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January

2019

| Event Location: Henn 318 | Speaker: Masahiro Hotta, Tohoku University, Japan

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 Where do entangled quantum systems store information in a total pure state? This question is nontrivial and interesting since the entanglement among subsystems delocalizes the information, and is significantly related to the information loss problem of evaporating black holes.  So far, a common picture is that of a subsystem and its purification partner sharing the information quantum mechanically.

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Add to Calendar 2019-01-16T13:00:00 2019-01-16T14:00:00 Partners and Quantum Information Capsules  Where do entangled quantum systems store information in a total pure state? This question is nontrivial and interesting since the entanglement among subsystems delocalizes the information, and is significantly related to the information loss problem of evaporating black holes.  So far, a common picture is that of a subsystem and its purification partner sharing the information quantum mechanically. Event Location: Henn 318

January

2019

| Event Location: Hennings 318 | Speaker: Stephen Portillo (U Washington)

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The depth of next generation surveys poses a great data analysis challenge: these surveys will suffer from crowding, making their images difficult to deblend and catalogue. Sources in crowded fields are extremely covariant with their neighbours and blending makes even the number of sources ambiguous. Probabilistic cataloguing returns an ensemble of catalogues inferred from the image and can address these difficulties. We present the first optical probabilistic catalogue, cataloguing a crowded Sloan Digital Sky Survey r band image cutout from Messier 2.

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Add to Calendar 2019-01-14T15:00:00 2019-01-14T16:00:00 Counting Stars: Developing Probabilistic Cataloguing for Crowded Fields The depth of next generation surveys poses a great data analysis challenge: these surveys will suffer from crowding, making their images difficult to deblend and catalogue. Sources in crowded fields are extremely covariant with their neighbours and blending makes even the number of sources ambiguous. Probabilistic cataloguing returns an ensemble of catalogues inferred from the image and can address these difficulties. We present the first optical probabilistic catalogue, cataloguing a crowded Sloan Digital Sky Survey r band image cutout from Messier 2. Event Location: Hennings 318

January

2019

| Event Location: Room 309, Hennings Building | Speaker: SAUL CUEN-ROCHIN

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Abstract:

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Add to Calendar 2019-01-11T10:00:00 2019-01-11T12:00:00 Departmental Oral Examination (Thesis Title: “Precise Measurement of Rare Pion Decay”) Abstract: Event Location: Room 309, Hennings Building

January

2019

| Event Location: Hennings 201 | Speaker: Cohl Furey (Cambridge)

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Grand unified theories envision the standard model of particle physics
as a piece of a larger system.  However, in this talk we will ask the
opposite question:  Could the standard model result from a set of
algebras much smaller than itself?

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Add to Calendar 2019-01-10T16:00:00 2019-01-10T17:00:00 Towards a more efficient model of particle physics Grand unified theories envision the standard model of particle physics as a piece of a larger system.  However, in this talk we will ask the opposite question:  Could the standard model result from a set of algebras much smaller than itself? Event Location: Hennings 201

January

2019

| Event Location: BRIM 311, Stewart Blusson Quantum Matter Institute, 2355 East Mall | Speaker: Hong Guo, Center for the Physics of Materials and Department of Physics, McGill University

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Materials informatics (MI) may be considered the 4th paradigm of scientific inquiry, in addition to experimental, theoretical and computational approaches. MI is made possible by the universal access to abundant scientific data, assisted by advances in software and machine learning (ML) to analyze the data. For materials problems with specific designing goals, physics-based indicators (or assumptions) are necessary to help narrowing down the informatics search.

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Add to Calendar 2019-01-10T14:00:00 2019-01-10T15:00:00 CM Seminar: Materials Informatics: the 4th paradigm Abstract Materials informatics (MI) may be considered the 4th paradigm of scientific inquiry, in addition to experimental, theoretical and computational approaches. MI is made possible by the universal access to abundant scientific data, assisted by advances in software and machine learning (ML) to analyze the data. For materials problems with specific designing goals, physics-based indicators (or assumptions) are necessary to help narrowing down the informatics search. Event Location: BRIM 311, Stewart Blusson Quantum Matter Institute, 2355 East Mall

January

2019

| Event Location: Hennings 318 | Speaker: Brett Gladman & Aaron Boley (UBC)

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On 1st January 2019 the New Horizons spacecraft encountered a small body beyond Neptune named Ultima Thule. In this informal collquium we will cover the initial results that have emerged this week and provide background on the importance of the science that can be addressed.

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Add to Calendar 2019-01-07T15:00:00 2019-01-07T16:00:00 The New Horizons spacecraft's encounter with the small Kuiper Belt object Ultima Thule On 1st January 2019 the New Horizons spacecraft encountered a small body beyond Neptune named Ultima Thule. In this informal collquium we will cover the initial results that have emerged this week and provide background on the importance of the science that can be addressed. Event Location: Hennings 318

December

2018

| Event Location: BRIM 311 2355 East Mall Vancouver BC V6T 1Z4 | Speaker: Can-Ming Hu

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Add to Calendar 2018-12-20T14:00:00 2018-12-20T15:00:00 CM Seminar: Cavity Spintronics Event Location: BRIM 311 2355 East Mall Vancouver BC V6T 1Z4

December

2018

| Event Location: Room 311, Brimacombe Building, 2355 East Mall | Speaker: ARASH KHAZRAIE ZAMANPOUR

