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Format results
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Talk
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Welcome and Opening Remarks
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Roger Melko University of Waterloo
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Shailesh Chandrasekharan Duke University
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Ribhu Kaul University of Kentucky
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Blackboard Talk 1 - Virtual
Senthil Todadri Massachusetts Institute of Technology (MIT) - Department of Physics
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Blackboard Talk 2
Senthil Todadri Massachusetts Institute of Technology (MIT) - Department of Physics
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Reducing the Sign Problem with Complex Neural Networks
Johann Ostmeyer University of Liverpool
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Self dual U(1) lattice field theory with a theta-term
Christoff Gatringer FWF Austrian Science Fund
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Quantum electrodynamics with massless fermions in three dimensions - Talk 1
Rajamani Narayanan Florida International University
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Quantum electrodynamics with massless fermions in three dimensions - Talk 2
Rajamani Narayanan Florida International University
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Talk
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Quantum Information and holography
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Aaron Szasz Alphabet (United States)
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Beni Yoshida Perimeter Institute for Theoretical Physics
PIRSA:22050006 -
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Quantum Information and holography
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Aaron Szasz Alphabet (United States)
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Beni Yoshida Perimeter Institute for Theoretical Physics
PIRSA:22050005 -
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Quantum Information and holography
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Aaron Szasz Alphabet (United States)
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Beni Yoshida Perimeter Institute for Theoretical Physics
PIRSA:22050004 -
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Quantum Information and holography
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Aaron Szasz Alphabet (United States)
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Beni Yoshida Perimeter Institute for Theoretical Physics
PIRSA:22040054 -
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Quantum Information and holography
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Aaron Szasz Alphabet (United States)
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Beni Yoshida Perimeter Institute for Theoretical Physics
PIRSA:22040053 -
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Quantum Information and holography
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Aaron Szasz Alphabet (United States)
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Beni Yoshida Perimeter Institute for Theoretical Physics
PIRSA:22040052 -
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Quantum Information and holography
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Aaron Szasz Alphabet (United States)
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Beni Yoshida Perimeter Institute for Theoretical Physics
PIRSA:22040051 -
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Quantum Information and holography
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Aaron Szasz Alphabet (United States)
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Beni Yoshida Perimeter Institute for Theoretical Physics
PIRSA:22040050 -
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Talk
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Talk
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Machine Learning (2021/2022)
Lauren Hayward Perimeter Institute for Theoretical Physics
PIRSA:22050009 -
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Machine Learning (2021/2022)
Lauren Hayward Perimeter Institute for Theoretical Physics
PIRSA:22040073 -
Machine Learning (2021/2022)
Lauren Hayward Perimeter Institute for Theoretical Physics
PIRSA:22040072 -
Machine Learning (2021/2022)
Lauren Hayward Perimeter Institute for Theoretical Physics
PIRSA:22040071
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Talk
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Cosmology
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Kendrick Smith Perimeter Institute for Theoretical Physics
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Gang Xu Perimeter Institute for Theoretical Physics
PIRSA:22050017 -
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Cosmology (2021/2022)
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Kendrick Smith Perimeter Institute for Theoretical Physics
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Gang Xu Perimeter Institute for Theoretical Physics
PIRSA:22050013 -
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Cosmology (2021/2022)
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Kendrick Smith Perimeter Institute for Theoretical Physics
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Gang Xu Perimeter Institute for Theoretical Physics
PIRSA:22050012 -
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Cosmology (2021/2022)
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Kendrick Smith Perimeter Institute for Theoretical Physics
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Gang Xu Perimeter Institute for Theoretical Physics
PIRSA:22040085 -
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Cosmology (2021/2022)
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Kendrick Smith Perimeter Institute for Theoretical Physics
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Gang Xu Perimeter Institute for Theoretical Physics
PIRSA:22040084 -
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Cosmology (2021/2022)
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Kendrick Smith Perimeter Institute for Theoretical Physics
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Gang Xu Perimeter Institute for Theoretical Physics
PIRSA:22040086 -
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Cosmology (2021/2022)
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Kendrick Smith Perimeter Institute for Theoretical Physics
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Gang Xu Perimeter Institute for Theoretical Physics
PIRSA:22040083 -
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Cosmology (2021/2022)
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Kendrick Smith Perimeter Institute for Theoretical Physics
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Gang Xu Perimeter Institute for Theoretical Physics
PIRSA:22040082 -
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Talk
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Talk
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Welcome and Opening Remarks
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William East Perimeter Institute for Theoretical Physics
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Reed Essick University of Toronto
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Luis Lehner Perimeter Institute for Theoretical Physics
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Daniel Siegel University of Greifswald
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Suvodip Mukherjee Tata Institute of Fundamental Research (TIFR)
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Huan Yang Tsinghua University
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Measure the cosmic expansion history of the Universe using GW sources
Jonathan Gair Max Planck Institute for Gravitational Physics (Albert Einstein Institute)
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Cross-correlation technique in GW cosmology
Benjamin Wandelt Institut d'Astrophysique de Paris
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Matter in Extreme Conditions
Katerina Chatziioannou California Institute of Technology (Caltech)
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Matter Effects in Waveform Models
Geraint Pratten University of Birmingham
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Dark matter, PBHs, boson clouds
Salvatore Vitale Massachusetts Institute of Technology (MIT)
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Multi-band GW observation from the third-generation detectors
Hsin-Yu Chen Massachusetts Institute of Technology (MIT)
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Pulsar Timing Arrays
Xavier Siemens Oregon State University
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Quantum Criticality: Gauge Fields and Matter
Quantum Criticality: Gauge Fields and Matter -
Physics with Trapped Atoms, Molecules and Ions (HYBRID)
The primary motivation of this meeting is to bring together investigators from diverse areas of ultracold AMO physics & quantum optics and discuss the nuts-and-bolts of recent developments in the field and find common grounds to cross-pollinate ideas. The primary emphasis will be on contemporary topics currently being pursued by Indian researchers. The meeting will be held in a hybrid offline-online mode.This is the second in the series of TAMIONs meetings. The topics are:Ultracold atoms, molecules and ionsQuantum opticsQuantum thermodynamics and simulationEligibility:Physical participation is by invitation only. For online participation, we encourage faculty members, young researchers and students (who have completed at least 1 year of MSc by May 2022) to apply online. ICTS is committed to building an environment that is inclusive, non-discriminatory and welcoming of diverse individuals. We especially encourage the participation of women and other under-represented groups.
