwSmlBRWVBdTR5OG1ZdlVSZz09
Meeting ID: 641 8301 1430
Passcode: 113399
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| Event Location: Connect via Zoom | Speaker: Richard Shaw (UBC)
CHIME will use Intensity Mapping of the 21cm line of neutral hydrogen to map large-scale structure between redshifts of 0.8 and 2.5.
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| Event Location: Connect via zoom | Speaker: Mike Webster (University of Nevada, Reno)
Sensory systems are constantly recalibrating their sensitivity and response properties to match the statistics of the current stimulus environment. These adaptations are intrinsic to neural coding and affect all stages of processing, profoundly impacting every perceptual experience. In our work we explore how vision is adapted to the natural visual world, and how it adjusts to changes in the world (e.g. as we move to a different environment) or to changes in the observer (e.g. as we age).
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| Event Location: Zoom | Speaker: Michel Devoret, Yale University
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| Event Location: Connect via Zoom | Speaker: Djuna Croon, TRIUMF
In this talk I will demonstrate the potential of the black hole mass gap to probe new physics. The mass gap, in which no black holes can be formed, is a standard prediction of stellar structure theory.
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| Event Location: Connect via zoom | Speaker: Qianjun Hang (Edinburgh)
Large-scale structures (LSS) can leave various imprints on the cosmic microwave background(CMB). Two main features come from the spatial and temporal perturbations of the CMB photon trajectory due to LSS: weak lensing and the integrated Sachs-Wolfe effect. I will give a summary of our paper "Galaxy clustering in Legacy Survey and its imprint on the CMB" (arXiv: 2010.00466), where we use the DESI Legacy Imaging Survey to extract cosmological information from the above effects in the redshift range 0<z<0.8.
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| Event Location: https://ubc.zoom.us/j/69495792445?pwd=RURFQmt1S3UwSE1FYk9YQUFweWxUZz09 Passcode: 764070 | Speaker: Andrew Potter
Building quantum technology, from electronic devices to quantum computers, requires achieving precision control over the quantum correlations and entanglement of many particles.
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| Event Location: Connect via zoom | Speaker: Noemie Globus (ELI Beamlines / Flatiron Institute) and Roger D Blandford (Stanford University/KIPAC)
Understanding the origin of life surely qualifies as one of the deepest and most perplexing questions facing humankind. While we have not yet reached a consensus on the definition of life, biological homochirality seems to be part of the definition as a necessary step for life's emergence. The unraveling of its origin require interdisciplinary research, by exploring each of fundamental physics, modern chemistry, astrophysics and biology. In this talk, We will focus on the origin of biological homochirality in the context of astrophysics and particle physics.
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| Event Location: Zoom link in description | Speaker: Speaker: Aline Ramires (Paul Scherrer Institute)
https://ubc.zoom.us/j/64183011430?pwd=U2lFNXEwSmlBRWVBdTR5OG1ZdlVSZz09
Meeting ID: 641 8301 1430
Passcode: 113399
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| Event Location: Connect via Zoom | Speaker: Maximiliano Isi, MIT
The LIGO and Virgo gravitational wave detectors carried out the first half of their third observing run from April through October, 2019. During this period, they collected 39 new detections of compact binary coalescences, which were compiled in the second LIGO-Virgo catalog (GWTC-2).
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| Event Location: Connect via zoom | Speaker: Steven Vance (JPL)
This lecture will describe recent research evaluating the magnetic induction characteristics of model Europa oceans (Vance et al. 2020). I will highlight how this work relates to efforts to understand the habitability of Europa and other icy ocean worlds. I will also provide an overview of NASA's planned Europa Clipper mission, set to conduct multiple flybys of Europa toward the end of the decade.
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| Event Location: https://ubc.zoom.us/j/62870796359?pwd=SkNWNnB4SW5mOWpEUUxCVE1pcWorUT09 Passcode: 581018 | Speaker: Ella Lachman
Quantum materials are rapidly emerging as the basis for possible novel computation devices. However,
fully understanding the interplay between magnetic and electronic excitations are preventing us from
realizing their full potential. In my talk I will show how realizing the microscopic magnetic textures in
quantum materials is crucial to the understanding of transport phenomena on the macro scale.
I will demonstrate this with two examples from two different types of materials. First, I will show how
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| Event Location: via Zoom | Speaker: ANNA HUGHES
Abstract:
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| Event Location: Connect via zoom | Speaker: Alexandre Blais (Sherbrooke)
By exploiting effects such as quantum superpositions and entanglement, quantum computers could solve problems that are intractable on standard, classical, computers. While building a full-scale quantum computer capable of rivalling today's supercomputers remains a challenge, the last few years have seen tremendous improvements in our ability to build small superconducting quantum processors and run simple algorithms on these processors. In this talk, I will review some of the basic concepts that could allow quantum computers to outperform their classical counterparts.
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| Event Location: Zoom link in description | Speaker: Jörg Schmalian, Karlsruhe Institute of Technology
https://ubc.zoom.us/j/64183011430?pwd=U2lFNXEwSmlBRWVBdTR5OG1ZdlVSZz09
Meeting ID: 641 8301 1430
Passcode: 113399
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