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Add to Calendar 2018-12-14T14:00:00 2018-12-14T16:00:00 Final PhD Oral Examination (Thesis Title: “A first principle study of the electronic structure of the bismuthates") Examination Programme Event Location: Room 311, Brimacombe Building, 2355 East Mall

December

2018

| Event Location: BRIM 311 Stewart Blusson Quantum Matter Institute 2355 East Mall Vancouver BC V6T 1Z4 | Speaker: Yuri V. Gusev Lebedev Research Center in Physics, Moscow

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The finite temperature field theory for condensed matter physics, based on the kernel of the evolution equation, was recently proposed. The field theory is scale-free formalism, so it denies the absolute scale of thermodynamic temperature and uses dimensionless thermal variables, which are defined by the group velocities of sound and the interatomic distances, combined with the defining constants of the New SI. The universal thermal functional is obtained and used to derive the specific heat of condensed matter.

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Add to Calendar 2018-12-13T14:00:00 2018-12-13T15:00:00 CM Seminar: The field theory of specific heat The finite temperature field theory for condensed matter physics, based on the kernel of the evolution equation, was recently proposed. The field theory is scale-free formalism, so it denies the absolute scale of thermodynamic temperature and uses dimensionless thermal variables, which are defined by the group velocities of sound and the interatomic distances, combined with the defining constants of the New SI. The universal thermal functional is obtained and used to derive the specific heat of condensed matter. Event Location: BRIM 311 Stewart Blusson Quantum Matter Institute 2355 East Mall Vancouver BC V6T 1Z4

December

2018

| Event Location: MCML 256, HR MacMillan Building, 2357 Main Mall | Speaker: HUAI-CHE (KEN) YEH

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Abstract:

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Add to Calendar 2018-12-11T12:30:00 2018-12-11T14:30:00 Final PhD Oral Examination (Thesis Title: “Emergent Spacetime in Matrix Models”) Abstract: Event Location: MCML 256, HR MacMillan Building, 2357 Main Mall

December

2018

| Event Location: Hennings 318 | Speaker: Natalie Batalha (UC Santa Cruz)

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On 30th October, the Kepler spacecraft was powered down, initiating the final closeout sequence to cease operations.  We'll pay homage to the mission by playing back some of the science highlights.  We'll also consider Kepler's exoplanet legacy - what it leaves behind and what roles it yet has to play in the next era of exoplanet exploration led by TESS and JWST.

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Add to Calendar 2018-12-10T15:00:00 2018-12-10T16:00:00 Goodnight, and thanks for all the planets On 30th October, the Kepler spacecraft was powered down, initiating the final closeout sequence to cease operations.  We'll pay homage to the mission by playing back some of the science highlights.  We'll also consider Kepler's exoplanet legacy - what it leaves behind and what roles it yet has to play in the next era of exoplanet exploration led by TESS and JWST. Event Location: Hennings 318

December

2018

| Event Location: LIFE building room 2201, 6138 Student Union Boulevard (UBC CAMPUS). The North Parkade is the closest parking lot to the LIFE Building. | Speaker: UBC faculty, staff, and students.

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WHERE: LIFE building room 2201, 6138 Student Union Boulevard (UBC CAMPUS). The North Parkade is the closest parking lot to the LIFE Building.

WHEN: SUNDAY, December 9, 2018, 2:00-3:30 PM

COST: FREE! (But bring non-perishable food items to support the Greater Vancouver Food Bank!) No RSVP required, though we recommend arriving 15-20 minutes earlier for good seats.

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Add to Calendar 2018-12-09T14:00:00 2018-12-09T15:30:00 Magic? Or Physics? 2019 Faraday Science Show WHERE: LIFE building room 2201, 6138 Student Union Boulevard (UBC CAMPUS). The North Parkade is the closest parking lot to the LIFE Building. WHEN: SUNDAY, December 9, 2018, 2:00-3:30 PM COST: FREE! (But bring non-perishable food items to support the Greater Vancouver Food Bank!) No RSVP required, though we recommend arriving 15-20 minutes earlier for good seats. Event Location: LIFE building room 2201, 6138 Student Union Boulevard (UBC CAMPUS). The North Parkade is the closest parking lot to the LIFE Building.

December

2018

| Event Location: LIFE building room 2201, 6138 Student Union Boulevard (UBC CAMPUS). The North Parkade is the closest parking lot to the LIFE Building. | Speaker: UBC faculty, staff, and students.

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FLAT Faraday Show poster 8.5x11 poster_0.jpgWHERE: LIFE building room 2201, 6138 Student Union Boulevard (UBC CAMPUS). The North Parkade is the closest parking lot to the LIFE Building.

WHEN: SUNDAY, December 9, 2018, 2:00-3:30 PM

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Add to Calendar 2018-12-09T14:00:00 2018-12-09T15:30:00 Magic? Or Physics? 2018 Faraday Science Show WHERE: LIFE building room 2201, 6138 Student Union Boulevard (UBC CAMPUS). The North Parkade is the closest parking lot to the LIFE Building. WHEN: SUNDAY, December 9, 2018, 2:00-3:30 PM Event Location: LIFE building room 2201, 6138 Student Union Boulevard (UBC CAMPUS). The North Parkade is the closest parking lot to the LIFE Building.