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Physics with Trapped Atoms, Molecules and Ions (HYBRID)
The primary motivation of this meeting is to bring together investigators from diverse areas of ultracold AMO physics & quantum optics and discuss the nuts-and-bolts of recent developments in the field and find common grounds to cross-pollinate ideas. The primary emphasis will be on contemporary topics currently being pursued by Indian researchers. The meeting will be held in a hybrid offline-online mode.This is the second in the series of TAMIONs meetings. The topics are:Ultracold atoms, molecules and ionsQuantum opticsQuantum thermodynamics and simulationEligibility:Physical participation is by invitation only. For online participation, we encourage faculty members, young researchers and students (who have completed at least 1 year of MSc by May 2022) to apply online. ICTS is committed to building an environment that is inclusive, non-discriminatory and welcoming of diverse individuals. We especially encourage the participation of women and other under-represented groups.
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Future Flavours: Prospects for Beauty, Charm and Tau Physics (ONLINE)
Flavour physics, the study of weak interactions of quarks and leptons, is in an exciting period with various anomalies observed in the decays of B mesons and processes involving muons, as well as LHC Run-3 starting operation in 2022 while the Belle II B factory steadily accumulating data. Conclusive evidence as to whether this sector of the standard model of particle physics is broken may be just around the corner. The programme will offer a pedagogical introduction to experimental and phenomenological flavour physics through seven brief lecture courses, followed by a three-day topical conference. The lecture courses will introduce flavour phenomenology within the standard model and beyond, as well as explaining the role of quantum chromodynamics. In addition, there will be lectures about the experimental techniques employed at the LHC and in electron-positron collisions. The concluding topical conference will review the latest results and prospects in the field of flavour physics.Elig...
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Future Flavours: Prospects for Beauty, Charm and Tau Physics (ONLINE)
Flavour physics, the study of weak interactions of quarks and leptons, is in an exciting period with various anomalies observed in the decays of B mesons and processes involving muons, as well as LHC Run-3 starting operation in 2022 while the Belle II B factory steadily accumulating data. Conclusive evidence as to whether this sector of the standard model of particle physics is broken may be just around the corner. The programme will offer a pedagogical introduction to experimental and phenomenological flavour physics through seven brief lecture courses, followed by a three-day topical conference. The lecture courses will introduce flavour phenomenology within the standard model and beyond, as well as explaining the role of quantum chromodynamics. In addition, there will be lectures about the experimental techniques employed at the LHC and in electron-positron collisions. The concluding topical conference will review the latest results and prospects in the field of flavour physics.Elig...
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Quantum Information and holography (2021/2022)
Topics will include (but are not limited to): - Quantum error correction in quantum gravity and condensed matter - Quantum information scrambling and black hole information - Physics of random tensor networks and random unitary circuits -
Quantum Gravity (2021-2022)
Topics will include (but are not limited to): Canonical formulation of constrained systems, The Dirac program, First order formalism of gravity, Loop Quantum Gravity, Spinfoam models, Research at PI and other approaches to quantum gravity. -
Machine Learning (2021/2022)
This course is designed to introduce modern machine learning techniques for studying classical and quantum many-body problems encountered in condensed matter, quantum information, and related fields of physics. Lectures will focus on introducing machine learning algorithms and discussing how they can be applied to solve problem in statistical physics. Tutorials and homework assignments will concentrate on developing programming skills to study the problems presented in lecture. -
Cosmology (2021/2022)
This class is an introduction to cosmology. We'll cover expansion history of the universe, thermal history, dark matter models, and as much cosmological perturbation theory as time permits. -
Strong Gravity (2021/2022)
This course will introduce some advanced topics in general relativity related to describing gravity in the strong field and dynamical regime. Topics covered include properties of spinning black holes, black hole thermodynamics and energy extraction, how to define horizons in a dynamical setting, formulations of the Einstein equations as constraint and evolution equations, and gravitational waves and how they are sourced. -
Gravitational Waves Beyond the Boxes II
Gravitational Waves Beyond the Boxes II -
Waves, Instabilities and Mixing in Rotating and Stratified Flows (ONLINE)
Waves are ubiquitous in natural fluid systems like the Earth's ocean, planetary atmosphere, and the interior of stars and planets. Stratification (owing to spatial variations of temperature, salinity, gravity or magnetic field) and/or Coriolis effects (owing to the rotation of planets & stars) represent key physical ingredients of wave generation, propagation and dissipation in many of these large-scale systems. Together with the significant amounts of energy input into them, the ability of waves to transport energy and momentum (and maybe mass too) through large spatial extents has significant implications for (i) global flow features like oceanic or atmospheric circulation, mean temperature distribution in planets/stars etc., (ii) the overall energy budget, and (iii) biological activity in the ocean. Furthermore, it is now widely recognized that wave dissipation mechanisms (and the resulting generation of heat and mixing) have to be accurately parameterized in global scale numerical ...