December

2018

| Event Location: Hennings 201 | Speaker: Chris Waltham (UBC)

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The Western violin and the erhu, the Chinese violin, are at first glance, markedly different instruments, being apparently related only by their bows. The violin soundbox is made of spruce and maple, has a complex shape, and an asymmetrical interior. The erhu soundbox is a simple cylinder closed on one side by a pre-tensioned python skin and open at the other. However, delving into the vibro-acoustics of each structure, deep similarities emerge, both with each other and with that most ancient musical instrument, the human voice.

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Add to Calendar 2018-12-06T16:00:00 2018-12-06T17:00:00 The human voice, the erhu and the violin The Western violin and the erhu, the Chinese violin, are at first glance, markedly different instruments, being apparently related only by their bows. The violin soundbox is made of spruce and maple, has a complex shape, and an asymmetrical interior. The erhu soundbox is a simple cylinder closed on one side by a pre-tensioned python skin and open at the other. However, delving into the vibro-acoustics of each structure, deep similarities emerge, both with each other and with that most ancient musical instrument, the human voice. Event Location: Hennings 201

December

2018

| Event Location: BRIM 311 2355 East Mall Vancouver BC V6T 1Z4 | Speaker: Kenji M. Kojima Research Scientist, TRIUMF and Affiliated Associate Professor, SBQMI

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A S=1/2 polarized particle, which may couple to the near-by electron is the simplest quantum mechanical object, as you may find in the standard text books. In reality, a particle called positive muon (µ+), provides such experimental observations. TRIUMF in the UBC south campus, which is also my home institute since this August, provides muon beams for material science research.

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Add to Calendar 2018-12-06T14:00:00 2018-12-06T15:00:00 CM Seminar: Muons for the Quantum Matter A S=1/2 polarized particle, which may couple to the near-by electron is the simplest quantum mechanical object, as you may find in the standard text books. In reality, a particle called positive muon (µ+), provides such experimental observations. TRIUMF in the UBC south campus, which is also my home institute since this August, provides muon beams for material science research. Event Location: BRIM 311 2355 East Mall Vancouver BC V6T 1Z4

December

2018

| Event Location: Henn 318. 6224 Agricultural Rd. | Speaker: Jordan Wilson-Gerow, UBC

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Add to Calendar 2018-12-05T12:30:00 2018-12-05T13:30:00 A Functional Approach to Soft Graviton Induced Decoherence Event Location: Henn 318. 6224 Agricultural Rd.

December

2018

| Event Location: Hennings 318 | Speaker: Kevin France (University of Colorado Boulder)

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ABSTRACT: High-energy photons and particles from stars regulate the atmospheric temperature structure and photochemistry on orbiting planets, influencing the long-term stability of planetary atmospheres and the production of potential “biomarker” gases.  Rocky planets orbiting low-mass stars (M dwarfs) will likely be the first exoplanets directly probed for signs of life, however, relatively few observational and theoretical constraints exist on the high-energy irradiance from typical (i.e., weakly active) M dwarf exoplanet host stars.  In this talk, I will describe results f

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Add to Calendar 2018-12-03T15:00:00 2018-12-03T16:00:00 The Potential Habitability of Rocky Planets around Red Dwarfs: Stellar Drivers for Atmospheric Chemistry and Stability ABSTRACT: High-energy photons and particles from stars regulate the atmospheric temperature structure and photochemistry on orbiting planets, influencing the long-term stability of planetary atmospheres and the production of potential “biomarker” gases.  Rocky planets orbiting low-mass stars (M dwarfs) will likely be the first exoplanets directly probed for signs of life, however, relatively few observational and theoretical constraints exist on the high-energy irradiance from typical (i.e., weakly active) M dwarf exoplanet host stars.  In this talk, I will describe results f Event Location: Hennings 318

December

2018

| Event Location: Hennings 318 | Speaker: Ilia Tutunnikov, Weizmann Institute of Science, Israel

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Orientation and alignment of molecules by ultrashort laser pulses is crucial for a variety of applications and have long been of interest in physics and chemistry, with the special emphasis on stereodynamics in chemical reactions and molecular orbitals imaging. As compared to the laser induced molecular alignment, which has been extensively studied and demonstrated, achieving molecular orientation is a much more challenging task, especially in the case of asymmetric-top molecules.

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Add to Calendar 2018-12-03T10:00:00 2018-12-03T11:00:00 All-optical Field-free Three-Dimensional Orientation of Asymmetric-Top Molecules Orientation and alignment of molecules by ultrashort laser pulses is crucial for a variety of applications and have long been of interest in physics and chemistry, with the special emphasis on stereodynamics in chemical reactions and molecular orbitals imaging. As compared to the laser induced molecular alignment, which has been extensively studied and demonstrated, achieving molecular orientation is a much more challenging task, especially in the case of asymmetric-top molecules. Event Location: Hennings 318

November

2018

| Event Location: Hennings 309 | Speaker: Philip W. Phillips University of Illinois at Urbana-Champaign

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It is well known that the dimension of conserved currents is determined simply from dimensional analysis. However, a recent proposal is that what is strange about the conserved currents in the strange metal in the cuprate superconductors is that they carry anomalous dimensions. The basic model invoked to exhibit such behaviour is a holographic dilatonic one in which the field strength couples to the radial coordinate. I will show that the anomalous dimension in such cases arises from a fractional electromagnetism that can be thought of as a general loop-hole in Noether's second theorem.

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Add to Calendar 2018-11-30T11:00:00 2018-11-30T12:00:00 Anomalous Dimensions for Conserved Currents from Holographic Dilatonic Models to Superconductivity It is well known that the dimension of conserved currents is determined simply from dimensional analysis. However, a recent proposal is that what is strange about the conserved currents in the strange metal in the cuprate superconductors is that they carry anomalous dimensions. The basic model invoked to exhibit such behaviour is a holographic dilatonic one in which the field strength couples to the radial coordinate. I will show that the anomalous dimension in such cases arises from a fractional electromagnetism that can be thought of as a general loop-hole in Noether's second theorem. Event Location: Hennings 309

November

2018

| Event Location: Hennings 201 | Speaker: David Jaffray (Toronto)

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Our characterization of cancer is advancing rapidly through the ever-increasing ability to make quantitative measurements of the cancerous tissues with new tools and technologies.

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Add to Calendar 2018-11-29T16:00:00 2018-11-29T17:00:00 The Future of Cancer Medicine: Personal or Industrial? Our characterization of cancer is advancing rapidly through the ever-increasing ability to make quantitative measurements of the cancerous tissues with new tools and technologies. Event Location: Hennings 201

November

2018

| Event Location: AMPL 311 | Speaker: Prof. Philip W. Phillips from the University of Illinois

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In a recent paper, the MIT group led Pablo Jarillo-Herrero has found that doping twisted bi-layer graphene can generate strongly correlated insulating states and superconductivity at particular twist angles called magic angles.  

This problem has excited the condensed matter community because it establishes that graphene, normally viewed as a weakly  interacting system, is a new platform for strongly correlated physics.   

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Add to Calendar 2018-11-29T14:00:00 2018-11-12T15:00:00 Moiré is Different: Wigner Solidification at Magic Angles in Doped Twisted bi-layer Graphene In a recent paper, the MIT group led Pablo Jarillo-Herrero has found that doping twisted bi-layer graphene can generate strongly correlated insulating states and superconductivity at particular twist angles called magic angles.   This problem has excited the condensed matter community because it establishes that graphene, normally viewed as a weakly  interacting system, is a new platform for strongly correlated physics.    Event Location: AMPL 311

November

2018

| Event Location: Hennings 301 | Speaker: Kathleen Foote, PHAS Science Education Specialist

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Physics 301 has been flagged as a challenging course in the department for a myraid of reasons.  First, this is one of the first “advanced” physics courses.  While the content is largely familiar, students must integrate ideas from previous physics and math courses and utilize a coordinated set of tools when solving problems.  Secondly, the class is comprised of 160-180 students from a variety of programs, with variations in prerequisite courses and incoming abilities.  This talk will cover how we’ve utilized the active learning theater (Henn200) to promote collaboration

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Add to Calendar 2018-11-28T15:30:00 2018-11-28T16:30:00 Leveraging Space to Promote Engagement in Intermediate Electricity & Magnetism Physics 301 has been flagged as a challenging course in the department for a myraid of reasons.  First, this is one of the first “advanced” physics courses.  While the content is largely familiar, students must integrate ideas from previous physics and math courses and utilize a coordinated set of tools when solving problems.  Secondly, the class is comprised of 160-180 students from a variety of programs, with variations in prerequisite courses and incoming abilities.  This talk will cover how we’ve utilized the active learning theater (Henn200) to promote collaboration Event Location: Hennings 301

November

2018

| Event Location: Henn 318. 6224 Agricultural Rd. | Speaker: Qingdi Wang, UBC

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We show that when the bare cosmological constant in the Einstein field equations takes large negative values, the average distance between any two nearby geodesics moving in the spacetime sourced by quantum fields vacuum would gradually increase at a slow accelerating rate due to the weak parametric resonance effect caused by the fluctuations of the quantum vacuum energy density.

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Add to Calendar 2018-11-28T13:00:00 2018-11-28T14:00:00 Extreme fine-tuning of the cosmological constant is not needed We show that when the bare cosmological constant in the Einstein field equations takes large negative values, the average distance between any two nearby geodesics moving in the spacetime sourced by quantum fields vacuum would gradually increase at a slow accelerating rate due to the weak parametric resonance effect caused by the fluctuations of the quantum vacuum energy density. Event Location: Henn 318. 6224 Agricultural Rd.

November

2018

| Event Location: Room D207, Buchanan Block D Building | Speaker: ALAN PATRICK MANNING

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Add to Calendar 2018-11-28T12:30:00 2018-11-28T14:30:00 Final Doctoral Oral Examination for ALAN PATRICK MANNING Event Location: Room D207, Buchanan Block D Building

November

2018

| Event Location: Hennings 318 | Speaker: Michael Cushing (University of Toledo)

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ABSTRACT: The study of brown dwarfs with effective temperatures less than 500 K can offer important insights into the complex physics of ultracool atmospheres, the shape of the initial mass function, and the low-mass limit of star formation. We have been using the Wide-field Infrared Survey Explorer (WISE) to search for just such a population of brown dwarfs and have identified roughly twenty cool browns dwarfs that populate a new spectral class, dubbed 'Y'.

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Add to Calendar 2018-11-26T15:00:00 2018-11-26T16:00:00 Hunting for Cool Brown Dwarfs with WISE ABSTRACT: The study of brown dwarfs with effective temperatures less than 500 K can offer important insights into the complex physics of ultracool atmospheres, the shape of the initial mass function, and the low-mass limit of star formation. We have been using the Wide-field Infrared Survey Explorer (WISE) to search for just such a population of brown dwarfs and have identified roughly twenty cool browns dwarfs that populate a new spectral class, dubbed 'Y'. Event Location: Hennings 318

November

2018

| Event Location: Hennings 201 | Speaker: Doug Altshuler (UBC Zoology)

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My research program is motivated by fascination with bird flight. My laboratory group uses a multi- disciplinary approach that includes biomechanics, physiology, and neuroscience to examine flight ability. Our current research is organized around two topics: 1) how birds morph their wings and what benefits this provides; and 2) how optic flow signals are encoded in the avian brain and used to guide their flight. As we gain understanding of flight mechanisms, we further endeavor to apply comparative approaches that provide deeper insight into avian ecology and evolution.

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Add to Calendar 2018-11-22T16:00:00 2018-11-22T17:00:00 Biomechanics and neural control of maneuvering flight My research program is motivated by fascination with bird flight. My laboratory group uses a multi- disciplinary approach that includes biomechanics, physiology, and neuroscience to examine flight ability. Our current research is organized around two topics: 1) how birds morph their wings and what benefits this provides; and 2) how optic flow signals are encoded in the avian brain and used to guide their flight. As we gain understanding of flight mechanisms, we further endeavor to apply comparative approaches that provide deeper insight into avian ecology and evolution. Event Location: Hennings 201

November

2018

| Event Location: BRIM 311 | Speaker: Jian-Hua Jiang, Ph.D., Professor

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Topological insulators are electronic systems with an insulating bulk and topologically protected boundary states. Conventional 2D topological insulators induce 1D edge states. Recent studies indicate that lower-dimensional topological states are also possible in electronic systems through higher-order topology, which, however, has been confirmed only in Bismuth in experiments [1]. In this talk, I will show that lower-dimensional topological wave trapping can be achieved in photonic and acoustic systems through several different mechanisms.

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Add to Calendar 2018-11-22T14:00:00 2018-11-22T15:00:00 CM Seminar: TOPOLOGICAL CAVITY STATES IN TWO-DIMENSIONAL PHOTONIC/PHONONIC CHIPS Topological insulators are electronic systems with an insulating bulk and topologically protected boundary states. Conventional 2D topological insulators induce 1D edge states. Recent studies indicate that lower-dimensional topological states are also possible in electronic systems through higher-order topology, which, however, has been confirmed only in Bismuth in experiments [1]. In this talk, I will show that lower-dimensional topological wave trapping can be achieved in photonic and acoustic systems through several different mechanisms. Event Location: BRIM 311

November

2018

| Event Location: Hennings 318 | Speaker: Megan Ansdell (Berkeley)

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Please join us before the Colloquium in Hennings 318 for coffee, tea and snacks at 2:45 pm

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Add to Calendar 2018-11-19T15:00:00 2018-11-19T16:15:00 To be announced: speaker Megan Ansdell (Berkeley) Please join us before the Colloquium in Hennings 318 for coffee, tea and snacks at 2:45 pm Event Location: Hennings 318

November

2018

| Event Location: Hennings 318 | Speaker: Megan Ansdell (UC Berkeley)

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The advent of space-based telescopes that provide high-precision time-series photometry, such as CoRoT and Kepler/K2, have revealed a zoo of stellar variability on timescales from minutes to months. In this talk, I will focus on classes of objects whose light curves show distinctive "dips" that can tell us a surprising amount about planet formation, evolution, and death. These include disintegrating planets, young dipper systems, likely exocomets, and unlikely alien megastructures.

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Add to Calendar 2018-11-19T15:00:00 2018-11-19T16:00:00 Things that go "dip" in the night: from disintegrating planets to alien megastructures The advent of space-based telescopes that provide high-precision time-series photometry, such as CoRoT and Kepler/K2, have revealed a zoo of stellar variability on timescales from minutes to months. In this talk, I will focus on classes of objects whose light curves show distinctive "dips" that can tell us a surprising amount about planet formation, evolution, and death. These include disintegrating planets, young dipper systems, likely exocomets, and unlikely alien megastructures. Event Location: Hennings 318

November

2018

| Event Location: TRIUMF Conference Room | Speaker: Jia Liu (Princeton)

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The non-zero mass of neutrinos suppresses the growth of cosmic structure on small scales. Since the level of suppression depends on the sum of the masses of the three active neutrino species, the evolution of large-scale structure is a promising tool to constrain the total mass of neutrinos and possibly shed light on the mass hierarchy. I will discuss recent progress and future prospects to constrain the neutrino mass sum with cosmology.

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Add to Calendar 2018-11-19T13:00:00 2018-11-19T14:00:00 Cosmology with Massive Neutrinos The non-zero mass of neutrinos suppresses the growth of cosmic structure on small scales. Since the level of suppression depends on the sum of the masses of the three active neutrino species, the evolution of large-scale structure is a promising tool to constrain the total mass of neutrinos and possibly shed light on the mass hierarchy. I will discuss recent progress and future prospects to constrain the neutrino mass sum with cosmology. Event Location: TRIUMF Conference Room

November

2018

| Event Location: Room 488, The Brimacombe Building, 2355 East Mall | Speaker: JOHN SOUS

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Thesis Abstract:
In this thesis, I investigate the behavior of particles dressed by quantum field excitations and random interactions.

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Add to Calendar 2018-11-16T12:30:00 2018-11-16T14:30:00 Final PhD Oral Examination (Thesis Title: “Peierls Bipolarons and Localization in Solid-State and Molecular Systems") Thesis Abstract: In this thesis, I investigate the behavior of particles dressed by quantum field excitations and random interactions. Event Location: Room 488, The Brimacombe Building, 2355 East Mall

November

2018

| Event Location: BRIM 311 | Speaker: Frank Marsiglio; Dept. of Physics, University of Alberta

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Superconductivity is more than 100 years old, and the established theory of conventional superconductors is more than half as old. But how established is it, and how conventional are the 'old' superconductors? This talk will provide a brief summary of the “state-of-the-art” of superconductivity, and discuss one aspect of pairing that has received some attention lately — “kinetic-energy-induced” pairing. A parable that describes the chemistry of the Helium atom will be used to explain this idea, and how this concept ties in to possible experimental signatures.

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Add to Calendar 2018-11-16T10:00:00 2018-11-16T11:00:00 CM Seminar: Theoretical Description of superconductivity in 2018: a personal assessment Superconductivity is more than 100 years old, and the established theory of conventional superconductors is more than half as old. But how established is it, and how conventional are the 'old' superconductors? This talk will provide a brief summary of the “state-of-the-art” of superconductivity, and discuss one aspect of pairing that has received some attention lately — “kinetic-energy-induced” pairing. A parable that describes the chemistry of the Helium atom will be used to explain this idea, and how this concept ties in to possible experimental signatures. Event Location: BRIM 311

November

2018

| Event Location: Hennings 201 | Speaker: Ian Fisher (Stanford)

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It is common to think of strains in solids in a somewhat passive sense, simply as the response of a material to external forces. However, for certain types of electronic order, strains of a specific symmetry can have much more important roles to play, acting as longitudinal, and even transverse, fields for the order parameter. In this talk, I will first describe how antisymmetric strain can act as a longitudinal field for electronic nematic order. I'll then go on to describe appropriate transverse fields for nematic order, including orthogonal antisymmetric

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Add to Calendar 2018-11-15T16:00:00 2018-11-15T17:00:00 Feeling the strain: fields for electronic nematic order It is common to think of strains in solids in a somewhat passive sense, simply as the response of a material to external forces. However, for certain types of electronic order, strains of a specific symmetry can have much more important roles to play, acting as longitudinal, and even transverse, fields for the order parameter. In this talk, I will first describe how antisymmetric strain can act as a longitudinal field for electronic nematic order. I'll then go on to describe appropriate transverse fields for nematic order, including orthogonal antisymmetric Event Location: Hennings 201

November

2018

| Event Location: Earth Sciences Building - RM 1013 (2207 Main Mall) UBC | Speaker: Matthew Fisher - University of California, Santa Barbara

The effort to design and build quantum computers in the laboratory is now a billion dollar enterprise. But might we, ourselves, be quantum computers? Most scientists think that in the warm wet brain, this is highly unlikely; and certainly it would be at variance with what the medical profession believes. My strategy is one of reverse engineering, seeking to identify the biochemical substrate and mechanisms that could host such putative quantum processing.

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Add to Calendar 2018-11-14T19:30:00 2018-11-14T21:00:00 Are We Quantum Brains, or Merely Clever Robots? The effort to design and build quantum computers in the laboratory is now a billion dollar enterprise. But might we, ourselves, be quantum computers? Most scientists think that in the warm wet brain, this is highly unlikely; and certainly it would be at variance with what the medical profession believes. My strategy is one of reverse engineering, seeking to identify the biochemical substrate and mechanisms that could host such putative quantum processing. Event Location: Earth Sciences Building - RM 1013 (2207 Main Mall) UBC

November

2018

| Event Location: Henn room 318, 6224 Agricultural Road | Speaker: Andrei O. Barvinsky, Theory Department, Lebedev Physics Institute, Russia.

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Using the background-field method we demonstrate the Becchi-Rouet-Stora-Tyutin (BRST) structure of counterterms in a broad class of gauge theories. Put simply, we show that gauge invariance is preserved by renormalization in local gauge field theories whenever they admit a sensible background-field formulation and anomaly-free path integral measure. This class encompasses Yang--Mills theories and relativistic gravity, including both renormalizable and non-renormalizable (effective) theories.

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Add to Calendar 2018-11-14T13:00:00 2018-11-14T14:00:00 Renormalization of gauge theories and asymptotic freedom of Horava-Lifshitz gravity Using the background-field method we demonstrate the Becchi-Rouet-Stora-Tyutin (BRST) structure of counterterms in a broad class of gauge theories. Put simply, we show that gauge invariance is preserved by renormalization in local gauge field theories whenever they admit a sensible background-field formulation and anomaly-free path integral measure. This class encompasses Yang--Mills theories and relativistic gravity, including both renormalizable and non-renormalizable (effective) theories. Event Location: Henn room 318, 6224 Agricultural Road

November

2018

| Event Location: Where you choose to observe |

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Add to Calendar 2018-11-12T15:00:00 2018-11-12T16:15:00 REMEMBRANCE DAY OBSERVANCE - No Astronomy Colloquium today Event Location: Where you choose to observe

November

2018

| Event Location: Hennings 201 | Speaker: Kari Dalnoki-Veress (McMaster)

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The physics of soft materials is distinct from hard matter, as the weaker intermolecular bonds can result in a large response to external stresses. In recent years, there has been a significant interest in understanding the interaction between a liquid’s surface tension and a solid’s elasticity: elastocapillarity. In particular, liquids can generate significant deformations of highly compliant materials.

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Add to Calendar 2018-11-08T16:00:00 2018-11-08T17:00:00 Soft Materials at surfaces and interfaces: Elastocapillarity The physics of soft materials is distinct from hard matter, as the weaker intermolecular bonds can result in a large response to external stresses. In recent years, there has been a significant interest in understanding the interaction between a liquid’s surface tension and a solid’s elasticity: elastocapillarity. In particular, liquids can generate significant deformations of highly compliant materials. Event Location: Hennings 201

November

2018

| Event Location: TRIUMF Auditorium | Speaker: Clifford Cheung (Caltech)

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Scattering amplitudes are fundamental observables that encode the dynamics of interacting particles. In this talk, I describe how to systematically construct these objects without reference to a Lagrangian or an underlying spacetime. The physics of real-world particles like gravitons, gluons, and pions are thus derived from the properties of amplitudes rather than vice versa. Remarkably, the expressions gleaned from this line of attack are marvelously simple, revealing new structures long hidden in plain sight.

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Add to Calendar 2018-11-08T14:00:00 2018-11-08T15:00:00 Unification from Scattering Amplitudes Scattering amplitudes are fundamental observables that encode the dynamics of interacting particles. In this talk, I describe how to systematically construct these objects without reference to a Lagrangian or an underlying spacetime. The physics of real-world particles like gravitons, gluons, and pions are thus derived from the properties of amplitudes rather than vice versa. Remarkably, the expressions gleaned from this line of attack are marvelously simple, revealing new structures long hidden in plain sight. Event Location: TRIUMF Auditorium

November

2018

| Event Location: Hennings 318 | Speaker: Nina Hernitschek (Caltech)

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Every night, telescopes around the world obtain a flood of new data as parts of deep and wide surveys. This amount of data will steeply rise once upcoming sureys such as the Large Synoptic Survey Telescope (LSST), which will image the entire visible sky every few nights, start their operation. To investigate this huge amount of data, machine-learning algorithms are absolutely necessary for image analysis, classification of sources, time-series analysis and also structure finding.

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Add to Calendar 2018-11-05T15:00:00 2018-11-05T16:00:00 A machine-learning view of our Milky Way Every night, telescopes around the world obtain a flood of new data as parts of deep and wide surveys. This amount of data will steeply rise once upcoming sureys such as the Large Synoptic Survey Telescope (LSST), which will image the entire visible sky every few nights, start their operation. To investigate this huge amount of data, machine-learning algorithms are absolutely necessary for image analysis, classification of sources, time-series analysis and also structure finding. Event Location: Hennings 318

November

2018

| Event Location: TRIUMF Auditorium | Speaker: Deborah Harris (Fermilab/York U)

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The fact that neutrinos have mass and change flavors means that we can learn a great deal about them by studying what are effectively interference patterns that arise after neutrinos propagate over hundreds of kilometers. The DUNE experiment will measure these interference patterns over a broad neutrino energy range after neutrinos have propagated 1300km. In addition, DUNE will use a detector technology that provides exquisite detail about the interactions that make up the interference pattern.

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Add to Calendar 2018-11-05T14:00:00 2018-11-05T15:00:00 Neutrino Interferometry at DUNE: Preparing for the Deep Underground Neutrino Experiment The fact that neutrinos have mass and change flavors means that we can learn a great deal about them by studying what are effectively interference patterns that arise after neutrinos propagate over hundreds of kilometers. The DUNE experiment will measure these interference patterns over a broad neutrino energy range after neutrinos have propagated 1300km. In addition, DUNE will use a detector technology that provides exquisite detail about the interactions that make up the interference pattern. Event Location: TRIUMF Auditorium

November

2018

| Event Location: Room 309, Hennings Building | Speaker: LEONARD RUOCCO

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I investigate the dynamics of multi-state central systems coupled bilinearly to an external oscillator bath within the noninteracting-blip approximation. I focus on both a 3-site configuration, as well as a 2-site model for the central systems of interest.

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Add to Calendar 2018-11-05T12:00:00 2018-11-05T14:00:00 Departmental Oral Examination (Thesis Title: “Modelling exciton dynamics in light-harvesting molecules”) I investigate the dynamics of multi-state central systems coupled bilinearly to an external oscillator bath within the noninteracting-blip approximation. I focus on both a 3-site configuration, as well as a 2-site model for the central systems of interest. Event Location: Room 309, Hennings Building

November

2018

| Event Location: Hennings 201 | Speaker: Erich Mueller (Cornell)

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Physicists have been exploring techniques for the controlled manipulation of large collections of quantum objects.  A valuable strategy has been placing collections of laser-cooled atoms in optical cavities.  I will review the state of the field, some of the underlying physics, and the outlook.

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Add to Calendar 2018-11-01T16:00:00 2018-11-01T17:00:00 Atoms in Cavities Physicists have been exploring techniques for the controlled manipulation of large collections of quantum objects.  A valuable strategy has been placing collections of laser-cooled atoms in optical cavities.  I will review the state of the field, some of the underlying physics, and the outlook. Event Location: Hennings 201

October

2018

| Event Location: Hennings 318 | Speaker: Marcel Pawlovski (UC Irvine)

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Major galaxies such as the Milky Way are surrounded by swarms of smaller dwarf satellite galaxies. Over the past 15 years, our knowledge of these satellite galaxies has exploded. The number of known Milky Way satellites has quadrupled, and highly precise measurements of their motions, with the Hubble Space Telescope and most recently with Gaia, have provided unprecedented insights into their complex orbital dance.

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Add to Calendar 2018-10-29T15:00:00 2018-10-29T16:15:00 Dark Matter and the Dance of Dwarf Galaxies Major galaxies such as the Milky Way are surrounded by swarms of smaller dwarf satellite galaxies. Over the past 15 years, our knowledge of these satellite galaxies has exploded. The number of known Milky Way satellites has quadrupled, and highly precise measurements of their motions, with the Hubble Space Telescope and most recently with Gaia, have provided unprecedented insights into their complex orbital dance. Event Location: Hennings 318

October

2018

| Event Location: Hennings 318 |

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What is the Equity and Inclusion in PHAS group? Come to our open house to learn about our mission, what we are doing to help promote opportunities for our community, how to get involved, and learn about equity issues. We are offering a lunch and poster session to mingle with everyone in our department to engage in the conversation around equity, inclusion and diversity.

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Add to Calendar 2018-10-26T12:30:00 2018-10-26T17:00:00 Equity and Inclusion Open House What is the Equity and Inclusion in PHAS group? Come to our open house to learn about our mission, what we are doing to help promote opportunities for our community, how to get involved, and learn about equity issues. We are offering a lunch and poster session to mingle with everyone in our department to engage in the conversation around equity, inclusion and diversity. Event Location: Hennings 318

October

2018

| Event Location: Hennings 201 | Speaker: Prineha Narang (Harvard)

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Add to Calendar 2018-10-25T16:00:00 2018-10-25T18:00:00 Excited-State Dynamics and Quantum Interaction from First Principles Event Location: Hennings 201

October

2018

| Event Location: AMPL 311 | Speaker: Prof. Prineha Narang, from Harvard University

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Today, we imagine a world where we can engineer materials and devices atom-by-atom. Exciting discoveries during the past few decades in quantum science and technology have brought us to this next step in the quantum revolution: the ability to fabricate, image and measure materials and their properties at the level of single atoms is almost within our grasp. Yet, at the most fundamental level a tractable quantum mechanical description and understanding of these materials does not exist.

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Add to Calendar 2018-10-25T14:00:00 2018-10-25T15:00:00 Linear-, Nonlinear- and Hydrodynamics in Quantum Materials. Today, we imagine a world where we can engineer materials and devices atom-by-atom. Exciting discoveries during the past few decades in quantum science and technology have brought us to this next step in the quantum revolution: the ability to fabricate, image and measure materials and their properties at the level of single atoms is almost within our grasp. Yet, at the most fundamental level a tractable quantum mechanical description and understanding of these materials does not exist. Event Location: AMPL 311

October

2018

| Event Location: Henn 318 | Speaker: Ramon Gonzales Masachs. He completed his MSc at the University of Barcelona and is currently pursuing his PhD at the University of Southampton, under the supervision of Dr Oscar Dias.

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Reissner-Nordstrom black holes (RN BH) in AdS suffer from two linear instabilities, superradiance and the near horizon instability. The endpoint of these instabilities is a hairy black hole. I will present an analytic perturbative construction of these hairy black holes and analyse the phase space of solutions. In asymptotically flat spacetime, inspired by the black hole bomb of Press and Teukolsky, one can surround a RN BH by a reflecting box. It is known that this system suffers from superradiant instability. We show that the near horizon instability is also present there.

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Add to Calendar 2018-10-24T13:00:00 2018-10-24T14:00:00 Instabilities of charged black holes and small hairy black holes Reissner-Nordstrom black holes (RN BH) in AdS suffer from two linear instabilities, superradiance and the near horizon instability. The endpoint of these instabilities is a hairy black hole. I will present an analytic perturbative construction of these hairy black holes and analyse the phase space of solutions. In asymptotically flat spacetime, inspired by the black hole bomb of Press and Teukolsky, one can surround a RN BH by a reflecting box. It is known that this system suffers from superradiant instability. We show that the near horizon instability is also present there. Event Location: Henn 318

October

2018

| Event Location: Hennings 318 | Speaker: Jessie Christensen (Caltech, NASA Exoplanet Science Institute)

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Please join us before the Colloquium in Hennings 318 for coffee, tea and snacks at 2:45 pm

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Add to Calendar 2018-10-22T15:00:00 2018-10-22T16:00:00 Ten Thousand Pieces of Blue Sky: Building towards the complete picture of exoplanet demographics Please join us before the Colloquium in Hennings 318 for coffee, tea and snacks at 2:45 pm Event Location: Hennings 318

October

2018

| Event Location: Life 2602 | Speaker: Corinne Manogue

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Physics is the study of change. In many cases, this change involves more than one independent and one dependent physical quantity. In these cases the partial derivative is an important tool, including the geometric combinations of partial derivatives in E & M (e.g. gradient) and the measurable combinations in thermodynamics (e.g. heat capacity).

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Add to Calendar 2018-10-19T10:00:00 2018-10-19T23:00:00 Exploring Rates of Change in Calculus and Upper-Level Physics Courses Physics is the study of change. In many cases, this change involves more than one independent and one dependent physical quantity. In these cases the partial derivative is an important tool, including the geometric combinations of partial derivatives in E & M (e.g. gradient) and the measurable combinations in thermodynamics (e.g. heat capacity). Event Location: Life 2602

October

2018

| Event Location: Hennings 201 | Speaker: Andy Bunn (Western Washington University)

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Add to Calendar 2018-10-18T16:00:00 2018-10-18T17:00:00 Occam's Razor and Climate Change: How to Explain Climate Change to Non-Scientists Event Location: Hennings 201